Published June 24, 2004
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OGLE-TR-56
Abstract
In early 2003 our team announced the discovery of the second extrasolar transiting planet, around the faint star OGLE-TR-56 (V = 16.6), based on the detection of small changes in the radial velocity of the primary. The star was originally identified as a candidate by the OGLE team from the shallow and periodic dips in its brightness. We present here new precise radial velocity measurements that confirm the variation measured earlier, supporting the conclusion that the companion is indeed a planet. Additional photometric observations are also available, which combined with the spectroscopy yield improved parameters (mass and radius) for the planet.
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© 2004 American Institute of Physics. Issue Date: June 24, 2004.Attached Files
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Additional details
- Eprint ID
- 9234
- Resolver ID
- CaltechAUTHORS:TORaipcp04
- Created
-
2007-11-28Created from EPrint's datestamp field
- Updated
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2021-11-08Created from EPrint's last_modified field
- Series Name
- AIP Conference Proceedings
- Series Volume or Issue Number
- 713