activity
20242026
collaborators

11 papers

astro-ph.HE2026

Evolution of Time-Lags of Swift J1727.8-1613 during the Rising Phase of Its Discovery Outburst

Sujoy Kumar Nath, Dipak Debnath, Hsiang-Kuang Chang

We investigate the accretion dynamics of the black hole X-ray binary Swift J1727.8-1613 during its discovery outburst that lasted for months. Insight-HXMT moni…

astro-ph.HE2026

Observational Relationship between Spectral Properties of Gamma-ray and X-ray Emissions from Pulsars

Ashwin Aravindaraj, Hsiang-Kuang Chang

Correlations between gamma-ray and X-ray spectral properties of pulsars are investigated in order to provide observational hints on physics involved in pulsars' high-energy emissio…

astro-ph.HE2026

Multi-wavelength properties of changing-state active galactic nuclei: I. the evolution of soft excess and X-ray continuum

Arghajit Jana, Claudio Ricci, Alessia Tortosa +11

Changing-state active galactic nuclei (CSAGNs) exhibit rapid variability, with mass accretion rates that can change by several orders of magnitude in a few years. This provides us…

astro-ph.HE2025

Investigating the Anti-Correlation between Photon Index and Flux of the Crab using RXTE and NuSTAR

Debjit Chatterjee, Hsiang-Kuang Chang, Dipak Debnath +2

We present a systematic study of the recently reported anti-correlation between X-ray flux and photon index () in the Crab Nebula, using archival RXTE/PCA (3 - 50 keV), RXTE/HEX…

astro-ph.HE2025

Evolution of QPO During Discovery Outburst of MAXI J1834-021: Estimation of Intrinsic Parameters from Spectro-Temporal Study

Dipak Debnath, Hsiang-Kuang Chang

The Galactic transient black hole candidate (BHC) MAXI~J1834-021 was detected for the first time by MAXI/GSC on February 05, 2023 and it was active for next ~months. A mon…

astro-ph.HE2025

Distinct Fe-K Line Complexes in MAXI J1744-294 Revealed by XRISM High-Resolution Spectroscopy

Kaushik Chatterjee, Santanu Mondal, Biswaraj Palit +7

The newly discovered Galactic transient MAXI J1744-294 went into its first X-ray outburst in 2025. We study the spectral properties of this source in the 2-10 keV energy band durin…