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Items where Person is "Beaulieu-J-P"

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Number of items: 13.

2018

Bhattacharya, A. and Beaulieu, J.-P. and Bennett, D. P. et al. (2018) WFIRST Exoplanet Mass-measurement Method Finds a Planetary Mass of 39 ± 8 M_⊕ for OGLE-2012-BLG-0950Lb. Astronomical Journal, 156 (6). Art. No. 289. ISSN 1538-3881. https://resolver.caltech.edu/CaltechAUTHORS:20181130-095502884

Beaulieu, J.-P. and Batista, V. and Bennett, D. P. et al. (2018) Combining Spitzer Parallax and Keck II Adaptive Optics Imaging to Measure the Mass of a Solar-like Star Orbited by a Cold Gaseous Planet Discovered by Microlensing. Astronomical Journal, 155 (2). Art. No. 78. ISSN 1538-3881. https://resolver.caltech.edu/CaltechAUTHORS:20180201-112823289

2014

McDonald, I. and Kerins, E. and Penny, M. et al. (2014) ExELS: an exoplanet legacy science proposal for the ESA Euclid mission – II. Hot exoplanets and sub-stellar systems. Monthly Notices of the Royal Astronomical Society, 445 (4). pp. 4137-4154. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20150122-083653200

2012

Deroo, Pieter and Swain, Mark and Vasisht, Gautam et al. (2012) Exoplanet Spectroscopy: The Hubble Case. In: Molecules in the Atmospheres of Extrasolar Planets. Astronomical Society of the Pacific conference series. No.450. Astronomical Society of the Pacific , San Francisco, CA, pp. 63-66. ISBN 978-1-58381-782-7. https://resolver.caltech.edu/CaltechAUTHORS:20141217-093958592

2011

Barry, Richard and Kruk, Jeffery and Anderson, Jay et al. (2011) The exoplanet microlensing survey by the proposed WFIRST Observatory. In: Techniques and Instrumentation for Detection of Exoplanets V. Proceedings of SPIE. No.8151. Society of Photo-Optical Instrumentation Engineers , Bellingham, WA, Art. No. 81510L. ISBN 978-0-81948-761-2. https://resolver.caltech.edu/CaltechAUTHORS:20161028-150534809

Beaulieu, J. -P. and Tinetti, G. and Kipping, D. M. et al. (2011) Methane in the Atmosphere of the Transiting Hot Neptune GJ436B? Astrophysical Journal, 731 (1). Art. No. 16. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20110506-141703127

2010

Beaulieu, J. P. and Kipping, D. M. and Batista, V. et al. (2010) Water in the atmosphere of HD 209458b from 3.6–8 μm IRAC photometric observations in primary transit. Monthly Notices of the Royal Astronomical Society, 409 (3). pp. 963-974. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20110106-100201080

Sumi, T. and Bennett, D. P. and Bond, I. A. et al. (2010) A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common. Astrophysical Journal, 710 (2). pp. 1641-1653. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20100224-162757796

2009

Albrow, M. D. and Horne, K. and Bramich, D. M. et al. (2009) Difference imaging photometry of blended gravitational microlensing events with a numerical kernel. Monthly Notices of the Royal Astronomical Society, 397 (4). pp. 2099-2105. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20090909-095412081

Dong, Subo and Gould, Andrew and Udalski, Andrzej et al. (2009) OGLE-2005-BLG-071Lb, the Most Massive M Dwarf Planetary Companion? Astrophysical Journal, 695 (2). pp. 970-987. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20090821-084434959

Kains, N. and Cassan, A. and Horne, K. et al. (2009) A systematic fitting scheme for caustic-crossing microlensing events. Monthly Notices of the Royal Astronomical Society, 395 (2). pp. 787-796. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20090904-142928631

2008

Beaulieu, J. P. and Carey, S. and Ribas, I et al. (2008) Primary transit of the planet HD 189733b at 3.6 and 5.8 µm. Astrophysical Journal, 677 (2). pp. 1343-1347. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:BEAapj08

2007

Tinetti, Giovanna and Vidal-Madjar, Alfred and Liang, Mao-Chang et al. (2007) Water vapour in the atmosphere of a transiting extrasolar planet. Nature, 448 (7150). pp. 169-171. ISSN 0028-0836. https://resolver.caltech.edu/CaltechAUTHORS:20140724-161026901

This list was generated on Sat Oct 19 00:39:40 2019 PDT.