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Characteristics of planetary candidates observed by Kepler II : Analysis of the first four months of data
Borucki, W.J.; Koch, D.G.; Basri, G.; Batalha, N.; Brown, T.M.; Bryson, S.T.; Caldwell, T.; Christensen-Dalsgaard, J.; Cochran, W.D.; DeVore, E.; Dunham, E.W.; Gautier, T.N.; Geary, J.C.; Gilliland, R.; Gould, A.; Howell, S.B.; Jenkins, J.M.; Latham, D.W.; Lissauer, J.J.; Marcy, G.W.; Rowe, J.; Sasselov, D.; Boss, A.; Charbonneau, D.; Ciardi, D.; Doyle, L.; Dupree, A.K.; Ford, E.B.; Fortney, J.; Holman, M.J.; Seager, S.; Steffen, J.H.; Tarter, J.; Welsh, W.F.; Allen, C.; Buchhave, L.A.; Christiansen, J.L.; Clarke, B.D.; Das, S.; Desert, J.M.; Endl, M.; Fabrycky, D.; Fressin, F.; Haas, M.; Horch, E.; Howard, A.; Isaacson, H.; Kjeldsen, H.; Kolodziejczak, J.; Kulesa, C.; Li, J.; Lucas, P.W.; Machalek, P.; McCarthy, D.; MacQueen, P.; Meibom, S.; Miquel, T.; Prsa, A.; Quinn, S.N.; Quintana, E.V.; Ragozzine, D.; Sherry, W.; Shpora, A.; Tenenbaum, P.; Torres, G.; Twicken, J.D.; Van Cleve, J.; Walkowicz, L.; Witteborn, F.C.; Still, M. (2011)On 2011 February 1 the Kepler mission released data for 156,453 stars observed from the beginning of the science observations on 2009 May 2 through September 16. There are 1235 planetary candidates with transit-like ... -
Discovery and atmospheric characterization of giant planet Kepler-12b : An inflated radius outlier
Fortney, J.J.; Nutzman, P.; Miller, N.; Demory, B.-O.; Seager, S.; Désert, J.-M.; Buchhave, L.A.; Charbonneau, D.; Fressin, F.; Latham, D.W.; Geary, J.C.; Rowe, J.; Caldwell, D.A.; Jenkins, J.M.; Christiansen, J.L.; Marcy, G.W.; Isaacson, H.; Howard, A.; Knutson, H.A.; Buchhave, L.A.; Ciardi, D.; Gautier, T.N.; Batalha, N.M.; Bryson, S.T.; Howell, S.B.; Borucki, W.J.; Koch, D.; Lissauer, J.J.; Haas, M.R.; Everett, M.; Deming, D.; Brown, T.M.; Ford, E.B.; Gilliland, R.L.; Fischer, D.A.; Still, M.; Lucas, P.W.; Gillon, M. (2011-11-01)We report the discovery of planet Kepler-12b (KOI-20), which at 1.695 ± 0.030 R is among the handful of planets with super-inflated radii above 1.65 R. Orbiting its slightly evolved G0 host with a 4.438 day period, this ... -
Kepler-15b : A hot Jupiter enriched in heavy elements and the first Kepler mission planet confirmed with the Hobby-Eberly Telescope
Endl, M.; MacQueen, P.J.; Cochran, W.D.; Brugamyer, E.J.; Buchhave, L.A.; Rowe, J.; Lucas, P.W.; Isaacson, H.; Bryson, S.; Howell, S.B.; Borucki, W.J.; Caldwell, D.; Christiansen, J.L.; Haas, M.R.; Koch, D.J.; Lissauer, J.J.; Still, M.; Fortney, J.J.; Hansen, T.; Ciardi, D.R.; Demory, B.-O.; Everett, M.; Ford, E.B.; Holman, M.J.; Horch, E.; Jenkins, J.M.; Sanderfer, D.T.; Seader, S.E.; Smith, J.C.; Thompson, S.E.; Twicken, J.D.; MacHalek, P.; Welsh, W.F. (2011-11-01)We report the discovery of Kepler-15b (KOI-128), a new transiting exoplanet detected by NASA's Kepler mission. The transit signal with a period of 4.94days was detected in the quarter 1 (Q1) Kepler photometry. For the first ... -
Kepler-18b, c, and d : A system of three planets confirmed by transit timing variations, light curve validation, Warm-Spitzer photometry, and radial velocity measurements
Cochran, W.D.; MacQueen, P.J.; Endl, M.; Fabrycky, D.C.; Fortney, J.J.; Miller, N.; Torres, G.; Fressin, F.; Désert, J.-M.; Ragozzine, D.; Sasselov, D.; Carter, J.A.; Quinn, S.N.; Latham, D.W.; Holman, M.J.; Charbonneau, D.; Rowe, J.F.; Bryson, S.T.; Howell, S.B.; Borucki, W.J.; Koch, D.G.; Uddin, K.; Tenenbaum, P.; Still, M.; Mullally, F.; Lissauer, J.J.; Kinemuchi, K.; Jenkins, J.M.; Henze, C.E.; Haas, M.R.; Caldwell, D.; Brugamyer, E.J.; Ciardi, D.R.; Steffen, J.H.; Winn, J.N.; Seager, S.; Demory, B.-O.; Welsh, W.F.; Uddin, K.; Tenenbaum, P.; Mullally, F.; Jenkins, J.M.; Caldwell, D.; Still, M.; Kinemuchi, K.; Marcy, G.W.; Knutson, H.; Isaacson, H.; Howard, A.; Lucas, P.W.; Johnson, J.A.; Horch, E.; Gilliland, R.L.; Gautier, T.N.; Ford, E.B.; Fischer, D.A.; Everett, M.; Deming, D.; Buchhave, L.; Brown, T.M.; Batalha, N. (2011-11-01)We report the detection of three transiting planets around a Sun-like star, which we designate Kepler-18. The transit signals were detected in photometric data from the Kepler satellite, and were confirmed to arise from ... -
A near-infrared spectroscopic search for very-low-mass cool companions to notable DA white dwarfs
Dobbie, P.D.; Burleigh, M.R.; Levan, A.; Barstow, M.A.; Napiwotzki, R.; Holberg, J.B.; Hubeny, I.; Howell, S.B. (2005) -
Phase-resolved Hubble Space Telescope ultraviolet spectroscopy of V795 Her
Rosen, S.R.; Prinja, R.K.; Drew, J.E.; Mason, K.O.; Howell, S.B. (1998)We present highly time-resolved HST FOS UV spectroscopy of the nova-like binary V795 Her. Several key results emerge. For the first time we find a strong 2.6-h signature in the variability of the UV lines. The HST data ...