output
20052026
most citedThe Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

5k citations

Showing 2022Show all

28 papers · 1 filter

astro-ph.HE2022★ 15 cited

Broadband mHz QPOs and spectral study of LMC X4 with AstroSat

Rahul Sharma, Chetana Jain, Ketan Rikame +1

We report the results of broadband timing and spectral analysis of data from an AstroSat observation of the High Mass X-ray binary LMC X4. The Large Area X-ray Proportional Coun…

astro-ph.HE2022★ 7 cited

Broadband Spectral properties of MAXI J1348--630 using AstroSat Observations

Gitika Mall, Jithesh Vadakkumthani, Ranjeev Misra

We present broadband X-ray spectral analysis of the black hole X-ray binary MAXI J1348--630, performed using five AstroSat observations. The source was in the soft spectral state f…

astro-ph.GA2022★ 13 cited

Barbell-shaped giant radio galaxy with ~100 kpc kink in the jet

Pratik Dabhade, Timothy W. Shimwell, Joydeep Bagchi +8

We present for the first time a study of peculiar giant radio galaxy (GRG) J223301+131502 using deep multi-frequency radio observations from GMRT (323, 612, and 1300 MHz) and LOFAR…

astro-ph.HE2022★ 2 cited

Spectral characteristics of the black hole binary 4U 1957+115: A multi-mission perspective

Sneha Prakash Mudambi, S. B. Gudennavar, R. Misra +1

We report spectral analysis of the persistent black hole X-ray binary, 4U 1957+115, using AstroSat, Swift and NuSTAR observations carried out between 2016-2019. Modelling with a di…

astro-ph.HE2022★ 5 cited

Long-term optical and ray variability of the blazar PKS~1222+216

Savithri H. Ezhikode, Amit Shukla, Gulab C. Dewangan +4

The ray emission from flat-spectrum radio quasars (FSRQs) is thought to be dominated by the inverse Compton scattering of the external sources of photon fields, e.g., accretion…

astro-ph.SR2022★ 2 cited

Study of the transient nature of classical Be stars using multi-epoch optical spectroscopy

Gourav Banerjee, Blesson Mathew, K. T. Paul +8

Variability is a commonly observed property of classical Be stars (CBe) stars. In extreme cases, complete disappearance of the Hα emission line occurs, indicating a disc-less state…