NICER observation list: Target ID 363101

Abstract

Quasi-periodic oscillations (QPOs) are potentially valuable tools for studying accretion disks, general relativity, and the environments around black holes. Despite proliferating theories, however, their physical origin is still unknown. Although common in the X-ray light curves of stellar mass black holes, only a handful have been observed in AGN. Bolstered by the discovery of an optical QPO in a Kepler AGN light curve, we have obtained TESS short-cadence monitoring for two AGN with known powerful X-ray QPOs. In this proposal, we request NICER monitoring of one of these AGN to occur simultaneously with TESS, to provide vital complementary insights into the nature of the quasiperiodic phenomenon and causality in the AGN central engine.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
3631010101 184.614 29.812 190.678 82.273 58897.9903 58898.0169 2198.0 52 3 VALIDATED 58904.0 58912
3631010201 184.611 29.813 190.680 82.271 58899.9887 58900.0132 1581.0 52 2 VALIDATED 58904.7 58914
3631010301 184.612 29.813 190.681 82.271 58903.9241 58903.9569 1261.0 52 4 VALIDATED 58907.8 58917
3631010401 184.611 29.813 190.680 82.270 58905.7968 58905.8228 2052.0 52 3 VALIDATED 58912.0 58919
3631010501 184.611 29.813 190.682 82.270 58907.2811 58907.3113 2470.0 52 1 VALIDATED 58912.2 58921
3631010601 184.610 29.813 190.680 82.269 58918.0676 58918.1403 2059.0 52 5 VALIDATED 58981.9 58932
3631010701 184.613 29.815 190.658 82.271 58919.8109 58919.8928 2579.3 52 3 VALIDATED 58924.1 58933
3631010801 184.614 29.816 190.653 82.272 58920.9103 58920.9842 1324.0 52 3 VALIDATED 58924.8 58934
3631010802 184.615 29.816 190.651 82.273 58921.0395 58921.1134 1259.0 52 3 VALIDATED 58925.6 58935
3631010901 184.613 29.814 190.666 82.272 58923.2363 58923.4412 2717.0 52 3 VALIDATED 58927.6 58937
3631011001 184.610 29.813 190.680 82.270 58925.3706 58925.4516 2329.0 52 3 VALIDATED 58930.7 58939