Mass loss from the exoplanet WASP-12b inferred from Spitzer phase curves
Taylor J. Bell(McGill University), Michael R. Line(Ames Research Center), Jonathan J. Fortney(University of California, Santa Cruz), Heather A. Knutson(California Institute of Technology), Ian J. M. Crossfield(Massachusetts Institute of Technology), Nicolas B. Cowan(Amherst College), Lisa Dang(McGill University), Kevin B. Stevenson(University of Chicago), Robert T. Zellem(Jet Propulsion Laboratory), Ian Dobbs‐Dixon(New York University Abu Dhabi), Patricio E. Cubillos(Austrian Academy of Sciences), L. Fossati(Austrian Academy of Sciences), Kamen Todorov(University of Amsterdam), Drake Deming(NASA Astrobiology Institute), Michael Zhang(California Institute of Technology)
Cited by 72
Related Papers
<i>SPITZER</i>SECONDARY ECLIPSES OF THE DENSE, MODESTLY-IRRADIATED, GIANT EXOPLANET HAT-P-$20{\rm b}$ USING PIXEL-LEVEL DECORRELATION
|The Astrophysical Journal|2015|283
An excess of massive stars in the local 30 Doradus starburst
|Science|2018|257
The spectroscopic Hertzsprung-Russell diagram of Galactic massive stars
|Astronomy and Astrophysics|2014|148
3.6 AND 4.5 μm SPITZER PHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b
|The Astrophysical Journal|2016|144