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##  Appendix A Outliers

###  A.1 Literature comparison outliers

Below, we list and discuss the discrepant periods between this work and the
literature described in Section 4.2 and shown in Fig. 3. We distinguish
between cases where the periods are likely harmonically related (Sect. A.1.1)
and those lacking a straightforward explanation (Sect. A.1.2). We note again
that this is not an exhaustive list of all instances where measured periods
disagree. Instead, these examples illustrate the type and extent of deviations
confronted, as well as the thought processes and evidence used to decide on
the best period we adopt. For each case, we also present final period
assessments, following the reasoning described here and mirroring the
guidelines given in Sect. 4.5.

####  A.1.1 Harmonics

When two contending periods are harmonics of each other, it is in general
expected that one of them, typically the larger one, is correct. This is
because the first harmonic of the true period can manifest itself as the
prevailing period of modulation when, for example, the star’s spot
distribution is bimodal across its hemispheres, resulting in a ‘double-
dipping’ feature throughout each full rotation (e.g. Basri & Shah 2020;
Jeffers et al. 2022; Schöfer et al. 2022). On the other hand, there is no
simple mechanism that may explain the production of one dip over two
rotations. While the double-dip phenomenon is usually temporary and minute
differences in the dip morphologies may be resolved with high-precision, high-
cadence photometric data, it is more difficult to distinguish nearly equal-
sized dips in ground-based data or data that cover only a short time baseline.
We evaluate the following cases with this principle in mind.

##### J01019+541.

The best TESS period of 0.139 d is exactly half that from MEarth data 0.278 d
(DA19, Newton et al. 2016b). We give preference to the longer period from the
literature.

##### J04173+088.

The period of this fast rotator was measured to be 0.185 d using MEarth data
(West et al. 2015). However, both the TESS light curve and SuperWASP data
spanning 6 seasons unambiguously indicate a period of 0.3697 d, exactly twice
as long (see discussion in Johnson et al. 2021). We strongly favour the longer
period from our work.

##### J10182$-$204.

Baroch et al. (2018) obtained a period of 7.3 d from archival SuperWASP data.
TESS SAP light curves resolve a double-dipping modulation pattern with
periodicity twice that at 14.5 d, which we deem to be convincing.

##### J16581+257.

The period measured from one season of SuperWASP observations is 11.73 d,
about half that reported from ASAS data in the literature (23.8 d, DA19,
Oelkers et al. 2018). We consider the longer periods to be correct.

##### J20450+444.

DA19 measured a 19.9 d period from archival SuperWASP data. However, a period
of $\sim 39$ d, about twice the literature period, is implicated in
spectroscopic indicators (the two Ca-IRT lines, H$\alpha$, and TiO). In fact,
TESS SAP light curves also rule the shorter period for J20450+444 as
implausible. Therefore, we update this period to the longer one from our work.

In a couple of cases, there is additional evidence in favour of the shorter
period:

##### J06371+175.

A 37 d period is strongly implicated by APT photometry presented in the planet
discovery paper of Luque et al. (2022) and also significant in both seasons of
SuperWASP data. Although the second season of SuperWASP data slightly prefers
a $\sim 74$ d period, we still adopted the shorter period.

##### J20525$-$169.

The literature period is $\sim$68 d (ASAS, DA19, Suárez Mascareño et al. 2016)
or 85 d (MEarth, Newton et al. 2018), which are approximately yearly aliases
of one another, and 134 d from our work in H$\alpha$ and Ca-IRTb, nearly
exactly twice the ASAS period. We adopted the 68 d period but note that it is
‘debated’.

####  A.1.2 Other discrepant cases

##### J03213+799.

The literature measurement of 32.4 d is based on photometric data from
AstroLAB that were available at the time. In this work, we perform a new
analysis using a more complete light curve from AstroLAB. To be conservative,
we indicate that the new period is still ‘debated’ and would benefit from
further confirmation.

##### J03463+262.

The literature value of $\sim 16$ d comes from KELT photometry (Oelkers et al.
2018), and is supported by SuperWASP data as well as Ca-IRTa. However,
multiple spectroscopic indicators H$\alpha$, Ca-IRTb, and TiO show a $\sim 10$
d period. We prefer the value derived from photometry, but indicate that it is
‘debated’.

##### J04153$-$076.

This active mid-M dwarf ($pEW^{\prime}_{\rm H\alpha}=-3.3\AA$) is expected to
have a relatively short period. Using CARMENES data, Lafarga et al. (2021)
detected a significant signal at 1.8 d in three spectroscopic indicators: RV,
CRX, and BIS. With the latest spectroscopic time series, we detect a 8.56 d
period in the two Ca-IRTab lines. The measured $v\sin i=2.2$ km/s indicates
that the $P_{\rm rot}\lesssim 6$ d, slightly preferring the value from Lafarga
et al. (2021). However, the limited precision in $v\sin i$ means the 8 d
period can also be easily accommodated. We take the period in this work as the
nominal ‘best’ period, but designate it as ‘debated’.

##### J05337+019.

SB1 analyzed in detail by Baroch et al. (2021). The rotation period of 0.6 d
robustly determined from TESS (see Figure 19) and unbinned SuperWASP data
agree with each other and also with the orbital period of the binary, as
measured from RV, which is consistent with tidal synchronization. One of the
reported periods in the literature is 2.8 d, which is an alias of the 0.6 d
period. Therefore, we are confident in the 0.6 d period derived in this work
and assign it a ‘secure’ rating.

##### J09140+196.

The literature period of 89.9 d comes from DA19’s analysis of archival ASAS
data, whereas the SuperWASP data exhibit an unequivocal sinusoidal signal at
39 d over a 127 d time baseline. The same SuperWASP data were analyzed in
Baroch et al. (2021), reaching a similar value. It is possible that the two
periods are harmonically related. However, a reanalysis of the data used by
DA19 shows that the 89.9 d peak, while formally significant, competes with
many other peaks of similar or greater height, therefore cannot be
unambiguously interpreted. Therefore, we prefer the $\sim 39$ d period, but
indicate it as ‘provisional’.

##### J11000+228.

The literature period is 171 d from longitudinal B-fields (Donati et al.
2023), which is rather long for an early-M dwarf. We see a much shorter, 53 d
period in both TiO and $R^{\prime}_{\rm HK}$ time series, corroborated at
least tentatively by SuperWASP light curves. We deem our period to be more
reasonable, and brand it as ‘secure’ owing to multiple lines of support.

##### J11509+483.

This star has many periods in the literature. Earlier works measured a period
of $\sim$125 d (Irwin et al. 2011; Newton et al. 2016b; Díez Alonso et al.
2019), all based on MEarth data. However, a new analysis of the latest MEarth
data presented a longer period at 149 d (Medina et al. 2022), and subsequent
measurements using spectropolarimetric time series support this longer period
of Medina et al. (2022) (158 d and 176 d, Fouqué et al. 2023; Donati et al.
2023, respectively). Three of our spectroscopic indicator time series
(H$\alpha$, Ca-IRTb, TiO) show an $\sim$83 d period, which could represent the
first harmonic of the longer periods. We list the $P_{\rm rot}$ of (Medina et
al. 2022), the middle ground within $\sim 15$% of all the available
measurements, as the best period with a ‘secure’ rating.

##### J12230+640.

The literature period of 32.9 d originates from the analysis of archival NSVS
photometry data by DA19. The Ca-IRT time series contains 151 epochs and
reveals a 51.5 d signal, which incidentally coincides with a smaller peak in
the NSVS data. While we deem the photometric period more likely to be correct,
the veracity of the other signal cannot be ruled out. Therefore, we list the
DA19 period as the best period with a ‘debated’ designation.

##### J14257+236E.

The period from DA19 is 17.6 d and is derived from unbinned public SuperWASP
data. A reanalysis of the same data with daily binning shows that this peak,
while present, is not formally significant. Multiple spectroscopic indicators
(H$\alpha$, Ca-IRT) reflect a period of $\sim 12.8$ d, casting further doubt
into the photometric period but not enough to flat-out refute it. Therefore,
we list the DA19 period as the best period but flag it as ‘debated’.

##### J14321+081.

The 0.757 d period comes from MEarth data recently presented by Pass et al.
(2023) and previously by Newton et al. (2016b) as a ‘U’-rotator. This is a
very faint ($V>$ 15 mag) but very active late-M star whose $v\sin i$ bounds
the period to $\lesssim 1.7$ d (see also Section 4.3). While our unbinned
SuperWASP data exhibit a highly significant period at 1.115 d and 1.025 d (and
their aliases) in the first season, the weight of the two literature values in
agreement tips the value in favour of the shorter period, which we indicate as
‘secure’.

##### J19346+045.

The literature value of 12.9 d (DA19) is from ASAS photometry with FAP =
0.33%. We find a 21.8 d period in H$\alpha$ and Ca-IRTab. An identical period
in dLW (Lafarga et al. 2021) strengthens our preference for the longer period
measured in this work, which we assign as the best period with a rating of
‘secure’.

##### J23381$-$162.

The literature value of 61.66 d comes from Watson et al. (2006), which refers
to the AAVSO database of variable stars. The SuperWASP data show conflicting
periods (therefore a U-designation). While there is a large-amplitude
sinusoidal signal of $\sim 91$ d in season 6, a similarly clear signal at
$\sim 54$ d in season 7 is only slightly less formally significant. In
summary, we consider the evidence insufficient to reject the period in the
literature, though flag it as ‘debated’.

###  A.2 $v\sin i$ outliers

Here we list and describe the $v\sin i$ outliers as shown in Figure 4 in
Section 4.3.

##### J05337+019.

This is an SB1 analyzed in detail in Baroch et al. (2021), with the companion
suspected to be a white dwarf (See also Section A.1). The $v\sin i$
measurement implicates a maximum rotation period of 2.5 d (1$\sigma$: 3.2 d),
which is completely consistent with the rotational modulation of 0.6 d well-
resolved in TESS and SuperWASP data. Oelkers et al. (2018) found a period of
2.8 d, which is an alias of 0.6 d. The clearly contradicting period of 18.4 d
is from Howard et al. (2020).

##### J10584$-$107.

The $v\sin i$ measurement implicates a maximum rotation period of 3.7 d
(1$\sigma$: 13 d). The SuperWASP data give a 28 d period which, as discussed
in Section 3.1.1, is suspected to be moon-related and likely to be unreliable.

##### J18356+329.

With $P_{\rm rot}\sim 0.1$ d, this is the fastest rotator in the sample.
$P_{\rm max}=0.089$ d and the $1\sigma$ upper bound is 0.103 d, which is only
marginally exceeded by all the photometric measurements of 0.118 d (e.g. DA19,
TESS). The discrepancy could be easily accounted for if the error on either
$v\sin i$ or $R_{\star}$ is slightly underestimated.

##### J19169+051S.

This very late-type (M8V) and faint star is in a wide binary with J19169+051N
(73$\aas@@fstack{\prime\prime}$8). It exhibits very large H$\alpha$ activity,
although at its radius ($\sim 0.1R_{\star}$) the saturation period is $\sim
150$ d (see Section 5.1), which implies that even extremely slow rotators can
be expected to display considerable level of activity. The $v\sin i$
measurement constrains the maximum period to be $\sim 1.4$ d ($1\sigma$ upper
limit is 3.2 d), which severely contradicts the photometric rotation period of
23.6 d reported by DA19. However, it is worth noting that the DA19 period
comes from MEarth, the same data that led Newton et al. (2016b) to conclude
that no reliable period can be derived.

##### J06574+740, J20305+654.

The measured $P_{\rm rot}$ for these stars exceed their expected $P_{\rm
rot,max}$ by 16%, just over the threshold of 15%. They could be easily
explained if errors in the stellar radius or rotational velocity are slightly
underestimated. J06574+740 is interesting because its light curve from every
sector shows a beat pattern of two closely-spaced frequencies at 0.61 and 0.63
d (see Fig. 20). This star is catalogued in Gaia as a duplicate source and has
a high astrometric excess noise. Furthermore, it has been classified as RV-
loud after the criteria of Tal-Or et al. (2018), exhibiting peak-to-peak RV
variability of ¿ 600 m/s over 11 epochs of monitoring (spread over 450 d).
Both clues indicate that this object could be an unresolved binary. However,
in this interpretation, the apparent spin-synchronization of the binary
components at $\sim 0.6$ d is more difficult to explain. The RV amplitude of
an equal-mass binary consistent with the observed spectral type and spin-orbit
synchronized at 0.6 d is expected to be of order $\sim 100$ km/s. On the other
hand, the fact that J06574+740 does not show overluminosity in a colour-
magnitude diagram argues against the binary hypothesis. The beating pattern
could also be due to two latitudinally displaced spots exhibiting differential
rotation (see, e.g. Nagel et al. 2016). In both possible scenarios, the
modulation signal is attributed to rotation and has relatively good
consistency with the measured H$\alpha$ activity and $v\sin i$. We consider
the most significant of the two peaks at 0.61 d to be the ‘securely’
determined $P_{\rm rot}$ for this target, and recommend follow-up observations
to resolve the nature of this system.

###  A.3 $pEW^{\prime}_{\rm H\alpha}$ outliers

In Fig. 5 of Sect. 4.4, the clump of extreme outliers with $P_{\rm
rot}\lesssim 1$ d correspond to measurements from Oelkers et al. (2018,
J00184+440, J09439+269, J17115+384, J22115+184) and a ‘U’ rotator from Newton
et al. (2016b, J01026+623). All five stars have $v\sin i<2$ km/s which, given
their radii, rules out $P_{\rm rot}<1$ d in all but a narrow range of
inclination angles. All except J00184+440 have alternative $P_{\rm rot}$
measurements in the literature longwards of 10 d.

The rest of the points in this quadrant have modestly rapid rotations with 3 d
$\lesssim P_{\rm rot}<10$ d. Though closer to the overall trend, there are
reasons to suspect these particular periods may be unreliable. The periods for
J04225+105, J08119+087 and J14155+046 are measured from MEarth light curves by
DA19 and Baroch et al. (2018), but have been deemed ‘N’ rotators by Newton et
al. (2016b) who analysed the same data. The period of J09561+627 is 8.54 d
according to Oelkers et al. (2018), which is about half of the $\sim 18$ d
measured by Lafarga et al. (2021) and 16.9 d from TESS SAP in this work, as
discussed in Section 4.2. The sub-10 d periods of J16554$-$083N, J19072+208,
and J20567$-$104 were measured by DA19 from rather noisy ASAS data, the latter
two with non-trivial FAPs (0.91 % and 0.28%).

##  Appendix B Rossby number computation

Since the dynamo mechanism relies on the motion of charged fluids in the
stellar interior, stellar rotation and convection are thought to be relevant.
Leading theories posit that if the timescale of rotation is short compared
with that of convection, then the dynamo would operate efficiently, inducing
more vigorous magnetic field generation (e.g. Parker 1955; Durney & Latour
1978; Noyes et al. 1984). Therefore, a commonly used parameter in physically
connecting stellar rotation and activity phenomena is the Rossby number
($Ro$), a dimensionless quantity that characterizes the ratio between the two
timescales: $Ro\equiv P_{\rm rot}/\tau_{\rm conv}$. $\tau_{\rm conv}$ is the
convective overturn time and depends on the stellar type, but cannot be
directly measured. While theoretical calculations of $\tau_{\rm conv}$ are
becoming available (e.g. Kim & Demarque 1996), they are subject to stellar
model assumptions and, importantly, do not work for fully convective stars. In
practice, $\tau_{\rm conv}$ is often estimated empirically from minimizing the
scatter in observed activity-rotation relations (e.g. Pizzolato et al. 2003;
Kiraga & Stepien 2007; Wright et al. 2011). A recent calibration as a function
of $(V-K_{s})$ colour comes from Wright et al. (2018), which is applicable
across the entire M dwarf range:

$\centering\log\tau_{\rm
conv}=0.64^{+0.1}_{-0.12}+0.25^{+0.08}_{-0.07}\leavevmode\nobreak\
(V-K_{s}).\@add@centering$ (8)

The relation is also given in terms of $M_{\star}$ as follows (Wright et al.
2018):

$\centering\log\tau_{\rm
conv}=2.33^{+0.06}_{-0.05}-1.50^{+0.21}_{-0.20}\leavevmode\nobreak\
(M_{\star}/M_{\sun})+0.31^{+0.16}_{-0.17}\leavevmode\nobreak\
(M_{\star}/M_{\sun})^{2}.\@add@centering$ (9)

These relations supersedes the previous widely-used versions from Wright et
al. (2011). The earlier version is less accurate for late-type stars,
deviating from the updated one by up to $\sim+0.2$ dex.

An alternative prescription, used by Reiners et al. (2022), is given in terms
of $L_{\star}$: $\tau_{\rm conv}=12.3{\rm d}\times(L_{\rm
bol}/L_{\sun})^{-1/2}$. Figure 17 shows the $\tau_{\rm conv}$ versus $(V-Ks)$
resulting from using different version of the relations for our sample.

Figure 17: Systemtic differences in calculated $\tau_{\rm conv}$ from popular
formulae for our sample, which can result in differences in $Ro$.

A number of authors have also remarked that activity measures, when not
luminosity normalized, are tightly correlated with rotation period itself, and
that $\tau_{\rm conv}$ in fact has a similar scaling with colour as $L_{\rm
bol}$. Therefore, the significance of the $Ro$ as the fundamental determinant
of magnetic activity over the simple and more readily measured $P_{\rm rot}$
has been questioned (e.g. Pizzolato et al. 2003; Reiners et al. 2014).
Furthermore, Reiners et al. (2014) advocated for the utility of the
generalized Rossby number $P_{\rm rot}^{-2}R_{\star}^{-4}$, demonstrating that
it provides a slightly tighter relation with normalized X-ray luminosity over
a wide range of dwarf spectral types (F to M) than the traditional $Ro$.
Nevertheless, many activity-rotation studies continue to use $Ro$. In order to
facilitate direct comparison with results from the literature, we present most
of our activity-rotation relations in terms of $Ro$ in addition to $P_{\rm
rot}$. We use $(V-K_{s})$ colours from Cifuentes et al. (2020) and Eqn. 8
combined with the measured $P_{\rm rot}$, where available, to compute $Ro$ for
our sample. For the stars without a $V$-mag measurement in our sample, we used
the $M_{\star}-Ro$ relation given in Equation 9.

##  Appendix C Long tables and additional figures

Tables LABEL:t:bestprots, LABEL:t:allprots, and LABEL:t:planets are available
in their entirety in electronic form at the CDS via anonymous ftp to
cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-
bin/qcat?J/A+A/. Below we show representative snapshots of each table to
provide guidance on their content.

