Zobrazeno 1 - 6
of 6
pro vyhledávání: '"François Fressin"'
Publikováno v:
Astronomy & Astrophysics 2008
Each transiting planet discovered is characterized by 7 measurable quantities, that may or may not be linked together (planet mass, radius, orbital period, and star mass, radius, effective temperature, and metallicity). Correlations between planet ma
Externí odkaz:
http://arxiv.org/abs/0901.3083
Publikováno v:
Comptes Rendus. Physique
Comptes Rendus. Physique, Académie des sciences (Paris), 2005, 6, pp.1169-1175. ⟨10.1016/j.crhy.2005.12.001⟩
Comptes Rendus. Physique, Académie des sciences (Paris), 2005, 6, pp.1169-1175. ⟨10.1016/j.crhy.2005.12.001⟩
On-axis achromatic interfero-coronagraph. We present a new type of stellar interfero-coronagraph, the "CIAXE", which is a variant of the "AIC", the Achromatic Interfero-Coronagraph [3,4]. The CIAXE is characterized by a very simple, compact and fully
Autor:
François Fressin
How hot is Venus? Can you distinguish between a pulsar and a quasar? Is there a universe or a multiverse? Where do we fit into the infinitely grand scheme of things? How do we map the Cosmic Microwave Background? Most tantalizing of all: Is there any
Autor:
Jean-Michel Désert, David Charbonneau, Brice-Olivier Demory, Sarah Ballard, Joshua A. Carter, Jonathan J. Fortney, William D. Cochran, Michael Endl, Samuel N. Quinn, Howard T. Isaacson, François Fressin, Lars A. Buchhave, David W. Latham, Heather A. Knutson, Stephen T. Bryson, Guillermo Torres, Jason F. Rowe, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Douglas A. Caldwell, Jessie L. Christiansen, Drake Deming, Daniel C. Fabrycky, Eric B. Ford, Ronald L. Gilliland, Michaël Gillon, Michaël R. Haas, Jon M. Jenkins, Karen Kinemuchi, David Koch, Jack J. Lissauer, Philip Lucas, Fergal Mullally, Phillip J. MacQueen, Geoffrey W. Marcy, Dimitar D. Sasselov, Sara Seager, Martin Still, Peter Tenenbaum, Kamal Uddin, Joshua N. Winn
Publikováno v:
Désert, Jean-Michel; Charbonneau, David; Demory, Brice-Olivier; Ballard, Sarah; Carter, Joshua A.; Fortney, Jonathan J.; Cochran, William D.; Endl, Michael; Quinn, Samuel N.; Isaacson, Howard T.; Fressin, François; Buchhave, Lars A.; Latham, David W.; Knutson, Heather A.; Bryson, Stephen T.; Torres, Guillermo; Rowe, Jason F.; Batalha, Natalie M.; Borucki, William J.; Brown, Timothy M.; ... (2011). THE HOT-JUPITER KEPLER-17b: DISCOVERY, OBLIQUITY FROM STROBOSCOPIC STARSPOTS, AND ATMOSPHERIC CHARACTERIZATION. Astrophysical journal-supplement series, 197(1), p. 14. Institute of Physics Publishing IOP 10.1088/0067-0049/197/1/14
Prof. Winn via Mat Willmott
Prof. Winn via Mat Willmott
This paper reports the discovery and characterization of the transiting hot giant exoplanet Kepler-17b. The planet has an orbital period of 1.486 days, and radial velocity measurements from the Hobby-Eberly Telescope show a Doppler signal of 419.5[su
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d7b511564ddf7eea702601697441bcae
Autor:
Guillermo Torres, François Fressin, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Stephen T. Bryson, Lars A. Buchhave, David Charbonneau, David R. Ciardi, Edward W. Dunham, Daniel C. Fabrycky, Eric B. Ford, Thomas N. Gautier III, Ronald L. Gilliland, Matthew J. Holman, Steve B. Howell, Howard Isaacson, Jon M. Jenkins, David G. Koch, David W. Latham, Jack J. Lissauer, Geoffrey W. Marcy, David G. Monet, Andrej Prsa, Samuel N. Quinn, Darin Ragozzine, Jason F. Rowe, Dimitar D. Sasselov, Jason H. Steffen, William F. Welsh
Publikováno v:
The Astrophysical Journal. 727:24
Light curves from the Kepler Mission contain valuable information on the nature of the phenomena producing the transit-like signals. To assist in exploring the possibility that they are due to an astrophysical false positive, we describe a procedure
Autor:
Jean-Michel Désert, David Charbonneau, Guillermo Torres, François Fressin, Sarah Ballard, Stephen T. Bryson, Heather A. Knutson, Natalie M. Batalha, William J. Borucki, Timothy M. Brown, Drake Deming, Eric B. Ford, Jonathan J. Fortney, Ronald L. Gilliland, David W. Latham, Sara Seager
Publikováno v:
Astrophysical Journal; 5/1/2015, Vol. 804 Issue 1, p1-1, 1p