activity
20102024
most cited4U 1626-67 Returns to Spin-Down: Timing features toe the line

13 citations · 30 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2024

The 2021 outburst of 2S 1417-624 revisited with AstroSat

Chetana Jain

This work presents the first ever broadband (0.7-25.0 keV) timing and spectral analysis of Be-HMXB 2S 1417-624 during its 2021 outburst. Using AstroSat observations, coherent pulsa…

astro-ph.HE2024

A comprehensive study of orbital evolution of LMC X-4: Existence of a second derivative of the orbital period

Chetana Jain, Rahul Sharma, Biswajit Paul

We report here results from pulse arrival time delay analysis of the eclipsing high mass X-ray binary pulsar LMC X-4 using observations made with the Rossi X-ray Timing Explorer, X…

astro-ph.HE20231 cited

AstroSat observation of the magnetar SGR J18300645 during its first detected X-ray outburst

Rahul Sharma, Chetana Jain, Biswajit Paul +1

We present here timing and spectral analyses of SGR J18300645 based on an AstroSat observation carried out on 2020 October 16, about a week after the onset of its first detected…

astro-ph.HE202313 cited

4U 1626-67 Returns to Spin-Down: Timing features toe the line

Rahul Sharma, Chetana Jain, Biswajit Paul

We present a comprehensive analysis of X-ray pulsar 4U 1626-67 during its current spin-down (2SD) state, following a recent torque reversal. Since its discovery, this ultra-compact…

astro-ph.HE20239 cited

Torque reversal and cyclotron absorption feature in HMXB 4U 1538-522

Prince Sharma, Chetana Jain, Anjan Dutta

We present a comprehensive timing and spectral analysis of the HMXB 4U 1538-522 by using the Nuclear Spectroscopic Telescope Array (NuSTAR) observatory data. Using three archived o…

astro-ph.HE2010

New measurement of orbital and spin period evolution of the Accretion Disk Corona source 4U 1822-37

Chetana Jain, Biswajit Paul, Anjan Dutta

4U 1822-37 is a Low Mass X-ray Binary (LMXB) system with an Accretion Disk Corona. We have obtained 16 new mid-eclipse time measurements of this source during the last 13 years usi…