Figure 18: Example SuperWASP light curve for J22330+093. Top: all three
seasons with black dots being the data points at every epoch. The purple
circles and corresponding error bars represent the daily-binned points,
computed as described in the text. In red we overplot the sinusoid
parametrized by the best period from the second season. The best period is at
37.8 d in the second season (HJD $\sim 5100$, middle panels) and agrees well
with that in season 3 (37.2 d, HJD $\sim 5400$, bottom panels). The pink
dashed line in the light curve denotes the best-fit mean magnitudes, whereas
in the periodograms it corresponds to FAP = 0.1%.  Figure 19: Summary page for
the analysis of PDCSAP light curves from J05337+019, TESS sector 6. Top left:
target pixel map; top right: PDCSAP light curve; bottom left: GLS periodogram;
bottom right: light curve phase-folded on the peak period (0.6048 d).

Figure 20: TESS light curve analysis for J06574+740. Top: PDCSAP light curves
for J06574+740 from sector 40 (left) and 47 (right). The light curves exhibit
a ‘beating’ pattern, suggestive of there being two stars with very similar
rotation periods. Bottom: periodograms showing a main peak at 0.608 d and a
smaller but still highly significant peak at $\sim$0.63 d, which could be the
rotational signal from a binary companion or from differential rotation.

