activity
20092026
most citedAccretion flow behaviour during the evolution of the Quasi Periodic Oscillation Frequency of XTE J1550-564 in 1998 outburst

54 citations · 140 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

Bridging X-ray Polarization with Timing & Spectroscopic Parameters of a galactic black hole: Swift J1727.8-1613

Arka Chatterjee, Sujoy K. Nath, Kaushik Chatterjee +5

We report the discovery of a correlated energy-dependent time lag and degree of polarization for Swift J1727.8-1613 during its 2023 outburst. The energy-dependent time lag is measu…

astro-ph.HE2026

Time-Lag properties associated with LFQPO in X-ray variability classes of GRS 1915+105: Findings from AstroSat

Prajjwal Majumder, Broja G. Dutta, Anuj Nandi

We present a comprehensive analysis of Low Frequency Quasi-periodic Oscillation (LFQPO) associated time-lags in the persistently variable black hole binary GRS 1915+105 using 441 k…

astro-ph.HE2025★ 1 cited

Decoding the Origin of HFQPOs of GRS 1915+105 during 'Canonical' Soft States: An In-depth View using Multi-mission observations

Prajjwal Majumder, Broja G. Dutta, Anuj Nandi

We present a comprehensive analysis of the 'canonical' soft state (, , and spectral variability classes) of the black hole binary GRS 1915+105, using RXTE, AstroSat, and…

astro-ph.HE2023

First detection of Soft-lag in GRS 1915+105 at HFQPO using AstroSat observations

Prajjwal Majumder, Broja G. Dutta, Anuj Nandi

The Galactic black hole GRS 1915+105 exhibits generic High-Frequency Quasi-periodic Oscillations (HFQPOs) at 67 Hz only during the radio-quiet 'softer' variability classes.…

astro-ph.HE2021★ 21 cited

Long term X-Ray Observations of Seyfert 1 Galaxy Ark 120: On the origin of soft-excess

Prantik Nandi, Arka Chatterjee, Sandip K. Chakrabarti +1

We present the long-term X-ray spectral and temporal analysis of a 'bare-type AGN' Ark 120. We consider the observations from XMM-Newton, Suzaku, Swift, and NuSTAR from 2003 to 201…

astro-ph.HE2020★ 13 cited

Time-domain variability properties of XTE J1650-500 during its 2001 outburst: Evidence of disc-jet connection

Arka Chatterjee, Broja G. Dutta, Prantik Nandi +1

Evolution of variability properties of Galactic transient sources is a diagnostic tool to understand various regimes of the accretion flow and its dynamics close to the central bla…

astro-ph.HE2019★ 3 cited

Discovery of Jet-Induced Soft Lags of XTE J1550-564 during Its 1998 Outburst

Arka Chatterjee, Broja G. Dutta, Dusmanta Patra +2

X-ray time lags are complicated in nature. The exact reasons for complex lag spectra are yet to be known. However, the hard lags, in general, are believed to be originated due to t…

astro-ph.HE2019★ 12 cited

Evidence of Outflow Induced Soft Lags of Galactic Black Holes

Dusmanta Patra, Arka Chatterjee, Broja G. Dutta +2

The nature of lag variation of Galactic black holes remains enigmatic mostly because of nonlinear and non-local physical mechanisms which contribute to the lag of the photons comin…

astro-ph.HE2018★ 11 cited

Evolution of Accretion Disc Geometry of GRS~1915+105 during its state as revealed by TCAF solution

Broja G Dutta, Partha Sarathi Pal, Sandip K Chakrabarti

The evolution of the C-type low frequency quasi-periodic oscillations (LFQPOs) and associated time lag in transient black hole sources as a function of time can be explained by var…

astro-ph.HE2016★ 25 cited

Temporal variability from the two-component advective flow solution and its observational evidence

Broja G. Dutta, Sandip K. Chakrabarti

In the propagating oscillatory shock model, the oscillation of the post-shock region, i.e., the Compton cloud, causes the observed low-frequency quasi-periodic oscillations (QPOs).…

astro-ph.HE2009★ 54 cited

Accretion flow behaviour during the evolution of the Quasi Periodic Oscillation Frequency of XTE J1550-564 in 1998 outburst

Sandip K. Chakrabarti, Broja G. Dutta, P. S. Pal

Low and intermediate frequency quasi-periodic oscillations (QPOs) are thought to be due to oscillations of Comptonizing regions or hot regions embedded in Keplerian discs. Observat…