Zobrazeno 1 - 10
of 22
pro vyhledávání: '"S. T. Bryson"'
Autor:
D Specht, R Poleski, M T Penny, E Kerins, I McDonald, Chung-Uk Lee, A Udalski, I A Bond, Y Shvartzvald, Weicheng Zang, R A Street, D W Hogg, B S Gaudi, T Barclay, G Barentsen, S B Howell, F Mullally, C B Henderson, S T Bryson, D A Caldwell, M R Haas, J E Van Cleve, K Larson, K McCalmont, C Peterson, D Putnam, S Ross, M Packard, L Reedy, Michael D Albrow, Sun-Ju Chung, Youn Kil Jung, Andrew Gould, Cheongho Han, Kyu-Ha Hwang, Yoon-Hyun Ryu, In-Gu Shin, Hongjing Yang, Jennifer C Yee, Sang-Mok Cha, Dong-Jin Kim, Seung-Lee Kim, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W Pogge, M K Szymański, I Soszyński, K Ulaczyk, P Pietrukowicz, Sz Kozłowski, J Skowron, P Mróz, Shude Mao, Pascal Fouqué, Wei Zhu, F Abe, R Barry, D P Bennett, A Bhattacharya, A Fukui, H Fujii, Y Hirao, Y Itow, R Kirikawa, I Kondo, N Koshimoto, Y Matsubara, S Matsumoto, S Miyazaki, Y Muraki, G Olmschenk, C Ranc, A Okamura, N J Rattenbury, Y Satoh, T Sumi, D Suzuki, S I Silva, T Toda, P J Tristram, A Vandorou, H Yama, C Beichman, G Bryden, S Calchi Novati
Publikováno v:
Specht, D, Poleski, R, Penny, M T, Kerins, E, McDonald, I, Lee, C-U, Udalski, A, Bond, I A, Shvartzvald, Y, Zang, W, Street, R A, Hogg, D W, Gaudi, B S, Barclay, T, Barentsen, G, Howell, S B, Mullally, F, Henderson, C B, Bryson, S T, Caldwell, D A, Haas, M R, Van Cleve, J E, Larson, K, McCalmont, K, Peterson, C, Putnam, D, Ross, S, Packard, M, Reedy, L, Albrow, M D, Chung, S-J, Jung, Y K, Gould, A, Han, C, Hwang, K-H, Ryu, Y-H, Shin, I-G, Yang, H, Yee, J C, Cha, S-M, Kim, D-J, Kim, S-L, Lee, D-J, Lee, Y, Park, B-G, Pogge, R W, Szymański, M K, Soszyński, I, Ulaczyk, K, Pietrukowicz, P, Kozłowski, S, Skowron, J, Mróz, P, Mao, S, Fouqué, P, Zhu, W, Abe, F, Barry, R, Bennett, D P, Bhattacharya, A, Fukui, A, Fujii, H, Hirao, Y, Itow, Y, Kirikawa, R, Kondo, I, Koshimoto, N, Matsubara, Y, Matsumoto, S, Miyazaki, S, Muraki, Y, Olmschenk, G, Ranc, C, Okamura, A, Rattenbury, N J, Satoh, Y, Sumi, T, Suzuki, D, Silva, S I, Toda, T, Tristram, P J, Vandorou, A, Yama, H, Beichman, C, Bryden, G & Novati, S C 2023, ' Kepler K2 Campaign 9: II. First space-based discovery of an exoplanet using microlensing ', Monthly Notices of the Royal Astronomical Society, vol. 520, no. 4, pp. 6350-6366 . https://doi.org/10.1093/mnras/stad212
We present K2-2016-BLG-0005Lb, a densely sampled, planetary binary caustic-crossing microlensing event found from a blind search of data gathered from Campaign 9 of the Kepler K2 mission (K2C9). K2-2016-BLG-0005Lb is the first bound microlensing exop
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c659b8d68423b8dea278f9ed53b96c7
https://doi.org/10.1093/mnras/stad212
https://doi.org/10.1093/mnras/stad212
Autor:
Elliott P. Horch, Jon M. Jenkins, Leslie A. Rogers, Jason F. Rowe, David W. Latham, Søren Meibom, Sydney A. Barnes, Christopher E. Henze, Guillermo Torres, David R. Ciardi, Geoffrey W. Marcy, Francois Fressin, Justin R. Crepp, Kenneth A. Janes, S. T. Bryson, Steve B. Howell, Howard Isaacson, Debra A. Fischer, Simon C. Schuler
Publikováno v:
Nature. 499:55-58