Figure 21: Example of spectroscopic indicator time series analysis for J14524+123. Top: time series data with sinusoids corresponding to the best-fitting period (23.3 d) overplotted; Middle: time series of the individual indicators over the entire baseline; Bottom left: phase-folded on the strongest period; Bottom right: GLS periodogram (middle) and zoom-in on the strongest period (right) of the 4 indicators, with horizontal dashed line denoting FAP = 0.1% and the peak highlighted by the vertical line. Black = H$\alpha$, blue = Ca-IRTa, green = Ca-IRTb, magenta = TiO. Red denotes the window function.  Figure 22: Posterior distributions for each parameter fit in the rotation-activity relation $L_{\rm X}/L_{\rm bol}$ versus $Ro$, as described in Sect. 5.1 and Eqn. 6. This MCMC fit is performed over the whole stellar mass range. The contours shown are $0.5\sigma$, $1\sigma$, $1.5\sigma$ and $2\sigma$. The median value for each parameter is marked in blue. This corner plot is generated using corner.py (https://corner.readthedocs.io/en/latest/).  Table 3: Stellar parameters of the investigated stars. Karmn | Spectral |  Best $P_{\rm rot}$ |  Source b | Secure | $M_{\star}$ | $\log\frac{\tau}{{\rm d}}$ | $\log Ro$ | $v\sin i$ | $R_{\star}$ | $P_{\rm rot,max}$ | $pEW^{\prime}_{\rm H\alpha}$ | $L_{\rm bol}$ | $\log\frac{L_{X}}{L_{\rm bol}}$ | $\log\frac{L_{\rm H\alpha}}{L_{\rm bol}}$ | $\log R^{\prime}_{HK}$ | $\log\frac{\langle B\rangle}{G}$ | SB |  Aged | Kin.
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---
|  Type a | (d) |  |  flag c |  ($M_{\sun}$) |  |  | (km/s) |  ($R_{\sun}$) | (d) |  ($\AA$) |  ($10^{-2}L_{\sun}$) |  |  |  |  | flag | (Myr) | Member
J00051+457 | M1.0 V | 15.37 | DA19 | D | 0.49 | 1.70 | -0.52 | ¡ 2.0 | 0.49 | … | -0.06 | 4.36 | … | -5.17 | -4.97 | … |  | 800 | YD
J00067-075 | M5.5 V | 93.00 | Fou23 | S | 0.11 | 2.24 | -0.27 | ¡ 2.0 | 0.12 | … | 0.00 | 0.14 | … | … | … | … |  | … | D
J00162+198E | M4.0 V | 105.00 | DA19 | S | 0.27 | 1.93 | 0.10 | ¡ 2.0 | 0.28 | … | 0.05 | 0.86 | … | -5.46 | -5.70 | … |  | … | TD-D
J00162+198W | M4.0 V | 4.83 | DA19 | S | 0.43 | 1.90 | -1.22 |  4.0$\pm$ 2.0 | 0.43 | 5.4 | -4.16 | 2.18 | -3.09 | -3.91 | … | … | SB2 | … | TD-D
J00183+440 | M1.0 V | 45.00 | SM18 | S | 0.39 | 1.71 | -0.05 | ¡ 2.0 | 0.40 | … | -0.07 | 2.39 | -4.68 | … | -5.33 | … |  | … | D
J00184+440 | M3.5 V | 113.30 | Don23 | S | 0.16 | 1.93 | 0.13 | ¡ 2.0 | 0.17 | … | -0.03 | 0.33 | … | -5.02 | -5.42 | … |  | … | D
J00286-066 | M4.0 V | … |  |  | 0.34 | 1.87 | … | ¡ 2.0 | 0.35 | … | 0.12 | 1.50 | … | … | … | … |  | … | D
J00389+306 | M2.5 V | 50.20 | DA19 | P | 0.41 | 1.74 | -0.04 | ¡ 2.0 | 0.41 | … | 0.04 | 2.46 | … | -5.28 | -5.11 | … |  | … | D
J00570+450 | M3.0 V | … |  |  | 0.33 | 1.82 | … | ¡ 2.0 | 0.34 | … | -0.08 | 1.50 | … | -4.88 | … | … |  | … | YD
J01013+613 | M2.0 V | 34.70 | SM18 | P | 0.37 | 1.72 | -0.18 | ¡ 2.0 | 0.37 | … | -0.07 | 2.00 | -4.65 | -4.93 | -5.10 | … |  | … | D
J01019+541 | M5.0 V | 0.28 | DA19 | S | 0.14 | 2.20 | -2.76 |  30.6$\pm$ 3.1 | 0.16 | 0.3 | -5.74 | 0.19 | … | -3.84 | … | … |  | 800 | D
J01025+716 | M3.0 V | 50.52 | T.W. | S | 0.47 | 1.79 | -0.09 | ¡ 2.0 | 0.46 | … | 0.08 | 2.99 | -5.48 | -5.33 | -5.03 | … |  | … | D
J01026+623 | M1.5 V | 18.82 | T.W. | S | 0.51 | 1.74 | -0.46 | ¡ 2.0 | 0.51 | … | -0.04 | 4.83 | … | -4.86 | -4.43 | … |  | 800 | YD
J01033+623 | M5.0 V | 1.02 | T.W. | S | 0.23 | 2.05 | -2.04 |  10.5$\pm$ 2.0 | 0.24 | 1.2 | -9.77 | 0.47 | -2.97 | -3.60 | … | … |  | 800 | YD
J01048-181 | M5.0 V | 143.20 | New18 | P | 0.14 | 2.16 | -0.01 | ¡ 2.0 | 0.15 | … | 0.00 | 0.22 | … | -5.36 | … | … |  | … | D
J01056+284 | M5.0 V | 16.32 | Bar18 | P | 0.14 | 2.05 | -0.83 |  …$\pm$ … | 0.16 | … | -0.12 | 0.32 | … | … | … | … | SB2 | … | TD
J01125-169 | M4.5 V | 70.10 | T.W. | S | 0.14 | 2.06 | -0.21 | ¡ 2.0 | 0.15 | … | -1.36 | 0.23 | -3.46 | -4.28 | -5.13 | … |  | … | D
J01339-176 | M4.0 V | 7.75 | T.W. | S | 0.27 | 1.91 | -1.02 | ¡ 2.0 | 0.28 | … | -1.62 | 0.90 | -3.36 | -4.08 | … | … |  | … | YD
J01352-072 | M4.0 V | 0.70 | T.W. | S | 0.38 | 1.98 | -2.13 |  59.8$\pm$ 6.9 | 0.72 | 0.6 | -7.74 | 4.77 | -2.96 | -3.63 | … | … |  | 25 | YD
J01433+043 | M2.0 V | 14.65 | T.W. | P | 0.40 | 1.70 | -0.53 | ¡ 2.0 | 0.40 | … | -0.08 | 2.27 | … | -5.07 | -5.05 | … |  | … | D
J01518+644 | M2.5 V | … |  |  | 0.46 | 1.76 | … | ¡ 2.0 | 0.46 | … | 0.03 | 3.30 | … | -4.99 | … | … |  | … | YD
J02002+130 | M3.5 V | 2.00 | T.W. | S | 0.14 | 2.08 | -1.78 | ¡ 2.0 | 0.16 | … | -1.91 | 0.25 | -3.55 | -4.25 | -4.73 | … |  | … | D
J02015+637 | M3.0 V | … |  |  | 0.42 | 1.80 | … | ¡ 2.0 | 0.42 | … | 0.05 | 2.63 | … | … | -5.06 | … |  | … | D
J02070+496 | M3.5 V | 7.20 | DA19 | S | 0.32 | 1.81 | -0.95 | ¡ 2.0 | 0.33 | … | -0.48 | 1.38 | … | -4.53 | … | … |  | … | YD
J02088+494 | M3.5 V | 0.75 | T.W. | S | 0.37 | 1.86 | -1.98 |  24.1$\pm$ 2.4 | 0.42 | 0.9 | -6.38 | 1.78 | -2.85 | -3.66 | … | … |  | 120 | YD
J02123+035 | M1.5 V | 17.11 | T.W. | D | 0.47 | 1.66 | -0.42 | ¡ 2.0 | 0.47 | … | 0.07 | 3.19 | … | -5.35 | -5.20 | … |  | … | TD
J02222+478 | M0.5 V | 29.50 | DA19 | S | 0.58 | 1.59 | -0.12 | ¡ 2.0 | 0.57 | … | 0.05 | 6.73 | -4.97 | … | -4.70 | … |  | … | D
J02336+249 | M4.0 V | 3.00 | T.W. | S | 0.22 | 1.98 | -1.50 |  3.0$\pm$ 2.0 | 0.23 | 3.8 | -2.73 | 0.56 | -3.35 | -4.03 | -4.52 | … |  | … | D
J02358+202 | M2.0 V | 31.90 | DA19 | D | 0.49 | 1.72 | -0.21 | ¡ 2.0 | 0.48 | … | 0.06 | 3.96 | … | -5.41 | -4.82 | … |  | … | YD
J02362+068 | M4.0 V | … |  |  | 0.26 | 1.91 | … | ¡ 2.0 | 0.27 | … | 0.08 | 0.81 | … | -5.22 | -5.31 | … |  | … | D
J02442+255 | M3.0 V | 38.70 | DA19 | P | 0.34 | 1.80 | -0.21 | ¡ 2.0 | 0.35 | … | 0.01 | 1.67 | -4.48 | -5.15 | -5.14 | … |  | … | YD
J02519+224 | M4.0 V | 0.86 | DA19 | S | 0.25 | 1.94 | -2.01 |  27.2$\pm$ 2.7 | 0.61 | 1.1 | -5.90 | 2.69 | -2.21 | -3.72 | … | … |  | 25 | YD
J02530+168 | M7.0 V | 97.56 | Laf21 | S | 0.08 | 2.51 | -0.52 | ¡ 2.0 | 0.10 | … | -0.50 | 0.07 | … | -4.63 | … | … |  | … | TD
J02565+554W | M1.0 V | 51.20 | SM18 | P | 0.62 | 1.62 | 0.09 | ¡ 2.0 | 0.61 | … | 0.11 | 7.22 | … | -5.10 | … | 2.58 |  | … | D
J03133+047 | M5.0 V | 126.20 | New16 | S | 0.16 | 2.18 | -0.08 | ¡ 2.0 | 0.18 | … | … | 0.30 | … | -5.25 | -5.25 | 2.40 |  | … | D
J03181+382 | M1.5 V | 77.20 | DA19 | P | 0.58 | 1.67 | 0.22 | ¡ 2.0 | 0.57 | … | 0.17 | 6.25 | … | -5.20 | -4.89 | … |  | … | D
J03213+799 | M2.0 V | 23.26 | T.W. | D | 0.40 | 1.69 | -0.33 | ¡ 2.0 | 0.40 | … | -0.01 | 2.48 | … | … | … | 2.51 |  | … | D
J03217-066 | M2.0 V | 21.00 | T.W. | S | 0.45 | 1.72 | -0.40 | ¡ 2.0 | 0.45 | … | -0.27 | 3.29 | -4.65 | … | -4.53 | 2.97 |  | 800 | YD
J03463+262 | M0.0 V | 16.40 | T.W. | D | 0.58 | 1.57 | -0.36 | ¡ 2.0 | 0.57 | … | -0.09 | 7.19 | -4.80 | … | -4.41 | 2.67 |  | … | YD
J03473-019 | M3.0 V | 3.88 | T.W. | S | 0.47 | 1.80 | -1.21 |  6.0$\pm$ 2.0 | 0.49 | 4.2 | -3.95 | 3.12 | -3.04 | -3.76 | -3.98 | 3.54 |  | 120 | YD
J03531+625 | M3.0 V | … |  |  | 0.35 | 1.76 | … | ¡ 2.0 | 0.35 | … | 0.06 | 1.69 | … | … | … | 2.42 |  | … | TD
J04153-076 | M4.5 V | 8.56 | T.W. | D | 0.25 | 1.52 | -0.59 |  2.2$\pm$ 2.0 | 0.26 | 6.1 | -3.36 | 0.64 | … | -3.97 | … | 3.48 |  | … | TD-D
J04167-120 | K7.0 V | 33.00 | Dre20 | P | 0.59 | 1.61 | -0.09 |  2.2$\pm$ 2.0 | 0.58 | 13.3 | … | 7.40 | … | … | … | 2.81 |  | … | D
J04173+088 | M4.5 V | 0.37 | T.W. | S | 0.27 | 2.06 | -2.49 |  37.3$\pm$ 3.7 | 0.28 | 0.4 | -11.15 | 0.66 | -3.10 | -3.70 | … | … |  | 120 | D
J04198+425 | M8.5 V | 0.99 | T.W. | S | 0.11 | 2.17 | -2.17 |  3.6$\pm$ 2.3 | 0.13 | 1.8 | -10.82 | 0.05 | … | -4.20 | … | … |  | … | D
J04225+105 | M3.5 V | 5.48 | DA19 | D | 0.42 | 1.88 | -1.14 | ¡ 2.0 | 0.42 | … | 0.06 | 2.49 | … | -4.74 | -5.37 | 2.29 |  | 800 | YD
J04290+219 | M0.5 V | 25.40 | DA19 | S | 0.68 | 1.55 | -0.14 | ¡ 2.0 | 0.66 | … | 0.19 | 11.50 | -4.54 | -4.86 | -4.62 | 2.58 |  | … | D
J04311+589 | M4.0 V | 91.90 | Fou23 | S | 0.28 | 1.96 | 0.01 | ¡ 2.0 | 0.29 | … | -0.01 | 0.96 | … | -5.09 | … | … |  | … | D
J04376-110 | M1.5 V | … |  |  | 0.45 | 1.70 | … | ¡ 2.0 | 0.45 | … | 0.07 | 3.31 | … | … | -5.06 | … |  | … | D
J04376+528 | M0.0 V | 15.47 | Laf21 | S | 0.55 | 1.59 | -0.40 | ¡ 2.0 | 0.55 | … | -0.01 | 7.16 | -4.77 | -5.09 | -4.56 | 2.63 |  | … | D
J04429+189 | M2.0 V | 40.70 | DA19 | S | 0.46 | 1.74 | -0.13 | ¡ 2.0 | 0.46 | … | 0.00 | 3.51 | -4.64 | -5.31 | -4.79 | 2.54 |  | … | D
J04429+214 | M3.5 V | 47.80 | DA19 | P | 0.36 | 1.85 | -0.17 | ¡ 2.0 | 0.37 | … | -0.05 | 1.82 | … | … | -5.80 | 2.63 |  | … | D
J04472+206 | M5.0 V | 0.34 | DA19 | S | 0.21 | 2.07 | -2.53 |  45.4$\pm$ 4.5 | 0.43 | 0.5 | -9.82 | 1.25 | -3.12 | -3.66 | … | 3.79 |  | 50 | YD
J04520+064 | M3.5 V | … |  |  | 0.36 | 1.90 | … | ¡ 2.0 | 0.36 | … | -0.05 | 1.65 | … | -5.23 | -5.06 | … |  | … | D
J04538-177 | M2.0 V | 53.10 | T.W. | P | 0.40 | 1.72 | 0.01 | ¡ 2.0 | 0.40 | … | 0.04 | 2.38 | … | … | -5.10 | … |  | … | D
J04588+498 | M0.0 V | 17.46 | T.W. | S | 0.60 | 1.57 | -0.33 | ¡ 2.0 | 0.59 | … | -0.05 | 7.98 | -5.02 | … | -4.42 | 2.66 |  | … | D
J05019-069 | M4.0 V | 93.87 | T.W. | S | 0.17 | 2.00 | -0.02 | ¡ 2.0 | 0.19 | … | -0.64 | 0.36 | -3.91 | -4.30 | -4.72 | 3.05 |  | … | D
J05019+011 | M4.0 V | 2.08 | T.W. | S | 0.30 | 1.94 | -1.62 |  7.0$\pm$ 2.0 | 0.65 | 4.7 | -6.36 | 3.38 | -3.04 | -3.69 | -4.30 | 3.52 |  | 25 | YD
J05033-173 | M3.0 V | … |  |  | 0.26 | 1.85 | … | ¡ 2.0 | 0.27 | … | -0.01 | 0.94 | … | -5.44 | -5.29 | 2.42 |  | … | YD
J05062+046 | M4.0 V | 0.89 | T.W. | S | 0.26 | 1.99 | -2.04 |  29.0$\pm$ 2.9 | 0.62 | 1.1 | -7.17 | 2.82 | -3.12 | -3.65 | -4.56 | 3.49 |  | 25 | YD
J05084-210 | M5.0 V | 0.28 | T.W. | S | 0.33 | 2.10 | -2.65 |  25.2$\pm$ 2.5 | 0.68 | 1.4 | -17.39 | 3.90 | -3.17 | -3.46 | … | … |  | 25 | YD
J05127+196 | M2.0 V | 32.70 | T.W. | P | 0.42 | 1.72 | -0.21 | ¡ 2.0 | 0.42 | … | 0.04 | 2.66 | … | -5.35 | -5.19 | … |  | … | D
J05280+096 | M3.5 V | 17.20 | DA19 | P | 0.22 | 1.87 | -0.63 | ¡ 2.0 | 0.23 | … | -0.05 | 0.68 | … | -4.93 | … | … |  | … | D
J05314-036 | M1.5 V | 33.80 | DA19 | S | 0.58 | 1.72 | -0.19 |  2.1$\pm$ 2.0 | 0.57 | 13.8 | 0.10 | 6.52 | -4.81 | … | -4.56 | 2.32 |  | … | D
J05337+019 | M2.5 V | 0.60 | T.W. | S | 0.49 | 1.80 | -2.02 |  9.8$\pm$ 2.0 | 0.49 | 2.5 | -5.00 | 2.95 | -3.01 | -3.58 | … | … | SB1 | … | YD
J05348+138 | M3.5 V | … |  |  | 0.34 | 1.86 | … | ¡ 2.0 | 0.34 | … | 0.02 | 1.54 | -4.28 | … | -5.20 | 2.54 |  | … | YD
J05360-076 | M4.0 V | … |  |  | 0.31 | 1.97 | … | ¡ 2.0 | 0.32 | … | 0.07 | 1.27 | … | -4.90 | … | … |  | … | D
J05365+113 | M0.0 V | 11.75 | T.W. | S | 0.58 | 1.63 | -0.56 | ¡ 2.0 | 0.57 | … | -0.43 | 7.95 | -4.09 | -4.43 | -4.53 | 3.05 |  | 800 | YD
J05366+112 | M4.0 V | 5.44 | T.W. | S | 0.27 | 1.93 | -1.20 |  3.4$\pm$ 2.0 | 0.28 | 4.2 | -2.96 | 0.90 | … | -3.95 | -4.16 | 3.40 |  | 800 | YD
J05394+406 | M8.0 V | … |  |  | 0.10 | 2.18 | … |  5.3$\pm$ 2.0 | 0.12 | 1.1 | -5.53 | 0.06 | … | -4.21 | … | 3.26 |  | … | D
J05415+534 | M1.0 V | 17.39 | T.W. | P | 0.55 | 1.64 | -0.40 | ¡ 2.0 | 0.54 | … | -0.04 | 5.71 | … | -5.02 | -4.74 | 2.62 |  | 120 | YD
J05421+124 | M4.0 V | … |  |  | 0.23 | 1.91 | … | ¡ 2.0 | 0.24 | … | 0.06 | 0.63 | -4.86 | -5.17 | -5.51 | … |  | … | TD
J05532+242 | M1.5 V | … |  |  | 0.60 | 1.69 | … | ¡ 3.0 | 0.59 | … | -0.03 | 6.92 | … | -5.39 | … | … | SB2 | … | D
J06000+027 | M4.0 V | 1.81 | T.W. | S | 0.23 | 1.96 | -1.70 |  6.2$\pm$ 2.0 | 0.24 | 2.0 | -2.69 | 0.63 | -3.41 | -3.88 | -4.79 | 3.40 |  | 800 | YD
J06011+595 | M3.5 V | 95.10 | Don23 | S | 0.25 | 1.91 | 0.06 | ¡ 2.0 | 0.26 | … | -0.01 | 0.84 | … | -5.02 | -5.17 | 2.32 |  | … | YD
J06024+498 | M5.0 V | 105.00 | DA19 | S | 0.13 | 2.16 | -0.14 | ¡ 2.0 | 0.15 | … | -0.04 | 0.21 | … | -5.57 | … | 2.57 |  | … | YD
