Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Dorothy A. Fraquelli"'
Autor:
Chris Stewart, V. Silva Aguirre, Forrest R. Girouard, Krzysztof G. Hełminiak, Peter Plavchan, Jason F. Rowe, Jeffrey C. Smith, Christopher E. Henze, Elisa V. Quintana, Y. Shah, Christopher J. Burke, Fergal Mullally, Dorothy A. Fraquelli, Riley M. Duren, Eric Bachtell, Jeremy Stober, Jason H. Steffen, Martin Still, Dustin Putnam, Scott W. Fleming, John Troeltzsch, Aviv Ofir, Daniel Huber, Thomas N. Gautier, Jennifer R. Campbell, Avi Shporer, Shawn Seader, Anima Patil-Sabale, Thomas Barclay, Douglas A. Caldwell, Joseph D. Twicken, Ji-Wei Xie, Jessie L. Christiansen, Vic S. Argabright, William J. Chaplin, Solange V. Ramirez, William J. Borucki, Jon M. Jenkins, Robert L. Morris, Angie Wolfgang, V. Van Eylen, Jie Li, Susan E. Thompson, Natalie M. Batalha, K. Larson, Khadeejah A. Zamudio, Joseph Catanzarite, Christopher J. Miller, Peter Tenenbaum, Scot McArthur, David W. Latham, Michael R. Haas, Rachel Akeson, Christa Van Laerhoven, William D. Cochran, Jeffrey L. Coughlin, Billy Quarles, Jack J. Lissauer, Steve B. Howell, Stephen T. Bryson
Publikováno v:
Mullally, F, Coughlin, J L, Thompson, S E, Rowe, J, Burke, C, Latham, D W, Batalha, N M, Bryson, S T, Christiansen, J, Henze, C E, Ofir, A, Quarles, B, Shporer, A, Van Eylen, V, Van Laerhoven, C, Shah, Y, Wolfgang, A, Chaplin, W J, Xie, J-W, Akeson, R, Argabright, V, Bachtell, E, Barclay, T, Borucki, W J, Caldwell, D A, Campbell, J R, Catanzarite, J H, Cochran, W D, Duren, R M, Fleming, S W, Fraquelli, D, Girouard, F R, Haas, M R, Hełminiak, K G, Howell, S B, Huber, D, Larson, K, Gautier, T N III, Jenkins, J M, Li, J, Lissauer, J J, McArthur, S, Miller, C, Morris, R L, Patil-Sabale, A, Plavchan, P, Putnam, D, Quintana, E V, Ramirez, S, Silva Aguirre, V, Seader, S, Smith, J C, Steffen, J H, Stewart, C, Stober, J, Still, M, Tenenbaum, P, Troeltzsch, J, Twicken, J D & Zamudio, K A 2015, ' Planetary Candidates Observed by Kepler. VI. Planet Sample from Q1--Q16 (47 Months) ', Astrophysical Journal Supplement Series, vol. 217, pp. 31 . https://doi.org/10.1088/0067-0049/217/2/31
\We present the sixth catalog of Kepler candidate planets based on nearly 4 years of high precision photometry. This catalog builds on the legacy of previous catalogs released by the Kepler project and includes 1493 new Kepler Objects of Interest (KO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4956e23786e8b0129aa420a9cdf3674b
http://arxiv.org/abs/1502.02038
http://arxiv.org/abs/1502.02038
Autor:
Dorothy A. Fraquelli, Richard G. Lyon, Kenneth G. Carpenter, A. B. Schultz, Jan M. Hollis, Helen M. Hart, Ian J. E. Jordan, Frederick C. Bruhweiler, M. Kochte
Publikováno v:
SPIE Proceedings.
The standard approach to achieving TPF-level starlight suppression has been to couple a few techniques together. Deployment of a low- or medium-performance external occulter as the first stage of starlight suppression reduces manufacturing challenges
Autor:
Dorothy A. Fraquelli, H. M. Hart, J. Leitner, M. Kochte, Ian J. E. Jordan, R. D. Burns, A. Schultz
Publikováno v:
Space OPS 2004 Conference.
Autor:
Dorothy A. Fraquelli, Kenneth G. Carpenter, Ian J. E. Jordan, Cherie L. Miskey, M. Rodrigue, M. Kochte, Mike A. DiSanti, A. Schultz, H. M. Hart, Dennis L. Skelton, Richard G. Lyon, F. Bruhweiler, M.S. Fadali, K. P. Cheng
Publikováno v:
AIP Conference Proceedings.
We present optical simulations of a new approach to directly image terrestrial planets. Terrestrial planets typically are 10 orders of magnitude fainter than the central star, a difficult challenge for any optical system. Our studies show that the co
Autor:
Scott R. Starin, Kenneth G. Carpenter, M. Kochte, M. Rodrigue, Jesse Leitner, Fred C. Bruhweiler, M.S. Fadali, Mike A. DiSanti, F. Hamilton, Jan M. Hollis, Richard Burns, Dorothy A. Fraquelli, Dennis L. Skelton, H. M. Hart, A. Schultz, Ian J. E. Jordan, Cherie L. Miskey, Richard G. Lyon, Kwang-Ping Cheng
Publikováno v:
SPIE Proceedings.
We describe a 1-meter space telescope plus free-flying occulter craft mission that would provide direct imaging and spectroscopic observations of Jovian and Uranus-sized planets about nearby stars not detectable by Doppler techniques. The Doppler tec
Publikováno v:
Observatory Operations to Optimize Scientific Return III.
This paper presents an overview of the history and technology by which tools placed in the Hubble Space Telescope (HST) data processing pipeline were used to feedback information on observation execution to the scheduling system and observers. Becaus
Autor:
Ian J. E. Jordan, Kwang-Ping Cheng, Cherie L. Miskey, Dorothy A. Fraquelli, John L. Hershey, Fred C. Bruhweiler, M. Rodrigue, Bruce Johnson, Mike A. DiSanti, H. M. Hart, M. Kochte, A. B. Schultz, M.S. Fadali, R. Clark, F. Hamilton, Daniel J. Schroeder
Publikováno v:
SPIE Proceedings.
We present a novel coronagraphic imaging technique and design for space-based telescopes. The Umbral Mission Blocking Radiating Astronomical Sources (UMBRAS) is a space mission design consisting of a free flying occulter, the Solar Powered Ion Driven
Autor:
Fred C. Bruhweiler, J. E. Jordan, H. M. Hart, Dorothy A. Fraquelli, Alfred B. Schultzt, John HersheyK
Publikováno v:
Space 2000 Conference and Exposition.
A free-flying occulter used with a space-based telescope can enhance the contrast in the region close to a star, allowing extrasolar planet searches. An occulting spacecraft design, emphasizing configuration, control, propulsion, mass estimates, and
Autor:
Dorothy A. Fraquelli
Publikováno v:
Close Binary Stars: Observations and Interpretation ISBN: 9789027711175
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::0341490dc0af5f7bd8847cdf2cdd803d
https://doi.org/10.1007/978-94-009-9038-8_72
https://doi.org/10.1007/978-94-009-9038-8_72
Autor:
Dorothy A. Fraquelli
Publikováno v:
Symposium - International Astronomical Union. 88:413-414
Spectrophotometry of the bright RS CVn binary HR 5110 is presented. The data consist of 42 red spectrograms obtained with the DDO 74″ telescope. All spectrograms were scanned using the PDS microdensitometer system at the DDO and rectified intensity