EIS had good signal strength only for spectral lines  186 and 195 [Å]{}, and 284 [Å]{} among the observed lines. The exposure time for IRIS in spectroscopic mode was 4 s that resulted into an effective cadence of 5 s in sit-and-stare mode. The IRIS-SJI were obtained with an exposure time of 4 s and effective cadence of 18 s, 15 s, and 15 s for SJI 1330 [Å]{}, 1400 [Å]{}, and 2796 [Å]{}, respectively. EIS spectra were obtained with an exposure time of 20 s. XRT images were obtained in several filters such as Al\_poly, C\_poly, Be\_thin, Be\_med, Al\_med, Ti\_poly, and Al\_thick with varying exposure time and hence the cadence. IRIS and AIA observations were co-aligned using IRIS-SJI 1400 [Å]{}, and AIA 1600 [Å]{} images. All the HMI and AIA images obtained in different passbands were co-aligned and de-rotated to AIA 1600 [Å]{} image obtained at 12:53:28 UT using the standard procedures provided in the Solar Software package [SSW; @1998SoPh..182..497F]. We have used IRIS level-2 data where slit-jaw images from different filters and detectors are already co-aligned. We used IRIS cool neutral line 1401.514 [Å]{} to perform the absolute wavelength calibration of IRIS spectral lines. We followed standard procedures 