Most stars and their planets form in open clusters. Over 95 per cent of such clusters have stellar densities too low (less than a hundred stars per cubic parsec) to withstand internal and external dynamical stresses and fall apart within a few hundre
Autor:
Peter Tenenbaum, Christopher E. Henze, Susan E. Thompson, Bruce D. Clarke, Miles T. Cote, Jon M. Jenkins, Anima Sabale, Robert L. Morris, Akm Kamal Uddin, Jessie L. Christiansen, Lee S. Brownston, Michael R. Haas, Jennifer R. Campbell, Bill Wohler, Christopher J. Burke, Dwight T. Sanderfer, Sean McCauliff, Jeffrey L. Coughlin, Todd C. Klaus, S. T. Bryson, Jie Li, Khadeejah A. Zamudio, Joseph Catanzarite, Forrest R. Girouard, Jeffrey C. Smith, Shawn Seader, Douglas A. Caldwell, Joseph D. Twicken
We present results of the final Kepler Data Processing Pipeline search for transiting planet signals in the full 17-quarter primary mission data set. The search includes a total of 198,709 stellar targets, of which 112,046 were observed in all 17 qua
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ba6625a08e1fc6ef23ae8cf00dd70616
http://arxiv.org/abs/1604.06140
http://arxiv.org/abs/1604.06140
Autor:
S. T. Bryson, D. W. Kurtz, Holger Lehmann, Nancy Remage Evans, L. N. Berdnikov, Gábor Fűrész, Douglas J. Mink, P. Moskalik, G. Champine, Christopher Allen, N. A. Gorynya, A. A. Henden, E. N. Pastukhova, J. M. Nemec, László Szabados, Róbert Szabó, Zoltán Kolláth, Jørgen Christensen-Dalsgaard, J. Van Cleve, Dennis Stello, Gerald Handler, J. Nuspl, József Benkő, Hans Kjeldsen, József Kovács, H. Bruntt, Jonathan E. Grindlay, László L. Kiss, Edward Los, A. Sliski, Aliz Derekas, Radosław Smolec, A. Doane, J. Molenda-Zakowicz, R. J. Simcoe, Chow-Choong Ngeow, Susan E. Thompson, Silas Laycock
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 413:2709-2720
We report results of initial work done on selected candidate Cepheids to be observed with the Kepler space telescope. Prior to the launch 40 candidates were selected from previous surveys and databases. The analysis of the first 322 days of Kepler ph
Autor:
L. A. Balona, M. S. Cunha, D. W. Kurtz, I. M. Brandão, M. Gruberbauer, H. Saio, R. Østensen, V. G. Elkin, W. J. Borucki, J. Christensen-Dalsgaard, H. Kjeldsen, D. G. Koch, S. T. Bryson
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 410:517-524
Observations of the A5p star KIC 8677585 obtained during the Kepler 10-d commissioning run with 1-min time resolution show that it is a roAp star with several frequencies with periods near 10 min. In addition, a low frequency at 3.142 cycles/day is a
Autor:
D. W. Kurtz, Zoltán Kolláth, J. Nuspl, Jørgen Christensen-Dalsgaard, Y-B. Jeon, William J. Borucki, J. M. Nemec, P. Moskalik, S. T. Bryson, Joseph D. Twicken, J. M. Benko, László Molnár, Katrien Kolenberg, Merieme Chadid, David G. Koch, Hans Kjeldsen, M. Di Criscienzo, Róbert Szabó
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 409:1244-1252
The first detection of the period doubling phenomenon is reported in the Kepler RR Lyrae stars RR Lyr, V808 Cyg and V355 Lyr. Interestingly, all these pulsating stars show Blazhko modulation. The period doubling manifests itself as alternating maxima
Autor:
