CDSD-4000: High-resolution, high-temperature carbon dioxide spectroscopic databank

By S. Tashkun, V. Perevalov. 2011

260 citations recorded by the source corpus.

Subfields: Atmospheric Science, Global and Planetary Change, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/b8b6339db74b2cdb7d4085865cdca87b28cf1d9d

How researchers see this paper

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

In Atmospheric Science

1. Sergei N. Yurchenko
2. Jonathan Tennyson
3. Giovanna Tinetti
4. Ingo P. Waldmann
5. D. Sing
6. H. Wakeford
7. Laura K. McKemmish
8. Oleg L. Polyansky

In Global and Planetary Change

1. Sergei N. Yurchenko
2. J. Lustig-Yaeger
3. Z. Rustamkulov
4. Jonathan Tennyson

In Spectroscopy

1. Sergei N. Yurchenko
2. Jonathan Tennyson
3. Giovanna Tinetti
4. Ingo P. Waldmann
5. Laura K. McKemmish
6. Oleg L. Polyansky
7. D. Sing
8. H. Wakeford

Citations in the corpus

• The 2020 release of the ExoMol database: Molecular line lists for exoplanet and other hot atmospheres (2020, background): “[181, 182, 183] ExoMol CO2 1 4000 1 628 324 454 CSSD-4000 Tashkun and Perevalov [184] Empirical H2O 1 300 1 WAT UV296 [185] ExoMol Niso Number of isotopologues considered; Tmax Maximum temperature for which the line list is complete; Nelec Number of electronic states considered; Nlines Number of lin”
• High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations (2023, background): “The opacity contributions from these gases include line opacity (Tashkun & Perevalov 2011; Li et al. 2015; Yurchenko et al. 2017; Polyansky et al. 2018) and collision-induced absorption (CIA) from H2–H2, H2–N2, H2–CH4, H2–CO2, CO2–CO2, CO2–CH4, and N2–N2 (Karman et al. 2019).”
• ExoMol: molecular line lists for exoplanet and other atmospheres (2012, methodology): “The recent CDSD-4000 CO2 line list of Tashkun & Perevalov (2011) extended their earlier work, which was used in the 2010 edition of HITEMP (Rothman et al. 2010), to higher temperatures.”
• The ExoMol database: Molecular line lists for exoplanet and other hot atmospheres (2016, background): “[181, 182, 183] ExoMol CO2 1 4000 1 628 324 454 CSSD-4000 Tashkun and Perevalov [184] Empirical H2O 1 300 1 WAT UV296 [185] ExoMol Niso Number of isotopologues considered; Tmax Maximum temperature for which the line list is complete; Nelec Number of electronic states considered; Nlines Number of lin”