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20092023
most citedThe lattice gradient flow at tree-level and its improvement

106 citations · 1.3k across the 67 of their papers we have counts for

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32 papers · 1 filter

astro-ph.HE2023

Spectral Properties of GX~339--4 in the Intermediate State Using AstroSat Observation

Arghajit Jana, Debjit Chatterjee, Hsiang-Kuang Chang +2

We present the results obtained from the spectral studies of black hole X-ray binary GX~339--4 using \astrosat~ observations during its 2021 outburst. \astrosat~ observed the sourc…

astro-ph.HE2023★ 3 cited

Broadband X-ray spectral analysis of the ULX NGC 1313\,X-1 using JeTCAF: Origin of the ULX bubble

Biswaraj Palit, Santanu Mondal

NGC 1313\,X-1 is a mysterious Ultra-luminous X-ray (ULX) source whose X-ray powering mechanism and a bubble-like structure surrounding the source are topics of intense study. Here,…

astro-ph.HE2023★ 8 cited

Spectral and Temporal Studies of Swift\,J1658.2--4242 using {\it AstroSat} Observations with {\tt JeTCAF} Model

Santanu Mondal, V. Jithesh

We present the X-ray spectral and temporal analysis of the black hole X-ray transient Swift J1658.2--4242 observed by {\it AstroSat}. Three epochs of data have been analysed using…

astro-ph.HE2023

Evolution of low frequency quasi-periodic oscillations in GX 339-4 during its 2021 outburst using AstroSat data

Santanu Mondal, Anirudh Salgundi, Debjit Chatterjee +3

The black hole X-ray binary GX\,339-4 showed an X-ray outburst during 2021. The {\it AstroSat} captured this outburst when the source entered into the intermediate flux state while…

astro-ph.HE2022★ 15 cited

Misaligned jets from Sgr A and the origin of Fermi/eROSITA bubbles

Kartick C. Sarkar, Santanu Mondal, Prateek Sharma +1

One of the leading explanations for the origin of Fermi Bubbles is a past jet activity in the Galactic center supermassive black hole Sgr A. The claimed jets are often assumed…

astro-ph.HE2022★ 7 cited

Study of accretion flows around an ultraluminous X-ray source M82 X-1 using NuSTAR data

Santanu Mondal, Biswaraj Palit, Sandip K. Chakrabarti

We study the spectral properties and accretion flow behavior of an ultraluminous X-ray source M82\,X-1 using {\it NuSTAR} observations. We use the physical two component advective…

astro-ph.HE2022★ 13 cited

Variable mass accretion and failed wind explain changing look phenomena in NGC 1365

Santanu Mondal, Tek P. Adhikari, Krzysztof Hryniewicz +2

Changing look active galactic nuclei (CLAGNs) show complex nature in their X-ray spectral shape and line of sight column density variation. The physical mechanisms responsible for…

astro-ph.HE2022★ 7 cited

Flux and spectral variability of Mrk 421 during its moderate activity state using NuSTAR: Possible accretion disc contribution?

Santanu Mondal, Priyanka Rani, C. S. Stalin +2

The X-ray emission in BL Lac objects is believed to be dominated by synchrotron emission from their relativistic jets. However, when the jet emission is not strong, one could expec…

astro-ph.HE2021★ 9 cited

Low Frequency Quasi Periodic Oscillations and Shocks in Accretion onto Black Hole

Chandra B. Singh, Santanu Mondal, David Garofalo

Low-frequency quasi-periodic oscillations (LFQPOs) have been routinely observed in black hole X-ray binaries (BHXRBs). These LFQPOs can be explained by axisymmetric shock oscillati…

astro-ph.HE2021★ 12 cited

Fermi bubbles: the collimated outburst needed to explain forward-shock edges

Santanu Mondal, Uri Keshet, Kartick C. Sarkar +1

The bipolar, nonthermal, high-latitude lobes known as the Fermi bubbles (FBs) are thought to originate from a massive energy release near the Galactic centre (GC). We constrain the…

astro-ph.HE2021

Spectral signature of mass outflow in Two Component Advective Flow Paradigm

Santanu Mondal, Sandip K. Chakrabarti

Outflows are common in many astrophysical systems. In the Two Component Advective Flow ({\fontfamily{qcr}\selectfont TCAF}) paradigm which is essentially a generalized Bondi flow i…

astro-ph.HE2021★ 5 cited

Emission lines from X-ray illuminated accretion disc in black hole binaries

Santanu Mondal, Tek P. Adhikari, Chandra B. Singh

X-ray flux from the inner hot region around central compact object in a binary system illuminates the upper surface of an accretion disc and it behaves like a corona. This region c…

astro-ph.HE2021★ 10 cited

Changing Accretion Geometry of Seyfert 1 Mrk 335 with {\it NuSTAR}: A Comparative Study