J06103+821 | M2.0 V | 44.60 | DA19 | P | 0.41 | 1.73 | -0.08 | ¡ 2.0 | 0.41 | … | 0.00 | 2.41 | -5.04 | -5.36 | -5.09 | … |  | … | D
J06105-218 | M0.5 V | 27.30 | DA19 | S | 0.54 | 1.87 | -0.43 | ¡ 2.0 | 0.54 | … | 0.00 | 5.46 | -5.19 | … | -4.64 | 2.57 |  | … | YD
J06246+234 | M4.0 V | … |  |  | 0.17 | 1.94 | … | ¡ 2.0 | 0.18 | … | 0.04 | 0.33 | … | -5.54 | … | 2.79 |  | … | D
J06318+414 | M5.0 V | 0.30 | T.W. | S | 0.35 | 2.13 | -2.66 |  54.0$\pm$ 5.4 | 0.36 | 0.3 | -11.19 | 1.34 | -2.96 | -3.68 | … | 3.34 |  | 120 | YD
J06371+175 | M0.0 V | 37.50 | Luq22 | S | 0.44 | 1.62 | -0.04 | ¡ 2.0 | 0.44 | … | -0.07 | 3.63 | -4.84 | -5.24 | -4.86 | 2.27 |  | … | TD-D
J06396-210 | M4.0 V | 79.15 | New18 | P | 0.33 | 1.92 | -0.02 | ¡ 2.0 | 0.33 | … | -0.12 | 1.37 | … | -4.98 | … | 2.79 |  | … | D
J06421+035 | M3.5 V | 83.40 | DA19 | P | 0.37 | 1.82 | 0.10 | ¡ 2.0 | 0.37 | … | 0.05 | 1.83 | … | -5.19 | -5.11 | 2.26 |  | … | D
J06548+332 | M3.0 V | 122.00 | Sto20b | S | 0.34 | 1.83 | 0.26 | ¡ 2.0 | 0.35 | … | 0.00 | 1.64 | … | -5.10 | -5.38 | … |  | … | YD
J06574+740 | M4.0 V | 0.61 | T.W. | S | 0.27 | 1.86 | -2.08 |  32.0$\pm$ 3.2 | 0.28 | 0.4 | -5.44 | 0.70 | -2.93 | -3.74 | … | 3.52 |  | 800 | D
J06594+193 | M5.0 V | … |  |  | 0.12 | 2.16 | … | ¡ 2.0 | 0.13 | … | -0.43 | 0.16 | … | -4.70 | -5.91 | 2.59 |  | … | D
J07001-190 | M5.0 V | … |  |  | 0.24 | 2.10 | … |  …$\pm$ … | … | … | -6.99 | 2.98 | … | -3.77 | … | … | SB2 | … | D
J07033+346 | M4.0 V | 8.00 | T.W. | S | 0.25 | 1.93 | -1.03 |  2.4$\pm$ 2.0 | 0.26 | 5.5 | -2.98 | 0.74 | … | -3.85 | … | 3.39 |  | … | D
J07044+682 | M3.0 V | … |  |  | 0.39 | 1.80 | … | ¡ 2.0 | 0.40 | … | 0.07 | 2.19 | … | … | … | … |  | … | D
J07274+052 | M3.5 V | 93.50 | SM17 | D | 0.28 | 1.90 | 0.07 | ¡ 2.0 | 0.29 | … | -0.05 | 0.98 | -5.33 | -5.24 | -5.29 | … |  | … | D
J07287-032 | M3.0 V | 115.40 | T.W. | P | 0.37 | 1.82 | 0.24 | ¡ 2.0 | 0.37 | … | 0.04 | 1.92 | … | … | -5.36 | … |  | … | D
J07319+362N | M3.5 V | 16.40 | DA19 | P | 0.41 | 1.89 | -0.67 | ¡ 2.0 | 0.40 | … | -2.78 | 1.86 | -2.76 | -4.03 | -4.28 | 3.40 |  | 800 | YD
J07353+548 | M2.0 V | 21.80 | DA19 | P | 0.36 | 1.73 | -0.39 | ¡ 2.0 | 0.36 | … | -0.03 | 1.91 | … | … | … | … |  | 800 | YD
J07361-031 | M1.0 V | 12.20 | T.W. | S | 0.54 | 1.67 | -0.58 |  3.1$\pm$ 2.0 | 0.55 | 8.9 | -0.86 | 6.14 | -4.25 | -4.23 | … | … | SB1 | 800 | D
J07386-212 | M3.0 V | … |  |  | 0.29 | 1.81 | … | ¡ 2.0 | 0.29 | … | 0.01 | 1.15 | … | … | -5.32 | … |  | … | D
J07393+021 | M0.0 V | 11.45 | T.W. | P | 0.59 | 1.61 | -0.55 | ¡ 2.0 | 0.58 | … | 0.02 | 7.68 | … | … | -4.53 | 2.44 |  | … | YD
J07403-174 | M6.0 V | … |  |  | 0.09 | 2.20 | … | ¡ 2.0 | 0.11 | … | 0.00 | 0.08 | … | … | … | 2.44 |  | … | D
J07446+035 | M4.5 V | 2.78 | T.W. | S | 0.19 | 1.97 | -1.53 |  4.6$\pm$ 2.0 | 0.34 | 3.8 | -7.28 | 1.12 | -2.98 | -3.61 | … | 3.66 |  | 50 | YD
J07472+503 | M4.0 V | 1.32 | T.W. | S | 0.27 | 1.90 | -1.78 |  10.3$\pm$ 2.0 | 0.28 | 1.4 | -3.77 | 0.79 | -3.76 | -3.87 | … | 3.47 |  | 800 | D
J07558+833 | M4.5 V | 1.11 | T.W. | S | 0.26 | 1.93 | -1.89 |  11.8$\pm$ 2.0 | 0.27 | 1.2 | -5.21 | 0.75 | -3.03 | -3.83 | … | 3.56 |  | 800 | YD
J07582+413 | M3.5 V | … |  |  | 0.26 | 1.92 | … | ¡ 2.0 | 0.27 | … | -0.03 | 0.88 | … | -5.19 | -5.34 | … |  | … | D
J08023+033 | M4.0 V | … |  |  | 0.34 | 1.87 | … | ¡ 2.0 | 0.35 | … | … | 1.50 | … | … | … | 2.41 |  | … | TD
J08119+087 | M4.5 V | 5.42 | DA19 | D | 0.15 | 1.93 | -1.20 | ¡ 2.0 | 0.16 | … | -0.01 | 0.26 | … | -5.62 | … | 2.96 |  | … | TD
J08126-215 | M4.0 V | … |  |  | 0.26 | 2.00 | … | ¡ 2.0 | 0.27 | … | 0.04 | 0.84 | … | … | -5.12 | … |  | … | D
J08161+013 | M2.0 V | 40.70 | DA19 | P | 0.44 | 1.72 | -0.11 | ¡ 2.0 | 0.44 | … | 0.01 | 2.80 | … | -5.18 | -5.02 | 2.40 |  | … | D
J08293+039 | M2.5 V | … |  |  | 0.48 | 1.74 | … | ¡ 2.0 | 0.47 | … | 0.05 | 3.59 | … | … | -4.65 | 2.61 |  | … | YD
J08298+267 | M6.5 V | 0.46 | DA19 | S | 0.09 | 2.20 | -2.54 |  11.5$\pm$ 2.0 | 0.11 | 0.5 | -4.55 | 0.08 | … | -4.11 | … | 3.43 |  | … | YD
J08315+730 | M4.0 V | 105.00 | DA19 | S | 0.28 | 1.86 | 0.16 | ¡ 2.0 | 0.29 | … | 0.07 | 0.94 | … | -5.09 | … | … |  | … | D
J08358+680 | M2.5 V | … |  |  | 0.36 | 1.78 | … | ¡ 2.0 | 0.36 | … | -0.19 | 1.77 | -4.48 | -4.89 | … | 2.76 |  | … | D
J08402+314 | M3.5 V | 118.00 | DA19 | S | 0.27 | 1.88 | 0.19 | ¡ 2.0 | 0.28 | … | 0.01 | 0.99 | … | -4.88 | … | 2.49 |  | … | TD-D
J08409-234 | M3.5 V | 57.50 | Irv23 | D | 0.40 | 1.88 | -0.12 | ¡ 2.0 | 0.40 | … | 0.04 | 2.19 | … | -5.10 | -5.04 | … |  | … | TD-D
J08413+594 | M5.5 V | 83.27 | Pas23 | S | 0.12 | 2.26 | -0.34 | ¡ 2.0 | 0.14 | … | -1.34 | 0.17 | … | -4.86 | … | 3.11 |  | … | D
J08526+283 | M4.5 V | … |  |  | 0.26 | 2.01 | … | ¡ 2.0 | 0.27 | … | 0.05 | 0.80 | … | -5.28 | -5.09 | … |  | … | YD
J08536-034 | M9.0 V | 0.46 | T.W. | S | 0.08 | 2.21 | -2.55 |  8.4$\pm$ 2.0 | 0.10 | 0.6 | … | 0.03 | … | … | … | 3.68 |  | … | D
J09003+218 | M6.5 V | 0.44 | New16 | S | 0.08 | 2.52 | -2.87 |  13.0$\pm$ 2.0 | 0.10 | 0.4 | -6.40 | 0.08 | … | -4.23 | … | 3.63 |  | 120 | YD
J09005+465 | M4.5 V | 8.00 | Wes15 | S | 0.20 | 2.03 | -1.13 | ¡ 2.0 | 0.21 | … | -0.95 | 0.47 | -3.80 | -4.36 | … | … |  | 120 | YD
J09028+680 | M4.0 V | … |  |  | 0.27 | 1.87 | … | ¡ 2.0 | 0.28 | … | 0.07 | 0.84 | … | -5.32 | … | … |  | … | D
J09033+056 | M7.0 V | … |  |  | 0.14 | 2.13 | … |  7.1$\pm$ 2.0 | 0.15 | 1.1 | -3.79 | 0.18 | … | -4.14 | … | 3.51 |  | 800 | D
J09133+688 | M2.5 V | 10.40 | SM18 | P | 0.58 | 1.71 | -0.69 | ¡ 2.0 | 0.59 | … | -0.54 | 7.19 | -3.89 | -4.42 | … | … |  | 800 | YD
J09140+196 | M3.0 V | 39.10 | T.W. | P | 0.49 | 1.80 | -0.21 | ¡ 2.0 | 0.49 | … | -0.10 | 3.31 | … | … | -4.67 | … | SB1 | … | YD
J09143+526 | M0.0 V | 17.54 | T.W. | S | 0.58 | 1.59 | -0.35 | ¡ 2.0 | 0.57 | … | -0.01 | 7.64 | … | … | -4.46 | 2.61 |  | 800 | YD
J09144+526 | M0.0 V | 16.88 | T.W. | S | 0.58 | 1.73 | -0.51 | ¡ 2.0 | 0.58 | … | -0.01 | 7.55 | -4.69 | … | -4.55 | 2.53 |  | 800 | YD
J09161+018 | M4.0 V | 1.43 | T.W. | S | 0.31 | 1.91 | -1.75 |  10.0$\pm$ 2.0 | 0.32 | 1.6 | -4.89 | 1.02 | -3.28 | -3.78 | -4.30 | 3.59 |  | 800 | D
J09163-186 | M1.5 V | … |  |  | 0.44 | 1.70 | … | ¡ 2.0 | 0.44 | … | -0.38 | 3.30 | -4.31 | -4.51 | -4.53 | 2.87 |  | 50 | YD
J09307+003 | M3.5 V | … |  |  | 0.29 | 1.85 | … | ¡ 2.0 | 0.30 | … | 0.00 | 1.16 | … | -5.29 | -5.38 | 2.25 |  | … | D
J09360-216 | M2.5 V | 74.30 | SM15 | S | 0.34 | 1.75 | 0.12 | ¡ 2.0 | 0.35 | … | -0.01 | 1.61 | … | … | -5.46 | … |  | … | D
J09411+132 | M1.5 V | … |  |  | 0.45 | 1.71 | … | ¡ 2.0 | 0.45 | … | 0.01 | 3.41 | -4.55 | -5.12 | -4.94 | 2.59 |  | … | YD
J09423+559 | M3.5 V | 74.30 | DA19 | S | 0.37 | 1.88 | -0.01 | ¡ 2.0 | 0.37 | … | -0.04 | 1.76 | … | -5.20 | … | 2.50 |  | … | D
J09425+700 | M2.0 V | 21.00 | DA19 | P | 0.50 | 1.77 | -0.44 |  2.1$\pm$ 2.0 | 0.49 | 11.9 | -0.58 | 3.49 | … | -4.66 | … | 3.01 |  | 800 | YD
J09428+700 | M3.0 V | 24.33 | T.W. | S | 0.42 | 1.83 | -0.45 | ¡ 2.0 | 0.42 | … | -0.80 | 2.40 | -3.69 | -4.18 | -5.05 | 3.14 |  | 800 | YD
J09439+269 | M3.5 V | 13.70 | DA19 | D | 0.36 | 1.86 | -0.72 | ¡ 2.0 | 0.37 | … | 0.08 | 1.80 | … | -5.12 | -5.26 | … |  | 800 | D
J09447-182 | M4.0 V | … |  |  | 0.27 | 1.94 | … | ¡ 2.0 | 0.28 | … | 0.09 | 0.93 | … | … | -5.32 | … |  | … | TD-D
J09449-123 | M5.0 V | 0.44 | T.W. | S | 0.17 | 2.18 | -2.53 |  35.3$\pm$ 3.5 | 0.32 | 0.5 | -14.00 | 0.90 | -2.90 | -3.54 | … | 3.69 |  | 50 | YD
J09468+760 | M1.5 V | 50.62 | T.W. | P | 0.53 | 1.63 | 0.08 | ¡ 2.0 | 0.53 | … | 0.12 | 4.28 | … | -5.21 | … | … |  | … | TD
J09511-123 | M0.5 V | … |  |  | 0.51 | 1.62 | … | ¡ 2.0 | 0.50 | … | -0.03 | 4.63 | … | … | -4.93 | 2.18 |  | … | TD
J09561+627 | M0.0 V | 16.88 | T.W. | S | 0.59 | 1.64 | -0.41 | ¡ 2.0 | 0.58 | … | -0.06 | 7.29 | -4.81 | -5.03 | -4.43 | 2.59 |  | … | YD
J10023+480 | M1.0 V | … |  |  | 0.59 | 1.62 | … | ¡ 2.0 | 0.58 | … | 0.09 | 5.96 | … | -5.44 | … | 2.29 |  | … | TD
J10088+692 | M0.5 V | 41.20 | Blu20 | S | 0.64 | 1.54 | 0.07 | ¡ 2.0 | 0.63 | … | … | 8.73 | … | … | … | 2.32 |  | … | D
J10122-037 | M1.5 V | 23.00 | T.W. | S | 0.50 | 1.78 | -0.42 | ¡ 2.0 | 0.49 | … | -0.03 | 4.21 | -4.86 | … | -4.78 | 2.65 |  | 800 | YD
J10125+570 | M3.5 V | … |  |  | 0.29 | 1.85 | … | ¡ 2.0 | 0.30 | … | -0.01 | 1.17 | … | -4.97 | -5.30 | 2.38 |  | … | YD
J10167-119 | M3.0 V | … |  |  | 0.48 | 1.78 | … | ¡ 2.0 | 0.47 | … | 0.08 | 3.22 | … | … | -5.08 | … |  | … | D
J10182-204 | M4.5 V | 14.50 | T.W. | S | 0.40 | 2.08 | -0.92 | … | 0.40 | … | -7.63 | 2.09 | -3.41 | … | … | … | SB2 | … | D
J10196+198 | M3.0 V | 2.24 | Mor08 | S | 0.45 | 1.87 | -1.52 |  3.3$\pm$ 2.0 | 0.43 | 6.6 | -4.52 | 2.36 | -3.08 | -3.76 | … | 3.55 |  | 800 | YD
J10251-102 | M1.0 V | 25.05 | T.W. | P | 0.51 | 1.69 | -0.29 | ¡ 2.0 | 0.51 | … | -0.11 | 4.63 | -5.09 | … | -4.74 | 2.58 |  | … | YD
J10289+008 | M2.0 V | 31.72 | T.W. | S | 0.41 | 1.74 | -0.24 | ¡ 2.0 | 0.41 | … | -0.00 | 2.56 | -5.17 | … | -4.92 | 2.44 |  | … | YD
J10350-094 | M3.0 V | … |  |  | 0.38 | 1.83 | … | ¡ 2.0 | 0.38 | … | 0.04 | 1.97 | … | … | -5.18 | … |  | … | D
J10354+694 | M3.5 V | 118.00 | DA19 | S | 0.32 | 1.80 | 0.27 | ¡ 3.0 | 0.33 | … | 0.07 | 1.60 | … | -5.03 | … | … | SB2 | … | TD
J10360+051 | M3.5 V | 6.90 | T.W. | S | 0.36 | 1.90 | -1.07 |  2.1$\pm$ 2.0 | 0.36 | 8.8 | -5.08 | 1.36 | -3.12 | -3.74 | … | 3.68 |  | 800 | D
J10396-069 | M2.5 V | … |  |  | 0.46 | 1.75 | … | ¡ 2.0 | 0.46 | … | 0.02 | 3.16 | … | … | -5.03 | … |  | … | YD
J10416+376 | M4.5 V | 54.30 | DA19 | D | 0.21 | 1.97 | -0.24 | ¡ 2.0 | 0.22 | … | 0.08 | 0.52 | … | -5.46 | … | … |  | … | D
J10482-113 | M6.5 V | 1.50 | Mor10 | S | 0.08 | 2.60 | -2.43 |  2.1$\pm$ 2.0 | 0.09 | 2.3 | -2.27 | 0.07 | … | -4.50 | … | … |  | … | D
J10504+331 | M4.0 V | … |  |  | 0.40 | 1.90 | … | ¡ 2.0 | 0.41 | … | 0.09 | 2.04 | … | -5.06 | … | … | SB1 | … | TD
J10508+068 | M4.0 V | 64.00 | DA19 | P | 0.25 | 1.97 | -0.17 | ¡ 2.0 | 0.26 | … | 0.05 | 0.79 | … | -5.28 | -5.32 | … |  | … | YD
J10564+070 | M6.0 V | 2.70 | DA19 | S | 0.09 | 2.50 | -2.07 | ¡ 2.0 | 0.11 | … | -7.22 | 0.10 | -3.54 | -4.14 | … | 3.48 |  | … | D
J10584-107 | M5.0 V | … |  |  | 0.19 | 2.05 | … |  2.8$\pm$ 2.0 | 0.21 | 3.7 | -0.62 | 0.41 | -3.30 | -4.58 | … | 3.61 |  | 120 | YD
J11000+228 | M2.5 V | 53.17 | T.W. | S | 0.37 | 1.78 | -0.06 | ¡ 2.0 | 0.37 | … | -0.01 | 1.95 | … | -5.14 | -5.11 | 2.56 |  | … | YD
J11026+219 | M1.0 V | 14.26 | T.W. | S | 0.54 | 1.62 | -0.46 |  2.3$\pm$ 2.0 | 0.54 | 11.8 | -0.49 | 5.65 | -3.94 | -4.48 | -4.20 | 3.02 |  | 800 | D
J11033+359 | M1.5 V | 56.15 | Dia19 | S | 0.39 | 1.70 | 0.05 | ¡ 2.0 | 0.40 | … | -0.04 | 2.25 | … | … | -5.50 | … |  | … | TD
J11054+435 | M1.0 V | 36.90 | Don23 | D | 0.38 | 1.65 | -0.09 | ¡ 2.0 | 0.38 | … | -0.09 | 2.31 | … | -4.94 | -5.48 | … |  | … | TD-D
J11055+435 | M5.5 V | 0.78 | Mor10 | S | 0.08 | 2.22 | -2.32 |  3.5$\pm$ 2.0 | 0.10 | 1.4 | -9.69 | 0.10 | -3.15 | -3.70 | … | 3.84 |  | … | TD-D
J11110+304E | K7.0 V | 40.00 | Ded21 | P | 0.67 | 1.61 | -0.01 | ¡ 2.0 | 0.66 | … | … | 12.33 | … | -5.11 | … | … |  | … | D
J11110+304W | M2.0 V | … |  |  | 0.55 | 1.70 | … | ¡ 2.0 | 0.54 | … | 0.05 | 5.10 | … | -5.21 | -4.78 | 2.45 |  | … | D
J11126+189 | M1.5 V | … |  |  | 0.51 | 1.69 | … | ¡ 2.0 | 0.51 | … | 0.07 | 4.58 | … | … | -4.59 | 2.47 |  | … | D
J11201-104 | M2.0 V | 5.64 | T.W. | S | 0.53 | 1.71 | -0.96 |  4.6$\pm$ 2.0 | 0.51 | 5.6 | -1.88 | 4.16 | -3.21 | -3.98 | … | 3.34 |  | 800 | YD
J11289+101 | M3.5 V | … |  |  | 0.27 | 1.87 | … | ¡ 2.0 | 0.28 | … | 0.01 | 0.92 | … | -5.19 | -5.02 | … |  | … | D
J11302+076 | M2.5 V | 36.40 | DA19 | S | 0.43 | 1.79 | -0.23 | ¡ 2.0 | 0.43 | … | 0.04 | 2.74 | … | … | -5.05 | 2.43 |  | … | D
J11306-080 | M3.5 V | … |  |  | 0.34 | 1.86 | … | ¡ 2.0 | 0.35 | … | -0.00 | 1.59 | … | … | … | 2.58 |  | … | D
