NICER observation list: Target ID 564101

Abstract

eROSITA is performing multiple all-sky X-ray surveys and monitoring almost half a million AGN every six months. It has the capability to identify exceptional AGN with periodic X-ray flux signals. These objects are potential supermassive black hole binaries (SMBHB). We request ToO monitoring campaigns for up to three eROSITA-selected candidate periodic AGN. Each ToO consists of six individual pointings, 10 ks each, spaced roughly four weeks apart. The campaigns are needed to track the flux modulation waveform on a monthly time-scale, accurately determine the period, and to determine the details of follow-up observations to confirm the binary nature. The most convincing case will be the target of a pre-approved 100 ks XMM-Newton observation.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
5641010101 23.395 -21.166 183.372 -78.695 59963.6167 59963.9516 1099.0 52 1 VALIDATED 59971.3 60157
5641010102 23.395 -21.166 183.371 -78.695 59964.0715 59964.9838 1155.5 52 1 VALIDATED 59971.4 60158
5641010103 23.396 -21.166 183.373 -78.695 59965.0964 59965.2345 1401.0 52 3 VALIDATED 59981.9 60159
5641010201 23.397 -21.166 183.375 -78.694 59992.0134 59992.6708 20.0 45 12 VALIDATED 60082.7 60186
5641010301 23.396 -21.166 183.375 -78.695 60076.0483 60076.3986 17.8 42 4 VALIDATED 60088.2 60270
5641010401 23.395 -21.162 183.356 -78.693 60110.4264 60110.8282 7053.0 51 3 VALIDATED 60121.8 60304
5641010501 23.396 -21.166 183.375 -78.694 60132.0558 60132.4025 7530.5 42 4 VALIDATED 60143.2 60326
5641010601 23.397 -21.167 183.381 -78.695 60160.8935 60160.9000 94.0 51 3 VALIDATED 60172.6 60354
5641010602 23.396 -21.166 183.377 -78.695 60161.0243 60161.4855 6311.2 51 3 VALIDATED 60172.7 60355