Zobrazeno 1 - 10
of 34
pro vyhledávání: '"Pedro V. Sada"'
Autor:
F. Colas, Florent Deleflie, Felipe Braga-Ribas, J. Normand, Hiromi Hamanowa, Alain Klotz, Pascal Descamps, P. Vingerhoets, J. A. Farrell, L. Maquet, K. Archer, G. Dubos, Vishnu Reddy, T. Pauwels, Frédéric Vachier, A. Peyrot, Joe Pollock, F. Marchis, A. Leroy, Pedro V. Sada, Jérôme Berthier, Sylvain Bouley, J.-P. Teng-Chuen-Yu
Publikováno v:
Icarus
Icarus, Elsevier, 2020, ⟨10.1016/j.icarus.2020.113990⟩
Icarus, 2020, ⟨10.1016/j.icarus.2020.113990⟩
HAL
Icarus, Elsevier, 2020, ⟨10.1016/j.icarus.2020.113990⟩
Icarus, 2020, ⟨10.1016/j.icarus.2020.113990⟩
HAL
International audience; We publish a set of 16 light curves of mutual events inside the synchronous system of the Jupiter Trojan (617) Patroclus. Patroclus is th only binary system of the six target asteroids of the forthcoming NASA Discovery-class m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c74b5d2ba0b746c13726ed44931ba404
https://hal.archives-ouvertes.fr/hal-03023849
https://hal.archives-ouvertes.fr/hal-03023849
Autor:
Raul Michel, Enric Palle, S. Brown Sevilla, Sergio Velasco, Chiara Righi, Hans J. Deeg, A. La Camera, Mauricio Reyes-Ruiz, Lorenzo Cabona, Jorge Prieto-Arranz, Davide Ricci, S. Navarro-Meza, Ricardo Lopez-Valdivia, Silvano Tosi, N. Truant, Steven W. Peterson, L. Fox Machado, C. Ayala-Loera, Pedro V. Sada, F. G. Ramón-Fox
We present a photometric follow-up of transiting exoplanets HAT-P-3b and TrES-3b, observed by using several optical and near-infrared filters, with four small-class telescopes (D = 36--152cm) in the Northern Hemisphere. Two of the facilities present
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab5598c3718d9f9434e4deb7850cd106
http://hdl.handle.net/11383/2069609
http://hdl.handle.net/11383/2069609
Autor:
Flynn Haase, Kevin Bays, Brian Jackson, E. O'Gorman, Drake Deming, Steven W. Peterson, Alan Lundsford, Pedro V. Sada, Donald E. Jennings
Publikováno v:
The Astrophysical Journal. 720:L215-L218
We report recent ground-based photometry of the transiting super-Earth exoplanet GJ1214b at several wavelengths, including the infrared near 1.25 microns (J-band). We observed a J-band transit with the FLAMINGOS infrared imager and the 2.1-meter tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e3592f2ea5e36c65a9b1af8c955d7f68
https://doi.org/10.1088/2041-8205/720/2/l215
https://doi.org/10.1088/2041-8205/720/2/l215
Autor:
R. J. Boyle, Carrie M. Anderson, Amy A. Simon-Miller, Brigette E. Hesman, Pedro V. Sada, Richard K. Achterberg, Leigh N. Fletcher, Conor A. Nixon, Gordon L. Bjoraker, George H. McCabe, Donald E. Jennings
Publikováno v:
Icarus. 202:249-259
Hydrocarbons in the upper atmosphere of Saturn are known, from Voyager, ground-based, and early Cassini results, to vary in emission intensity with latitude. Of particular interest is the marked increase in hydrocarbon line intensity near the south p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d7af24124a87f7807d8761f6fdfa755c
https://doi.org/10.1016/j.icarus.2009.02.013
https://doi.org/10.1016/j.icarus.2009.02.013
Autor:
Conor A. Nixon, R. J. Boyle, Brigette E. Hesman, George H. McCabe, Allen Lunsford, Donald E. Jennings, Pedro V. Sada, Gordon L. Bjoraker, Paul N. Romani
Publikováno v:
The Journal of Physical Chemistry A. 113:11101-11106
The (12)C/(13)C abundance ratio in ethane in the atmosphere of Titan has been measured at 822 cm(-1) from high spectral resolution ground-based observations. The value, 89(8), coincides with the telluric standard and also agrees with the ratio seen i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af69460aee6a36246a1d831834fcdc7b
https://doi.org/10.1021/jp903637d
https://doi.org/10.1021/jp903637d
Publikováno v:
Icarus. 200:265-270
Highly accurate astrometric positions obtained from eclipses and occultations of planetary satellites are reported. These measurements may be used to test existing ephemerides, to improve upon them, and to fit system constants such as satellite masse
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b9ec59a0322183156e63da5a40e00912
https://doi.org/10.1016/j.icarus.2008.11.022
https://doi.org/10.1016/j.icarus.2008.11.022
Autor:
Gordon L. Bjoraker, Donald E. Jennings, R. J. Boyle, Pedro V. Sada, Paul N. Romani, George H. McCabe
Publikováno v:
Icarus. 198:420-434
Ethylene (C2H4) emission has been measured in the poles and equator of Jupiter. The 949 cm(sup -1) spectra were recorded with a high resolution spectrometer at the McMath-Pierce telescope at Kitt Peak in October-November 1998 and at the Infrared Tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92481e7462e7ee7ae5f2854963a7598d
https://doi.org/10.1016/j.icarus.2008.05.027
https://doi.org/10.1016/j.icarus.2008.05.027
Autor:
George H. McCabe, Pedro V. Sada, Donald E. Jennings, Thomas G. Moran, R. J. Boyle, L. Drake Deming
Publikováno v:
Solar Physics. 241:213-222
We present the first solar vector magnetogram constructed from measurements of infra-red Mg I 12.32-μm line spectra. Observations were made at the McMath-Pierce Telescope using the Celeste spectrometer/polarimeter. Zeeman-split Stokes line spectra w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::aff27bc14ac623fa9da141604b71da96
https://doi.org/10.1007/s11207-007-0271-1
https://doi.org/10.1007/s11207-007-0271-1
Publikováno v:
Scopus-Elsevier
An analysis of the optical flashes produced by Leonid meteoroids impacting the Moon in 1999 November is carried out in order to estimate the fraction of kinetic energy converted into radiation, the so-called luminous efficiency η. It is shown that t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0e0fd9c58e783085cdfd226ffceeef24
https://doi.org/10.1086/312914
https://doi.org/10.1086/312914
Publikováno v:
Icarus. 147:405-420
We present an analysis of new cloud motion measurements in Saturn's atmosphere from Voyager 1 and 2 images and define a nominal zonal wind velocity vs latitude profile for the cloud top level that can be used as reference for the upcoming Cassini mis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e417a83541623a28831ed96f9150fecd
https://doi.org/10.1006/icar.2000.6449
https://doi.org/10.1006/icar.2000.6449