NICER observation list: Target ID 463401

Abstract

The puzzling variety of orbital phase locked X-ray flares and super-orbital modulations in the Supergiant Fast X-ray Transient (SFXT) IGR J16479-4514 indicates the presence of stable large scale structures in the stellar wind of the supergiant star. To investigate these structures in the stellar wind, we propose 25 kilosec observations of IGR J16479-4514 each at two orbital phase 0.3 and 0.7 (50 kilosec total), where these X-ray flares occur. The time of observations will be matched to the super-orbital maximum phase, where many of these X-ray bright flares are coincident. The results from hardness ratio and spectral analysis during the rise and decay of these flares will be used to constrain stellar wind models predicting the existence of these large scale structures in the wind.
Obsid RA DEC l b Start End Exposure Number of modules Status of Processing Date of Processing Public date
4634010101 252.026 -45.202 340.16259 -0.12325 59403.8854 59403.9609 768.00000 52 VALIDATED 59413.8 59597
4634010102 252.026 -45.202 340.16260 -0.12297 59404.0110 59404.9912 12840.00000 52 VALIDATED 59415.7 59598
4634010103 252.026 -45.202 340.16244 -0.12338 59405.0440 59405.6368 8319.00000 52 VALIDATED 59415.8 59599