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P. Gandhi

49 papers hereh-index 221.4k citations82 works total

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

author position
  • sole author2
  • first author5
  • middle author32
  • last author2

Across the 41 of 49 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE31
  • astro-ph.CO5
  • astro-ph4
  • astro-ph.IM4
  • astro-ph.SR3
  • astro-ph.GA2
same name
  • P. Gandhi — 206 papers, h 56
  • P. Gandhi — 46 papers, h 9
  • P. Gandhi — 27 papers, h 12
  • P. Gandhi — 18 papers, h 3
  • P. Gandhi — 17 papers, h 4
  • P. Gandhi — 13 papers, h 11

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
20062026
most citedThe XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

272 citations · 1.7k across the 49 of their papers we have counts for

collaborators
Showing 2018Show all

3 papers · 1 filter

astro-ph.HE2018★ 13 cited

The Curious Case of Swift J1753.5-0127: A Black Hole Low-mass X-ray Binary Analogue to Z Cam Type Dwarf Novae

A. W. Shaw, B. E. Tetarenko, G. Dubus +5

Swift J1753.5-0127 (J1753) is a candidate black hole low-mass X-ray binary (BH-LMXB) that was discovered in outburst in May 2005. It remained in outburst for ∼12 years, exhibi…

astro-ph.HE2018★ 35 cited

A high-density relativistic reflection origin for the soft and hard X-ray excess emission from Mrk 1044

Labani Mallick, William N. Alston, Michael L. Parker +7

We present the first results from a detailed spectral-timing analysis of a long (∼130 ks) XMM-Newton observation and quasi-simultaneous NuSTAR and Swift observations of the hi…

astro-ph.HE2018★ 22 cited

Measuring the masses of Intermediate Polars with NuSTAR: V709 Cas, NY Lup and V1223 Sgr

A. W. Shaw, C. O. Heinke, K. Mukai +3

The X-ray spectra of intermediate polars can be modelled to give a direct measurement of white dwarf mass. Here we fit accretion column models to NuSTAR spectra of three intermedia…

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