Zobrazeno 1 - 10
of 73
pro vyhledávání: '"Collier Cameron, Andrew"'
Autor:
Billot, Nicolas, Hellmich, Stephan, Benz, Willy, Fortier, Andrea, Ehrenreich, David, Broeg, Christopher, Heitzmann, Alexis, Bekkelien, Anja, Brandeker, Alexis, Alibert, Yann, Alonso, Roi, Bárczy, Tamas, Barrado Navascues, David, Barros, Susana C.C., Baumjohann, Wolfgang, Biondi, Federico, Borsato, Luca, Collier Cameron, Andrew, Corral van Damme, Carlos, Correia, Alexandre C.M., Csizmadia, Szilard, Cubillos, Patricio E., Davies, Melvyn B., Deleuil, Magali, Deline, Adrien, Demangeon, Olivier D.S., Demory, Brice-Olivier, Derekas, Aliz, Edwards, Billy, Egger, Jo Ann, Erikson, Anders, Fossati, Luca, Fridlund, Malcolm, Gandolfi, Davide, Gazeas, Kosmas, Gillon, Michaël, Güdel, Manuel, Günther, Maximilian N., Helling, Ch., Isaak, Kate G., Kiss, Laszlo L., Korth, Judith, Lam, Kristine W.F., Laskar, Jacques, Lecavelier des Etangs, Alain, Lendl, Monika, Magrin, Demetrio, Maxted, Pierre F.L., Mecina, Marko, Merín, Bruno, Mordasini, Christoph, Nascimbeni, Valerio, Olofsson, Göran, Ottensamer, Roland, Pagano, Isabella, Pallé, Enric, Peter, Gisbert, Piazza, Daniele, Piotto, Giampaolo, Pollacco, Don, Queloz, Didier, Ragazzoni, Roberto, Rando, Nicola, Rauer, Heike, Ribas, Ignasi, Rieder, Martin, Santos, Nuno C., Scandariato, Gaetano, Ségransan, Damien, Simon, Attila E., Smith, Alexis M.S., Sousa, Sérgio G., Stalport, Manu, Sulis, Sophia, Szabó, Gyula M., Udry, Stéphane, Ulmer, Bernd, Ulmer-Moll, Solène, Van Grootel, Valérie, Venturini, Julia, Villaver, Eva, Walton, Nicholas A., Wilson, Thomas G.
Publikováno v:
In The Journal of Space Safety Engineering September 2024 11(3):498-506
Autor:
Gill, Samuel, Bayliss, Daniel, Cooke, Benjamin F., Wheatley, Peter J., Nielsen, Louise D., Lendl, Monika, McCormac, James, Bryant, Edward M., Acton, Jack S., Anderson, David R., Belardi, Claudia, Bouchy, Francois, Burleigh, Matthew R., Collier-Cameron, Andrew, Casewell, Sarah L., Goad, Michael R., Gunther, Maximilian N., Hellier, Coel, Jackman, James A. G., Jenkins, James S., Moyano, Maximiliano, Pollacco, Don, Raynard, Liam, Smith, Alexis M. S., Tilbrook, Rosanna H., Turner, Oliver, Udry, Stephane, West, Richard G.
