most citedA New Planet Around an M Dwarf: Revealing a Correlation Between Exoplanets and Stellar Mass

326 citations · 1.1k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2009162 cited

Variable Sodium Absorption in a Low-Extinction Type Ia Supernova

Joshua D. Simon, Avishay Gal-Yam, Orly Gnat +18

Recent observations have revealed that some Type Ia supernovae exhibit narrow, time-variable Na I D absorption features. The origin of the absorbing material is controversial, but…

astro-ph2007263 cited

Five Planets Orbiting 55 Cancri

Debra A. Fischer, Geoffrey W. Marcy, R. Paul Butler +9

We report 18 years of Doppler shift measurements of a nearby star, 55 Cancri, that exhibit strong evidence for five orbiting planets. The four previously reported planets are stron…

astro-ph2007142 cited

An Accurate Distance to High-Velocity Cloud Complex C

C. Thom, J. E. G. Peek, M. E. Putman +3

We report an accurate distance of d = 10+/-2.5kpc to the high-velocity cloud Complex C. Using high signal-to-noise Keck/HIRES spectra of two horizontal-branch stars, we have detect…

astro-ph200796 cited

Retired A Stars and Their Companions II: Jovian planets orbiting kappa Coronae Borealis and HD167042

John A. Johnson, Geoffrey W. Marcy, Debra A. Fischer +5

We report precise Doppler measurements of two evolved stars, kappa CrB (HD142091) and HD 167042, obtained at Lick Observatory as part of our search for planets orbiting intermediat…

astro-ph2007326 cited

A New Planet Around an M Dwarf: Revealing a Correlation Between Exoplanets and Stellar Mass

John A. Johnson, R. Paul Butler, Geoffrey W. Marcy +4

We report precise Doppler measurements of GJ317 (M3.5V) that reveal the presence of a planet with a minimum mass Msini = 1.2 Mjup in an eccentric, 692.9 day orbit. GJ317 is only th…

astro-ph200792 cited

Spin-Orbit Alignment for the Eccentric Exoplanet HD 147506b

Joshua N. Winn, John Asher Johnson, Kathryn M. G. Peek +7

The short-period exoplanet HD 147506b (also known as HAT-P-2b) has an eccentric orbit, raising the possibility that it migrated through planet-planet scattering or Kozai oscillatio…