NICER observation list: Target ID 366701

Abstract

The puzzling variety of super-orbital modulations seen in the long term light-curves of Supergiant High Mass X-ray binaries (sgHMXBs), opens up new questions on the stellar wind interaction with a highly magnetised neutron star. We propose a joint 40 ks NuSTAR + 10 ks NICER observation of the persistent sgHMXB 4U 1538-52 at its super-orbital maximum and minimum to conclusively understand the mechanisms driving these flux modulations. The results of energy resolved pulsation studies, pulse phase resolved spectroscopic study of photon indices, absorption column density and cyclotron lines will be used to differentiate or constrain the various models explaining these super-orbital modulations.
Obsid RA DEC l b Start End Exposure Number of
Modules
Number of
Processing
Status of
Processing
Date of
Processing
Public
date
3667010101 235.603 -52.388 327.421 2.160 59216.0467 59216.2044 0.0 47 3 VALIDATED 59220.7 59590
3667010201 235.602 -52.386 327.422 2.162 59221.9155 59221.9470 0.0 47 4 VALIDATED 59244.0 59595
3667010202 235.601 -52.386 327.421 2.162 59221.9813 59222.0759 0.0 47 6 VALIDATED 59244.0 59596
3667010301 235.597 -52.386 327.419 2.164 59261.3666 59261.8324 7272.0 52 2 VALIDATED 59270.9 59635
3667010302 235.594 -52.384 327.419 2.167 59267.0324 59267.1123 41.0 52 1 VALIDATED 59271.1 59641
3667010401 235.595 -52.385 327.419 2.165 59267.1630 59267.5641 1625.0 52 1 VALIDATED 59271.1 59641