redshifts ($z_{photo}$) within $1.90<z_{\mathrm{photo}}<2.66$. 160 of these galaxies with $1.90<z_{\mathrm{photo}}<2.66$ were targeted in K band out of which 128[^3] were detected with at least one emission line with SNR $>5$. None of the [H$\alpha$]{} detected galaxies had spectroscopic redshifts outside the considered redshift interval. However, 3 additional galaxies (1 object with Q$_z=2$, 2 objects with Q$_z=3$) fell within $1.90<z<2.66$ due to inaccurate photometric redshifts. There were 8 galaxies targeted in K band that did not have [H$\alpha$]{} detections but do have other emission line detections (i.e. No [H$\alpha$]{} but have [\[\]]{}, [\[\]]{}, [H$\beta$]{} etc). Furthermore, there were no galaxies that were targeted in K band expecting [H$\alpha$]{} but resulted in other emission line detections.

There were 151 objects within $1.90<z<2.66$ with [H$\alpha$]{} detections (Q$_z>1$) and 26 of them were flagged as AGN following selection criteria from @Coil2015 and @Cowley2016. In the remaining 125 galaxies, 8 galaxies did not have matching ZFOURGE counterparts and 8 galaxies had low confidence for redshift detection (Q$_z=2$) from @Nanayakkara2016. We removed those 16 galaxies from the sample. Out of the 109 remaining galaxies, seven are removed due to the following reasons: four galaxies due to negative spectroscopic flux, one galaxy due to multiple objects overlapping 