NICER observation list: Target ID 767601

Abstract

LMC X-3 is a persistently active black-hole X-ray binary whose behavior more resembles transient BHs than the other persistent black holes. LMC X-3 is nearly always in a disk-dominated soft state, but infrequently will enter a hard state. Crucially, the line-of-sight absorption to LMC X-3, 4e20/cm^2, is an order of magnitude (or more) lower than other Galactic black-hole X-ray binaries. This uniquely low-absorption column allows for an unobscured view of the hard-state's thermal disk, which is key to determining whether the accretion disk extends to the ISCO or is truncated at larger radii in hard states. We propose a 30ks observation of LMC X-3 to be triggered upon the detection of a hard state in LMC X-3.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
7676010101 84.734 -64.087 273.579 -32.082 60619.1314 60619.9782 0.0 41 4 VALIDATED 60629.9 60813
7676010102 84.737 -64.084 273.577 -32.081 60620.0317 60620.9449 0.0 41 4 VALIDATED 60632.0 60814
7676010103 84.737 -64.084 273.577 -32.081 60620.9948 60621.9757 0.0 41 4 VALIDATED 60632.1 60815