Exoplanet Characterization and the Search for Life (2009)
Kasting, J., Traub, W., Roberge, A., Leger, A., Schwartz, A., Wooten, A., ...
Over 300 extrasolar planets (exoplanets) have been detected orbiting nearby stars. We now hope to conduct a census of all planets around nearby stars and to characterize their atmospheres and...
Titan's Prolific Propane: The Cassini CIRS Perspective (2009)
Nixon, C. A., Jennings, D. E., Bezard, B., Teanby, N. A., Irwin, P. G. J., ...
In this paper we select large spectral averages of data from the Cassini Composite Infrared Spectrometer (CIRS) obtained in limb-viewing mode at low latitudes (30S--30N), greatly increasing the path...
TandEM: Titan and Enceladus mission (2009)
Coustenis, A., Atreya, S. K., Balint, T., Brown, R. H., Dougherty, M. K., Ferri, F., ...
TandEM was proposed as an L-class (large) mission in response to ESA’s Cosmic Vision 2015–2025 Call, and accepted for further studies, with the goal of exploring Titan and Enceladus. The mission...
What makes a planet habitable? (2009)
Lammer, H, Bredehöft, J, Coustenis, A, Khodachenko, M, Kaltenegger, L, Grasset, O, ...
E. Gendron, A. Coustenis, P. Drossart, M. Combes, M. Hirtzig, F. Lacombe, ...
Abstract. The advent of the NAOS/CONICA adaptive optics system at the ESO Very Large Telescope recently gave us the opportunity to map the surface of Titan and to search for atmospheric variations at...
TandEM: Titan and Enceladus mission (2008)
Coustenis, A., Atreya, S. K., Balint, T., Brown, R. H., Dougherty, M. K., Ferri, F., ...
54 pages, 8 figures.-- In press.
Jacquinet-Husson, N, Scott, N.A., Chedin, N., Crépeau, A., Armante, R., Capelle, V., ...
The development of Gestion et Etude des Informations Spectroscopiques Atmospheriques (GEISA: Management and Study of Spectroscopic Information) was started over three decades at Laboratoire de...
Surfaces and atmospheres of the outer planets, their satellites and ring systems: Part IV (2008)
Coustenis, A., Atreya, S., Casavecchia, P., Castillo, J., Dutuit, O., Hussmann, H., ...
This special issue of PSS is composed of selected articles based on research, presented during several different planetary meetings in 2007, including the European Geosciences Union (EGU) meeting (in...
H. Rauer, A. Coustenis, T. Guillot, J. Schneider
A&A manuscript no. (will be inserted by hand later) Your thesaurus codes are:
RECENT APPLICATIONS AND FUTURE PROSPECTS OF METHANE SPECTROSCOPY TO THE ATMOSPHERE OF TITAN (2007)
Boudon, V., Coustenis, A., Lellouch, E., Drossart, P., Negrão, A., Griffith, C. A.
Author Institution: Institut Carnot de Bourgogne, UMR 5209 CNRS-Universite de Bourgogne, 9. Av. A. Savary, BP 47870, F-21078 Dijon Cedex, France; LESIA, Observatoire de Paris-Meudon, 5 Place Jules...
Solar system objects with the NACO Fabry-Perot and SINFONI (2007)
Hartung, M., Dumas, C., Herbst, T. M., Coustenis, A., Hirtzig, M., Adámkovics, M., ...
Evidence for a Polar Ethane Cloud on Titan (2006)
Griffith, C. A., Penteado, P., Rannou, P., Brown, R., Boudon, V., Baines, K. H., ...
Spectra from Cassini’s Visual and Infrared Mapping Spectrometer reveal the presence of a vast tropospheric cloud on Titan at latitudes 51- to 68- north and all longitudes observed (10- to 190-...
In situ measurements of the physical characteristics of Titan's environment (2005)
Fulchignoni, M., Ferri, F., Angrilli, F., Ball, A.J., Bar-Nun, A., Barucci, M.A., ...
On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and pressure profiles were poorly constrained...
Temperature variations in Titan's upper atmosphere: Impact on Cassini/Huygens (2005)
Kazeminejad, B., Lammer, H., Coustenis, A., Witasse, O., Fischer, G., Schwingenschuh, K., ...
Temperature variations of Titan's upper atmosphere due to the plasma interaction of the satellite with Saturn's magnetosphere and Titan's high altitude monomer haze particles can imply an offset of...
Rain, winds and haze during Huygens probe's descent to Titan's surface (2005)
Tomasko, M. G., Archinal, A., Becker, T., Bezard, B., Bushroe, M., Combes, M., ...
Temperature variations in Titan's upper atmosphere: Impact on Cassini/Huygens (2005)
Kazeminejad, B., Lammer, H., Coustenis, A., Witasse, O., Fischer, G., Schwingenschuh, K., ...
Temperature variations of Titan's upper atmosphere due to the plasma interaction of the satellite with Saturn's magnetosphere and Titan's high altitude monomer haze particles can imply an offset of...
Temperature variations in Titan's upper atmosphere: Impact on Cassini/Huygens (2005)
Kazeminejad, B., Lammer, H., Coustenis, A., Witasse, O., Fischer, G., Schwingenschuh, K., ...
Temperature variations of Titan's upper atmosphere due to the plasma interaction of the satellite with Saturn's magnetosphere and Titan's high altitude monomer haze particles can imply an offset of...
Observe Jupiter's atmosphere (2004)
Orton, G. S., Fisher, B., Barnard, L., Edberg, S., Martin, T., Spilker, L., ...
FOURIER TRANSFORM SPECTROSCOPY AT JUPITER AND SATURN (2004)
Jennings, D. E., Flasar, F. M., Bjoraker, G. L., Romani, P. N., Brasunas, J. C., Kunde, V. G., ...
Author Institution: NASA/Goddard Space Flight Center; Department of Astronomy, University of Maryland; Department of Astronomy, Space Science and Applications, Inc.; LESIA, CNRS-UMR8632, Observatoire...
Search For Exospheric Signatures From Transiting Planets (2003)
Iro, N., Coustenis, A., Moutou, C., Lajous, N., Mayor, M., Queloz, D.
We searched for spectral signatures from the exosphere of HD209458 in the UV and the near-IR with UVES and ISAAC at the VLT. We looked in particular for the helium absorption feature at 10 830 \AA...
Fulchignoni, M., Ferri, F., Angrilli, F., Bar-Nun, A., Barucci, M.A., Bianchini, G., ...
The Huygens Atmospheric Structure Instrument (HASI) is a multi-sensor package which has been designed to measure the physical quantities characterising the atmosphere of Titan during the Huygens...
Observations of planetary satellites with ISO (2002)
Coustenis, A., Encrenaz, T., Lellouch, E., Salama, A., Müller, T., Burgdorf, M. J., ...
Several observational programmes were conducted with ISO (Kessler et al., 1996) aiming at the investigation of the near- and far- infrared spectrum of the satellites of the giant planets. Thus,...
Search for an exosphere around 51 Pegasi B with ISO (2000)
Rauer, H., Bockelee-Morvan, D., Coustenis, A., Guillot, T., Schneider, J.
The detection of absorption features in spectra of 51 Peg obtained during transit of its planet would provide a first clue on the physical nature of the planet. We have searched for signatures of an...