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researcher

S. Bhattacharyya

28 papers hereh-index 6489 citations44 works total

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

author position
  • first author1
  • middle author15
  • last author7

Across the 23 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE22
  • astro-ph4
  • astro-ph.IM1
  • gr-qc1
same name
  • S. Bhattacharyya — 94 papers, h 24
  • S. Bhattacharyya — 23 papers, h 36
  • S. Bhattacharyya — 22 papers, h 19
  • S. Bhattacharyya — 21 papers, h 9
  • S. Bhattacharyya — 20 papers, h 11
  • S. Bhattacharyya — 18 papers, h 15

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
20052026
most citedRelativistic Lines and Reflection from the Inner Accretion Disks Around Neutron Stars

185 citations · 536 across the 27 of their papers we have counts for

collaborators
Showing 2026Show all

3 papers · 1 filter

astro-ph.HE2026

Why most neutron star low-mass X-ray binaries accrete transiently: an evolutionary study of transient and persistent phases

Divyansh Tripathi, Sudip Bhattacharyya, Pulkit Ojha

A neutron star (NS) low-mass X-ray binary (LMXB), in which an NS accretes matter from a low-mass donor star, is an ideal source for probing some fundamental aspects of physics and…

astro-ph.HE2026

Circumstellar Disc and X-ray Variability in the Be/X-ray Binary SXP 5.05 During its 2024 Outburst

Chintan Patel, Sayantan Bhattacharya, Karan Akbari +3

Be/X-ray binaries provide a unique opportunity to study the interaction between neutron stars and circumstellar discs. SXP 5.05 is a particularly rare system, exhibiting eclipse-li…

astro-ph.HE2026

Probing heartbeat oscillations from the black hole X-ray binary GRS 1915+105 using spectral-timing analysis

Karan Akbari, Chintan Patel, Sayantan Bhattacharya +2

GRS 1915+105 is a black hole X-ray binary whose ρ-class ("heartbeat") oscillations (∼50--100 s) are attributed to radiation-pressure instabilities in the inner accretion dis…

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