Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Scientist
Harvard-Smithsonian Center for Astrophysics
CfA;
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA, USA
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138.
Harvard-Smithsonian, CfA
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
California, University, Los Angeles
Harvard-Smithsonian Center for Astrophysics 60 Garden St., Cambridge, MA, 02139, USA
Harvard-Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA, 02138 MS16
Instituto de Astrofí sica de Canarias, 38205, La Laguna, Tenerife, Spain
Harvard-Smithsonian Center for Astrophysics, 60 Garden St. Cambridge, MA, 02138, USA
ULL
Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, USA
CfA
Crimean Astrophysical Observatory;, The University of Southern California
California Univ., Los Angeles
Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, USA
Harvard-Smithsonican Center for Astrophysics, Cambridge, MA, US
California Institute of Technology, Pasadena.
University of Southern California, Los Angeles.
California Univ., Los Angeles.
Consejo Superior de Investigaciones Cientificas, Tenerife, Spain
A High-Eccentricity Low-Mass Companion to HD 89744
A Keck HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. II. On the Frequency of Giant Planets in the Metal-Poor Regime
A Keck/HIRES Doppler Search for Planets Orbiting Metal-Poor Dwarfs. I. Testing Giant Planet Formation and Migration Scenarios
A Mode Fitting Methodology Optimized for Very Long Time Series
A Mode-Fitting Methodology Optimized for Very Long Helioseismic Time Series
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Profile ID: LFWR-SCP-P-19425