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- Inter-University Centre for Astronomy and AstrophysicsIN16 papers
- National Centre for Radio AstrophysicsIN7 papers
- Physical Research LaboratoryIN6 papers
- Tata Institute of Fundamental ResearchIN6 papers
- North-West UniversityZA5 papers
- Raman Research InstituteIN4 papers
- Aryabhatta Research Institute of Observational SciencesIN3 papers
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- Manipal Academy of Higher EducationIN3 papers
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11 papers · 1 filter
Sloshing Cold Fronts in Galaxy Cluster Abell 2566
S. K. Kadam, Satish S. Sonkamble, N. D. Vagshette +1
This paper presents properties of the intracluster medium (ICM) in the environment of a cool core cluster Abell 2566 (redshift = 0.08247) based on the analysis of 20 ks Chandra…
Cool-core, X-ray cavities and cold front revealed in RXCJ0352.9+1941 cluster by Chandra and GMRT observations
Satish S. Sonkamble, S. K. Kadam, Surajit Paul +3
This paper presents a comprehensive analysis of 30 ks Chandra and 46.8 ks (13 Hr) 1.4 GHz GMRT radio data on the cool-core cluster RXCJ0352.9+1941 with an objective to investigate…
X-ray Studies of Blazar 1ES 1959+650 Using SWIFT & XMM-NEWTON Satellite
Kiran A Wani, Haritma Gaur, M K Patil
High synchrotron energy peaked blazar 1ES 1959+650 is studied with Swift and XMM-Newton satellite in total 127 observations during the period June 2018-December 2020. We extensivel…
Study of Intra-Day Flux Distributions of Blazars Using XMM-Newton Satellite
Kiran Wani, Haritma Gaur
We present a study of the flux distribution of a sample of 15 Intermediate and Low-energy peaked blazars using XMM-Newton observations in a total of 57 epochs on short-term timesca…
A stochastic propagation model to the energy dependent rapid temporal behaviour of Cygnus X-1 as observed by AstroSat in the hard state
Bari Maqbool, M. Sneha Prakash, R. Misra +8
We report the results from analysis of six observations of Cygnus X-1 by Large Area X-ray Proportional Counters (LAXPC) and Soft X-ray Telescope (SXT) on-board AstroSat, when the s…
UV to X-ray Comptonization delay in Mrk 493
Oluwashina Adegoke, Gulab C. Dewangan, Pramod Pawar +1
The broadband X-ray emission from type 1 active galactic nuclei, dominated by a powerlaw continuum, is thought to arise from repeated inverse Compton scattering of seed optical/UV…