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G. Benedict

45 papers hereh-index 303.4k citations207 works total

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

author position
  • first author21
  • middle author8
  • last author7

Across the 36 of 45 papers where every author was matched, so the position is known.

fields
  • astro-ph27
  • astro-ph.SR13
  • astro-ph.EP4
  • astro-ph.IM1
same name
  • G. Benedict — 8 papers, h 8

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
19962023
most citedHubble Space Telescope Fine Guidance Sensor Parallaxes of Galactic Cepheid Variable Stars: Period-Luminosity Relations

370 citations · 3.5k across the 45 of their papers we have counts for

collaborators
Showing 1999 · astro-phShow all

3 papers · 2 filters

astro-ph1999★ 321 cited

Interferometric Astrometry of Proxima Centauri and Barnard's Star Using Hubble Space Telescope Fine Guidance Sensor 3: Detection Limits for sub-Stellar Companions

G. Fritz Benedict, Barbara McArthur, D. W. Chappell +13

We report on a sub-stellar companion search utilizing interferometric fringe-tracking astrometry acquired with Fine Guidance Sensor 3 (FGS 3) on the Hubble Space Telescope. Our tar…

astro-ph1999★ 41 cited

Astrometry with Hubble Space Telescope Fine Guidance Sensor 3: The Parallax of the Cataclysmic Variable RW Triangulum

B. E. McArthur, G. F. Benedict, J. Lee +12

RW Triangulum (RW Tri) is a 13th magnitude Nova-like Cataclysmic Variable star with an orbital period of 0.2319 days (5.56 hours). Infrared observations of RW Tri indicate that its…

astro-ph1999★ 85 cited

HST Fine Guidance Sensor Astrometric Parallaxes for Three Dwarf Novae: SS Aurigae, SS Cygni, and U Geminorum

Thomas E. Harrison, Bernard J. McNamara, Paula Szkody +4

We report astrometric parallaxes for three well known dwarf novae obtained using the Fine Guidance Sensors on the Hubble Space Telescope. We found a parallax for SS Aurigae of Pi =…

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