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researcher

K. Hill

6 papers hereh-index 81.5k citations10 works total

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

author position
  • middle author2
  • last author1

Across the 3 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph3
  • astro-ph.SR2
  • astro-ph.EP1
same name
  • K. Hill — 38 papers, h 26
  • K. Hill — 24 papers, h 11
  • K. Hill — 22 papers, h 36
  • K. Hill — 3 papers, h 18
  • K. Hill — 3 papers, h 42
  • K. Hill — 2 papers, h 16

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
20042022
most citedOne or more bound planets per Milky Way star from microlensing observations

588 citations · 749 across the 6 of their papers we have counts for

collaborators
Showing astro-phShow all

3 papers · 1 filter

astro-ph2007★ 27 cited

Limits on additional planetary companions to OGLE-2005-BLG-390L

D. Kubas, A. Cassan, M. Dominik +1

We investigate constraints on additional planets orbiting the distant M-dwarf star OGLE-2005-BLG-390L, around which photometric microlensing data has revealed the existence of the…

astro-ph2004★ 42 cited

Potential Direct Single-Star Mass Measurement

H. Ghosh

We analyze the lightcurve of the microlensing event OGLE-2003-BLG-175/MOA-2003-BLG-45 and show that it has two properties that, when combined with future high resolution astrometry…

astro-ph2004★ 75 cited

OGLE-2003-BLG-238: Microlensing Mass Estimate of an Isolated Star

Guangfei Jiang, D. L. DePoy, A. Gal-Yam +38

Microlensing is the only known direct method to measure the masses of stars that lack visible companions. In terms of microlensing observables, the mass is given by M=(c^2/4G)\tild…

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