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researcher

K. Collins

248 papers hereh-index 407.6k citations335 works total

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

author position
  • first author5
  • middle author189
  • last author2

Across the 196 of 248 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP230
  • astro-ph.SR14
  • astro-ph.IM3
  • cs.NI1
same name
  • K. Collins — 127 papers, h 14
  • K. Collins — 124 papers, h 27
  • K. Collins — 46 papers, h 6
  • K. Collins — 5 papers, h 6
  • K. Collins — 2 papers, h 10
  • K. Collins — 2 papers, h 2

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
20122026
most citedAstroImageJ: Image Processing and Photometric Extraction for Ultra-Precise Astronomical Light Curves (Expanded Edition)

706 citations · 11k across the 245 of their papers we have counts for

collaborators
Showing 2012Show all

3 papers · 1 filter

astro-ph.EP2012★ 74 cited

KELT-3b: A Hot Jupiter Transiting a V=9.8 Late-F Star

Joshua Pepper, Robert J. Siverd, Thomas G. Beatty +31

We report the discovery of KELT-3b, a moderately inflated transiting hot Jupiter with a mass of 1.477 (-0.067, +0.066) M_J, and radius of 1.345 +/- 0.072 R_J, with an orbital perio…

astro-ph.EP2012★ 300 cited

KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star

Robert J. Siverd, Thomas G. Beatty, Joshua Pepper +29

We present the discovery of KELT-1b, the first transiting low-mass companion from the wide-field Kilodegree Extremely Little Telescope-North (KELT-North) survey. The V=10.7 primary…

astro-ph.EP2012★ 69 cited

KELT-2Ab: A Hot Jupiter Transiting the Bright (V=8.77) Primary Star of a Binary System

Thomas G. Beatty, Joshua Pepper, Robert J. Siverd +28

We report the discovery of KELT-2Ab, a hot Jupiter transiting the bright (V=8.77) primary star of the HD 42176 binary system. The host is a slightly evolved late F-star likely in t…

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