J/A+A/609/A34       VUV absorption cross section of CO_2_         (Venot+, 2018)
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VUV-absorption cross section of carbon dioxide from 150 to 800 K and
applications to warm exoplanetary atmospheres.
    Venot O., Benilan Y., Fray N., Gazeau M.-C., Lefevre F., Es-sebbar Et.,
    Hebrard E., Schwell M., Bahrini C., Montmessin F., Lefevre M., Waldmann I.P.
    <Astron. Astrophys. 609, A34 (2018)>
    =2018A&A...609A..34V        (SIMBAD/NED BibCode)
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ADC_Keywords: Atomic physics ; Spectra, ultraviolet
Keywords: molecular data - methods: laboratory: molecular -
          planets and satellites: atmospheres

Abstract:
    We quantify the temperature dependency of the VUV absorption cross
    section of carbon dioxide. The VUV absorption cross section of CO_2_
    increases with the temperature. The absorption we measured at 150K
    seems to be close to the absorption of CO_2_ in the fundamental ground
    state. The absorption cross section can be separated in two parts: a
    continuum and a fine structure superimposed on the continuum. The
    variation of the continuum of absorption can be represented by the sum
    of three gaussian functions. We used these data in our 1D
    thermo-photochemical model in order to study their impact on the
    predicted atmospheric composition of warm exoplanets. Using data at
    high temperature in thermo-photochemical models modifies significantly
    the abundance and the photodissociation rates of many species, in
    addition to carbon dioxide, such as methane and ammonia. These
    deviations have an impact on synthetic transmission spectra, leading
    to variations of up to 5ppm.

Description:
    We performed experimental measurements of CO_2_ absorption cross
    section with synchrotron radiation for the wavelength range
    (115-200nm). For longer wavelengths (195-230nm), we used a deuterium
    lamp and a 1.5m Jobin-Yvon spectrometer. We present a full set of
    high resolution ({Delta}{lambda}=0.03nm) absorption cross sections
    of CO_2_ from 115 to 230nm for temperatures ranging from 150 to 800K.

File Summary:
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 FileName      Lrecl  Records   Explanations
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ReadMe            80        .   This file
co2_150k.dat      22     1985   Absorption cross section of CO_2_ at 150K
co2_170k.dat      22     2154   Absorption cross section of CO_2_ at 170K
co2_195k.dat      22     2345   Absorption cross section of CO_2_ at 195K
co2_230k.dat      22     2367   Absorption cross section of CO_2_ at 230K
co2_300k.dat      22     2167   Absorption cross section of CO_2_ at 300K
co2_420k.dat      22     2040   Absorption cross section of CO_2_ at 420K
co2_500k.dat      22     2101   Absorption cross section of CO_2_ at 500K
co2_585k.dat      22     3031   Absorption cross section of CO_2_ at 585K
co2_700k.dat      22     3127   Absorption cross section of CO_2_ at 700K
co2_800k.dat      22     3394   Absorption cross section of CO_2_ at 800K
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Byte-by-byte Description of file: co2*.dat
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   Bytes Format Units   Label     Explanations
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   1-  9  F9.5  nm      lambda    [114/230] Wavelength
  12- 22  E11.5 cm2     CS        Absorption cross section
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Acknowledgements:
     Olivia Venot, olivia.venot(at)lisa.u-pec.fr

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(End)      Olivia Venot [LISA, France], Patricia Vannier [CDS]       26-Sep-2017
