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A. Gould

156 papers hereh-index 6213.9k citations372 works total

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

author position
  • sole author38
  • first author30
  • middle author40
  • last author41

Across the 149 of 156 papers where every author was matched, so the position is known.

fields
  • astro-ph94
  • astro-ph.EP28
  • astro-ph.GA15
  • astro-ph.SR15
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • A. Gould — 239 papers, h 46
  • A. Gould — 87 papers, h 19
  • A. Gould — 75 papers, h 63
  • A. Gould — 52 papers, h 23
  • A. Gould — 10 papers, h 14
  • A. Gould — 1 paper

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
19932022
most citedReddening and Extinction Toward the Galactic Bulge from OGLE-III: The Inner Milky Way's Rv ~ 2.5 Extinction Curve

590 citations · 8.8k across the 153 of their papers we have counts for

collaborators
Showing 2015Show all

3 papers · 1 filter

astro-ph.SR2015★ 129 cited

Slingshot Mechanism in Orion: Kinematic Evidence For Ejection of Protostars by Filaments

Amelia M. Stutz, Andrew Gould

By comparing 3 constituents of Orion A (gas, protostars, and pre-main-sequence stars), both morhologically and kinematically, we derive the following. The gas surface density near…

astro-ph.EP2015★ 43 cited

KELT-4Ab: An inflated Hot Jupiter transiting the bright (V~10) component of a hierarchical triple

Jason D. Eastman, Thomas G. Beatty, Robert J. Siverd +42

We report the discovery of KELT-4Ab, an inflated, transiting Hot Jupiter orbiting the brightest component of a hierarchical triple stellar system. The host star is an F star with $…

astro-ph.EP2015★ 2 cited

KELT-7b: A hot Jupiter transiting a bright V=8.54 rapidly rotating F-star

Allyson Bieryla, Karen Collins, Thomas G. Beatty +31

We report the discovery of KELT-7b, a transiting hot Jupiter with a mass of 1.28±0.18 MJ, radius of 1.53−0.047+0.046​ RJ, and an orbital period of $2.7347749 \pm 0.000…

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