J11417+427 | M4.0 V | 71.50 | DA19 | D | 0.35 | 1.92 | -0.07 | ¡ 2.0 | 0.35 | … | 0.11 | 1.47 | … | -5.21 | -5.35 | … |  | … | YD
J11421+267 | M2.5 V | 44.60 | DA19 | S | 0.41 | 1.77 | -0.13 | ¡ 2.0 | 0.41 | … | 0.00 | 2.41 | -5.18 | -5.28 | -5.27 | … |  | … | D
J11467-140 | M3.0 V | … |  |  | 0.50 | 1.80 | … | ¡ 2.0 | 0.50 | … | 0.08 | 3.64 | … | … | -4.79 | 2.43 |  | … | D
J11474+667 | M5.0 V | 13.30 | T.W. | S | 0.29 | 2.10 | -0.98 |  3.1$\pm$ 2.0 | 0.30 | 4.9 | -7.99 | 0.81 | … | -3.72 | … | 3.68 |  | 800 | YD
J11476+002 | M4.0 V | 11.60 | DA19 | S | 0.34 | 1.95 | -0.89 |  2.3$\pm$ 2.0 | 0.34 | 7.5 | -5.05 | 1.23 | -3.14 | -3.73 | -4.40 | 3.57 |  | 120 | YD
J11476+786 | M3.5 V | … |  |  | 0.25 | 1.84 | … | ¡ 2.0 | 0.26 | … | -0.00 | 0.80 | … | -5.08 | -5.59 | … |  | … | TD
J11477+008 | M4.0 V | 112.83 | Ste16 | S | 0.17 | 2.01 | 0.05 | ¡ 2.0 | 0.19 | … | 0.00 | 0.38 | -4.32 | -5.19 | -5.27 | 2.45 |  | … | D
J11509+483 | M4.5 V | 148.95 | Med22 | S | 0.16 | 2.04 | 0.13 | ¡ 2.0 | 0.18 | … | -0.09 | 0.33 | … | -5.17 | … | … |  | … | D
J11511+352 | M1.5 V | 22.80 | DA19 | S | 0.45 | 1.69 | -0.33 | ¡ 2.0 | 0.45 | … | -0.06 | 3.32 | -4.44 | … | -4.74 | 2.82 |  | … | D
J12054+695 | M4.0 V | 100.00 | DA19 | S | 0.30 | 1.95 | 0.05 | ¡ 2.0 | 0.30 | … | 0.02 | 1.04 | … | -5.03 | … | … |  | … | YD
J12100-150 | M3.5 V | 79.30 | T.W. | P | 0.36 | 1.95 | -0.05 | ¡ 2.0 | 0.36 | … | -0.02 | 1.60 | … | … | -5.22 | … |  | … | TD
J12111-199 | M3.0 V | … |  |  | 0.34 | 1.80 | … | ¡ 2.0 | 0.35 | … | 0.01 | 1.68 | … | -5.37 | -5.19 | … |  | … | YD
J12123+544S | M0.0 V | 96.70 | Sto20b | P | 0.59 | 1.55 | 0.44 | ¡ 2.0 | 0.58 | … | 0.04 | 7.04 | … | … | … | 2.32 |  | … | D
J12156+526 | M4.0 V | 0.73 | T.W. | S | 0.49 | 1.84 | -1.98 |  37.6$\pm$ 3.8 | 0.48 | 0.6 | -5.52 | 3.30 | -2.98 | -3.74 | … | 3.81 |  | 800 | D
J12189+111 | M5.0 V | 0.49 | DA19 | S | 0.15 | 2.22 | -2.53 |  13.0$\pm$ 2.0 | 0.16 | 0.6 | -5.84 | 0.21 | … | -3.85 | -4.85 | 3.60 |  | 800 | YD
J12230+640 | M3.0 V | 32.90 | DA19 | D | 0.49 | 1.76 | -0.24 | ¡ 2.0 | 0.48 | … | 0.12 | 3.39 | … | -4.74 | -5.07 | … |  | … | D
J12248-182 | M2.0 V | … |  |  | 0.27 | 1.74 | … | ¡ 2.0 | 0.28 | … | -0.02 | 0.98 | … | … | -5.47 | 2.45 |  | … | TD
J12312+086 | M0.5 V | … |  |  | 0.56 | 1.60 | … | ¡ 2.0 | 0.55 | … | 0.01 | 6.26 | … | -4.90 | -4.52 | 2.56 |  | … | D
J12350+098 | M2.5 V | 36.60 | DA19 | P | 0.48 | 1.70 | -0.14 | ¡ 2.0 | 0.48 | … | 0.12 | 3.34 | … | -5.26 | -5.10 | … |  | … | D
J12373-208 | M4.0 V | … |  |  | 0.40 | 1.94 | … | ¡ 2.0 | 0.40 | … | 0.10 | 2.00 | … | … | -5.24 | 2.46 |  | … | D
J12388+116 | M3.0 V | 55.35 | T.W. | S | 0.45 | 1.84 | -0.10 | ¡ 2.0 | 0.45 | … | -0.00 | 2.79 | … | -5.04 | -5.05 | 2.52 |  | … | D
J12428+418 | M4.0 V | 16.20 | DA19 | P | 0.38 | 1.93 | -0.72 |  2.1$\pm$ 2.0 | 0.38 | 9.2 | -2.41 | 1.61 | -3.29 | -3.87 | … | 3.37 |  | 800 | YD
J12479+097 | M3.5 V | 49.90 | Cab22 | D | 0.31 | 1.90 | -0.20 | ¡ 2.0 | 0.32 | … | -0.01 | 1.21 | … | -5.21 | -5.48 | … |  | … | D
J13005+056 | M4.5 V | 0.60 | T.W. | S | 0.20 | 2.08 | -2.30 |  16.4$\pm$ 2.0 | 0.21 | 0.6 | -5.13 | 0.39 | -3.22 | -3.88 | -4.60 | 3.58 |  | … | D
J13102+477 | M5.0 V | 29.06 | T.W. | S | 0.16 | 2.12 | -0.65 | ¡ 2.0 | 0.17 | … | -3.02 | 0.29 | -3.08 | -3.82 | … | 3.36 |  | … | D
J13196+333 | M1.5 V | 48.00 | SM18 | P | 0.54 | 1.69 | -0.01 | ¡ 2.0 | 0.54 | … | 0.14 | 5.37 | … | … | -4.81 | 2.35 |  | … | YD
J13209+342 | M1.0 V | … |  |  | 0.54 | 1.65 | … | ¡ 2.0 | 0.53 | … | -0.00 | 4.88 | … | -5.43 | … | 2.45 |  | … | D
J13229+244 | M4.0 V | 95.00 | Luq18 | D | 0.27 | 1.90 | 0.07 | ¡ 2.0 | 0.28 | … | 0.06 | 0.86 | … | -5.19 | … | 2.64 |  | … | D
J13283-023W | M3.0 V | 46.42 | Rae20 | P | 0.42 | 1.80 | -0.14 | ¡ 2.0 | 0.42 | … | 0.06 | 2.54 | … | … | -5.19 | … |  | … | D
J13293+114 | M3.5 V | … |  |  | 0.44 | 1.82 | … | ¡ 2.0 | 0.44 | … | 0.05 | 2.49 | … | -4.81 | -5.03 | … |  | … | TD
J13299+102 | M0.5 V | 30.00 | SM17 | S | 0.48 | 1.72 | -0.24 | ¡ 2.0 | 0.48 | … | -0.01 | 4.15 | -4.80 | -5.25 | -4.81 | 2.20 |  | … | D
J13427+332 | M3.5 V | … |  |  | 0.26 | 1.89 | … | ¡ 2.0 | 0.27 | … | -0.03 | 0.90 | … | -5.09 | -5.16 | 2.37 |  | … | D
J13450+176 | M0.0 V | … |  |  | 0.49 | 1.54 | … | ¡ 2.0 | 0.49 | … | -0.03 | 4.63 | … | -5.26 | -4.99 | … |  | … | TD
J13457+148 | M1.5 V | 52.30 | SM15 | P | 0.49 | 1.67 | 0.05 | ¡ 2.0 | 0.49 | … | 0.13 | 3.65 | … | -5.52 | -4.99 | 2.25 |  | … | D
J13458-179 | M3.5 V | … |  |  | 0.33 | 1.88 | … | ¡ 2.0 | 0.33 | … | 0.00 | 1.42 | … | … | -5.34 | … |  | … | D
J13536+776 | M4.0 V | 1.23 | T.W. | S | 0.29 | 1.91 | -1.82 |  9.7$\pm$ 2.0 | 0.30 | 1.6 | -3.77 | 0.86 | -3.13 | -3.81 | … | 3.42 |  | 800 | D
J13582+125 | M3.0 V | … |  |  | 0.21 | 1.85 | … | ¡ 2.0 | 0.22 | … | -0.04 | 0.62 | … | … | -5.00 | … |  | … | D
J13591-198 | M4.0 V | 3.32 | T.W. | S | 0.26 | 2.01 | -1.49 |  4.2$\pm$ 2.0 | 0.27 | 3.3 | -3.07 | 0.75 | -3.21 | -3.84 | -4.27 | 3.28 |  | 800 | YD
J14010-026 | M1.0 V | 43.90 | SM17 | S | 0.51 | 1.65 | -0.01 | ¡ 2.0 | 0.50 | … | 0.01 | 4.39 | … | … | -4.77 | 2.36 |  | … | D
J14082+805 | M1.0 V | … |  |  | 0.60 | 1.63 | … | ¡ 2.0 | 0.59 | … | 0.05 | 6.52 | … | -5.27 | -4.70 | 2.60 |  | … | D
J14152+450 | M3.0 V | 52.80 | DA19 | P | 0.43 | 1.80 | -0.07 | ¡ 2.0 | 0.43 | … | 0.04 | 2.55 | … | -5.38 | … | 2.50 |  | … | D
J14155+046 | M5.0 V | 8.92 | Bar18 | D | 0.16 | 2.08 | -1.13 |  …$\pm$ … | 0.17 | … | 0.10 | 0.42 | … | … | … | … | SB2 | … | D
J14173+454 | M5.0 V | 0.37 | T.W. | S | 0.27 | 2.02 | -2.46 |  14.9$\pm$ 2.0 | 0.28 | 1.0 | -3.89 | 0.77 | -3.05 | -3.96 | … | 3.77 |  | … | D
J14251+518 | M2.5 V | … |  |  | 0.39 | 1.74 | … | ¡ 2.0 | 0.40 | … | 0.01 | 2.24 | … | … | … | … |  | … | D
J14257+236E | M0.5 V | 17.60 | DA19 | D | 0.60 | 1.60 | -0.35 | ¡ 2.0 | 0.59 | … | 0.03 | 7.48 | -4.41 | -5.38 | -4.65 | 2.43 |  | … | TD-D
J14257+236W | M0.0 V | 111.00 | DA19 | P | 0.61 | 1.57 | 0.47 | ¡ 2.0 | 0.61 | … | 0.00 | 8.33 | … | -5.48 | -4.55 | 2.35 |  | … | D
J14294+155 | M2.0 V | 43.50 | SM18 | P | 0.50 | 1.72 | -0.08 | ¡ 2.0 | 0.50 | … | 0.05 | 3.99 | … | -5.39 | -4.89 | 2.62 |  | … | TD
J14307-086 | M0.5 V | … |  |  | 0.64 | 1.63 | … | ¡ 2.0 | 0.63 | … | 0.17 | 9.60 | … | … | -4.61 | 2.32 |  | … | TD-D
J14310-122 | M3.5 V | … |  |  | 0.31 | 1.88 | … | ¡ 2.0 | 0.31 | … | 0.00 | 1.25 | … | … | -5.56 | … |  | … | YD
J14321+081 | M6.0 V | 0.76 | Pas23 | S | 0.13 | 2.27 | -2.39 |  6.8$\pm$ 2.0 | 0.14 | 1.1 | -5.11 | 0.18 | … | -4.12 | … | 3.45 |  | 800 | YD
J14342-125 | M4.0 V | 94.77 | T.W. | S | 0.29 | 1.98 | -0.00 | ¡ 2.0 | 0.30 | … | 0.02 | 1.01 | … | … | -5.24 | … |  | … | D
J14524+123 | M2.0 V | 26.03 | T.W. | S | 0.50 | 1.75 | -0.34 | ¡ 2.0 | 0.50 | … | -0.05 | 4.20 | … | … | -4.77 | 2.66 |  | … | D
J14544+355 | M3.5 V | … |  |  | 0.35 | 1.85 | … | ¡ 2.0 | 0.35 | … | -0.00 | 1.56 | … | -5.28 | … | … |  | … | D
J15013+055 | M3.0 V | … |  |  | 0.33 | 1.85 | … | ¡ 2.0 | 0.34 | … | -0.05 | 1.55 | … | -6.30 | -5.12 | 2.64 |  | … | D
J15095+031 | M3.0 V | … |  |  | 0.43 | 1.79 | … | ¡ 2.0 | 0.43 | … | 0.05 | 2.59 | … | -5.38 | -5.13 | … |  | … | D
J15194-077 | M3.0 V | 132.50 | SM15 | S | 0.30 | 1.82 | 0.30 | ¡ 2.0 | 0.30 | … | 0.00 | 1.24 | … | … | -5.52 | 2.19 |  | … | YD
J15218+209 | M1.5 V | 3.35 | T.W. | S | 0.52 | 1.71 | -1.18 |  4.1$\pm$ 2.0 | 0.52 | 6.4 | -2.88 | 4.57 | -3.20 | -3.92 | -4.00 | 3.53 |  | … | D
J15305+094 | M5.5 V | 0.30 | DA19 | S | 0.11 | 2.26 | -2.77 |  13.4$\pm$ 2.0 | 0.13 | 0.5 | -4.20 | 0.13 | … | -3.91 | … | 3.68 |  | … | D
J15369-141 | M4.0 V | … |  |  | 0.30 | 1.93 | … | ¡ 2.0 | 0.30 | … | 0.08 | 1.15 | … | -6.00 | -5.52 | … |  | … | D
J15412+759 | M3.0 V | 83.40 | DA19 | S | 0.32 | 1.80 | 0.12 | ¡ 3.0 | 0.32 | … | -0.11 | 1.29 | … | -4.97 | … | … | SB2 | … | D
J15474-108 | M2.0 V | 46.71 | T.W. | P | 0.35 | 1.77 | -0.10 | ¡ 3.0 | … | … | -0.03 | 3.49 | … | … | … | … | ST3 | … | D
J15499+796 | M5.0 V | 0.19 | T.W. | S | 0.29 | 2.11 | -2.84 |  31.0$\pm$ 3.1 | 0.30 | 0.5 | -5.17 | 0.74 | -3.62 | -3.85 | … | 3.51 |  | 120 | YD
J15598-082 | M1.0 V | 20.00 | SM18 | P | 0.48 | 1.69 | -0.39 | ¡ 2.0 | 0.47 | … | -0.14 | 3.83 | -4.48 | … | -4.61 | 2.72 |  | … | D
J16028+205 | M4.0 V | … |  |  | 0.24 | 1.92 | … | ¡ 2.0 | 0.25 | … | 0.04 | 0.71 | … | -5.15 | -5.52 | 2.33 |  | … | TD-D
J16092+093 | M3.0 V | 44.30 | T.W. | P | 0.35 | 1.79 | -0.14 | ¡ 2.0 | 0.35 | … | -0.05 | 1.70 | … | … | -4.84 | 2.70 |  | … | D
J16102-193 | M3.0 V | 6.26 | DA19 | S | 0.51 | 2.06 | -1.27 |  7.3$\pm$ 2.0 | 0.94 | 6.5 | -1.43 | 10.26 | … | -4.10 | … | … |  | 10 | YD
J16167+672N | M3.0 V | 40.40 | Don23 | P | 0.45 | 1.78 | -0.17 | ¡ 2.0 | 0.45 | … | 0.06 | 2.97 | … | -5.19 | -4.92 | … |  | … | YD
J16167+672S | M0.0 V | 22.00 | Laf21 | P | 0.65 | 1.63 | -0.28 | ¡ 2.0 | 0.63 | … | 0.06 | 9.60 | -4.89 | -5.42 | -5.34 | 2.71 |  | … | D
J16254+543 | M1.5 V | 76.79 | DA19 | S | 0.30 | 1.70 | 0.19 | ¡ 2.0 | 0.31 | … | 0.00 | 1.42 | -5.03 | … | -5.33 | 2.46 |  | … | YD
J16303-126 | M3.5 V | 119.00 | DA19 | S | 0.29 | 1.90 | 0.18 | ¡ 2.0 | 0.30 | … | 0.01 | 1.09 | -5.09 | … | -5.31 | … |  | … | YD
J16313+408 | M5.0 V | 0.51 | T.W. | S | 0.16 | 2.20 | -2.49 |  7.4$\pm$ 2.0 | 0.17 | 1.2 | -7.46 | 0.27 | … | -3.64 | … | 3.62 |  | 50 | YD
J16327+126 | M3.0 V | … |  |  | 0.40 | 1.75 | … | ¡ 2.0 | 0.40 | … | 0.11 | 2.12 | … | -6.10 | -5.29 | … |  | … | TD-D
J16462+164 | M2.5 V | … |  |  | 0.41 | 1.79 | … | ¡ 2.0 | 0.42 | … | 0.02 | 2.50 | … | -5.46 | -5.11 | … |  | … | D
J16554-083N | M3.5 V | 6.52 | DA19 | D | 0.21 | 1.90 | -1.09 | ¡ 2.0 | 0.22 | … | -0.00 | 0.57 | … | … | -5.44 | 2.41 |  | … | D
J16555-083 | M7.0 V | 1.09 | Laf21 | S | 0.07 | 2.23 | -2.19 |  4.0$\pm$ 2.0 | 0.09 | 1.1 | -4.54 | 0.06 | … | -4.29 | … | 3.48 |  | … | D
J16570-043 | M3.5 V | 1.21 | Kir12 | S | 0.25 | 1.93 | -1.85 |  9.7$\pm$ 2.0 | 0.26 | 1.4 | -4.53 | 0.66 | -3.10 | -3.86 | -4.28 | 3.56 |  | … | YD
J16581+257 | M1.0 V | 23.80 | DA19 | S | 0.50 | 1.69 | -0.32 | ¡ 2.0 | 0.50 | … | -0.05 | 4.53 | … | -5.68 | -4.70 | 2.73 |  | … | D
J17033+514 | M4.5 V | 115.00 | Gor23 | P | 0.18 | 2.07 | -0.01 | ¡ 2.0 | 0.20 | … | 0.01 | 0.40 | … | -5.09 | … | … |  | … | D
J17052-050 | M1.5 V | 50.20 | DA19 | P | 0.48 | 1.69 | 0.01 | ¡ 2.0 | 0.48 | … | 0.11 | 3.38 | -4.82 | … | -5.09 | … |  | … | TD-D
J17071+215 | M3.0 V | … |  |  | 0.38 | 1.80 | … | ¡ 2.0 | 0.38 | … | 0.06 | 2.06 | … | -5.19 | -5.19 | … |  | … | D
J17115+384 | M3.5 V | 62.60 | DA19 | P | 0.37 | 1.85 | -0.05 | ¡ 2.0 | 0.37 | … | 0.08 | 1.83 | … | -5.11 | -5.28 | … |  | … | D
J17166+080 | M2.0 V | … |  |  | 0.40 | 1.74 | … | ¡ 2.0 | 0.40 | … | -0.01 | 2.31 | … | -5.36 | … | … |  | … | YD
J17198+417 | M2.5 V | 71.50 | DA19 | P | 0.35 | 1.76 | 0.10 | ¡ 2.0 | 0.36 | … | 0.00 | 1.80 | … | -5.43 | -5.38 | … |  | … | D
J17303+055 | M0.0 V | 34.60 | T.W. | S | 0.52 | 1.64 | -0.10 | ¡ 2.0 | 0.52 | … | -0.02 | 5.18 | … | -5.29 | -4.67 | 2.43 |  | … | YD
J17338+169 | M5.5 V | 0.27 | T.W. | S | 0.29 | 2.24 | -2.81 |  38.0$\pm$ 3.8 | 0.32 | 0.4 | -12.09 | 0.95 | -3.26 | -3.63 | … | 3.91 |  | 120 | YD
J17355+616 | M0.5 V | 18.39 | T.W. | S | 0.55 | 1.62 | -0.35 | ¡ 2.0 | 0.55 | … | -0.08 | 5.91 | … | -5.04 | … | 2.87 |  | … | D
J17378+185 | M1.0 V | 35.02 | T.W. | S | 0.43 | 1.66 | -0.11 | ¡ 2.0 | 0.43 | … | -0.07 | 2.97 | … | -5.24 | -5.09 | … |  | … | D
J17542+073 | M4.0 V | … |  |  | 0.30 | 1.95 | … | ¡ 2.0 | 0.31 | … | 0.09 | 1.02 | … | -5.82 | … | 2.45 |  | … | D
J17578+046 | M3.5 V | 145.00 | TP19 | S | 0.17 | 1.89 | 0.27 | ¡ 2.0 | 0.19 | … | 0.00 | 0.35 | -5.41 | -5.22 | -5.52 | 2.64 |  | … | TD
J17578+465 | M2.5 V | 30.30 | DA19 | S | 0.39 | 1.83 | -0.34 | ¡ 2.0 | 0.39 | … | -0.14 | 2.10 | -4.42 | -4.94 | … | 2.45 |  | … | YD
J18022+642 | M5.0 V | 0.28 | T.W. | S | 0.16 | 2.07 | -2.62 |  12.9$\pm$ 2.0 | 0.18 | 0.7 | -5.13 | 0.30 | -3.18 | -3.93 | … | 3.69 |  | 800 | D