Santanu Mondal, C. S. Stalin

We present a detailed spectral study of the narrow-line Seyfert~1 galaxy, Markarian~335, using eight epoch observations made between 2013 and 2020 with the Nuclear Spectroscopic Te…

astro-ph.HE2019★ 16 cited

Spectral properties of NGC 4151 and the Estimation of black hole mass using TCAF solution

Prantik Nandi, Sandip K. Chakrabarti, Santanu Mondal

We present X-ray spectral analysis of Seyfert 1.5 Active Galactic Nuclei (AGN) NGC~4151 using \textit{NuSTAR} observation during 2012. This is the first attempt to fit an AGN data…

astro-ph.HE2019★ 1 cited

Evolution of spectral and temporal properties of MAXI J1836-194 during 2011 outburst

Arghajit Jana, Dipak Debnath, Sandip K. Chakrabarti +3

We study transient Galatic black hole candidate MAXI~J1836-194 during its 2011 outburst using RXTE/PCA archival data. 2.5-25~keV spectra are fitted with Two Component Advective Flo…

astro-ph.HE2018★ 11 cited

Implications on accretion flow dynamics from spectral study of Swift~J1357.2-0933

Santanu Mondal, Sandip K Chakrabarti

We report a detailed spectral study of Swift~J1357.2-0933 low-mass X-ray binary during its 2017 outburst using {\it Swift} and {\it NuSTAR} observations. We fit the data with two c…

astro-ph.HE2017★ 22 cited

Possible range of viscosity parameter to trigger black hole candidates to exhibit different states of outbursts

Santanu Mondal, Sandip K. Chakrabarti, Shreeram Nagarkoti +1

In a two component advective flow around a compact object, a high viscosity Keplerian disk is flanked by a low angular momentum and low viscosity flow which forms a centrifugal pre…

astro-ph.HE2017★ 40 cited

Accretion Flow Properties of Swift J1753.5-0127 during its 2005 outburst

Dipak Debnath, Arghajit Jana, Sandip K. Chakrabarti +2

Galactic X-ray binary black hole candidate Swift~J1753.5-0127 was discovered on June 30 2005 by Swift/BAT instrument. In this paper, we make detailed analysis of spectral and timin…

astro-ph.HE2016★ 74 cited

Estimation of Mass of Compact Object in H 1743-322 from 2010 and 2011 Outbursts using TCAF Solution and Spectral Index - QPO Frequency Correlation

Aslam Ali Molla, Sandip K. Chakrabarti, Dipak Debnath +1

The well known black hole candidate H~1743-322 exhibited temporal and spectral variabilities during several outbursts. Daily variation of the accretion rates and the flow geometry…

astro-ph.HE2016★ 59 cited

Accretion Flow Properties of MAXI J1543-564 During 2011 Outburst from TCAF Solution

Debjit Chatterjee, Dipak Debnath, Sandip K. Chakrabarti +2

We derive accretion flow properties of the transient black hole candidate (BHC) MAXI~J1543-564 using the RXTE data. We use Two-Component Advective Flow (TCAF) solution to fit the d…

astro-ph.HE2016★ 63 cited

Estimation of Mass of the Black Hole Candidate MAXI J1659-152 using TCAF and POS Models

Aslam Ali Molla, Dipak Debnath, Sandip K. Chakrabarti +2

The Galactic transient black hole candidate (BHC) MAXI~J1659-152 exhibited temporal and spectral evolution during its very first X-ray outburst (2010) after its discovery on 25th S…

astro-ph.HE2016★ 32 cited

Spectral study of GX 339-4 with TCAF using Swift/XRT and NuSTAR Observation

Santanu Mondal, Sandip K. Chakrabarti, Dipak Debnath

We fit spectra of galactic transient source GX~339-4 during its 2013 outburst using Two Component Advective Flow (TCAF) solution. For the first time, we are fitting combined NuSTAR…

astro-ph.HE2016★ 72 cited

Accretion flow dynamics of MAXI J1836-194 during its 2011 outburst from TCAF solution

Arghajit Jana, Dipak Debnath, Sandip K. Chakrabarti +2

The Galactic transient X-ray binary MAXI~J1836-194 was discovered on 29th August 2011. Here we make a detailed study of the spectral and timing properties of its 2011 outburst usin…

astro-ph.HE2015

Spectral and Temporal Properties of MAXI J1836-194 during 2011 Outburst

A. Jana, D. Debnath, S. Mondal +3

We study black hole candidate (BHC) MAXI~J1836-194 during its 2011 outburst with Two Component Advective Flow (TCAF) model using RXTE/PCU2 data in ~keV band. From spectral…