output
20192026
most citedAstroSat view of MAXI J1535-571: broadband spectro-temporal features

78 citations

Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2026

Tracing the outburst decay of soft X-ray transients Aql X-1 and 4U 1608-52 with XSPECT

Rwitika Chatterjee, Vivek Kumar Agrawal, V. P. Shyam Prakash +2

XSPECT instrument on-board XPoSat mission is a soft X-ray spectrometer sensitive in the energy band 0.815 keV. XSPECT has observed several bright neutron star low mass X-ray bin…

astro-ph.HE2023★ 4 cited

Multiwavelength study of radio galaxy Pictor A: detection of western hotspot in far-UV and possible origin of high energy emissions

Sanna Gulati, Debbijoy Bhattacharya, M. C. Ramadevi +2

A comprehensive study of the nucleus and western hotspot of Pictor A is carried out using AstroSat observations, 13 years of Fermi, and archival Swift observations, along with othe…

astro-ph.HE2023★ 29 cited

IXPE and NICER view of Black hole X-ray binary 4U 1630-47: First significant detection of polarized emission in thermal state

Ankur Kushwaha, Kiran M. Jayasurya, Vivek K. Agrawal +1

We present a detailed spectro-polarimetric study of Black hole X-ray binary 4U during its outburst with IXPE and NICER observations. The source is observed in disk…

astro-ph.HE2023★ 16 cited

Detection of significant X-ray polarization from transient NS-LMXB XTE J1701-462 with IXPE and its implication on the coronal geometry

Kiran M. Jayasurya, Vivek K. Agrawal, Rwitika Chatterjee

In this paper, we performed a spectro-polarimetric analysis of the transient NS-LMXB XTE J1701-462 using IXPE, NICER, and NuSTAR data during its 2022 outburst. We report the signif…

astro-ph.HE2021★ 2 cited

Swift J1753.5-0127 : Understanding the accretion geometry through frequency resolved spectroscopy

Blessy E. Baby, Ramadevi M. C

The Black Hole Binary source Swift J175.5-0127 remained in outburst for 12 years from May 2005 to April 2017. For most part of the outburst, the source remained in the Low H…

astro-ph.HE2021★ 17 cited

Revealing the nature of the transient source MAXI J0637-430 through spectro-temporal analysis

Blessy E. Baby, Bhuvana G. R., Radhika D. +3

We study the spectral and temporal properties of MAXI J0637-430 during its 2019-2020 outburst using \textit{NICER}, \textit{AstroSat} and \textit{Swift-XRT} data. The source was in…