J18027+375 | M5.0 V | 123.80 | New16 | P | 0.14 | 2.16 | -0.07 | ¡ 2.0 | 0.16 | … | 0.01 | 0.25 | … | … | … | … |  | … | D
J18051-030 | M1.0 V | 127.80 | SM15 | D | 0.44 | 1.66 | 0.45 | ¡ 2.0 | 0.44 | … | 0.00 | 3.30 | -4.87 | … | -4.96 | 2.42 |  | … | D
J18075-159 | M4.5 V | 3.87 | DA19 | S | 0.16 | 2.07 | -1.48 | ¡ 2.0 | 0.17 | … | -3.74 | 0.29 | -3.07 | -3.94 | … | 3.50 |  | … | D
J18131+260 | M4.0 V | 2.28 | T.W. | S | 0.33 | 1.94 | -1.58 |  6.3$\pm$ 2.0 | 0.34 | 2.7 | -5.86 | 1.18 | -2.68 | -3.71 | … | 3.65 |  | … | D
J18165+048 | M5.0 V | … |  |  | 0.18 | 2.09 | … | ¡ 2.0 | 0.19 | … | 0.05 | 0.37 | … | … | … | … |  | … | D
J18174+483 | M2.0 V | 15.83 | T.W. | S | 0.52 | 1.74 | -0.55 |  2.2$\pm$ 2.0 | 0.52 | 11.9 | -1.58 | 4.49 | -3.61 | -4.04 | … | 3.28 |  | 120 | YD
J18180+387E | M3.0 V | … |  |  | 0.28 | 1.93 | … | ¡ 2.0 | 0.29 | … | 0.02 | 1.15 | … | -5.15 | … | … |  | … | D
J18189+661 | M4.5 V | 0.52 | T.W. | S | 0.15 | 2.00 | -2.29 |  14.5$\pm$ 2.0 | 0.16 | 0.6 | -2.56 | 0.24 | -3.61 | -4.18 | … | 3.60 |  | … | D
J18198-019 | K7.0 V | 31.69 | T.W. | S | 0.59 | 1.55 | -0.05 | ¡ 2.0 | 0.59 | … | … | 9.24 | … | … | … | 2.44 |  | … | YD
J18221+063 | M4.0 V | … |  |  | 0.29 | 1.81 | … | ¡ 2.0 | 0.29 | … | 0.14 | 1.03 | … | -5.59 | -5.48 | … |  | … | TD
J18224+620 | M4.0 V | … |  |  | 0.16 | 2.04 | … | ¡ 2.0 | 0.18 | … | -0.07 | 0.33 | … | -5.26 | … | 2.70 |  | … | D
J18319+406 | M3.5 V | 50.20 | DA19 | P | 0.34 | 1.86 | -0.15 | ¡ 2.0 | 0.35 | … | -0.07 | 1.61 | -4.77 | -4.88 | -5.05 | … |  | … | YD
J18346+401 | M3.5 V | 40.20 | DA19 | S | 0.41 | 1.73 | -0.13 | ¡ 2.0 | 0.41 | … | -0.05 | 2.14 | -4.75 | … | -5.05 | 2.38 |  | … | D
J18353+457 | M0.5 V | 34.00 | DA19 | S | 0.60 | 1.58 | -0.05 | ¡ 2.0 | 0.59 | … | 0.11 | 7.03 | -5.17 | -5.26 | -4.74 | 2.20 |  | … | D
J18356+329 | M8.5 V | 0.12 | T.W. | S | 0.07 | 2.23 | -3.16 |  49.2$\pm$ 4.9 | 0.09 | 0.1 | -1.65 | 0.03 | … | -4.83 | … | … |  | … | D
J18363+136 | M4.0 V | 50.20 | DA19 | D | 0.30 | 1.88 | -0.18 | ¡ 2.0 | 0.31 | … | -0.85 | 1.06 | -3.54 | -4.49 | -5.06 | 3.17 |  | … | YD
J18409-133 | M1.0 V | 28.23 | T.W. | P | 0.53 | 1.66 | -0.21 | ¡ 2.0 | 0.52 | … | 0.05 | 5.12 | … | … | -4.66 | 2.49 |  | … | D
J18419+318 | M3.0 V | … |  |  | 0.34 | 1.86 | … | ¡ 2.0 | 0.34 | … | 0.04 | 1.63 | … | -5.18 | -5.44 | … |  | … | D
J18427+596N | M3.0 V | 103.10 | Don23 | P | 0.34 | 1.80 | 0.22 | ¡ 2.0 | 0.34 | … | … | 1.55 | … | -5.14 | … | … |  | … | D
J18427+596S | M3.5 V | 135.00 | Don23 | P | 0.26 | 1.86 | 0.27 | ¡ 2.0 | 0.27 | … | … | 0.85 | -5.04 | … | … | … |  | … | D
J18480-145 | M2.5 V | … |  |  | 0.36 | 1.76 | … | ¡ 2.0 | 0.37 | … | 0.03 | 1.90 | … | … | … | … |  | … | D
J18482+076 | M5.0 V | 2.76 | DA19 | S | 0.14 | 2.22 | -1.78 |  3.6$\pm$ 2.0 | 0.16 | 2.2 | -3.37 | 0.22 | -3.65 | -4.06 | … | 3.08 |  | 800 | YD
J18498-238 | M3.5 V | 2.87 | DA19 | S | 0.18 | 1.91 | -1.45 |  4.4$\pm$ 2.0 | 0.19 | 2.2 | -2.22 | 0.40 | … | -4.09 | -4.44 | 3.32 |  | 800 | D
J18580+059 | M0.5 V | 35.20 | DA19 | S | 0.58 | 1.64 | -0.10 | ¡ 2.0 | 0.58 | … | 0.00 | 6.62 | … | … | -4.59 | 2.75 |  | … | D
J19070+208 | M2.0 V | … |  |  | 0.31 | 1.89 | … | ¡ 2.0 | 0.32 | … | -0.11 | 1.45 | … | -4.90 | -5.83 | … |  | … | D
J19072+208 | M2.0 V | 3.80 | DA19 | D | 0.31 | 1.90 | -1.32 | ¡ 2.0 | 0.31 | … | -0.10 | 1.42 | … | -4.90 | -5.67 | … |  | … | D
J19084+322 | M3.0 V | 74.10 | DA19 | P | 0.33 | 1.87 | 0.00 | ¡ 2.0 | 0.34 | … | 0.03 | 1.55 | … | -5.24 | -5.41 | … |  | … | YD
J19098+176 | M4.5 V | 80.10 | DA19 | P | 0.19 | 2.06 | -0.16 | ¡ 2.0 | 0.20 | … | 0.02 | 0.42 | … | -5.13 | -5.15 | … |  | … | D
J19169+051N | M2.5 V | 46.00 | DA19 | S | 0.48 | 1.76 | -0.09 | ¡ 2.0 | 0.47 | … | 0.06 | 3.32 | … | -5.37 | -4.94 | 2.37 |  | … | D
J19169+051S | M8.0 V | 23.60 | DA19 | D | 0.08 | 2.21 | -0.83 |  3.7$\pm$ 2.0 | 0.10 | 1.4 | -5.24 | 0.04 | … | -4.39 | … | 3.08 |  | … | D
J19216+208 | M4.5 V | 133.00 | DA19 | S | 0.20 | 2.05 | 0.08 | ¡ 2.0 | 0.21 | … | 0.00 | 0.45 | … | -5.39 | -5.40 | 2.53 |  | … | D
J19251+283 | M3.0 V | … |  |  | 0.35 | 1.84 | … | ¡ 2.0 | 0.35 | … | -0.06 | 1.64 | … | … | -5.14 | 2.40 |  | … | D
J19255+096 | M8.0 V | … |  |  | 0.16 | 2.10 | … |  34.7$\pm$ 3.5 | 0.17 | 0.3 | -1.60 | 0.11 | … | -4.77 | … | … |  | … | YD
J19346+045 | M0.0 V | 21.79 | T.W. | S | 0.56 | 1.48 | -0.14 | ¡ 2.0 | 0.55 | … | 0.10 | 7.65 | … | -5.46 | -5.07 | 2.33 |  | … | D
J19422-207 | M5.1 V | 1.34 | T.W. | S | 0.21 | 2.02 | -1.89 |  6.7$\pm$ 2.0 | 0.22 | 1.7 | -5.80 | 0.48 | -2.91 | -3.83 | … | 3.58 |  | … | YD
J19511+464 | M4.0 V | 0.59 | T.W. | S | 0.27 | 1.94 | -2.16 |  24.6$\pm$ 2.5 | 0.28 | 0.6 | -4.46 | 0.71 | -3.36 | -3.74 | -4.89 | 3.62 |  | 800 | YD
J20093-012 | M5.0 V | 1.37 | T.W. | S | 0.14 | 2.12 | -1.99 |  5.5$\pm$ 2.0 | 0.16 | 1.5 | -5.15 | 0.27 | -3.35 | -3.72 | … | 3.57 |  | … | D
J20198+229 | M3.0 V | 1.13 | T.W. | S | 0.62 | 1.79 | -1.74 |  …$\pm$ … | 0.61 | … | -3.03 | 6.77 | -3.05 | … | … | … | SB2 | … | YD
J20260+585 | M5.0 V | 159.88 | Med22 | S | 0.16 | 2.11 | 0.09 | ¡ 2.0 | 0.17 | … | -0.07 | 0.29 | … | -5.24 | … | … |  | … | D
J20305+654 | M2.5 V | 32.80 | DA19 | S | 0.37 | 1.78 | -0.27 |  2.7$\pm$ 2.0 | 0.38 | 7.0 | -0.23 | 1.93 | -4.09 | -4.74 | -5.16 | 2.34 |  | … | D
J20336+617 | M4.0 V | 12.60 | DA19 | P | 0.38 | 1.81 | -0.71 | ¡ 2.0 | 0.38 | … | 0.06 | 1.74 | … | -4.92 | … | 2.42 |  | … | D
J20405+154 | M4.5 V | 106.00 | DA19 | S | 0.19 | 2.04 | -0.01 | ¡ 2.0 | 0.20 | … | -0.22 | 0.41 | … | -4.85 | -5.45 | 2.62 |  | … | D
J20450+444 | M1.5 V | 39.12 | T.W. | P | 0.41 | 1.68 | -0.09 | ¡ 2.0 | 0.41 | … | 0.07 | 2.60 | … | -5.52 | -4.94 | 2.23 |  | 800 | YD
J20451-313 | M0.5 V | 4.89 | T.W. | S | 0.61 | 1.73 | -1.04 |  8.2$\pm$ 2.0 | 0.86 | 5.3 | … | 9.88 | -2.85 | … | … | 3.48 |  | 25 | YD
J20525-169 | M4.0 V | 67.60 | DA19 | D | 0.22 | 1.97 | -0.14 | ¡ 2.0 | 0.23 | … | 0.01 | 0.63 | … | -5.40 | -5.12 | 2.58 |  | … | D
J20533+621 | M1.0 V | … |  |  | 0.53 | 1.68 | … | ¡ 2.0 | 0.52 | … | -0.00 | 5.22 | -4.87 | -5.28 | -4.83 | 2.54 |  | … | D
J20556-140N | M4.0 V | 137.37 | New18 | P | 0.25 | 1.87 | 0.27 | … | 0.26 | … | -0.01 | 1.05 | … | -5.05 | … | … | SB2 | … | TD
J20556-140S | M5.0 V | 134.63 | New18 | P | 0.15 | 2.05 | 0.08 | ¡ 2.0 | 0.16 | … | 0.08 | 0.25 | … | … | … | 2.57 |  | … | TD
J20567-104 | M2.5 V | 9.63 | DA19 | D | 0.46 | 1.70 | -0.72 | ¡ 2.0 | 0.46 | … | 0.04 | 3.06 | … | … | -5.00 | 2.47 |  | … | TD
J21019-063 | M2.5 V | 49.29 | T.W. | S | 0.45 | 1.79 | -0.09 | ¡ 2.0 | 0.45 | … | 0.04 | 2.97 | -4.74 | … | -4.96 | 2.38 |  | … | D
J21152+257 | M3.0 V | 34.80 | DA19 | P | 0.55 | 1.78 | -0.24 | ¡ 2.0 | 0.54 | … | 0.10 | 4.54 | … | -4.74 | … | 2.33 |  | … | D
J21164+025 | M3.0 V | 42.68 | T.W. | S | 0.40 | 1.80 | -0.17 | ¡ 2.0 | 0.41 | … | 0.10 | 2.36 | … | … | -5.07 | … |  | … | YD
J21221+229 | M1.0 V | 38.40 | T.W. | S | 0.49 | 1.63 | -0.05 | ¡ 2.0 | 0.48 | … | -0.03 | 4.21 | … | … | -4.85 | 2.71 |  | … | D
J21348+515 | M3.0 V | 54.30 | DA19 | S | 0.44 | 1.75 | -0.02 | ¡ 2.0 | 0.44 | … | 0.06 | 2.71 | … | -5.24 | … | … |  | … | YD
J21463+382 | M4.0 V | 93.90 | Don23 | P | 0.20 | 1.89 | 0.08 | ¡ 2.0 | 0.21 | … | 0.10 | 0.46 | … | -4.94 | … | 2.49 |  | … | TD
J21466-001 | M4.0 V | … |  |  | 0.27 | 1.94 | … | ¡ 2.0 | 0.28 | … | 0.08 | 0.96 | … | … | … | … |  | … | D
J21466+668 | M4.0 V | 100.00 | Ama21 | P | 0.29 | 1.91 | 0.09 | ¡ 2.0 | 0.29 | … | 0.08 | 1.04 | … | -4.68 | … | … |  | … | YD
J22012+283 | M4.0 V | 0.45 | DA19 | S | 0.32 | 1.95 | -2.30 |  36.4$\pm$ 3.6 | 0.32 | 0.5 | -4.47 | 0.99 | -3.13 | -3.76 | -5.05 | 3.56 |  | 800 | YD
J22020-194 | M3.5 V | … |  |  | 0.33 | 1.85 | … | ¡ 2.0 | 0.33 | … | 0.06 | 1.44 | … | … | -5.32 | … |  | … | D
J22021+014 | M0.5 V | 22.06 | T.W. | S | 0.57 | 1.66 | -0.32 | ¡ 2.0 | 0.56 | … | 0.02 | 6.42 | … | -5.49 | -4.59 | 2.61 |  | … | D
J22057+656 | M1.5 V | 120.47 | Laf21 | P | 0.47 | 1.64 | 0.44 | ¡ 2.0 | 0.47 | … | 0.11 | 3.72 | … | … | … | 2.45 |  | … | D
J22096-046 | M3.5 V | 39.20 | SM15 | S | 0.45 | 1.83 | -0.24 | ¡ 2.0 | 0.45 | … | 0.14 | 2.90 | … | … | -5.07 | 2.28 |  | … | YD
J22114+409 | M5.5 V | 30.00 | DA19 | S | 0.16 | 2.23 | -0.75 | ¡ 2.0 | 0.18 | … | -5.74 | 0.27 | -2.94 | -3.88 | … | 3.27 |  | … | YD
J22115+184 | M2.0 V | 36.30 | DA19 | S | 0.51 | 1.74 | -0.18 | ¡ 2.0 | 0.50 | … | 0.03 | 4.29 | … | -5.08 | … | 2.41 |  | … | D
J22125+085 | M3.0 V | … |  |  | 0.36 | 1.76 | … | ¡ 2.0 | 0.36 | … | 0.04 | 1.83 | … | -5.06 | -5.31 | … |  | … | D
J22137-176 | M4.5 V | 116.40 | Ste16 | P | 0.18 | 2.03 | 0.04 | ¡ 2.0 | 0.19 | … | 0.06 | 0.36 | … | -5.04 | -5.06 | 2.50 |  | … | YD
J22231-176 | M4.5 V | 4.57 | T.W. | S | 0.18 | 2.14 | -1.48 |  2.3$\pm$ 2.0 | 0.19 | 4.2 | -3.93 | 0.35 | -3.23 | -4.00 | -5.18 | 3.33 |  | 120 | D
J22252+594 | M4.0 V | 64.60 | DA19 | S | 0.40 | 1.90 | -0.09 | ¡ 2.0 | 0.40 | … | 0.08 | 2.04 | … | -5.08 | … | 2.32 |  | … | D
J22298+414 | M4.0 V | 99.80 | DA19 | P | 0.25 | 1.97 | 0.02 | ¡ 2.0 | 0.26 | … | 0.08 | 0.75 | … | -5.10 | … | … |  | … | D
J22330+093 | M1.0 V | 37.80 | T.W. | S | 0.45 | 1.64 | -0.06 | ¡ 2.0 | 0.45 | … | -0.03 | 3.49 | … | -5.18 | -4.85 | 2.50 |  | … | YD
J22468+443 | M3.5 V | 4.35 | T.W. | S | 0.34 | 1.88 | -1.24 |  4.1$\pm$ 2.0 | 0.34 | 4.2 | -4.98 | 1.25 | -2.59 | -3.76 | -4.46 | 3.64 |  | 800 | D
J22503-070 | M0.5 V | … |  |  | 0.55 | 1.59 | … | ¡ 2.0 | 0.54 | … | -0.03 | 6.07 | … | … | -4.49 | 2.64 |  | … | D
J22518+317 | M3.0 V | 1.63 | DA19 | S | 0.35 | 1.82 | -1.61 |  12.7$\pm$ 2.0 | 0.54 | 2.1 | -5.17 | 2.64 | -3.03 | -3.71 | … | 3.59 |  | 50 | YD
J22532-142 | M4.0 V | 81.00 | DA19 | S | 0.31 | 1.94 | -0.03 | ¡ 2.0 | 0.32 | … | 0.06 | 1.27 | … | … | -5.18 | 2.29 |  | … | YD
J22559+178 | M1.0 V | 27.00 | SM18 | P | 0.55 | 1.67 | -0.24 | ¡ 2.0 | 0.54 | … | -0.03 | 5.58 | … | … | -4.55 | 2.76 |  | … | D
J22565+165 | M1.5 V | 39.50 | DA19 | S | 0.53 | 1.79 | -0.20 | ¡ 2.0 | 0.52 | … | 0.07 | 5.13 | -5.17 | -5.12 | -4.65 | 2.52 |  | … | D
J23064-050 | M8.0 V | 3.30 | DA19 | S | 0.09 | 2.19 | -1.68 | ¡ 2.0 | 0.11 | … | -1.98 | 0.05 | … | -4.69 | … | … |  | … | D
J23113+085 | M3.5 V | 44.82 | T.W. | P | 0.43 | 1.90 | -0.25 | ¡ 2.0 | 0.43 | … | 0.03 | 2.42 | … | -5.07 | … | 2.35 |  | … | D
J23216+172 | M4.0 V | 74.70 | DA19 | S | 0.37 | 1.94 | -0.07 | ¡ 2.0 | 0.38 | … | 0.02 | 1.69 | … | -5.05 | -5.06 | 2.40 |  | … | D
J23245+578 | M1.0 V | 36.48 | T.W. | S | 0.54 | 1.70 | -0.14 | ¡ 2.0 | 0.54 | … | 0.02 | 5.44 | -5.10 | … | -4.54 | 2.64 |  | … | D
J23340+001 | M2.5 V | … |  |  | 0.43 | 1.69 | … | ¡ 2.0 | 0.43 | … | 0.08 | 2.63 | … | -5.24 | -5.26 | … |  | … | D
J23351-023 | M5.5 V | 178.00 | Don23 | S | 0.11 | 2.16 | 0.09 | ¡ 2.0 | 0.13 | … | -0.82 | 0.15 | … | -4.53 | … | 2.96 |  | … | D
J23381-162 | M2.0 V | 61.66 | Wat06 | D | 0.36 | 1.71 | 0.08 | ¡ 2.0 | 0.36 | … | 0.01 | 1.95 | … | … | -5.37 | … |  | … | D
J23419+441 | M5.0 V | 106.00 | DA19 | S | 0.14 | 2.12 | -0.10 | ¡ 2.0 | 0.16 | … | -0.38 | 0.23 | -3.67 | -5.11 | -5.03 | 2.62 |  | … | TD-D
J23431+365 | M4.0 V | 73.66 | Don23 | S | 0.22 | 2.02 | -0.15 | ¡ 2.0 | 0.23 | … | -0.88 | 0.57 | -3.62 | -4.50 | … | 3.13 |  | … | YD
J23492+024 | M1.0 V | 49.90 | SM18 | S | 0.42 | 1.73 | -0.04 | ¡ 2.0 | 0.42 | … | -0.02 | 2.56 | -4.84 | -5.05 | -5.21 | … |  | … | TD
J23505-095 | M4.0 V | … |  |  | 0.29 | 1.92 | … | ¡ 2.0 | 0.30 | … | 0.01 | 1.03 | … | … | -4.77 | … |  | … | D
J23548+385 | M4.0 V | 4.80 | T.W. | S | 0.31 | 1.91 | -1.23 |  3.6$\pm$ 2.0 | 0.32 | 4.5 | -3.35 | 1.04 | -2.86 | -3.66 | … | 3.69 |  | 800 | D
J23556-061 | M2.5 V | … |  |  | 0.52 | 1.75 | … | ¡ 2.0 | 0.51 | … | 0.07 | 4.61 | … | … | … | … | SB1 | … | D
J23585+076 | M3.0 V | 55.40 | T.W. | P | 0.46 | 1.80 | -0.06 | ¡ 2.0 | 0.45 | … | 0.04 | 2.93 | … | -5.74 | … | … | ST3 | … | YD

