NICER observation list: Target ID 564103

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
5641030101 230.564 -37.380 333.373 16.421 59966.4905 59966.9104 3895.0 52 2 VALIDATED 59975.6 60160
5641030201 230.564 -37.379 333.373 16.422 59993.4657 59993.9880 8873.0 51 4 VALIDATED 60002.9 60187
5641030202 230.560 -37.377 333.372 16.425 59994.0399 59994.0505 15.0 51 4 VALIDATED 60006.7 60188
5641030203 230.567 -37.380 333.375 16.421 60022.0678 60022.9840 7368.0 51 6 VALIDATED 60036.2 60216
5641030204 230.566 -37.379 333.375 16.421 60023.1012 60023.1134 913.0 51 7 VALIDATED 60036.3 60217
5641030301 230.565 -37.380 333.374 16.421 60049.5625 60049.9563 1946.0 51 7 VALIDATED 60069.8 60243
5641030302 230.565 -37.380 333.374 16.421 60050.0139 60050.9907 5983.5 51 4 VALIDATED 60062.1 60244
5641030501 230.564 -37.380 333.373 16.421 60107.1872 60107.6650 8646.0 51 5 VALIDATED 60118.7 60301
5641030601 230.564 -37.380 333.373 16.422 60134.3478 60134.9426 9639.0 51 4 VALIDATED 60145.1 60328