… Te /5 keV and ν1 ν/1 kHz, with Te and ν1 the electron temperature and oscillation frequency
respectively, which is reasonably consistent with hydrodynamical calculations of the shock …

… A very brief summary of the analysis in this paper was previously presented by Strohmayer
(… [53 in support of RXT E proposal 50030 (PI : TE Strohmayer). An analysis of this burst will be …

We report the discovery with the Proportional Counter Array on board the Rossi X-Ray
Timing Explorer of a 450 Hz quasi-periodic oscillation (QPO) in the hard X-ray flux from the …

We report on Bayesian parameter estimation of the mass and equatorial radius of the
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …

We report the discovery with the European Photon Imaging Camera CCDs on board XMM-Newton
of a 54 mHz quasi-periodic oscillation (QPO) in the greater than 2 keV X-ray flux from …

We report the discovery of complex high-frequency variability during the 1998 August 27
giant flare from SGR 1900+ 14 using the Rossi X-Ray Timing Explorer (RXTE). We detect an≈ …

Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear
physicists because their attributes can be used to determine the properties of the dense matter …

… (2005) and Watts & Strohmayer (2006), we began our study by computing average power
spectra around this phase range, but for a sequence of different time intervals during the flare. …

We report a study of the temporal and spectral characteristics of the rising portions of X-ray
bursts from 4U 1728-34 observed with the Rossi X-Ray Timing Explorer (RXTE). We find that …

We present the calibration and background model for the Proportional Counter Array on board
the Rossi X-Ray Timing Explorer. The energy calibration is systematics-limited below 10 …