scispace - formally typeset
B

B. Scott Gaudi

Researcher at Ohio State University

Publications -  190
Citations -  10637

B. Scott Gaudi is an academic researcher from Ohio State University. The author has contributed to research in topics: Planet & Gravitational microlensing. The author has an hindex of 45, co-authored 189 publications receiving 9780 citations. Previous affiliations of B. Scott Gaudi include Harvard University & Princeton University.

Papers
More filters
Journal ArticleDOI

Sdss-iii: massive spectroscopic surveys of the distant universe, the milky way, and extra-solar planetary systems

Daniel J. Eisenstein, +263 more
TL;DR: SDSS-III as mentioned in this paper is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars.
Journal ArticleDOI

SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Daniel J. Eisenstein, +239 more
TL;DR: SDSS-III as discussed by the authors is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars.
Journal ArticleDOI

Prospects for the characterization and confirmation of transiting exoplanets via the rossiter-mclaughlin effect

TL;DR: In this paper, the Rossiter-McLaughlin (RM) effect is used to measure the alignment of planetary orbits with the spin axes of their parent stars, and to confirm exoplanetary transits.
Journal ArticleDOI

A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host

B. Scott Gaudi, +65 more
- 05 Jun 2017 - 
TL;DR: Observations of the bright star HD 195689 are reported, which reveal a close-in (orbital period of about 1.48 days) transiting giant planet, KELT-9b, which is as hot as stars of stellar type K4 and receives 700 times more extreme-ultraviolet radiation than WASP-33b.
Journal ArticleDOI

Periodic Flux Variability of Stars due to the Reflex Doppler Effect Induced by Planetary Companions

TL;DR: In this paper, the authors show that the Doppler flux variability induced by the reflex motion of stars due to planetary companions has an amplitude of (3 - α)K/c, where K is the reflex radial velocity amplitude and α ≈ is the logarithmic slope of the source spectral flux in the observed frequency band.