NICER observation list: Target ID 555702

Abstract

The ultracompact white dwarf systems HM Cnc and V407 Vul represent unique opportunities to probe binary evolution driven by gravitational radiation and mass transfer. NICER observations to date have provided new, precise frequency measurements in both systems, and the first measurement of an orbital frequency second derivative in an ultracompact binary. We propose observations of both sources to continue to extend their temporal baselines, enabling new, unique probes of their orbital evolution.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
5557020101 288.608 24.946 57.728 6.401 59647.4435 59647.8590 3858.0 52 5 VALIDATED 59662.2 59661
5557020201 288.609 24.946 57.728 6.400 59831.5024 59831.9831 14494.0 52 8 VALIDATED 59846.0 59845
5557020202 288.609 24.946 57.728 6.400 59832.0206 59832.0472 1848.0 52 5 VALIDATED 59844.1 59846