The Transiting Exoplanet Survey Satellite (\tess) produces a large number of single-transit event candidates, since the mission monitors most stars for only $\sim$27\,days. Such candidates correspond to long-period planets or eclipsing binaries. Usin
Externí odkaz:
http://arxiv.org/abs/1910.05282
Publikováno v:
Monthly Notices of the Royal Astronomical Society; Oct2024, Vol. 534 Issue 1, p843-851, 9p
Autor:
Otor, Oderah Justin, Montet, Benjamin T., Johnson, John Asher, Charbonneau, David, Collier-Cameron, Andrew, Howard, Andrew W., Isaacson, Howard, Latham, David W., Lopez-Morales, Mercedes, Lovis, Christophe, Mayor, Michel, Micela, Giusi, Molinari, Emilio, Pepe, Francesco, Piotto, Giampaolo, Phillips, David F., Queloz, Didier, Rice, Ken, Sasselov, Dimitar, Ségransan, Damien, Sozzetti, Alessandro, Udry, Stéphane, Watson, Chris
While the vast majority of multiple-planet systems have their orbital angular momentum axes aligned with the spin axis of their host star, Kepler-56 is an exception: its two transiting planets are coplanar yet misaligned by at least 40 degrees with r
Externí odkaz:
http://arxiv.org/abs/1608.03627
Autor:
Plavchan, Peter, Latham, Dave, Gaudi, Scott, Crepp, Justin, Dumusque, Xavier, Furesz, Gabor, Vanderburg, Andrew, Blake, Cullen, Fischer, Debra, Prato, Lisa, White, Russel, Makarov, Valeri, Marcy, Geoff, Stapelfeldt, Karl, Haywood, Raphaëlle, Collier-Cameron, Andrew, Quirrenbach, Andreas, Mahadevan, Suvrath, Anglada, Guillem, Muirhead, Philip
[Abridged] The Study Analysis Group 8 of the NASA Exoplanet Analysis Group was convened to assess the current capabilities and the future potential of the precise radial velocity (PRV) method to advance the NASA goal to "search for planetary bodies a
Externí odkaz:
http://arxiv.org/abs/1503.01770
Autor:
Madhusudhan, Nikku, Harrington, Joseph, Stevenson, Kevin B., Nymeyer, Sarah, Campo, Christopher J., Wheatley, Peter J., Deming, Drake, Blecic, Jasmina, Hardy, Ryan A., Lust, Nate B., Anderson, David R., Collier-Cameron, Andrew, Britt, Christopher B. T., Bowman, William C., Hebb, Leslie, Hellier, Coel, Maxted, Pierre F. L., Pollacco, Don, West, Richard G.
The carbon-to-oxygen ratio (C/O) in a planet provides critical information about its primordial origins and subsequent evolution. A primordial C/O greater than 0.8 causes a carbide-dominated interior as opposed to a silicate-dominated composition as
Externí odkaz:
http://arxiv.org/abs/1012.1603
Autor:
Nymeyer, Sarah, Harrington, Joseph, Hardy, Ryan A., Stevenson, Kevin B., Campo, Christopher J., Madhusudhan, Nikku, Collier-Cameron, Andrew, Loredo, Thomas J., Blecic, Jasmina, Bowman, William C., Britt, Christopher B. T., Cubillos, Patricio, Hellier, Coel, Gillon, Michael, Maxted, Pierre F. L., Hebb, Leslie, Wheatley, Peter J., Pollacco, Don, Anderson, David R.
Publikováno v:
2011 ApJ 742 35
The transiting exoplanet WASP-18b was discovered in 2008 by the Wide Angle Search for Planets (WASP) project. The Spitzer Exoplanet Target of Opportunity Program observed secondary eclipses of WASP-18b using Spitzer's Infrared Array Camera (IRAC) in
Externí odkaz:
http://arxiv.org/abs/1005.1017
Autor:
Campo, Christopher J., Harrington, Joseph, Hardy, Ryan A., Stevenson, Kevin B., Nymeyer, Sarah, Ragozzine, Darin, Lust, Nate B., Anderson, David R., Collier-Cameron, Andrew, Blecic, Jasmina, Britt, Christopher B. T., Bowman, William C., Wheatley, Peter J., Loredo, Thomas J., Deming, Drake, Hebb, Leslie, Hellier, Coel, Maxted, Pierre F. L., Pollaco, Don, West, Richard G.
We observed two secondary eclipses of the exoplanet WASP-12b using the Infrared Array Camera on the Spitzer Space Telescope. The close proximity of WASP-12b to its G-type star results in extreme tidal forces capable of inducing apsidal precession wit
Externí odkaz:
http://arxiv.org/abs/1003.2763
We present statistically robust observational evidence which imposes new limits on dynamo saturation in young solar-type stars. These are inferred from the increasing amplitude of the V-band optical flux with rotation, caused by the filling of the di
Externí odkaz:
http://arxiv.org/abs/astro-ph/9409023
Publikováno v:
Mon.Not.Roy.Astron.Soc. 265 (1993) 983
We present a new technique for estimating the distance to young open clusters. The method requires accurate measurement of the axial rotation period of late-type members of the cluster: rotation periods are first combined with projected rotation velo
Externí odkaz:
http://arxiv.org/abs/astro-ph/9310035