Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
Steward Observatory, University of Arizona, Tucson, AZ;
Steward Observatory, University of Arizona;
Steward Obs., Univ. of Arizona
Steward Observatory, USA
Steward Observatory, Univ. of Arizona
University of Arizona, Tucson
Steward Observatory, University of Arizona, Tucson, AZ 85721.
Steward Observatory, University of Arizona
Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065
University of Arizona, Tucson, AZ
Steward Observatory, Tucson, AZ
Arizona, University, Tucson, AZ
Steward Observatory, University of Arizona, Tucson, AZ 85721, USA
University of Arizona, Tucson, AZ, US
Mount Wilson and Las Campanas Observatoires, Pasadena
Steward Observatory, Tucson, AC
Steward Univ., Tucson, AZ
Steward Observatory, Tucson, AZ; Mount Wilson and Las Campanas Observatoires, Pasadena, CA
Department of Astronomy, University of Arizona, Tucson, AZ 85721, USA
Steward Observatory / University of Arizona, USA
Steward Observatory
U. Arizona
U.Arizona
Steward Observatory, University of Arizona, Tucson, AZ
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA
University of Arizona / Steward
Department of Astronomy, University of Arizona
Steward Observatory, UA
Steward Obs / University of Arizona
Harvard-Smithsonian Center for Astrophysics, Amado, AZ.
European Space Astronomy Center of ESA
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA; Steward Observatory, Tucson, AZ
UofA
University of Arizona, Steward Observatory
Havard-Smithsonian Center for Astrophysics, Cambridge, Mass.
Arizona University
Harvard Smithsonian Center for Astrophysics
150 keV Emission from PKS2149-306 with BeppoSAX
150 keV Emission from PKS2149-306 with BeppoSAX: A Compton Suppressed Jet and the Origin of Radio-quiet Quasars
A approximately 10 MPC void in the Ly-alpha forest at Z = 3.17
A comparison between the rest-frame optical UV continua of high (z ≥ 3) and low (z ≡ 0.1) redshift quasars.
A comparison between the rest-frame optical/UV continua of high (z>=3) and low (z ~ 0.1) redshift quasars
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Profile ID: LFWR-SCP-P-15555