activity
20112026
most citedDiscovery of pulsations from NGC 300 ULX1 and its fast period evolution

292 citations · 1.6k across the 78 of their papers we have counts for

collaborators
Showing 2020Show all

7 papers · 1 filter

astro-ph.GA2020★ 231 cited

Detection of large-scale X-ray bubbles in the Milky Way halo

P. Predehl, R. A. Sunyaev, W. Becker +25

The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is observational evidence of e…

astro-ph.HE2020★ 29 cited

New Optically Identified Supernova Remnants in the Large Magellanic Cloud

Miranda Yew, Miroslav D. Filipović, Milorad Stupar +20

We present a new optical sample of three Supernova Remnants and 16 Supernova Remnant (SNR) candidates in the Large Magellanic Cloud(LMC). These objects were originally selected usi…

astro-ph.HE2020★ 13 cited

Evolution of timing and spectral characteristics of 4U 1901+03 during its 2019 outburst using the Swift and NuSTAR observatories

Aru Beri, Tinku, Nirmal K. Iyer +1

We report the results from a detailed timing and spectral study of transient X-ray pulsars, 4U 1901+03 during its 2019 outburst. We performed broadband spectroscopy in the 1-70 keV…

astro-ph.HE2020★ 26 cited

AstroSat Observations of the first Galactic ULX Pulsar Swift J0243.6+6124

Aru Beri, Sachindra Naik, K. P Singh +11

SwiftJ0243.6+6124, the first Galactic ultra-luminous X-ray pulsar, was observed during its 2017-2018 outburst with \emph{AstroSat} at both sub- and super-Eddington levels of accret…

astro-ph.HE2020★ 16 cited

Time Evolution Of Cyclotron Line of Her X-1; A Detailed StatisticalAnalysis Including New ASTROSAT Data

S. Bala, D. Bhattacharya, R. Staubert +1

The cyclotron line feature in the X-ray spectrum of the accretion powered pulsar Her X-1 has been observed and monitored for over three decades. The line energy exhibited a slow se…

astro-ph.HE2020★ 18 cited

Is superorbital modulation in SMC X-1 caused by absorption in warped precessing accretion disc?

Pragati Pradhan, Chandreyee Maitra, Biswajit Paul

We present a broadband spectral-timing analysis of SMC X-1 at different intensity states of its super-orbital variation using 10 Suzaku and 6 NuSTAR observations. The spectrum in a…