The 2003 edition of the GEISA/IASI spectroscopic database

By N. Jacquinet-Husson, N. Scott, A. Chédin, K. Garceran, R. Armante, A. A. Chursin, A. Barbe, M. Birk, L. Brown, C. Camy‐Peyret and 32 more. 2005

180 citations recorded by the source corpus.

Subfields: Atmospheric Science, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/b26782807bbb4981fe8e8fc0e5488c7f71ac74c0

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In Atmospheric Science

1. Adam Burrows
2. C. Sharp
3. M. Marley
4. D. Spiegel
5. Jon Fortney
6. N. Madhusudhan
7. K. Lodders
8. R. Freedman

In Spectroscopy

1. Adam Burrows
2. M. Marley
3. Jonathan Tennyson
4. Sergei N. Yurchenko
5. K. Lodders
6. R. Freedman
7. Jon Fortney

Citations in the corpus

• Atomic and Molecular Opacities for Brown Dwarf and Giant Planet Atmospheres (2006, methodology): “This is in addition to those in the latest versions of HITRAN (Rothman et al. 2005) and GEISA (Jacquinet-Husson et al. 2005).”
• Chemical abundance analysis of the open clusters Cr 110, NGC 2099 (M 37), NGC 2420, NGC 7789, and M 67 (NGC 2682) (2009, methodology): “…laborat ry wavelengths of the H2O absorption bands around 5800, 6500, 7000, 7200, 8000 and 8900 Å and of the O2 absorption bands around 6300, 6900 and 7600 Å were obtained from the GEISA5 database (Jacquinet-Husson et al., 1999, 2005) and we measured their radial velocity in our programme stars.”
• The GEISA spectroscopic database: Current and future archive for Earth and planetary atmosphere studies (2008, unknown): “For each molecule listed in column 1, coded index of quality have been given (from conclusions of IASI/ISSWG working group [6]) for the spectroscopic parameters of columns 2–7, if applicable, as the following: ‘‘1’’ parameters that need to be improved; ‘‘2’’ and ‘‘3’’ second and third priority for i”
• Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission I. Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles (2010, methodology): “Spectroscopic parameters of CH4, CH3D, C2H2, C2H4, C3H8, and CO2 were extracted from GEISA 2003 database (Jacquinet-Husson et al., 2005). We applied a scaling factor of 0.420 to the intensities of the C3H8 lines in GEISA 2003 as explained in Nixon et al. (2009). For all transitions, we adopted a Lor”