Jason F. Rowe, Jon M. Jenkins, Martin Still, Susan E. Thompson, David W. Latham, Aviv Ofir, Jeffrey C. Smith, S. T. Bryson, Khadeejah A. Zamudio, Jason H. Steffen, Forrest R. Girouard, Hannah Jang-Condell, Thomas Barclay, Avi Shporer, Joseph Catanzarite, Robert L. Morris, Jack J. Lissauer, Krzysztof G. Hełminiak, Steve B. Howell, Victoria Antoci, Christa Van Laerhoven, Michael R. Haas, Natalie M. Batalha, Fergal Mullally, Anima Sabale, Billy Quarles, Peter Tenenbaum, Sean McCauliff, Todd C. Klaus, Roger C. Hunter, Jeffrey L. Coughlin, Jie Li, Kelsey Hoffman, Ronald L. Gilliland, William D. Cochran, William J. Borucki, Shawn Seader, Douglas A. Caldwell, Joseph D. Twicken, Jessie L. Christiansen, Christopher E. Henze, Elisa V. Quintana, Daniel Huber, Jennifer R. Campbell, Angie Wolfgang, Christopher J. Burke
Publikováno v:
Rowe, J F, Coughlin, J L, Antoci, V, Barclay, T, Batalha, N M, Borucki, W J, Burke, C J, Bryson, S T, Caldwell, D A, Campbell, J R, Catanzarite, J H, Christiansen, J L, Cochran, W, Gilliland, R L, Girouard, F R, Haas, M R, Hełminiak, K G, Henze, C E, Hoffman, K L, Howell, S B, Huber, D, Hunter, R C, Jang-Condell, H, Jenkins, J M, Klaus, T C, Latham, D W, Li, J, Lissauer, J J, McCauliff, S D, Morris, R L, Mullally, F, Ofir, A, Quarles, B, Quintana, E, Sabale, A, Seader, S, Shporer, A, Smith, J C, Steffen, J H, Still, M, Tenenbaum, P, Thompson, S E, Twicken, J D, Van Laerhoven, C, Wolfgang, A & Zamudio, K A 2015, ' Planetary Candidates Observed by Kepler. V. Planet Sample from Q1–Q12 (36 Months) ', Astrophysical Journal Supplement Series, vol. 217, no. 1, pp. 16 . https://doi.org/10.1088/0067-0049/217/1/16
The Kepler mission discovered 2842 exoplanet candidates with 2 years of data. We provide updates to the Kepler planet candidate sample based upon 3 years (Q1-Q12) of data. Through a series of tests to exclude false-positives, primarily caused by ecli
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fdc6e3697fdb2d0ad3216590de1a038a
Autor:
F. Kugel, C Drillaud, E. Conseil, J. F. Le Borgne, Alain Klotz, E. Poretti, D Loughney, Kenji Hirosawa, S. T. Bryson, E. Denoux, Katrien Kolenberg, Róbert Szabó, K. Graham, P. M Ruscitti, J Caron, Mónica Rodríguez, C. Buil, A. Klotz, Horace A. Smith, Kenneth Menzies, L Corp, M. Audejean
Publikováno v:
Monthly notices of the Royal Astronomical Society
RR Lyr is one of the most studied variable stars. Its light curve has been regularly monitored since the discovery of its periodic variability in 1899. The analysis of all observed maxima allows us to identify two primary pulsation states, defined as
Autor:
Andrea Miglio, Lars A. Buchhave, D. W. Kurtz, Amanda P. Doyle, Daniel Huber, Péter Pápics, Giovanni Catanzaro, Joanna Molenda-Żakowicz, G. Doğan, Tiago L. Campante, Antonio Frasca, J. A. Guzik, Martin Still, Maryline Briquet, William J. Chaplin, Fergal Mullally, Diana Dragomir, T. S. Metcalfe, J. Christensen-Dalsgaard, Barry Smalley, Sarbani Basu, Rasmus Handberg, M. Gruberbauer, O. Benomar, Timothy R. White, Jason F. Rowe, B. Mosser, Guy R. Davies, T. Appourchaux, J. Ballot, S. G. Sousa, Conny Aerts, K. Uytterhoeven, Patrick Gaulme, S. T. Bryson, Simon J. Murphy, Clara Régulo, S. Hekker, H. Bruntt, D. W. Latham, V. Ripepi, Victoria Antoci, Rafael A. García, Tabetha S. Boyajian, Christoffer Karoff, Holger Lehmann, D. Salabert, G. Houdek, S. Mathur, Yvonne Elsworth, T. R. Bedding, D. Stello, P. Mathias, R. L. Gilliland, H. Kjeldsen
