There are two substantial X-ray dips (very strong in the 15 - 50
keV band, weaker at lower energies) that are separated by an interval equal to the X-ray period.
The same periodicity is present in both the 2 - 20 keV and 15 - 50
keV bands, but with a 0.1 phase offset 40d).
Not exact matches
We characterized the evolution in the hard X-ray
band and showed that for the joint ISGRI - XRT fits, the e-folding energy decreased from 350
keV to 130
keV, while the energy where the exponential cut - off starts increased from 75
keV to 112
keV as the decay progressed.We investigated the claim that high energy cut - offs disappear with the compact jet turning on during outburst decays, and showed that spectra taken with HEXTE on RXTE provide insufficient quality to characterize cut - offs during the decay for typical hard X-ray fluxes.
HEFT will be the world's largest hard X-ray telescope, operating in the 20 - 120
keV energy
band and flown from a balloon.
The longitudinal variation of the GRXE in the energy
band above 4
keV shows a large enhancement within l < 30 deg.
Also, we derived the LogN - LogS relations of the resolved sources in the energy
bands below and above 2
keV.
Abstract: The X-ray emission from the central region of the Galactic plane, l < 45 deg and b < 0.4 deg, was studied in the 0.7 - 10
keV energy
band with a spatial resolution of ~ 3» with the ASCA observatory.
Many point sources are detected either in the soft X-ray
band (below 2
keV) or in the hard
band (above 2
keV), and only a small number of sources are detected in both energy
bands.
(
Kev's in a
band ya know!)