VizieR Online Data Catalog: FUV imaging of Dorado galaxies (Rampazzo+, 2022)

Astrosat is an X-ray-UV observatory launched by the Indian Space Research Organization on September 28, 2015. The Ultra-Violet Imaging Telescope facility UVIT is composed of two Ritchey-Chretien telescopes, each with a 37.5 cm aperture and a circular field of view with a diameter of 28'. Originally, one telescope observed FUV wavelengths (1300-1800Å) and the other both NUV (2000-3000Å) and optical band (VIS) wavelengths (3200-5500Å), by means of a beam-splitter directing NUV and VIS to individual cameras.

Images reconstructed from the photon-counting data with 0416 sub-sampling were rebinned for our analysis, to enhance the signal-to-noise ratio (S/N) to 1664px^-1. The nominal zero point magnitude of the FUV.CaF2 filter is 18.08mag (Tandon et al., 2017AJ....154..128T).

(2 data files).