NICER observation list: Target ID 570301

Abstract

Active galactic nuclei (AGN) are powered by accreting supermassive black holes, surrounded by a torus of obscuring material. Recent observations have detected variability in the line of sight column density, giving rise to the 'patchy torus' hypothesis. Other observations, however, fail to find the variability expected from a patchy torus in Sy2 galaxies. Here, we propose to monitor a Sy2 galaxy, with confirmed yearly column density variability, but that shows no variability in timescales of days. We need additional observations on timescales of months to properly constrain the obscurer properties. The number of sources for which a monitoring campaign (i.e. > two observations) has shown variability is only a handful, making the addition of every possible source vital.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
5703010101 220.159 53.504 93.036 56.818 59927.0003 59927.9808 12263.0 52 1 VALIDATED 59936.6 60121
5703010201 220.159 53.504 93.036 56.819 59944.7382 59944.9639 6720.0 52 6 VALIDATED 59956.0 60138
5703010202 220.159 53.504 93.036 56.819 59944.9963 59945.1998 3913.0 52 6 VALIDATED 59956.0 60139
5703010301 220.159 53.505 93.037 56.818 59976.7076 59976.9831 4249.8 51 4 VALIDATED 59988.3 60170
5703010302 220.160 53.505 93.037 56.817 59977.0305 59977.2331 2880.5 51 5 VALIDATED 59990.7 60171
5703010401 220.155 53.503 93.038 56.821 60029.0993 60029.6222 10762.0 51 7 VALIDATED 60042.2 60223
5703010501 220.160 53.505 93.036 56.818 60123.0032 60123.5984 7330.0 51 3 VALIDATED 60133.8 60317