NICER observation list: Target ID 252001

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. Initial {\it NICER} observations have provided new, precise frequency measurements in both systems, and a first indication for a slowing of the spin-up in HM Cnc. We propose additional observations to extend the timing baselines for each source, enabling new, unique probes of their orbital evolution.
Obsid RA DEC l b Start End Exposure Number of modules Status of Processing Date of Processing Public date
2520010101 121.597 15.458 206.92553 23.39645 58617.2073 58617.8157 18528.00000 52 VALIDATED 58624.1 58811
2520010201 121.597 15.458 206.92545 23.39586 58813.9908 58814.7292 16153.00000 52 VALIDATED 58818.6 59008