Zobrazeno 1 - 10
of 139
pro vyhledávání: '"Vuitton, Véronique"'
Autor:
He, Chao, Radke, Michael, Moran, Sarah E., Horst, Sarah M., Lewis, Nikole K., Moses, Julianne I., Marley, Mark S., Batalha, Natasha E., Kempton, Eliza M. -R., Morley, Caroline V., Valenti, Jeff A., Vuitton, Veronique
JWST has begun its scientific mission, which includes the atmospheric characterization of transiting exoplanets. Some of the first exoplanets to be observed by JWST have equilibrium temperatures below 1000 K, which is a regime where photochemical haz
Externí odkaz:
http://arxiv.org/abs/2301.02745
Autor:
Moses, Julianne I., Brown, Zarah L., Koskinen, Tommi T., Fletcher, Leigh N., Serigano, Joseph, Guerlet, Sandrine, Moore, Luke, Waite Jr., J. Hunter, Ben-Jaffel, Lotfi, Galand, Marina, Chadney, Joshua M., Hörst, Sarah M., Sinclair, James A., Vuitton, Veronique, Müller-Wodarg, Ingo
During the Grand Finale stage of the Cassini mission, organic-rich ring material was discovered to be flowing into Saturn's equatorial upper atmosphere at a surprisingly large rate. Through a series of photochemical models, we have examined the conse
Externí odkaz:
http://arxiv.org/abs/2211.05253
Autor:
Moran, Sarah E., Hörst, Sarah M., He, Chao, Radke, Michael J., Sebree, Joshua A., Izenberg, Noam R., Vuitton, Véronique, Flandinet, Laurène, Orthous-Daunay, François-Régis, Wolters, Cédric
Triton is the largest moon of the Neptune system and possesses a thin nitrogen atmosphere with trace amounts of carbon monoxide and methane, making it of similar composition to that of the dwarf planet Pluto. Like Pluto and Saturn's moon Titan, Trito
Externí odkaz:
http://arxiv.org/abs/2112.11627
Autor:
Isa, Junko, Orthous-Daunay, François-régis, Beck, Pierre, Herd, Christopher D. K., Vuitton, Veronique, Flandinet, Laurène
Publikováno v:
ApJL 920 L39 (2021)
Biologically relevant abiotic extraterrestrial soluble organic matter (SOM) has been widely investigated to study the origin of life and the chemical evolution of protoplanetary disks. Synthesis of biologically relevant organics, in particular, seems
Externí odkaz:
http://arxiv.org/abs/2111.10004
Autor:
Rodriguez, Sébastien, Vinatier, Sandrine, Cordier, Daniel, Tobie, Gabriel, Achterberg, Richard K., Anderson, Carrie M., Badman, Sarah V., Barnes, Jason W., Barth, Erika L., Bézard, Bruno, Carrasco, Nathalie, Charnay, Benjamin, Clark, Roger N., Coll, Patrice, Cornet, Thomas, Coustenis, Athena, Couturier-Tamburelli, Isabelle, Dobrijevic, Michel, Flasar, F. Michael, de Kok, Remco, Freissinet, Caroline, Galand, Marina, Gautier, Thomas, Geppert, Wolf D., Griffith, Caitlin A., Gudipati, Murthy S., Hadid, Lina Z., Hayes, Alexander G., Hendrix, Amanda R., Jauman, Ralf, Jennings, Donald E., Jolly, Antoine, Kalousova, Klara, Koskinen, Tommi T., Lavvas, Panayotis, Lebonnois, Sébastien, Lebreton, Jean-Pierre, Gall, Alice Le, Lellouch, Emmanuel, Mouélic, Stéphane Le, Lopes, Rosaly M. C., Lora, Juan M., Lorenz, Ralph D., Lucas, Antoine, MacKenzie, Shannon, Malaska, Michael J., Mandt, Kathleen, Mastrogiuseppe, Marco, Newman, Claire E., Nixon, Conor A., Radebaugh, Jani, Rafkin, Scot C., Rannou, Pascal, Sciamma-O-Brien, Ella M., Soderblom, Jason M., Solomonidou, Anezina, Sotin, Christophe, Stephan, Katrin, Strobel, Darrell, Szopa, Cyril, Teanby, Nicholas A., Turtle, Elizabeth P., Vuitton, Véronique, West, Robert A.
