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    The NOMAD spectrometer suite on ExoMars Trace Gas Orbiter: Data processing status after one year of observing the Red Planet

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    Authors
    Thomas, I.R.
    Vandaele, A.C.
    Aoki, S.
    Depiesse, C.
    Willame, Y.
    Erwin, J.
    Trompet, L.
    Villanueva, G.
    Liuzzi, G.
    Crismani, M.
    Lopez-Valverde, M.A.
    Bellucci, G.
    Oliva, F.
    Robert, S.
    Piccialli, A.
    Ristic, B.
    Queirolo, C.
    Daerden, F.
    Berkenbosch, S.
    Clairquin, R.
    Beeckman, B.
    Neefs, E.
    Mason, J.
    Patel, M.
    Lopez Moreno, J.J.
    the NOMAD Team
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    Discipline
    Physical sciences
    Audience
    Scientific
    Date
    2019
    Metadata
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    Description
    NOMAD is one of four scientific instruments on the ExoMars Trace Gas Orbiter. It consists of three spectrometers operating in the ultraviolet-visible and infrared [2]. The nominal science phase began in April 2018, almost exactly one year ago at the time of writing this abstract; and recently the first results of the TGO mission were published [1, 5]. Here we will describe the first results from the first year of NOMAD observations; with an emphasis on calibration and data processing, detailing the work that has been done so far, and improvements that will be made in future.
    Citation
    Thomas, I.R.; Vandaele, A.C.; Aoki, S.; Depiesse, C.; Willame, Y.; Erwin, J.; Trompet, L.; Villanueva, G.; Liuzzi, G.; Crismani, M.; Lopez-Valverde, M.A.; Bellucci, G.; Oliva, F.; Robert, S.; Piccialli, A.; Ristic, B.; Queirolo, C.; Daerden, F.; Berkenbosch, S.; Clairquin, R.; Beeckman, B.; Neefs, E.; Mason, J.; Patel, M.; Lopez Moreno, J.J.; the NOMAD Team (2019). The NOMAD spectrometer suite on ExoMars Trace Gas Orbiter: Data processing status after one year of observing the Red Planet. , EPSC-DPS Joint Meeting 2019, 15-20 September 2019, Geneva, Switzerland, Vol. 13, EPSC-DPS2019-477-1,
    Identifiers
    uri: https://orfeo.belnet.be/handle/internal/7496
    Type
    Conference
    Peer-Review
    No
    Language
    eng
    Links
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