A MULTI-SITE CAMPAIGN TO MEASURE SOLAR-LIKE OSCILLATIONS IN PROCYON. II. MODE FREQUENCIES

@article{Bedding2010AMC,
  title={A MULTI-SITE CAMPAIGN TO MEASURE SOLAR-LIKE OSCILLATIONS IN PROCYON. II. MODE FREQUENCIES},
  author={Timothy R. Bedding and Hans Kjeldsen and Tiago L. Campante and Thierry P. Appourchaux and Alfio Bonanno and William J. Chaplin and R. A. Garcı́a and Milena Marti{\'c} and Beno{\^i}t Mosser and R. Paul Butler and Hans Bruntt and L{\'a}szl{\'o} L. Kiss and S. O’Toole and Eiji Kambe and H. Ando and Hideyuki Izumiura and Bun’ei Sato and Michael Hartmann and A. P. Hatzes and Caroline Barban and Gabrielle Berthomieu and Eric Michel and Janine Provost and S. Turck-chi{\`e}ze and J. C. Lebrun and J{\'e}r{\^o}me Schmitt and J L Bertaux and Serena Benatti and Riccardo Claudi and Rosario Cosentino and S. Leccia and Soeren Frandsen and K. Brogaard and L. Glowienka and Frank Grundahl and Eric Stempels and Torben Arentoft and Mich{\"a}el Bazot and J{\o}rgen Christensen-Dalsgaard and Thomas H. Dall and Christoffer Karoff and J. Lundgreen-Nielsen and Fabien Carrier and Patrick Eggenberger and Danuta Sosnowska and Robert A. Wittenmyer and Michael Endl and Travis S. Metcalfe and Saskia Hekker and Sabine Reffert},
  journal={The Astrophysical Journal},
  year={2010},
  volume={713},
  pages={935-949}
}
We have analyzed data from a multi-site campaign to observe oscillations in the F5 star Procyon. The data consist of high-precision velocities that we obtained over more than three weeks with 11 telescopes. A new method for adjusting the data weights allows us to suppress the sidelobes in the power spectrum. Stacking the power spectrum in a so-called echelle diagram reveals two clear ridges, which we identify with even and odd values of the angular degree (l = 0 and 2, and l = 1 and 3… Expand
Solar-like Oscillations and Activity in Procyon: A Comparison of the 2007 MOST and Ground-based Radial Velocity Campaigns
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Hubble Space Telescope Astrometry of the Procyon System
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We have carried out a multisite campaign to measure oscillations in the F5 star Procyon A. We obtained high-precision velocity observations over more than three weeks with 11 telescopes, with almostExpand
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