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researcher

D. Bhattacharya

99 papers hereh-index 294k citations267 works total

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

author position
  • sole author2
  • first author2
  • middle author60
  • last author28

Across the 92 of 99 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE49
  • astro-ph24
  • astro-ph.IM19
  • astro-ph.SR5
  • hep-ph2
same name
  • D. Bhattacharya — 42 papers, h 20
  • D. Bhattacharya — 24 papers, h 7
  • D. Bhattacharya — 22 papers, h 25
  • D. Bhattacharya — 18 papers, h 7
  • D. Bhattacharya — 17 papers, h 14
  • D. Bhattacharya — 9 papers, h 9

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
19982023
most citedThe Cadmium Zinc Telluride Imager on AstroSat

103 citations · 1.7k across the 98 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

hep-ph2003★ 5 cited

A new window on Strange Quark Matter as the ground state of strongly interacting matter

Vikram Soni, Dipankar Bhattacharya

If strange quark matter is the true ground state of matter, it must have lower energy than nuclear matter. Simultaneously, two-flavour quark matter must have higher energy than nuc…

astro-ph2003

SN 2002ap, the hypernova of class Ic

S. B. Pandey, D. K. Sahu, G. C. Anupama +2

The supernova SN 2002ap was discovered in the outer regions of the nearby spiral M74 on January 29.4 UT. Early photometric and spectroscopic observations indicate the supernova bel…

astro-ph2003★ 38 cited

Optical afterglow of the not so dark GRB 021211

S. B. Pandey, G. C. Anupama, R. Sagar +5

We determine Johnson B,V and Cousins R,I photometric CCD magnitudes for the afterglow of GRB 021211 during the first night after the GRB trigger. The afterglow was very faint a…

astro-ph2003★ 2 cited

Evolution of an afterglow with a hard electron spectrum

D Bhattacharya, L Resmi

Diffusive shock acceleration theory suggests that the ``universal'' energy spectrum of electrons with a power-law index p approximately equal to 2.3, commonly used to model GRB aft…

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