Zobrazeno 1 - 10
of 18
pro vyhledávání: '"Robert C. Morehead"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 426:342-353
Using the Optical System for Imaging and low Resolution Integrated Spectroscopy (OSIRIS) instrument installed on the 10.4-m Gran Telescopio Canarias (GTC), we acquired multicolour transit photometry of four small () short-period (P ≲ 6 d) planet ca
Autor:
Mark Pfeifer, Robert C. Morehead, Monica Ann Shaw, Ruth B. Greenberg, Barbara Head, Lori Earnshaw
Publikováno v:
Journal of Palliative Medicine. 15:535-541
To use reflective writing to evaluate a new required palliative care experience for third year medical students.The authors used a constant comparison method based on grounded theory to conduct a thematic analysis of reflective writings produced by t
Publikováno v:
The Astronomical Journal. 155:205
We present a new framework to characterize the occurrence rates of planet candidates identified by Kepler based on hierarchical Bayesian modeling, Approximate Bayesian Computing (ABC), and sequential importance sampling. For this study we adopt a sim
We present new multi-band transit photometry of three small (R$_{p}$ < 6 R$_{\oplus}$), short-period (P < 6 days) Kepler planet candidates acquired with the Gran Telescopio Canarias. These observations supplement the results presented in Col��n &
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::87748dc2ed129bf0c60063bb4f2aff30
http://arxiv.org/abs/1506.07057
http://arxiv.org/abs/1506.07057
Autor:
William J. Borucki, Jon M. Jenkins, Jeffrey C. Smith, Thomas N. Gautier, Martin Still, Eric Agol, Jack J. Lissauer, Eric B. Ford, Avi Shporer, Matthew J. Holman, Jie Li, Thomas Barclay, Robert C. Morehead, David R. Ciardi, Robert L. Morris, Natalie M. Batalha, Darin Ragozzine, John C. Geary, Jason H. Steffen, Jeffrey Van Cleve, Jason F. Rowe, Daniel C. Fabrycky
Publikováno v:
NASA Astrophysics Data System
We report on the orbital architectures of Kepler systems having multiple planet candidates identified in the analysis of data from the first six quarters of Kepler data and reported by Batalha et al. (2013). These data show 899 transiting planet cand
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::973707280ef6b5a7c3b83dbc038049a0
https://resolver.caltech.edu/CaltechAUTHORS:20140815-092737225
https://resolver.caltech.edu/CaltechAUTHORS:20140815-092737225
Autor:
Christopher J. Burke, Stephen T. Bryson, F. Mullally, Jason F. Rowe, Jessie L. Christiansen, Susan E. Thompson, Jeffrey L. Coughlin, Michael R. Haas, Natalie M. Batalha, Douglas A. Caldwell, Jon M. Jenkins, Martin Still, Thomas Barclay, William J. Borucki, William J. Chaplin, David R. Ciardi, Bruce D. Clarke, William D. Cochran, Brice-Olivier Demory, Gilbert A. Esquerdo, Thomas N. Gautier, Ronald L. Gilliland, Forrest R. Girouard, Mathieu Havel, Christopher E. Henze, Steve B. Howell, Daniel Huber, David W. Latham, Jie Li, Robert C. Morehead, Timothy D. Morton, Joshua Pepper, Elisa Quintana, Darin Ragozzine, Shawn E. Seader, Yash Shah, Avi Shporer, Peter Tenenbaum, Joseph D. Twicken, Angie Wolfgang
Publikováno v:
