QUANTITATIVELY ASSESSING THE ROLE OF CLOUDS IN THE TRANSMISSION SPECTRUM OF GJ 1214b
Authors:
- Caroline V. MorleyCMCaroline V. Morley
- Jonathan J. FortneyJFJonathan J. Fortney
- Eliza M.-R. KemptonEKEliza M.-R. Kempton
- Mark S. MarleyMMMark S. Marley
- Channon VissherCVChannon Vissher
- Kevin ZahnleKZKevin Zahnle
- 30 August 2013
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 775 (1)
Abstract
No abstract availableAll Related Versions
This publication has 89 references indexed in Scilit:
- GJ 1214 reviewedAstronomy & Astrophysics, 2013
- CARBON-RICH GIANT PLANETS: ATMOSPHERIC CHEMISTRY, THERMAL INVERSIONS, SPECTRA, AND FORMATION CONDITIONSThe Astrophysical Journal, 2011
- DISEQUILIBRIUM CARBON, OXYGEN, AND NITROGEN CHEMISTRY IN THE ATMOSPHERES OF HD 189733b AND HD 209458bThe Astrophysical Journal, 2011
- HIGH-RESOLUTION, DIFFERENTIAL, NEAR-INFRARED TRANSMISSION SPECTROSCOPY OF GJ 1214bThe Astrophysical Journal, 2011
- BROADBAND TRANSMISSION SPECTROSCOPY OF THE SUPER-EARTH GJ 1214b SUGGESTS A LOW MEAN MOLECULAR WEIGHT ATMOSPHEREThe Astrophysical Journal, 2011
- THE NATURE OF THE ATMOSPHERE OF THE TRANSITING SUPER-EARTH GJ 1214bThe Astrophysical Journal Letters, 2010
- THE ATMOSPHERIC SIGNATURES OF SUPER-EARTHS: HOW TO DISTINGUISH BETWEEN HYDROGEN-RICH AND HYDROGEN-POOR ATMOSPHERESThe Astrophysical Journal, 2008
- Latitudinal Variations in Uranus' Vertical Cloud Structure from UKIRT UIST ObservationsThe Astrophysical Journal, 2007
- Subvisible CO2 ice clouds detected in the mesosphere of MarsIcarus, 2006
- Fresh Ammonia Ice Clouds in JupiterIcarus, 2002