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Confirmation of Hot Jupiter Kepler-41b via Phase Curve Analysis

Quintana, Elisa V. and Rowe, Jason F. and Barclay, Thomas and Howell, Steve B. and Ciardi, David R. and Demory, Brice-Olivier and Caldwell, Douglas A. and Borucki, William J. and Christiansen, Jessie L. and Jenkins, Jon M. and Klaus, Todd C. and Fulton, Benjamin J. and Morris, Robert L. and Sanderfer, Dwight T. and Shporer, Avi and Smith, Jeffrey C. and Still, Martin and Thompson, Susan E. (2013) Confirmation of Hot Jupiter Kepler-41b via Phase Curve Analysis. Astrophysical Journal, 767 (2). Art. No. 137. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130521-150946275

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Abstract

We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity measurements. We have developed a new method to confirm giant planets solely from the photometric light curve, and we apply this method herein to Kepler-41 to establish the validity of this technique. We generate a full phase photometric model by including the primary and secondary transits, ellipsoidal variations, Doppler beaming, and reflected/emitted light from the planet. Third light contamination scenarios that can mimic a planetary transit signal are simulated by injecting a full range of dilution values into the model, and we re-fit each diluted light curve model to the light curve. The resulting constraints on the maximum occultation depth and stellar density combined with stellar evolution models rules out stellar blends and provides a measurement of the planet's mass, size, and temperature. We expect about two dozen Kepler giant planets can be confirmed via this method.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/767/2/137DOIArticle
http://iopscience.iop.org/0004-637X/767/2/137PublisherArticle
ORCID:
AuthorORCID
Rowe, Jason F.0000-0002-5904-1865
Barclay, Thomas0000-0001-7139-2724
Howell, Steve B.0000-0002-2532-2853
Ciardi, David R.0000-0002-5741-3047
Demory, Brice-Olivier0000-0002-9355-5165
Caldwell, Douglas A.0000-0003-1963-9616
Christiansen, Jessie L.0000-0002-8035-4778
Jenkins, Jon M.0000-0002-4715-9460
Fulton, Benjamin J.0000-0003-3504-5316
Shporer, Avi0000-0002-1836-3120
Thompson, Susan E.0000-0001-7106-4683
Additional Information:© 2013 American Astronomical Society. Received 2012 September 20; accepted 2013 March 3; published 2013 April 5. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. Some/all of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASANAS5-26555
NASANNX09AF08G
Subject Keywords:planetary systems; techniques: photometric
Issue or Number:2
Record Number:CaltechAUTHORS:20130521-150946275
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130521-150946275
Official Citation:Confirmation of Hot Jupiter Kepler-41b via Phase Curve Analysis Elisa V. Quintana, Jason F. Rowe, Thomas Barclay, Steve B. Howell, David R. Ciardi, Brice-Olivier Demory, Douglas A. Caldwell, William J. Borucki, Jessie L. Christiansen, Jon M. Jenkins, Todd C. Klaus, Benjamin J. Fulton, Robert L. Morris, Dwight T. Sanderfer, Avi Shporer, Jeffrey C. Smith, Martin Still, and Susan E. Thompson doi:10.1088/0004-637X/767/2/137
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:38620
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:21 May 2013 22:31
Last Modified:14 Oct 2019 23:33

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