Methane absorption coefficients for the jovian planets from laboratory, Huygens, and HST data

By E. Karkoschka, M. Tomasko. 2010

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/cd062ae0ce0c0e2f489ebfbaa8b740bf9e32a7f3

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. N. Madhusudhan
2. Jon Fortney
3. M. Marley
4. D. Deming
5. H. Knutson
6. A. Showman
7. Adam Burrows
8. Sara Seager

In Atmospheric Science

1. Jon Fortney
2. N. Madhusudhan
3. M. Marley
4. Kerri L. Cahoy
5. A. Mandell
6. Travis S. Barman
7. B. Macintosh
8. Q. Konopacky

Citations in the corpus

• SIMULTANEOUS DETECTION OF WATER, METHANE, AND CARBON MONOXIDE IN THE ATMOSPHERE OF EXOPLANET HR 8799 b (2015, methodology): “For this study, the grid of exoplanet atmospheres models described in B11 was updated to include the methane linelist from Yurchenko & Tennyson (2014) supplemented with optical opacities from Karkoschka & Tomasko (2010).”
• EXOPLANET ALBEDO SPECTRA AND COLORS AS A FUNCTION OF PLANET PHASE, SEPARATION, AND METALLICITY (2010, methodology): “We note that we have yet to incorporate the recent tabulation of methane opacities presented in Karkoschka & Tomasko (2010).”
• An Accurate, Extensive, and Practical Line List of Methane for the HITEMP Database (2020, unknown): “For the line positions beyond 12,000 cm−1, the accuracy of this work is known to be insufficient and differences are observed when compared to low-resolution absorption coefficient band models of (Karkoschka & Tomasko 2010).”
• SPECTROSCOPIC EVIDENCE FOR A TEMPERATURE INVERSION IN THE DAYSIDE ATMOSPHERE OF HOT JUPITER WASP-33b (2015, methodology): “Our molecular line lists are obtained from Freedman et al. (2008), Freedman (personal communication, 2009), Rothman (2005), Karkoschka & Tomasko (2010), and Karkoschka (personal communication, 2011).”
• C/O RATIO AS A DIMENSION FOR CHARACTERIZING EXOPLANETARY ATMOSPHERES (2012, methodology): “Our molecular line data are from Freedman et al. 2008, Freedman (personal communication, 2009), Rothman et al. (2005), Karkoschka & Tomasko (2010), and Karkoschka (personal communication, 2011), and Harris et al. (2008).”