NICER observation list: Target ID 866602

Abstract

Supermassive black hole binaries (SMBHB) are rare and elusive objects that are expected to produce periodically variable X-ray emission. eROSITA opened a window to search and discover peculiar AGNs and provide an unprecedented opportunity to discover SMBHBs. We request five monitoring campaigns for eROSITA-selected candidates that have not been observed previously. Each campaign consists of 6 individual pointings of 10 ks each, spaced roughly 4 weeks apart. The campaigns are needed to track the flux modulation of the source on a monthly time scale, discriminate red-noise-induced variability, and determine the details of follow-up observations to confirm the binary nature. The most convincing cases will be the target of higher and longer cadence NICER follow-up.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
8666020101 336.983 -43.560 353.796 -56.803 60831.1866 60831.9692 9077.0 50 5 VALIDATED 60842.9 61025