Note: This table is available in its entirety in ASCII format online.
a: For known SBs, we tabulate the combined spectral type or that of the
primary.
b: T.W. refers to This Work.
c: Secure flags: ‘S’ = secure; ‘P’ = provisional; ‘D’ = debated.
d: Ages of 800 Myr are upper limits.

Table 4: Adopted, literature, and all measured $P_{\rm rot}$ of our investigated stars. Karmn |  Best $P_{\rm rot}$ | Source | Secure |  $P$1 b |  $\delta P$1 | Ref1 |  $P$ (Planet) | Ref |  $P$ (Laf21) |  $P$ (Other | Other phot |  $P$ (TESS) | TESS |  $P$ (SWASP) | SWASP |  $P$ (Spect)
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---
| (d) |  |  flaga | (d) | (d) |  | (d) | (Planet) | (d) | phot) (d) | facility | (d) | LC type | (d) | flag | (d)
J00051+457 | 15.37 | DA19 | D | 15.37 | 0.09 | DA19 | … |  | … | … |  | … |  | … |  | …
J00067-075 | 93.00 | Fou23 | S | 93.00 | 1.60 | Fou23 | 126.00 | SM23 | … | … |  | … |  | … |  | …
J00162+198E | 105.00 | DA19 | S | 105.00 | 44.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J00162+198W | 4.83 | DA19 | S | 4.83 | 0.06 | DA19 | … |  | … | … |  | … |  | … |  | …
J00183+440 | 45.00 | SM18 | S | 45.00 | 4.40 | SM18 | 43.82 | How14 | 46.19 | … |  | … |  | … |  | …
J00184+440 | 113.30 | Don23 | S | 113.30 | 4.30 | Don23 | … |  | … | … |  | … |  | … |  | …
J00286-066 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J00389+306 | 50.20 | DA19 | P | 50.20 | 1.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J00570+450 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J01013+613 | 34.70 | SM18 | P | 34.70 | 0.10 | SM18 | … |  | … | … |  | … |  | … |  | …
J01019+541 | 0.28 | DA19 | S | 0.28 | 0.00 | DA19 | … |  | … | … |  | 0.14 | PDCSAP | … |  | …
J01025+716 | 50.52 |  LCO-$V$ | S | 51.50 | 2.60 | DA19 | … |  | 51.73 | 50.52 |  LCO-$V$ | … |  | … |  | 51.37
J01026+623 | 18.82 |  OSN-$R$ | S | 19.90 | 0.40 | DA19 | 18.90 | Per19 | 20.00 | 18.82 |  OSN-$R$ | 18.94 | SAP | … |  | 18.89
J01033+623 | 1.02 | TESS | S | 1.02 | 0.01 | DA19 | … |  | … | … |  | 1.02 | PDCSAP | … |  | …
J01048-181 | 143.20 | New18 | P | 143.20 | … | New18 | … |  | … | … |  | … |  | … |  | …
J01056+284 | 16.32 | Bar18 | P | 16.32 | 0.24 | Bar18 | … |  | … | … |  | … |  | … |  | …
J01125-169 | 70.10 | SWASP | S | 69.20 | 2.40 | DA19 | 83.00 | AD17b | 80.67 | … |  | … |  | 70.10 |  | …
J01339-176 | 7.75 | TESS-SAP | S | 7.85 | … | Pas23 | … |  | … | … |  | 7.75 | SAP | … |  | …
J01352-072 | 0.70 | TESS | S | 0.70 | … | Kir12 | … |  | … | … |  | 0.70 | PDCSAP | … |  | …
J01433+043 | 14.65 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 14.65 |  | …
J01518+644 | … |  |  | 31.37 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J02002+130 | 2.00 | SWASP | S | 1.96 | … | Pas23 | … |  | 1.95 | … |  | … |  | 2.00 |  | …
J02015+637 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J02070+496 | 7.20 | DA19 | S | 7.20 | 0.13 | DA19 | … |  | … | … |  | … |  | … |  | …
J02088+494 | 0.75 | TESS | S | 0.75 | 0.00 | DA19 | … |  | … | … |  | 0.75 | PDCSAP | … |  | …
J02123+035 | 17.11 | SWASP | D | … | … |  | … |  | … | … |  | … |  | 17.11 |  | 52.33
J02222+478 | 29.50 | DA19 | S | 29.50 | 0.40 | DA19 | … |  | 28.88 | … |  | … |  | … |  | 31.05
J02336+249 | 3.00 | TESS | S | 3.00 | … | Pas23 | … |  | … | … |  | 3.00 | PDCSAP | 2.98 |  | …
J02358+202 | 31.90 | DA19 | D | 31.90 | 0.60 | DA19 | … |  | … | … |  | … |  | … |  | …
J02362+068 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J02442+255 | 38.70 | DA19 | P | 38.70 | 3.70 | DA19 | … |  | … | … |  | … |  | … |  | …
J02519+224 | 0.86 | DA19 | S | 0.86 | 0.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J02530+168 | 97.56 | Laf21 | S | 99.60 | 1.40 | Ter22 | … |  | 97.56 | … |  | … |  | … |  | …
J02565+554W | 51.20 | SM18 | P | 51.20 | 4.40 | SM18 | … |  | … | … |  | … |  | … |  | …
J03133+047 | 126.20 | New16 | S | 126.20 | … | New16 | … |  | 140.81 | … |  | … |  | … |  | …
J03181+382 | 77.20 | DA19 | P | 77.20 | 3.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J03213+799 | 23.26 | Astrolab- | D | 32.40 | 1.00 | DA19 | … |  | … | 23.26 |  Astrolab-$V$ | … |  | … |  | …
J03217-066 | 21.00 | TESS-SAP | S | 21.10 | 0.10 | DA19 | … |  | … | … |  | 21.00 | SAP | … |  | …
J03463+262 | 16.40 | SWASP | D | 16.24 | … | Oel18 | … |  | … | … |  | … |  | 16.40 |  | 10.27
J03473-019 | 3.88 | TESS | S | 3.87 | 0.01 | DA19 | … |  | … | … |  | 3.88 | PDCSAP | … |  | …
J03531+625 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J04153-076 | 8.56 | Spect | D | … | … |  | … |  | 1.80 | … |  | … |  | … |  | 8.56
J04167-120 | 33.00 | Dre20 | P | … | … |  | 33.00 | Dre20 | … | … |  | … |  | … |  | …
J04173+088 | 0.37 | TESS | S | 0.18 | … | Wes15 | … |  | … | … |  | 0.37 | PDCSAP | 0.37 |  | …
J04198+425 | 0.99 | TESS | S | … | … |  | … |  | … | … |  | 0.99 | PDCSAP | … |  | …
J04225+105 | 5.48 | DA19 | D | 5.48 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J04290+219 | 25.40 | DA19 | S | 25.40 | 0.30 | DA19 | … |  | 25.14 | … |  | … |  | … |  | 25.65
J04311+589 | 91.90 | Fou23 | S | 91.90 | 3.40 | Fou23 | … |  | … | … |  | … |  | … |  | …
J04376-110 | … |  |  | … | … |  | … |  | … | … |  | … |  | 28.64 | U | …
J04376+528 | 15.47 | Laf21 | S | … | … |  | … |  | 15.47 | … |  | … |  | … |  | …
J04429+189 | 40.70 | DA19 | S | 40.70 | 0.40 | DA19 | … |  | … | … |  | … |  | … |  | 39.48
J04429+214 | 47.80 | DA19 | P | 47.80 | 1.10 | DA19 | … |  | … | … |  | … |  | … |  | …
J04472+206 | 0.34 | DA19 | S | 0.34 | 0.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J04520+064 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J04538-177 | 53.10 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 53.10 |  | …
J04588+498 | 17.46 | TESS-SAP | S | … | … |  | … |  | 19.19 | … |  | 17.46 | SAP | … |  | 19.19
J05019-069 | 93.87 | SWASP | S | 94.60 | … | New18 | … |  | … | … |  | … |  | 93.87 |  | …
J05019+011 | 2.08 | TESS | S | 2.12 | 0.02 | DA19 | … |  | 2.09 | … |  | 2.08 | PDCSAP | … |  | …
J05033-173 | … |  |  | 87.79 | … | New18(U) | … |  | … | … |  | … |  | … |  | …
J05062+046 | 0.89 | TESS | S | 0.87 | 0.00 | DA19 | … |  | … | … |  | 0.89 | PDCSAP | … |  | …
J05084-210 | 0.28 | TESS | S | … | … |  | … |  | … | … |  | 0.28 | PDCSAP | … |  | …
J05127+196 | 32.70 | Spect | P | … | … |  | … |  | … | … |  | … |  | … |  | 32.70
J05280+096 | 17.20 | DA19 | P | 17.20 | 0.10 | DA19 | … |  | … | … |  | … |  | … |  | …
J05314-036 | 33.80 | DA19 | S | 33.80 | 0.60 | DA19 | … |  | 34.07 | … |  | … |  | … |  | 34.80
J05337+019 | 0.60 | TESS | S | 18.40 | 0.40 | How20 | … |  | … | … |  | 0.60 | PDCSAP | 0.60 |  | …
J05348+138 | … |  |  | 43.53 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J05360-076 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J05365+113 | 11.75 |  OSN-$V$ | S | 12.30 | 0.10 | DA19 | … |  | 11.77 | 11.75 |  OSN-$V$ | 11.61 | SAP | … |  | 11.81
J05366+112 | 5.44 | TESS-FFI | S | 5.31 | … | Pas22 | … |  | … | … |  | 5.44 | FFI | … |  | …
J05394+406 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J05415+534 | 17.39 |  OSN-$R$ | P | … | … |  | … |  | … | 17.39 |  OSN-$R$ | … |  | … |  | …
J05421+124 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J05532+242 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J06000+027 | 1.81 | TESS | S | 1.81 | 0.01 | DA19 | … |  | … | … |  | 1.81 | PDCSAP | … |  | …
J06011+595 | 95.10 | Don23 | S | 95.10 | 2.30 | Don23 | … |  | … | … |  | … |  | … |  | …
J06024+498 | 105.00 | DA19 | S | 105.00 | 6.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J06103+821 | 44.60 | DA19 | P | 44.60 | 1.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J06105-218 | 27.30 | DA19 | S | 27.30 | 0.20 | DA19 | … |  | … | … |  | … |  | … |  | …
J06246+234 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J06318+414 | 0.30 | TESS | S | 0.30 | 0.00 | DA19 | … |  | … | … |  | 0.30 | PDCSAP | … |  | …
J06371+175 | 37.50 | Luq22 | S | … | … |  | 37.50 | Luq22 | … | … |  | … |  | 74.58 | U | …
J06396-210 | 79.15 | New18 | P | 79.15 | … | New18 | … |  | … | … |  | … |  | … |  | …
J06421+035 | 83.40 | DA19 | P | 83.40 | 7.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J06548+332 | 122.00 | Sto20b | S | 90.00 | … | Mou17 | 122.10 | Sto20b | … | … |  | … |  | … |  | …
J06574+740 | 0.61 | TESS-FFI | S | … | … |  | … |  | … | … |  | 0.61 | FFI | … |  | …
J06594+193 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J07001-190 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J07033+346 | 8.00 | TESS-SAP | S | 8.04 | 0.03 | DA19 | … |  | … | … |  | 8.00 | SAP | … |  | …
J07044+682 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J07274+052 | 93.50 | SM17 | D | 93.50 | 16.00 | SM17 | … |  | … | … |  | … |  | … |  | …
J07287-032 | 115.40 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 115.40 |  | …
J07319+362N | 16.40 | DA19 | P | 16.40 | 0.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J07353+548 | 21.80 | DA19 | P | 21.80 | 1.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J07361-031 | 12.20 | SWASP | S | 12.20 | 0.10 | DA19 | … |  | … | 12.19 |  SNO-$R$ | 12.41 | SAP | 12.20 |  | …
J07386-212 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J07393+021 | 11.45 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 11.45 |  | …
J07403-174 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J07446+035 | 2.78 | TESS | S | 2.78 | 0.01 | DA19 | … |  | 2.78 | … |  | 2.78 | PDCSAP | … |  | …
J07472+503 | 1.32 | TESS | S | 1.32 | 0.01 | DA19 | … |  | … | … |  | 1.32 | PDCSAP | … |  | …
J07558+833 | 1.11 | TESS | S | 1.11 | 0.01 | DA19 | … |  | … | … |  | 1.11 | PDCSAP | … |  | …
J07582+413 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08023+033 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08119+087 | 5.42 | DA19 | D | 5.42 | 0.15 | DA19 | … |  | … | … |  | … |  | … |  | …
J08126-215 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08161+013 | 40.70 | DA19 | P | 40.70 | 0.40 | DA19 | … |  | … | … |  | … |  | … |  | …
J08293+039 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08298+267 | 0.46 | DA19 | S | 0.46 | 0.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J08315+730 | 105.00 | DA19 | S | 105.00 | 11.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J08358+680 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08402+314 | 118.00 | DA19 | S | 118.00 | 14.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J08409-234 | 57.50 | Irv23 | D | 57.50 | 1.70 | Irv23 | … |  | … | … |  | … |  | … |  | …
J08413+594 | 83.27 | Pas23 | S | 83.27 | … | Pas23 | 87.00 | Mor19 | 88.65 | … |  | … |  | … |  | …
J08526+283 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J08536-034 | 0.46 | TESS | S | … | … |  | … |  | … | … |  | 0.46 | PDCSAP | … |  | …
J09003+218 | 0.44 | New16 | S | 0.44 | … | New16 | … |  | … | … |  | … |  | … |  | …
J09005+465 | 8.00 | Wes15 | S | 8.00 | … | Wes15 | … |  | … | … |  | … |  | … |  | …
J09028+680 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09033+056 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09133+688 | 10.40 | SM18 | P | 10.40 | 0.10 | SM18 | … |  | … | … |  | … |  | … |  | …
J09140+196 | 39.10 | SWASP | P | 89.90 | 2.00 | DA19 | … |  | … | … |  | … |  | 39.10 |  | …
J09143+526 | 17.54 | Spect | S | … | … |  | … |  | 16.37 | … |  | … |  | … |  | 17.54
J09144+526 | 16.88 | Spect | S | 42.20 | 4.10 | Don23 (U) | 16.61 | GA20 | 16.69 | … |  | … |  | … |  | 16.88
J09161+018 | 1.43 | TESS | S | … | … |  | … |  | … | … |  | 1.43 | PDCSAP | … |  | …
J09163-186 | … |  |  | 1.05 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J09307+003 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09360-216 | 74.30 | SM15 | S | 74.30 | 1.70 | SM15 | 77.80 | Luq19 | … | … |  | … |  | … |  | …
J09411+132 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09423+559 | 74.30 | DA19 | S | 74.30 | 2.80 | DA19 | … |  | … | … |  | … |  | … |  | …
J09425+700 | 21.00 | DA19 | P | 21.00 | 0.40 | DA19 | … |  | … | … |  | … | SAP | … |  | …
J09428+700 | 24.33 |  LCO-$V$ | S | 23.90 | 0.60 | DA19 | … |  | … | 24.33 |  LCO-$V$ | … | SAP | … |  | …
J09439+269 | 13.70 | DA19 | D | 13.70 | 0.90 | DA19 | … |  | … | … |  | … |  | … |  | …
J09447-182 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09449-123 | 0.44 | TESS | S | 0.44 | … | Med20 | … |  | … | … |  | 0.44 | PDCSAP | … |  | …
J09468+760 | 50.62 | Spect | P | … | … |  | … |  | … | … |  | … |  | … |  | 50.62
J09511-123 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J09561+627 | 16.88 | TESS-SAP | S | 8.55 | … | Oel18 | … |  | 17.79 | … |  | 16.88 | SAP | … |  | 17.77
J10023+480 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J10088+692 | 41.20 | Blu20 | S | … | … |  | 41.20 | Blu20 | … | … |  | … |  | … |  | …
J10122-037 | 23.00 | TESS-SAP | S | 21.60 | 0.20 | DA19 | … |  | … | … |  | 23.00 | SAP | … |  | 21.43
J10125+570 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J10167-119 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J10182-204 | 14.50 | TESS-SAP | S | 7.31 | 0.04 | Bar18 | … |  | … | … |  | 14.50 | SAP | … |  | …
J10196+198 | 2.24 | Mor08 | S | 2.24 | 0.00 | Mor08 | … |  | 2.24 | … |  | … |  | … |  | …
J10251-102 | 25.05 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 25.05 |  | …
J10289+008 | 31.72 | SWASP | S | 35.10 | 13.00 | Rei20 | 34.15 | Ama21 | … | … |  | … |  | 31.72 |  | …
J10350-094 | … |  |  | 47.64 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J10354+694 | 118.00 | DA19 | S | 118.00 | 10.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J10360+051 | 6.90 | TESS-SAP | S | … | … |  | … |  | … | … |  | 6.90 | SAP | … |  | …
J10396-069 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J10416+376 | 54.30 | DA19 | D | 54.30 | 4.40 | DA19 | … |  | … | … |  | … |  | … |  | …
J10482-113 | 1.50 | Mor10 | S | 1.50 | 0.20 | Mor10 | … |  | … | … |  | … |  | … |  | …
J10504+331 | … |  |  | 19.35 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J10508+068 | 64.00 | DA19 | P | 64.00 | 19.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J10564+070 | 2.70 | DA19 | S | 2.70 | 0.00 | DA19 | … |  | 2.70 | … |  | … |  | … |  | …
J10584-107 | … |  |  | … | … |  | … |  | … | … |  | … |  | 27.87 | U | …
J11000+228 | 53.17 | Spect | S | 171.00 | 8.40 | Don23 | … |  | … | … |  | … |  | 53.66 | U | 53.17
J11026+219 | 14.26 | SWASP | S | 14.60 | 0.20 | DA19 | … |  | … | … |  | 13.48 | SAP | 14.26 |  | 14.93
J11033+359 | 56.15 | Dia19 | S | 48.00 | … | KS07 | 56.15 | Dia19 | … | … |  | … |  | … |  | …
J11054+435 | 36.90 | Don23 | D | 36.90 | 2.50 | Don23 | … |  | … | … |  | … |  | … |  | …
J11055+435 | 0.78 | Mor10 | S | 0.78 | 0.02 | Mor10 | … |  | … | … |  | … |  | … |  | …
J11110+304E | 40.00 | Ded21 | P | 38.55 | … | Oel18 | 40.00 | Ded21 | … | … |  | … |  | … |  | …
J11110+304W | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J11126+189 | … |  |  | … | … |  | … |  | … | … |  | … |  | 87.15 | U | …
J11201-104 | 5.64 | TESS | S | … | … |  | … |  | … | … |  | 5.64 | PDCSAP | … |  | …
J11289+101 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J11302+076 | 36.40 | DA19 | S | 36.40 | 0.30 | DA19 | 39.63 | Sar18 | 35.05 | … |  | … |  | 36.91 | U | …
J11306-080 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J11417+427 | 71.50 | DA19 | D | 71.50 | 5.10 | DA19 | 98.10 | Hag10 | … | … |  | … |  | … |  | …
J11421+267 | 44.60 | DA19 | S | 44.60 | 2.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J11467-140 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J11474+667 | 13.30 | TESS-SAP | S | … | … |  | … |  | … | … |  | 13.30 | SAP | … |  | …
J11476+002 | 11.60 | DA19 | S | 11.60 | 0.04 | DA19 | … |  | … | … |  | … |  | … |  | …
J11476+786 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J11477+008 | 112.83 | Ste16 | S | 112.83 | … | Ste16 | 121.00 | Bon18 | … | … |  | … |  | 105.00 |  | …
J11509+483 | 148.95 | Med22 | S | 148.95 | … | Med22 | 140.00 | Bla23 | … | … |  | … |  | … |  | 83.57
J11511+352 | 22.80 | DA19 | S | 22.80 | 1.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J12054+695 | 100.00 | DA19 | S | 100.00 | 10.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J12100-150 | 79.30 |  LCO-$B$ | P | … | … |  | … |  | … | 79.30 |  LCO-$B$ | … |  | … |  | …
J12111-199 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J12123+544S | 96.70 | Sto20b | P | … | … |  | 96.70 | Sto20b | … | … |  | … |  | … |  | …
J12156+526 | 0.73 | TESS | S | … | … |  | … |  | … | … |  | 0.73 | PDCSAP | … |  | …
J12189+111 | 0.49 | DA19 | S | 0.49 | 0.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J12230+640 | 32.90 | DA19 | D | 32.90 | 1.10 | DA19 | … |  | … | … |  | … |  | … |  | 51.51
J12248-182 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J12312+086 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J12350+098 | 36.60 | DA19 | P | 36.60 | 1.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J12373-208 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J12388+116 | 55.35 | SWASP | S | 25.00 | 0.24 | Don23 (U) | 49.30 | Fen20 | … | … |  | … |  | 55.35 |  | …
J12428+418 | 16.20 | DA19 | P | 16.20 | 0.10 | DA19 | … |  | … | … |  | … |  | … |  | …
J12479+097 | 49.90 | Cab22 | D | 49.90 | 5.50 | Cab22 | 130.10 | Tri21 | … | … |  | … |  | … |  | …
J13005+056 | 0.60 | TESS | S | 0.60 | 0.00 | DA19 | … |  | … | … |  | 0.60 | PDCSAP | … |  | …
J13102+477 | 29.06 | SWASP | S | 28.80 | 0.80 | DA19 | … |  | … | … |  | … |  | 29.06 |  | …
J13196+333 | 48.00 | SM18 | P | 48.00 | 4.80 | SM18 | … |  | … | … |  | … |  | … |  | …
J13209+342 | … |  |  | 43.53 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J13229+244 | 95.00 | Luq18 | D | 132.88 | … | Med22 | 95.00 | Luq18 | … | … |  | … |  | … |  | …
J13283-023W | 46.42 | Rae20 | P | 46.42 | … | Rae20 | … |  | … | … |  | … |  | … |  | …
J13293+114 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J13299+102 | 30.00 | SM17 | S | 30.00 | 0.90 | SM17 | … |  | … | … |  | … |  | … |  | 30.92
J13427+332 | … |  |  | 16.50 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J13450+176 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J13457+148 | 52.30 | SM15 | P | 52.30 | 1.70 | SM15 | … |  | … | … |  | … |  | … |  | …
J13458-179 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J13536+776 | 1.23 | TESS | S | 1.23 | 0.01 | DA19 | … |  | … | … |  | 1.23 | PDCSAP | … |  | …
J13582+125 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J13591-198 | 3.32 | TESS | S | 3.33 | … | New18 | … |  | … | … |  | 3.32 | PDCSAP | … |  | …
J14010-026 | 43.90 | SM17 | S | 43.90 | 0.80 | SM17 | … |  | … | … |  | … |  | … |  | …
J14082+805 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J14152+450 | 52.80 | DA19 | P | 52.80 | 1.40 | DA19 | … |  | … | … |  | … |  | … |  | …
J14155+046 | 8.92 | Bar18 | D | 8.92 | 0.24 | Bar18 | … |  | … | … |  | … |  | … |  | …
J14173+454 | 0.37 | TESS | S | … | … |  | … |  | … | … |  | 0.37 | PDCSAP | … |  | …
J14251+518 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J14257+236E | 17.60 | DA19 | D | 17.60 | 0.50 | DA19 | … |  | … | … |  | … |  | … |  | 12.61
J14257+236W | 111.00 | DA19 | P | 111.00 | 12.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J14294+155 | 43.50 | SM18 | P | 43.50 | 1.50 | SM18 | … |  | … | … |  | … |  | … |  | …
J14307-086 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J14310-122 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J14321+081 | 0.76 | Pas23 | S | 0.76 | … | Pas23 | … |  | … | … |  | … |  | 1.12 |  | …
J14342-125 | 94.77 |  TJO-$R$ | S | … | … |  | 96.00 | GA23 | … | 94.77 |  TJO-$R$ | … |  | … |  | …
J14524+123 | 26.03 | SWASP | S | … | … |  | … |  | … | … |  | … |  | 26.03 |  | 23.31
J14544+355 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J15013+055 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J15095+031 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J15194-077 | 132.50 | SM15 | S | 132.50 | 6.30 | SM15 | … |  | … | … |  | … |  | … |  | …
J15218+209 | 3.35 | TESS | S | 3.37 | 0.01 | DA19 | … |  | … | … |  | 3.35 | PDCSAP | … |  | …
J15305+094 | 0.30 | DA19 | S | 0.30 | 0.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J15369-141 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J15412+759 | 83.40 | DA19 | S | 83.40 | 10.40 | DA19 | … |  | … | … |  | … |  | … |  | …
J15474-108 | 46.71 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 46.71 |  | …
J15499+796 | 0.19 | TESS | S | … | … |  | … |  | … | … |  | 0.19 | PDCSAP | … |  | …
J15598-082 | 20.00 | SM18 | P | 20.00 | 2.00 | SM18 | … |  | … | … |  | … |  | … |  | …
J16028+205 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J16092+093 | 44.30 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 44.30 |  | …
J16102-193 | 6.26 | DA19 | S | 6.26 | 0.15 | DA19 | … |  | … | … |  | … |  | … |  | …
J16167+672N | 40.40 | Don23 | P | 40.40 | 3.00 | Don23 | … |  | … | … |  | … |  | … |  | …
J16167+672S | 22.00 | Laf21 | P | … | … |  | … |  | 22.00 | … |  | … |  | … |  | …
J16254+543 | 76.79 | DA19 | S | 76.79 | 0.13 | DA19 | … |  | … | … |  | … |  | … |  | …
J16303-126 | 119.00 | DA19 | S | 119.00 | 1.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J16313+408 | 0.51 | TESS | S | 0.51 | 0.00 | DA19 | … |  | … | … |  | 0.51 | PDCSAP | … |  | …
J16327+126 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J16462+164 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J16554-083N | 6.52 | DA19 | D | 6.52 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J16555-083 | 1.09 | Laf21 | S | … | … |  | … |  | 1.09 | … |  | … |  | … |  | …
J16570-043 | 1.21 | Kir12 | S | 1.21 | … | Kir12 | … |  | … | … |  | … |  | … |  | …
J16581+257 | 23.80 | DA19 | S | 23.80 | 0.10 | DA19 | 24.80 | Joh10 | … | … |  | … |  | 11.73 |  | 23.31
J17033+514 | 115.00 | Gor23 | P | … | … |  | 115.00 | Gor23 | … | … |  | … |  | … |  | …
J17052-050 | 50.20 | DA19 | P | 50.20 | 1.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J17071+215 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J17115+384 | 62.60 | DA19 | P | 62.60 | 2.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J17166+080 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J17198+417 | 71.50 | DA19 | P | 71.50 | 2.60 | DA19 | … |  | … | … |  | … |  | … |  | …
J17303+055 | 34.60 | SWASP | S | … | … |  | … |  | 33.51 | … |  | … |  | 34.60 |  | 34.02
J17338+169 | 0.27 | TESS | S | 0.27 | 0.00 | DA19 | … |  | … | … |  | 0.27 | PDCSAP | … |  | …
J17355+616 | 18.39 | TESS-SAP | S | 19.30 | 0.30 | DA19 | 18.00 | Pin19 | … | … |  | 18.39 | SAP | … |  | …
J17378+185 | 35.02 | Spect | S | … | … |  | 37.79 | Aff19 | 37.99 | … |  | … |  | … |  | 35.02
J17542+073 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J17578+046 | 145.00 | TP19 | S | 145.00 | 15.00 | TP19 | 140.00 | Rib18 | 135.15 | … |  | … |  | … |  | 129.28
J17578+465 | 30.30 | DA19 | S | 30.30 | 0.90 | DA19 | … |  | … | … |  | … |  | … |  | …
J18022+642 | 0.28 | TESS | S | 0.28 | 0.00 | DA19 | … |  | … | … |  | 0.28 | PDCSAP | … |  | …
J18027+375 | 123.80 | New16 | P | 123.80 | … | New16 | … |  | … | … |  | … |  | … |  | …
J18051-030 | 127.80 | SM15 | D | 127.80 | 3.20 | SM15 | … |  | … | … |  | … |  | … |  | …
J18075-159 | 3.87 | DA19 | S | 3.87 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J18131+260 | 2.28 | TESS | S | 2.28 | 0.01 | DA19 | … |  | … | … |  | 2.28 | PDCSAP | … |  | …
J18165+048 | … |  |  | 145.20 | … | New16(U) | … |  | … | … |  | … |  | … |  | …
J18174+483 | 15.83 | SWASP | S | 15.80 | 0.10 | DA19 | … |  | 16.02 | … |  | 15.10 | SAP | 15.83 |  | 15.79
J18180+387E | … |  |  | 41.74 | … | Oel18 | … |  | … | … |  | … |  | … |  | …
J18189+661 | 0.52 | TESS | S | 0.52 | … | Med22 | … |  | … | … |  | 0.52 | PDCSAP | … |  | …
J18198-019 | 31.69 | Spect | S | … | … |  | … |  | 31.61 | … |  | … |  | … |  | 31.69
J18221+063 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J18224+620 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J18319+406 | 50.20 | DA19 | P | 50.20 | 1.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J18346+401 | 40.20 | DA19 | S | 40.20 | 0.80 | DA19 | … |  | … | … |  | … |  | … |  | …
J18353+457 | 34.00 | DA19 | S | 34.00 | 2.90 | DA19 | 40.00 | GA21 | … | … |  | … |  | … |  | …
J18356+329 | 0.12 | TESS | S | 0.12 | 0.00 | DA19 | … |  | … | … |  | 0.12 | PDCSAP | … |  | …
J18363+136 | 50.20 | DA19 | D | 50.20 | 1.60 | DA19 | … |  | … | … |  | … |  | … |  | …
J18409-133 | 28.23 |  OSN-$V$ | P | … | … |  | 57.00 | Gor23 | … | 28.23 |  OSN-$V$ | … |  | … |  | …
J18419+318 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J18427+596N | 103.10 | Don23 | P | 103.10 | 6.10 | Don23 | … |  | … | … |  | … |  | … |  | …
J18427+596S | 135.00 | Don23 | P | 135.00 | 15.00 | Don23 | … |  | … | … |  | … |  | … |  | …
J18480-145 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J18482+076 | 2.76 | DA19 | S | 2.76 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J18498-238 | 2.87 | DA19 | S | 2.87 | 0.01 | DA19 | … |  | 2.86 | … |  | … |  | … |  | …
J18580+059 | 35.20 | DA19 | S | 35.20 | 0.30 | DA19 | 35.56 | TP21 | 36.65 | … |  | … |  | … |  | 36.43
J19070+208 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J19072+208 | 3.80 | DA19 | D | 3.80 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J19084+322 | 74.10 | DA19 | P | 74.10 | 2.80 | DA19 | … |  | … | … |  | … |  | … |  | …
J19098+176 | 80.10 | DA19 | P | 80.10 | 3.20 | DA19 | … |  | … | … |  | … |  | … |  | …
J19169+051N | 46.00 | DA19 | S | 46.00 | 0.20 | DA19 | … |  | … | … |  | … |  | … |  | 49.15
J19169+051S | 23.60 | DA19 | D | 23.60 | 0.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J19216+208 | 133.00 | DA19 | S | 133.00 | 9.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J19251+283 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J19255+096 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J19346+045 | 21.79 | Spect | S | 12.90 | 0.80 | DA19 | … |  | 21.75 | … |  | … |  | … |  | 21.79
J19422-207 | 1.34 | SWASP | S | … | … |  | … |  | … | … |  | … |  | 1.34 |  | …
J19511+464 | 0.59 | TESS | S | 0.59 | 0.00 | DA19 | … |  | … | … |  | 0.59 | PDCSAP | … |  | …
J20093-012 | 1.37 | SWASP | S | 1.37 | … | New18 | … |  | … | … |  | … |  | 1.37 |  | …
J20198+229 | 1.13 | TESS | S | 1.13 | 0.01 | DA19 | … |  | … | … |  | 1.13 | PDCSAP | … |  | …
J20260+585 | 159.88 | Med22 | S | 159.88 | … | Med22 | 169.30 | Kos22 | … | … |  | … |  | … |  | …
J20305+654 | 32.80 | DA19 | S | 32.80 | 0.50 | DA19 | … |  | … | … |  | … |  | … |  | …
J20336+617 | 12.60 | DA19 | P | 12.60 | 0.70 | DA19 | … |  | … | … |  | … |  | … |  | …
J20405+154 | 106.00 | DA19 | S | 106.00 | 6.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J20450+444 | 39.12 | Spect | P | 19.90 | 0.60 | DA19 | … |  | … | … |  | … |  | … |  | 39.12
J20451-313 | 4.89 | TESS | S | 4.84 | 0.04 | Mes11 | … |  | … | … |  | 4.89 | PDCSAP | … |  | …
J20525-169 | 67.60 | DA19 | D | 67.60 | 0.60 | DA19 | … |  | … | … |  | … |  | … |  | 133.50
J20533+621 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J20556-140N | 137.37 | New18 | P | 137.37 | … | New18 | … |  | … | … |  | … |  | … |  | …
J20556-140S | 134.63 | New18 | P | 134.63 | … | New18 | … |  | … | … |  | … |  | … |  | …
J20567-104 | 9.63 | DA19 | D | 9.63 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J21019-063 | 49.29 | SWASP | S | … | … |  | … |  | … | 22.99 |  SNO-$V$ | … |  | 49.29 |  | …
J21152+257 | 34.80 | DA19 | P | 34.80 | 0.20 | DA19 | … |  | … | … |  | … |  | … |  | …
J21164+025 | 42.68 | Spect | S | … | … |  | 42.00 | Lal19 | 41.77 | … |  | … |  | … |  | 42.68
J21221+229 | 38.40 | SWASP | S | 41.00 | 1.70 | DA19 | 40.00 | Qui22 | 39.90 | … |  | … |  | 38.40 |  | 39.79
J21348+515 | 54.30 | DA19 | S | 54.30 | 1.50 | DA19 | … |  | … | … |  | … |  | … |  | …
J21463+382 | 93.90 | Don23 | P | 93.90 | 3.40 | Don23 | … |  | … | … |  | … |  | … |  | …
J21466-001 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J21466+668 | 100.00 | Ama21 | P | … | … |  | 100.00 | Ama21 | … | … |  | … |  | … |  | …
J22012+283 | 0.45 | DA19 | S | 0.45 | 0.00 | DA19 | … |  | … | … |  | 0.45 | PDCSAP | … |  | …
J22020-194 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J22021+014 | 22.06 | Spect | S | 21.84 | 0.14 | Don23 | … |  | … | … |  | … |  | … |  | 22.06
J22057+656 | 120.47 | Laf21 | P | … | … |  | … |  | 120.47 | … |  | … |  | … |  | …
J22096-046 | 39.20 | SM15 | S | 39.20 | 6.30 | SM15 | … |  | … | … |  | … |  | 35.98 | U | …
J22114+409 | 30.00 | DA19 | S | 30.00 | 1.30 | DA19 | … |  | … | … |  | … |  | … |  | …
J22115+184 | 36.30 | DA19 | S | 36.30 | 0.20 | DA19 | … |  | 37.30 | … |  | … |  | … |  | 35.46
J22125+085 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J22137-176 | 116.40 | Ste16 | P | 116.40 | … | Ste16 | … |  | … | … |  | … |  | … |  | …
J22231-176 | 4.57 | TESS | S | 4.59 | … | New18 | … |  | … | … |  | 4.57 | PDCSAP | 4.60 |  | …
J22252+594 | 64.60 | DA19 | S | 64.60 | 2.10 | DA19 | 63.90 | Nag19 | … | … |  | … |  | … |  | …
J22298+414 | 99.80 | DA19 | P | 99.80 | 1.20 | DA19 | … |  | … | … |  | … |  | … |  | …
J22330+093 | 37.80 | SWASP | S | … | … |  | … |  | … | … |  | … |  | 37.80 |  | 37.59
J22468+443 | 4.35 | TESS | S | 4.38 | 0.03 | DA19 | … |  | … | … |  | 4.35 | PDCSAP | … |  | 4.38
J22503-070 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J22518+317 | 1.63 | DA19 | S | 1.63 | 0.01 | DA19 | … |  | … | … |  | … |  | … |  | …
J22532-142 | 81.00 | DA19 | S | 81.00 | 0.80 | DA19 | 96.70 | Riv05 | … | … |  | … |  | … |  | …
J22559+178 | 27.00 | SM18 | P | 27.00 | 2.50 | SM18 | … |  | … | … |  | … |  | … |  | …
J22565+165 | 39.50 | DA19 | S | 39.50 | 0.20 | DA19 | … |  | 38.65 | … |  | … |  | … |  | 37.63
J23064-050 | 3.30 | DA19 | S | 3.30 | 0.01 | DA19 | 1.40 | Gil16 | … | … |  | … |  | … |  | …
J23113+085 | 44.82 |  LCO-$V$ | P | … | … |  | … |  | … | 44.82 |  LCO-$V$ | … |  | … |  | …
J23216+172 | 74.70 | DA19 | S | 74.70 | 0.70 | DA19 | … |  | … | … |  | … |  | … |  | …
J23245+578 | 36.48 | Spect | S | … | … |  | … |  | … | … |  | … |  | 37.42 | U | 36.48
J23340+001 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J23351-023 | 178.00 | Don23 | S | 178.00 | 15.00 | Don23 | … |  | … | … |  | … |  | … |  | …
J23381-162 | 61.66 | Wat06 | D | 61.66 | … | Wat06 | … |  | … | … |  | … |  | 91.43 | U | …
J23419+441 | 106.00 | DA19 | S | 106.00 | 6.00 | DA19 | … |  | … | … |  | … |  | … |  | …
J23431+365 | 73.66 | Don23 | S | 73.66 | 0.92 | Don23 | … |  | … | … |  | … |  | … |  | …
J23492+024 | 49.90 | SM18 | S | 49.90 | 3.50 | SM18 | … |  | 53.82 | … |  | … |  | … |  | 53.77
J23505-095 | … |  |  | … | … |  | … |  | … | … |  | … |  | … |  | …
J23548+385 | 4.80 | TESS | S | 4.70 | 0.04 | DA19 | … |  | … | … |  | 4.80 | PDCSAP | … |  | …
J23556-061 | … |  |  | … | … |  | … |  | … | … |  | … |  | 28.53 | U | …
J23585+076 | 55.40 | SWASP | P | … | … |  | … |  | … | … |  | … |  | 55.40 |  | …