In response to ESA Voyage 2050 announcement of opportunity, we propose an ambitious L-class mission to explore one of the most exciting bodies in the Solar System, Saturn largest moon Titan. Titan, a "world with two oceans", is an organic-rich body w
Externí odkaz:
http://arxiv.org/abs/2110.10466
Autor:
Yu, Xinting, He, Chao, Zhang, Xi, Hörst, Sarah M., Dymont, Austin H., McGuiggan, Patricia, Moses, Julianne I., Lewis, Nikole K., Fortney, Jonathan J., Gao, Peter, Kempton, Eliza M. -R., Moran, Sarah E., Morley, Caroline V., Powell, Diana, Valenti, Jeff A., Vuitton, Véronique
Photochemical hazes are important opacity sources in temperate exoplanet atmospheres, hindering current observations from characterizing exoplanet atmospheric compositions. The haziness of an atmosphere is determined by the balance between haze produ
Externí odkaz:
http://arxiv.org/abs/2107.07069
Autor:
Furusho, Aogu, Ishii, Chiharu, Akita, Takeyuki, Oyaide, Mai, Mita, Masashi, Naraoka, Hiroshi, Takano, Yoshinori, Dworkin, Jason P., Oba, Yasuhiro, Koga, Toshiki, Fukushima, Kazuhiko, Aoki, Dan, Hashiguchi, Minako, Mita, Hajime, Chikaraishi, Yoshito, Ohkouchi, Naohiko, Ogawa, Nanako O., Sakai, Saburo, Glavin, Daniel P., Elsila, Jamie E., Parker, Eric T., Aponte, José C., McLain, Hannah L., Orthous-Daunay, Francois-Regis, Vuitton, Véronique, Thissen, Roland, Wolters, Cédric, Schmitt-Kopplin, Philippe, Ruf, Alexander, Isa, Junko, Hertkorn, Norbert, Eiler, John M., Yoshimura, Toshihiro, Sugahara, Haruna, Graham, Heather V., Furukawa, Yoshihiro, Araoka, Daisuke, Tanaka, Satoru, Yoshikawa, Takaaki, Kabashima, Fumie, Sasaki, Kazunori, Sato, Hajime, Yamazaki, Tomoya, Onose, Morihiko, Morita, Mayu, Kimura, Yuki, Kano, Kuniyuki, Aoki, Junken, Fujishima, Kosuke, Nomura, Shin-ichiro, Tachibana, Shogo, Nakamura, Tomoki, Noguchi, Takaaki, Okazaki, Ryuji, Yabuta, Hikaru, Yurimoto, Hisayoshi, Sakamoto, Kanako, Yada, Toru, Nishimura, Masahiro, Nakato, Aiko, Miyazaki, Akiko, Yogata, Kasumi, Abe, Masanao, Usui, Tomohiro, Yoshikawa, Makoto, Saiki, Takanao, Tanaka, Satoshi, Terui, Fuyuto, Nakazawa, Satoru, Okada, Tatsuaki, Watanabe, Sei-ichiro, Tsuda, Yuichi, Hamase, Kenji
Publikováno v:
In Journal of Chromatography Open May 2024 5
Autor:
Haythornthwaite, Richard P., Coates, Andrew J., Jones, Geraint H., Wellbrock, Anne, Waite, J. Hunter, Vuitton, Veronique, Lavvas, Panayotis
Titan's ionosphere contains a plethora of hydrocarbons and nitrile cations and anions as measured by the Ion Neutral Mass Spectrometer and Cassini Plasma Spectrometer (CAPS) onboard the Cassini spacecraft. Data from the CAPS Ion Beam Spectrometer (IB
Externí odkaz:
http://arxiv.org/abs/2009.08749
Autor:
He, Chao, Horst, Sarah M., Lewis, Nikole K., Yu, Xinting, Moses, Julianne I., McGuiggan, Patricia, Marley, Mark S., Kempton, Eliza M. -R., Morley, Caroline V., Valenti, Jeff A., Vuitton, Veronique
New observing capabilities coming online over the next few years will provide opportunities for characterization of exoplanet atmospheres. However, clouds/hazes could be present in the atmospheres of many exoplanets, muting the amplitude of spectral
Externí odkaz:
http://arxiv.org/abs/2008.09700
Autor:
Nixon, Conor A., Abshire, James, Ashton, Andrew, Barnes, Jason W., Carrasco, Nathalie, Choukroun, Mathieu, Coustenis, Athena, Couston, Louis-Alexandre, Edberg, Niklas, Gagnon, Alexander, Hofgartner, Jason D., Iess, Luciano, Mouélic, Stéphane Le, Lopes, Rosaly, Lora, Juan, Lorenz, Ralph D., Luspay-Kuti, Adrienn, Malaska, Michael, Mandt, Kathleen, Mastrogiuseppe, Marco, Mazarico, Erwan, Neveu, Marc, Perron, Taylor, Radebaugh, Jani, Rodriguez, Sébastien, Salama, Farid, Schoenfeld, Ashley, Soderblom, Jason M., Solomonidou, Anezina, Snowden, Darci, Sun, Xioali, Teanby, Nicholas, Tobie, Gabriel, Trainer, Melissa G., Tucker, Orenthal J., Turtle, Elizabeth P., Vinatier, Sandrine, Vuitton, Véronique, Zhang, Xi
We outline a flagship-class mission concept focused on studying Titan as a global system, with particular emphasis on the polar regions. Investigating Titan from the unique standpoint of a polar orbit would enable comprehensive global maps to uncover
Externí odkaz:
http://arxiv.org/abs/2008.05680