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A. Cameron

61 papers hereh-index 212.2k citations63 works total

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

author position
  • first author2
  • middle author48
  • last author3

Across the 53 of 61 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP37
  • astro-ph.SR15
  • astro-ph6
  • astro-ph.IM3
same name
  • A. Cameron — 341 papers, h 70
  • A. Cameron — 91 papers, h 31
  • A. Cameron — 57 papers, h 22
  • A. Cameron — 35 papers, h 6
  • A. Cameron — 19 papers, h 10
  • A. Cameron — 16 papers, h 4

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 citedSearching for Star-Planet interactions within the magnetosphere of HD 189733

205 citations · 2.3k across the 58 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

4 papers · 2 filters

astro-ph2003★ 54 cited

A search for starlight reflected from HD 75289 b

C. Leigh, A. Collier Cameron, S. Udry +4

We have used a doppler tomographic analysis to conduct a deep search for the starlight reflected from the planetary companion to HD 75289. In 4 nights on VLT2/UVES in January 2003,…

astro-ph2003★ 15 cited

Prospects for Spectroscopic Reflected-light Planet Searches

C. Leigh, A. Collier Cameron, T. Guillot

High-resolution spectroscopic searches for the starlight reflected from close-in extra-solar giant planets have the capability of determining the optical albedo spectra and scatter…

astro-ph2003★ 83 cited

A new upper limit on the reflected starlight from Tau Bootis b

C. Leigh, A. Collier Cameron, K. Horne +2

Using improved doppler tomographic signal-analysis techniques we have carried out a deep search for starlight reflected from the giant planet orbiting the star Tau Bootis. We combi…

astro-ph2003

Rationale for the use of color information on Eddington

P. Borde, A. Leger, D. Rouan +1

For the Eddington mission, the intrinsic stellar variability can be a major source of noise in the detection of extrasolar planets by the transit method. We derive that most detect…

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