Abstract:
In the present work, recent characterization results of the 4K 4K CCD imager (a first light
instrument of the 3.6m devasthal optical telescope; DOT) and photometric calibrations are discussed along with
measurements of the extinction coefficients and sky brightness values at the location of the 3.6m DOT site based
on the imaging data taken between 2016 and 2021. For the 4K 4K CCD imager, all given combinations of
gains (1, 2, 3, 5 and 10 e /ADU) and readout noise values for the three readout speeds (100 kHz, 500 kHz and 1
MHz) are verified using the sky flats and bias frames taken during early 2021; measured values resemble well
with the theoretical ones. Using color–color and color–magnitude transformation equations, color coefficients
(a) and zero-points (b) are determined to constrain and examine their long-term consistencies and any possible
evolution based on UBVRI observations of several Landolt standard fields observed during 2016–2021. Our
present analysis exhibits consistency among estimated a values within the 1r and does not show any noticeable
trend with time. We also found that the photometric errors and limiting magnitudes computed using the data
taken using the CCD imager follow the simulated ones published earlier. The average extinction coefficients,
their seasonal variations and zenith night-sky brightness values for the moon-less nights for all ten Bessell and
SDSS filters are also estimated and found comparable to those reported for other good astronomical sites.