Burke, Christopher J.; Bryson, Stephen T.; Mullally, F.; Rowe, Jason F.; Christiansen, Jessie L.; Thompson, Susan E.; Coughlin, Jeffrey L.; Haas, Michael R.; Batalha, Natalie M.; Caldwell, Douglas A.; Jenkins, Jon M.; Still, Martin; Barclay, Thomas; Borucki, William J.; Chaplin, William J.; Ciardi, David R.; Clarke, Bruce D.; Cochran, William D.; Demory, Brice-Olivier; Esquerdo, Gilbert A.; ... (2014). PLANETARY CANDIDATES OBSERVED BY KEPLER IV: PLANET SAMPLE FROM Q1-Q8 (22 MONTHS). Astrophysical journal-supplement series, 210(2), p. 19. Institute of Physics Publishing IOP 10.1088/0067-0049/210/2/19
We provide updates to the Kepler planet candidate sample based upon nearly two years of high-precision photometry (i.e., Q1-Q8). From an initial list of nearly 13,400 Threshold Crossing Events (TCEs), 480 new host stars are identified from their flux
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56d0d4d389dfb4d65cabff17917d1e63
https://resolver.caltech.edu/CaltechAUTHORS:20140313-074312078
https://resolver.caltech.edu/CaltechAUTHORS:20140313-074312078
Autor:
Eric B. Ford, Matthew J. Holman, Lars A. Buchhave, Guillermo Torres, Jack J. Lissauer, David R. Ciardi, Peter G. Tanenbaum, Geoffrey W. Marcy, Francois Fressin, Jon M. Jenkins, Darin Ragozzine, Steve B. Howell, Daniel C. Fabrycky, Elisabeth R. Adams, Stephen T. Bryson, William D. Cochran, Jason F. Rowe, Shawn Seader, Karen Kinemuchi, Joseph D. Twicken, Ronald L. Gilliland, John C. Geary, Robert C. Morehead, David G. Koch
We present a statistical analysis that demonstrates that the overwhelming majority of Kepler candidate multiple transiting systems (multis) indeed represent true, physically-associated transiting planets. Binary stars provide the primary source of fa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eebfcb55757e47c36e8899404b11d490
https://resolver.caltech.edu/CaltechAUTHORS:20120530-140026379
https://resolver.caltech.edu/CaltechAUTHORS:20120530-140026379
Autor:
Jason F. Rowe, Khadeejah A. Ibrahim, Jack J. Lissauer, Darin Ragozzine, Douglas A. Caldwell, Joseph D. Twicken, Althea V. Moorhead, Bill Wohler, Guillermo Torres, Jie Li, Debra A. Fischer, Eric B. Ford, Elliott P. Horch, Phillip J. MacQueen, Samuel N. Quinn, Sean McCauliff, Elisa V. Quintana, Martin Still, Howard Isaacson, Jason H. Steffen, R. L. Gilliland, William D. Cochran, Christopher Allen, Michael R. Haas, David W. Latham, Avi Shporer, Jean-Michel Desert, Joshua A. Carter, Stephen T. Bryson, Lars A. Buchhave, Francois Fressin, Susan E. Thompson, William J. Borucki, Matthew J. Holman, Philip W. Lucas, Thomas N. Gautier, Michael Endl, Geoffrey W. Marcy, Natalie M. Batalha, Robert C. Morehead, David Charbonneau, Daniel C. Fabrycky, Fergal Mullally, William F. Welsh, Mark E. Everett, Peter Tenenbaum, Bruce D. Clarke, Jon M. Jenkins, Steve B. Howell, Christopher J. Burke, David G. Koch
We present a new method for confirming transiting planets based on the combination of transit timingn variations (TTVs) and dynamical stability. Correlated TTVs provide evidence that the pair of bodies are in the same physical system. Orbital stabili
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2a347d457de5f0f4173f5e87f00e4e53
Autor:
William J. Borucki, Shawn Seader, Robert C. Morehead, Douglas A. Caldwell, Jack J. Lissauer, Eric B. Ford, Joseph D. Twicken, Paul Robertson, William D. Cochran, Susan E. Thompson, Jason F. Rowe, Eric Agol, Daniel C. Fabrycky, Andrea K. Dupree, Jon M. Jenkins, Jason H. Steffen, Elisabeth R. Adams, Steve Bryson
We confirm 27 planets in 13 planetary systems by showing the existence of statistically significant anti-correlated transit timing variations (TTVs), which demonstrates that the planet candidates are in the same system, and long-term dynamical stabil
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f38e886d54a9bd040ef7bf804a6c23aa
Autor:
Andrew W. Howard, Geoffrey W. Marcy, Stephen T. Bryson, Jon M. Jenkins, Jason F. Rowe, Natalie M. Batalha, William J. Borucki, David G. Koch, Edward W. Dunham, Thomas N. Gautier, Jeffrey Van Cleve, William D. Cochran, David W. Latham, Jack J. Lissauer, Guillermo Torres, Timothy M. Brown, Ronald L. Gilliland, Lars A. Buchhave, Douglas A. Caldwell, Jørgen Christensen-Dalsgaard, David Ciardi, Francois Fressin, Michael R. Haas, Steve B. Howell, Hans Kjeldsen, Sara Seager, Leslie Rogers, Dimitar D. Sasselov, Jason H. Steffen, Gibor S. Basri, David Charbonneau, Jessie Christiansen, Bruce Clarke, Andrea Dupree, Daniel C. Fabrycky, Debra A. Fischer, Eric B. Ford, Jonathan J. Fortney, Jill Tarter, Forrest R. Girouard, Matthew J. Holman, John Asher Johnson, Todd C. Klaus, Pavel Machalek, Althea V. Moorhead, Robert C. Morehead, Darin Ragozzine, Peter Tenenbaum, Joseph D. Twicken, Samuel N. Quinn, Howard Isaacson, Avi Shporer, Philip W. Lucas, Lucianne M. Walkowicz, William F. Welsh, Alan Boss, Edna Devore, Alan Gould, Jeffrey C. Smith, Robert L. Morris, Andrej Prsa, Timothy D. Morton, Martin Still, Susan E. Thompson, Fergal Mullally, Michael Endl, Phillip J. MacQueen
Publikováno v:
Howard, A W, Marcy, G W, Bryson, S T, Jenkins, J M, Rowe, J F, Batalha, N M, Borucki, W J, Koch, D G, Dunham, E W, Gautier, T N III, Van Cleve, J, Cochran, W D, Latham, D W, Lissauer, J J, Torres, G, Brown, T M, Gilliland, R L, Buchhave, L A, Caldwell, D A, Christensen-Dalsgaard, J, Ciardi, D, Fressin, F, Haas, M R, Howell, S B, Kjeldsen, H, Seager, S, Rogers, L, Sasselov, D D, Steffen, J H, Basri, G S, Charbonneau, D, Christiansen, J, Clarke, B, Dupree, A, Fabrycky, D C, Fischer, D A, Ford, E B, Fortney, J J, Tarter, J, Girouard, F R, Holman, M J, Johnson, J A, Klaus, T C, Machalek, P, Moorhead, A V, Morehead, R C, Ragozzine, D, Tenenbaum, P, Twicken, J D, Quinn, S N, Isaacson, H, Shporer, A, Lucas, P W, Walkowicz, L M, Welsh, W F, Boss, A, Devore, E, Gould, A, Smith, J C, Morris, R L, Prsa, A, Morton, T D, Still, M, Thompson, S E, Mullally, F, Endl, M & MacQueen, P J 2012, ' Planet Occurrence within 0.25 AU of Solar-type Stars from Kepler ', The Astrophysical Journal Letters, vol. 201, no. 2 . https://doi.org/10.1088/0067-0049/201/2/15
We report the distribution of planets as a function of planet radius (R_p), orbital period (P), and stellar effective temperature (Teff) for P < 50 day orbits around GK stars. These results are based on the 1,235 planets (formally "planet candidates"
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5268c70b46421898fe3386fdea97916e
http://arxiv.org/abs/1103.2541
http://arxiv.org/abs/1103.2541