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Ritesh Ghosh
Ritesh Ghosh
AT, MKHS
Verified email at umbc.edu
Title
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Cited by
Year
A study of X-ray emission of galaxies hosting molecular outflows (MOX sample)
S Laha, M Guainazzi, E Piconcelli, P Gandhi, C Ricci, R Ghosh, ...
The Astrophysical Journal 868 (1), 10, 2018
272018
A radio, optical, UV, and X-ray view of the enigmatic changing-look active galactic nucleus 1ES 1927+ 654 from its pre-to postflare states
S Laha, E Meyer, A Roychowdhury, JB Gonzalez, JA Acosta–Pulido, ...
The Astrophysical Journal 931 (1), 5, 2022
252022
An X-ray view of central engines of low-luminosity quasars (LLQSO) in the local Universe
S Laha, R Ghosh, M Guainazzi, AG Markowitz
Monthly Notices of the Royal Astronomical Society 480 (2), 1522-1546, 2018
252018
Broad-band spectral study of the jet-disc emission in the radio-loud narrow-line Seyfert 1 galaxy 1H 0323+ 342
R Ghosh, GC Dewangan, L Mallick, B Raychaudhuri
Monthly Notices of the Royal Astronomical Society 479 (2), 2464-2475, 2018
252018
Accretion disc/corona emission from a radio-loud narrow-line Seyfert 1 galaxy PKS 0558–504
R Ghosh, GC Dewangan, B Raychaudhuri
Monthly Notices of the Royal Astronomical Society 456 (1), 554-564, 2016
222016
Blazar Variability: A Study of Nonstationarity and the Flux–Rms Relation
J Bhattacharyya, R Ghosh, R Chatterjee, N Das
The Astrophysical Journal 897 (1), 25, 2020
212020
Investigating the origin of the Fe emission lines of the Seyfert 1 galaxy Mrk 205
S Laha, R Ghosh, S Tripathi, M Guainazzi
Monthly Notices of the Royal Astronomical Society 486 (3), 3124-3133, 2019
152019
An X-ray spectral study of the origin of reflection features in bare Seyfert 1 galaxy ESO 511–G030
R Ghosh, S Laha
The Astrophysical Journal 908 (2), 198, 2021
132021
A Weakening Compton Hump and Soft X-Ray Excess Detected in the Seyfert 1 Galaxy MCG–02–58–22
S Laha, R Ghosh
The Astrophysical Journal 915 (2), 93, 2021
92021
Simultaneous View of FRB 180301 with FAST and NICER during a Bursting Phase
S Laha, G Younes, Z Wadiasingh, BJ Wang, KJ Lee, N Klingler, B Zhang, ...
The Astrophysical Journal 930 (2), 172, 2022
82022
Short-timescale variability of the blazar Mrk 421 from AstroSat and simultaneous multi-wavelength observations
R Chatterjee, S Das, A Khasnovis, R Ghosh, N Kumari, S Naik, ...
Journal of Astrophysics and Astronomy 42 (2), 80, 2021
82021
Limits on the hard X-ray emission from the periodic fast radio burst FRB 180916. J0158+ 65
S Laha, Z Wadiasingh, T Parsotan, A Lien, G Younes, B Zhang, SB Cenko, ...
The Astrophysical Journal 929 (2), 173, 2022
52022
The origin of the vanishing soft X-ray excess in the changing-look Active Galactic Nucleus Mrk 590
R Ghosh, S Laha, K Deshmukh, V Bhalerao, GC Dewangan, R Chatterjee
The Astrophysical Journal 937 (1), 31, 2022
42022
The Correlated Response of the Narrow FeKα Emission Line to the Primary Continuum Changes in the Seyfert Galaxy NGC 2992
R Ghosh, M Pal
Research Notes of the AAS 5 (2), 35, 2021
42021
A reemerging bright soft X-ray state of the changing-look active galactic nucleus 1ES 1927+ 654: a multiwavelength view
R Ghosh, S Laha, E Meyer, A Roychowdhury, X Yang, JA Acosta–Pulido, ...
The Astrophysical Journal 955 (1), 3, 2023
2023
Multi-wavelength study of the bare intermediate AGN Mrk 926 with AstroSat
SH Ezhikode, S Chakravorty, PO Petrucci, GC Dewangan, R Misra, G Matt, ...
44th COSPAR Scientific Assembly. Held 16-24 July 44, 2246, 2022
2022
The Nature of the Absorbed Soft X-Ray Variations in Compton-thin Type-II Active Galactic Nuclei
R Ghosh
Research Notes of the AAS 5 (2), 28, 2021
2021
A broad-band X-ray spectral study of the Seyfert 1 galaxy ESO 141–G055 with XMM–Newton and NuSTAR
R Ghosh, S Laha
Monthly Notices of the Royal Astronomical Society 497 (4), 4213-4221, 2020
2020
A study of X-ray emission of galaxies hosting molecular outflows (MOX sample).
S Laha, M Guainazzi, E Piconcelli, P Gandhi, C Ricci, R Ghosh, ...
AAS/High Energy Astrophysics Division 17, 106.53, 2019
2019
On the He-like triplet emission lines detected in the soft X-ray spectra of Active Galactic Nuclei: An insight into the electron density of the emitting gas.
R Ghosh
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