Deepto Chakrabarty

TL;DR: The BATSE experiment on the Compton Gamma Ray Observatory provides data with suitable time and energy resulution to monitor numerous pulsed systems as mentioned in this paper, including radio pulsars, disk-fed and wind-fed X-ray binary systems, and Be/transient systems.

TL;DR: The Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) as discussed by the authors is a probe-class mission concept that will provide an unprecedented view of the X-ray sky, performing timing and spectroscopy over both a broad energy band and a wide range of timescales from microseconds to years.

TL;DR: STROBE-X is a probe-class mission concept, selected for study by NASA, for X-ray spectral timing of compact objects across the mass scale as mentioned in this paper, which combines huge collecting area, high throughput, broad energy coverage, and excellent spectral and temporal resolution in a single facility, enabling a broad portfolio of high priority astrophysics.

TL;DR: In this paper, a detailed spectral and timing analysis of the coherent pulsations of a millisecond X-ray pulsar IGR 17379-3747 was performed and it was shown that they show a strong energy dependence, with soft thermal emission lagging about 640 μs behind the hard Comptonized emission.

TL;DR: In this paper, a 7-year timing study of the 2.5 ms X-ray pulsar SAX J1808.4-3658 was presented, where the authors verified that the 401 Hz pulsation traces the spin frequency fundamental and not a harmonic, and showed that the pulsar is undergoing long-term spin down at a rate nudot = (-5.6+/-2.0)x10^{-16} Hz/s.