Note: This table is available in its entirety in ASCII format online.
a: Secure flags: ‘S’ = secure; ‘P’ = provisional; ‘D’ = debated.
b: Other literature periods can be found in online version of table.

Table 5: List of reference abbreviations to Table LABEL:t:allprots.  Abbreviation | Reference
---|---
AD17b | Astudillo-Defru et al. 2017b
AD17c | Astudillo-Defru et al. 2017c
Aff19 | Affer et al. 2019
Ama21 | Amado et al. 2021
Bar18 | Baroch et al. 2018
Bla23 | Blanco-Pozo et al. 2023
Blu20 | Bluhm et al. 2020
Bon18 | Bonfils et al. 2018
Bou18 | Bourrier et al. 2018
Cab22 | Caballero et al. 2022
Clo17 | Cloutier et al. 2017
Clo20 | Cloutier et al. 2020
DA19 | Díez Alonso et al. 2019
Don08 | Donati et al. 2008
Dav16 | David et al. 2016
Ded21 | Dedrick et al. 2021
Dia19 | Díaz et al. 2019
Don23 | Donati et al. 2023
Dre20 | Dreizler et al. 2020
Fen20 | Feng et al. 2020
Fek00 | Fekel & Henry 2000
Fou23 | Fouqué et al. 2023
GA20 | González-Álvarez et al. 2020
GA21 | González-Álvarez et al. 2021
GA23 | González-Álvarez et al. 2023
Gil16 | Gillon et al. 2016
Gor23 | Gorrini et al. 2023
GR98 | Greimel & Robb 1998
Hal08 | Hallinan et al. 2008
Hag10 | Haghighipour et al. 2010
Har11 | Hartman et al. 2011
Heb16 | Hébrard et al. 2016
Hob18 | Hobson et al. 2018
Hob19 | Hobson et al. 2019
How14 | Howard et al. 2014
How20 | Howard et al. 2020
Irv23 | Irving et al. 2023
Irw11 | Irwin et al. 2011
Joh07 | Johnson et al. 2007
Joh10 | Johnson et al. 2010
Kir12 | Kiraga 2012
Kos23 | Kossakowski et al. 2023
KS07 | Kiraga & Stepien 2007
KS13 | Kiraga & Stepień 2013
Laf21 | Lafarga et al. 2021
Lal19 | Lalitha et al. 2019
Table 5: Continued. Abbreviation | Reference
---|---
Lot18 | Lothringer et al. 2018
Luq18 | Luque et al. 2018
Luq19 | Luque et al. 2019
Luq22 | Luque et al. 2022
Med20 | Medina et al. 2020
Med22 | Medina et al. 2022
Mes11 | Messina et al. 2011
Mor08 | Morin et al. 2008
Mor10 | Morin et al. 2010
Mor19 | Morales et al. 2019
Mou17 | Moutou et al. 2017
Nag19 | Nagel et al. 2019
New16 | Newton et al. 2016b
New18 | Newton et al. 2018
Nor07 | Norton et al. 2007
Oel18 | Oelkers et al. 2018
Ola16 | Oláh et al. 2016
Pas22 | Pass et al. 2022
Pas23 | Pass et al. 2023
Per19 | Perger et al. 2019
Pin19 | Pinamonti et al. 2019
Poj05 | Pojmanski et al. 2005
Qui22 | Quirrenbach et al. 2022
Rae20 | Raetz et al. 2020
Rei20 | Reinhold & Hekker 2020
Rib18 | Ribas et al. 2018
Riv05 | Rivera et al. 2005
Sar18 | Sarkis et al. 2018
SM15 | Suárez Mascareño et al. 2015
SM16 | Suárez Mascareño et al. 2016
SM17 | Suárez Mascareño et al. 2017b
SM17b | Suárez Mascareño et al. 2017a
SM18 | Suárez Mascareño et al. 2018
SM23 | Suárez Mascareño et al. 2023
Ste16 | Stelzer et al. 2016
Sto20a | Stock et al. 2020a
Sto20b | Stock et al. 2020b
Ter22 | Terrien et al. 2022
Tes04 | Testa et al. 2004
TP19 | Toledo-Padrón et al. 2019
TP21 | Toledo-Padrón et al. 2021
Tri21 | Trifonov et al. 2021
Vid17 | Vida et al. 2017
Wat06 | Watson et al. 2006
Wes15 | West et al. 2015
Table 6: Planets table. Karmn |  Best $P_{\rm rot}$ | Secure | Transit |  $P_{\rm orb}$1 | $m_{p}\sin i1$ | Ref1 |  $P_{\rm orb}$2 | $m_{p}\sin i2$ | Ref2 |  $P_{\rm orb}$3 | $m_{p}\sin i3$ | Ref3 | Add.
---|---|---|---|---|---|---|---|---|---|---|---|---|---
| (d) | flag | flag | (d) |  ($m_{\oplus}$) |  | (d) |  ($m_{\oplus}$) |  | (d) |  ($m_{\oplus}$) |  | planets
J00067-075 | 93.00 | S |  | 10.35 | 1.08 | SM23 | 21.20 | 1.36 | SM23 | … | … |  |
J00183+440 | 45.00 | S |  | 11.44 | 3.98 | Tri22 Rib23 | 6694.00 | 50.40 | Tri22 Rib23 | … | … |  |
J01026+623 | 18.82 | S |  | 13.85 | 5.63 | Per19 | … | … |  | … | … |  |
J01125-169 | 70.10 | S |  | 2.02 | 0.70 | Sto20a | 3.06 | 1.14 | Sto20a | 4.66 | 1.09 | Sto20a |
J02002+130 | 2.00 | S |  | 771.40 | 67.00 | Qui22 | … | … |  | … | … |  |
J02530+168 | 97.56 | S |  | 4.91 | 1.05 | Zec19 | 11.41 | 1.11 | Zec19 | … | … |  |
J03133+047 | 126.20 | S |  | 2.29 | 3.95 | Bau20 | … | … |  | … | … |  |
J04167-120 | 33.00 | P | Y | 4.05 | 30.80 | Dre20 | … | … |  | … | … |  |
J04429+189 | 40.70 | S |  | 8.78 | 9.10 | Tri18 | … | … |  | … | … |  |
J04520+064 | … |  |  | 2288.00 | 260.00 | How10 | … | … |  | … | … |  |
J04538-177 | 53.10 | P |  | 17.13 | 6.49 | Fen20 | 106.30 | 7.56 | Fen20 | … | … |  |
J05019-069 | 93.87 | S |  | 5.36 | 2.02 | AD17c | 40.54 | 2.31 | AD17c | … | … |  |
J06105-218 | 27.30 | S |  | 122.00 | 7.27 | Fen20 | 526.00 | 8.48 | Fen20 | … | … |  |
J06371+175 | 37.50 | S |  | 2.77 | 2.14 | Luq22 | 5.71 | 3.09 | Luq22 | … | … |  |
J06548+332 | 122.00 | S |  | 14.24 | 4.27 | Sto20b Rib23 | … | … |  | … | … |  |
J07274+052 | 93.50 | D |  | 4.72 | 1.18 | AD17c | 18.65 | 2.89 | AD17c | … | … |  |
J08023+033 | … |  | Y | 1.20 | 1.86 | Kem20 | 15.51 | 7.41 | Kem20 | … | … |  |
J08409-234 | 57.50 | D |  | 695.66 | 557.10 | Fen20 | 6739.00 | 522.50 | Fen20 | … | … |  |
J08413+594 | 83.27 | S |  | 203.13 | 146.00 | Mor19 Rib23 | 2350.00 | 143.00 | Mor19 Rib23 | … | … |  |
J09144+526 | 16.88 | S |  | 24.45 | 10.27 | GA20 | … | … |  | … | … |  |
J09360-216 | 74.30 | S | Y | 3.93 | 1.84 | Luq19 | 9.12 | 3.40 | Luq19 | 55.66 | 6.10 | Luq19 |
J10023+480 | … |  |  | 3.82 | 13.02 | Hob19 | … | … |  | … | … |  |
J10088+692 | 41.20 | S | Y | 3.44 | 5.90 | Blu20 | … | … |  | … | … |  |