activity
19952020
most citedThe Cosmic Origins Spectrograph

491 citations · 6.2k across the 106 of their papers we have counts for

collaborators

107 papers

astro-ph.EP2020★ 4 cited

The Hubble Space Telescope's near-UV and optical transmission spectrum of Earth as an exoplanet

Allison Youngblood, Giada N. Arney, Antonio García Muñoz +3

We observed the 2019 January total lunar eclipse with the Hubble Space Telescope's STIS spectrograph to obtain the first near-UV (1700-3200 ) observation of Earth as a transitin…

astro-ph.GA2019★ 33 cited

A Search for Intrinsic HI 21 cm and OH 18 cm Absorption Toward Compact Radio Sources

Kathryn Grasha, Jeremy Darling, Alberto Bolatto +2

We present the results of a large search for intrinsic HI 21 cm and OH 18 cm absorption in 145 compact radio sources in the redshift range 0.02< z <3.8 with the Green Bank Telescop…

astro-ph.GA2018★ 16 cited

The Ultraviolet Detection of Diffuse Gas in Galaxy Groups

John T. Stocke, Brian A. Keeney, Charles W. Danforth +5

A small survey of the UV-absorbing gas in 12 low- galaxy groups has been conducted using the Cosmic Origins Spectrograph (COS) on-board the Hubble Space Telescope (HST). Targets…

astro-ph.HE2018★ 124 cited

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters

Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…

astro-ph.GA2018★ 34 cited

A Galaxy Redshift Survey near HST/COS AGN Sight Lines

Brian A. Keeney, John T. Stocke, Cameron T. Pratt +8

To establish the connection between galaxies and UV-detected absorption systems in the local universe, a deep () and wide ( radius) galaxy redshift survey…

astro-ph.SR2017★ 12 cited

H Fluorescence in M Dwarf Systems: A Stellar Origin

Nicholas Kruczek, Kevin France, William Evonosky +7

Observations of molecular hydrogen (H) fluorescence are a potentially useful tool for measuring the H abundance in exoplanet atmospheres. This emission was previously obser…