Publikováno v:
The Astrophysical Journal, 831, 1-22
NASA Astrophysics Data System
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2016, 831 (1), pp.17. ⟨10.3847/0004-637X/831/1/17⟩
Guzik, J A, Houdek, G, Chaplin, W J, Smalley, B, Kurtz, D W, Gilliland, R L, Mullally, F, Rowe, J F, Bryson, S T, Still, M D, Antoci, V, Appourchaux, T, Basu, S, Bedding, T R, Benomar, O, Garcia, R A, Huber, D, Kjeldsen, H, Latham, D W, Metcalfe, T S, Papics, P I, White, T R, Aerts, C, Ballot, J, Boyajian, T S, Briquet, M, Bruntt, H, Buchhave, L A, Campante, T L, Catanzaro, G, Christensen-Dalsgaard, J, Davies, G R, Dogan, G, Dragomir, D, Doyle, A P, Elsworth, Y, Frasca, A, Gaulme, P, Gruberbauer, M, Handberg, R, Hekker, S, Karoff, C, Lehmann, H, Mathias, P, Mathur, S, Miglio, A, Molenda-Zakowicz, J, Mosser, B, Murphy, S J, Regulo, C, Ripepi, V, Salabert, D, Sousa, S G, Stello, D & Uytterhoeven, K 2016, ' DETECTION OF SOLAR-LIKE OSCILLATIONS, OBSERVATIONAL CONSTRAINTS, AND STELLAR MODELS FOR theta CYG, THE BRIGHTEST STAR OBSERVED BY THE KEPLER MISSION ', The Astrophysical Journal, vol. 831, no. 1, 17 . https://doi.org/10.3847/0004-637X/831/1/17
The Astrophysical Journal, 2016, 831 (1), pp.17. ⟨10.3847/0004-637X/831/1/17⟩
The Astrophysical Journal, 831, 1, pp. 1-22
CIÊNCIAVITAE
NASA Astrophysics Data System
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2016, 831 (1), pp.17. ⟨10.3847/0004-637X/831/1/17⟩
Guzik, J A, Houdek, G, Chaplin, W J, Smalley, B, Kurtz, D W, Gilliland, R L, Mullally, F, Rowe, J F, Bryson, S T, Still, M D, Antoci, V, Appourchaux, T, Basu, S, Bedding, T R, Benomar, O, Garcia, R A, Huber, D, Kjeldsen, H, Latham, D W, Metcalfe, T S, Papics, P I, White, T R, Aerts, C, Ballot, J, Boyajian, T S, Briquet, M, Bruntt, H, Buchhave, L A, Campante, T L, Catanzaro, G, Christensen-Dalsgaard, J, Davies, G R, Dogan, G, Dragomir, D, Doyle, A P, Elsworth, Y, Frasca, A, Gaulme, P, Gruberbauer, M, Handberg, R, Hekker, S, Karoff, C, Lehmann, H, Mathias, P, Mathur, S, Miglio, A, Molenda-Zakowicz, J, Mosser, B, Murphy, S J, Regulo, C, Ripepi, V, Salabert, D, Sousa, S G, Stello, D & Uytterhoeven, K 2016, ' DETECTION OF SOLAR-LIKE OSCILLATIONS, OBSERVATIONAL CONSTRAINTS, AND STELLAR MODELS FOR theta CYG, THE BRIGHTEST STAR OBSERVED BY THE KEPLER MISSION ', The Astrophysical Journal, vol. 831, no. 1, 17 . https://doi.org/10.3847/0004-637X/831/1/17
The Astrophysical Journal, 2016, 831 (1), pp.17. ⟨10.3847/0004-637X/831/1/17⟩
The Astrophysical Journal, 831, 1, pp. 1-22
CIÊNCIAVITAE
$\theta$ Cygni is an F3 spectral-type main-sequence star with visual magnitude V=4.48. This star was the brightest star observed by the original Kepler spacecraft mission. Short-cadence (58.8 s) photometric data using a custom aperture were obtained
Autor:
Guillermo Torres, G. W. Marcy, David R. Ciardi, J. Chen, Chris Henze, David M. Kipping, S. T. Bryson, Lars A. Buchhave, Erik A. Petigura, Emily Sandford, Alex Teachey, Howard Isaacson
Publikováno v:
The Astrophysical Journal. 822:118