The Rossiter-McLaughlin Effect of the Transiting Exoplanet XO-4b
We report photometric and radial velocity observations of the XO-4 transiting planetary system, conducted with the FLWO 1.2 m telescope and the 8.2 m Subaru Telescope. Based on the new light curves, the refined transit ephemeris of XO-4b is $P$ $=$ 4.1250828$\ \pm\ $0.0000040 d and $T_{\rm c}$ [BJD$...
Main Authors: | Narita, Norio, Hirano, Teruyuki, Sanchis Ojeda, Roberto, Winn, Joshua Nathan, Holman, Matthew J., Sato, Bunei, Aoki, Wako, Tamura, Motohide |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics |
Format: | Article |
Language: | en_US |
Published: |
Astronomical Society of Japan
2012
|
Online Access: | http://hdl.handle.net/1721.1/73119 https://orcid.org/0000-0002-4265-047X |
Similar Items
-
Improved modeling of the Rossiter-McLaughlin effect for transiting exoplanets
by: Hirano, Teruyuki, et al.
Published: (2012) -
Improved Measurement of the Rossiter-McLaughlin Effect in the Exoplanetary System HD 17156
by: Winn, Joshua Nathan, et al.
Published: (2013) -
Analytic Description of the Rossiter-McLaughlin Effect for Transiting Exoplanets: Cross-Correlation Method and Comparison with Simulated Data
by: Hirano, Teruyuki, et al.
Published: (2011) -
The spin-orbit alignment of the transiting exoplanet WASP-3b from Rossiter-McLaughlin observations
by: Simpson, E, et al.
Published: (2010) -
Studying the atmosphere of HD 189733 b using the Rossiter-McLaughlin effect
by: Minsky, Charlotte(Charlotte L.)
Published: (2021)