Mathieu Hirtzig

Affiliations: 
Paris-Sud XI University, Orsay, Essonne, France 
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"Mathieu Hirtzig"

Parents

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Athéna Coustenis grad student 2005 Paris-Sud University
 (Etude de Titan dans l'infrarouge proche par spectro-imagerie couplée à l'optique adaptative)
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Publications

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Rodriguez S, Le Mouélic S, Barnes JW, et al. (2018) Observational evidence for active dust storms on Titan at equinox Nature Geoscience. 11: 727-732
Brossier JF, Rodriguez S, Cornet T, et al. (2018) Geological Evolution of Titan's Equatorial Regions: Possible Nature and Origin of the Dune Material Journal of Geophysical Research: Planets. 123: 1089-1112
Solomonidou A, Coustenis A, Lopes RMC, et al. (2018) The Spectral Nature of Titan's Major Geomorphological Units: Constraints on Surface Composition Journal of Geophysical Research: Planets. 123: 489-507
Solomonidou A, Coustenis A, Hirtzig M, et al. (2014) Temporal variations of Titan's surface with Cassini/VIMS Icarus
Solomonidou A, Hirtzig M, Coustenis A, et al. (2014) Surface albedo spectral properties of geologically interesting areas on Titan Journal of Geophysical Research E: Planets. 119: 1729-1747
Solomonidou A, Bampasidis G, Hirtzig M, et al. (2013) Morphotectonic features on Titan and their possible origin Planetary and Space Science. 77: 104-117
Hirtzig M, Bézard B, Lellouch E, et al. (2013) Corrigendum to “Titan’s surface and atmosphere from Cassini/VIMS data with updated methane opacity” [Icarus 226 (2013) 470–486] Icarus. 226: 1182-1182
Hirtzig M, Bézard B, Lellouch E, et al. (2013) Titan's surface and atmosphere from Cassini/VIMS data with updated methane opacity Icarus. 226: 470-486
Bergh Cd, Courtin R, Bézard B, et al. (2012) Applications of a new set of methane line parameters to the modeling of Titan’s spectrum in the 1.58 μm window Planetary and Space Science. 61: 85-98
Campargue A, Wang L, Mondelain D, et al. (2012) An empirical line list for methane in the 1.26–1.71 μm region for planetary investigations (T = 80–300 K). Application to Titan Icarus. 219: 110-128
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