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researcher

A. Roychowdhury

15 papers hereh-index 6113 citations18 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author3
  • first author6
  • middle author5
  • last author1

Across the 15 of 15 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE12
  • astro-ph.GA1
  • astro-ph.IM1
  • quant-ph1
same name
  • A. Roychowdhury — 4 papers, h 24
  • A. Roychowdhury — 3 papers, h 2

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20182026
most citedPossible Accretion Disk Origin of the Emission Variability of a Blazar Jet

34 citations · 81 across the 14 of their papers we have counts for

collaborators
Showing 2026Show all

4 papers · 1 filter

astro-ph.HE2026

First Detection of Radio Polarization During Jet Formation in the Changing-Look AGN 1ES 1927+654

Onic I. Shuvo, Eileen T. Meyer, Sibasish Laha +10

We present a multiwavelength radio study of the changing-look AGN 1ES 1927+654 following its renewed X-ray brightening since mid-2022, combining VLBA imaging with multi-band and ti…

astro-ph.HE2026

Reconnection-driven State Transitions in Flat Spectrum Radio Quasars

Agniva Roychowdhury

We extend the work of Roychowdhury (2026) on skewness variations of the logarithmic flux, driven by large GeV flares in FSRQs, to a sample of 18 FSRQs. We find that they can be cat…

astro-ph.HE2026

Parameter Estimation Limits in Blazars

Agniva Roychowdhury

Parameter degeneracy in blazar spectral energy distributions (SEDs) is known but rarely quantified. This paper introduces a Fisher Information approach to determine theoretical lim…

astro-ph.HE2026

An Afterglow Study of the "New Year's Burst" GRB 220101A

Agniva Roychowdhury, Tuomas Kangas, Andrew Fruchter +12

We present a detailed broadband afterglow study of GRB 220101A (104≲ΔT≲107 s) combining multi-wavelength data from soft X-rays until 6 GHz. The afterglow light cu…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.