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researcher

D. Farrah

315 papers hereh-index 7819.2k citations454 works total

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

author position
  • first author23
  • middle author215
  • last author9

Across the 247 of 315 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA124
  • astro-ph.CO108
  • astro-ph60
  • astro-ph.HE14
  • astro-ph.IM5
  • gr-qc3
same name
  • D. Farrah — 20 papers, h 15
  • D. Farrah — 13 papers, h 9
  • D. Farrah — 9 papers
  • D. Farrah — 3 papers, h 2
  • D. Farrah — 2 papers, h 3

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
20012026
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 25.3k across the 312 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.HEShow all

4 papers · 2 filters

astro-ph.HE2016★ 41 cited

Broadband X-ray spectral analysis of the Seyfert 1 galaxy GRS 1734-292

A. Tortosa, A. Marinucci, G. Matt +14

We discuss the broadband X-ray spectrum of GRS 1734-292 obtained from non-simultaneous XMM-Newton and NuSTAR observations, performed in 2009 and 2014, respectively. GRS1734-292 is…

astro-ph.HE2016★ 72 cited

NuSTAR observations of WISE J1036+0449, a Galaxy at z∼1 obscured by hot dust

C. Ricci, R. J. Assef, D. Stern +34

Hot, Dust-Obscured Galaxies (Hot DOGs), selected from the WISE all sky infrared survey, host some of the most powerful Active Galactic Nuclei (AGN) known, and might represent an im…

astro-ph.HE2016★ 7 cited

The Phoenix galaxy as seen by NuSTAR

A. Masini, A. Comastri, S. Puccetti +18

Aims. We study the long-term variability of the well-known Seyfert 2 galaxy Mrk 1210 (a.k.a. UGC 4203, or the Phoenix galaxy). Methods. The source was observed by many X-ray facili…

astro-ph.HE2016★ 37 cited

A growth-rate indicator for Compton-thick active galactic nuclei

M. Brightman, A. Masini, D. R. Ballantyne +10

Due to their heavily obscured central engines, the growth rate of Compton-thick (CT) active galactic nuclei (AGN) is difficult to measure. A statistically significant correlation b…

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