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researcher

D. Brown

48 papers hereh-index 261.7k citations78 works total

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

author position
  • sole author1
  • first author4
  • middle author39

Across the 44 of 48 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP44
  • astro-ph.SR3
  • astro-ph.GA1
same name
  • D. Brown — 157 papers, h 80
  • D. Brown — 128 papers, h 35
  • D. Brown — 125 papers
  • D. Brown — 115 papers, h 37
  • D. Brown — 84 papers, h 40
  • D. Brown — 71 papers, h 67

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
20102026
most citedThe GAPS programme with HARPS-N at TNG. I: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1

139 citations · 2.3k across the 48 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.EP2013★ 24 cited

Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii

Y. Gómez Maqueo Chew, F. Faedi, D. Pollacco +38

We report the discovery of two transiting hot Jupiters, WASP-65b (M_pl = 1.55 +/- 0.16 M_J; R_pl = 1.11 +/- 0.06 R_J), and WASP-75b (M_pl = 1.07 +/- 0.05 M_J; R_pl = 1.27 +/- 0.05…

astro-ph.SR2013★ 139 cited

The GAPS programme with HARPS-N at TNG. I: Observations of the Rossiter-McLaughlin effect and characterisation of the transiting system Qatar-1

E. Covino, M. Esposito, M. Barbieri +67

A long-term multi-purpose observational programme has started with HARPS-N@TNG aimed to characterise the global architectural properties of exoplanetary systems. In this first pape…

astro-ph.EP2013★ 51 cited

Analysis of spin-orbit alignment in the WASP-32, WASP-38, and HAT-P-27/WASP-40 systems

D. J. A. Brown, A. Collier Cameron, R. F. Díaz +14

We present measurements of the spin-orbit alignment angle, lambda, for the hot Jupiter systems WASP-32, WASP-38, and HAT-P-27/WASP-40, based on data obtained using the HARPS spectr…

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