Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Vic S. Argabright"'
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:
S. Franka, J. B. Hutchings, Edward B. Jenkins, Chuck Bowers, D. Rose, Richard F. Green, Alan W. Delamere, M. Bottema, D. Hood, W. Meyer, Sara R. Heap, Morley M. Blouke, Charles L. Joseph, George F. Hartig, Fred L. Roesler, Lee Feinberg, Randy A. Kimble, Jeffrey L. Linsky, J. J. Loiacono, J. F. Grady, Albert Boggess, J. C. Hetlinger, David A. Dorn, H. Garner, Steven B. Kraemer, David Michika, Vic S. Argabright, C. Ludtke, B. E. Woodgate, Mark D. Brumfield, Theodore R. Gull, H. W. Moos, Anthony C. Danks, J. G. Timothy, C. VanHouten, Mary Elizabeth Kaiser, Donna Weistrop, R. Stocker, Robert A. Woodruff, D. J. Lindler, Stephen P. Maran, I. Becker, Richard L. Bybee, Joe H. Sullivan
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:1183-1204
The Space Telescope Imaging Spectrograph (STIS) instrument was installed on the Hubble Space Telescope (HST) during the second servicing mission, in 1997 February. Four bands cover the wavelength range of 115–1000 nm, with spectral resolving powers
Autor:
Randy A. Kimble, Ronald L. Gilliland, Ralph C. Bohlin, Mary Elizabeth Kaiser, Don J. Lindler, Vic S. Argabright
Publikováno v:
Publications of the Astronomical Society of the Pacific. 110:978-990
The Space Telescope Imaging Spectrograph (STIS) was designed as a versatile spectrograph for the Hubble Space Telescope (HST) capable of maintaining or exceeding the spectroscopic capabilities of both the Goddard High Resolution Spectrograph (GHRS) a
Publikováno v:
Review of Scientific Instruments. 69:1898-1905
We conducted a study to estimate the impact that thermal variations and electronic drifts would have on the photometric stability of the multianode microchannel array (MAMA) detectors that are currently flying aboard the space telescope imaging spect
Autor:
Dennis Ebbets, Mark D. Brumfield, R. Breyer, Stefi A. Baum, Mary Elizabeth Kaiser, P. R. Christon, S. I. Becker, Chuck Bowers, Randy A. Kimble, Sara R. Heap, R. J. Hill, Richard F. Green, Alan W. Delamere, L. W. Brown, S. Downey, Melissa A. McGrath, J. F. Grady, Richard D. Robinson, J. J. Yagelowich, D. Rose, A. Grusczak, David A. Dorn, C. Standley, A. Boggess, Vic S. Argabright, J. C. Blades, Anthony C. Danks, C. Ludtke, Stephen P. Maran, P. A. Driggers, Theodore R. Gull, J. G. Timothy, W. B. Fowler, W. Meyer, Mark Clampin, V. L. Krueger, M. N. Isaacs, J. A. Valenti, Wayne B. Landsman, George F. Hartig, J. J. Loiacono, Ralph C. Bohlin, Richard L. Bybee, R. Stocker, Fred L. Roesler, H. W. Moos, D. Hood, R. L. Lettieri, Eliot M. Malumuth, V. Balzano, C. Biagetti, Steven B. Kraemer, Henry C. Ferguson, David Michika, Robert S. Hill, R. Nyquist, Paul Goudfrooij, J. C. Hetlinger, M. Bottema, T. Wolfe, T. L. Beck, R. W. Melcher, Robert A. Woodruff, D. J. Lindler, Morley M. Blouke, Jennifer L. Sandoval, Lee Feinberg, F. J. Rebar, Charles L. Joseph, Nicholas R. Collins, C. N. Van Houten, J. F. Sullivan, J. K. Feggans, J. S. Gallegos, Carolyn A. Krebs, R. Doxsey, D. Weistrop, Stephen J. Hulbert, P. Plait, Bruce E. Woodgate, R. Kutina, R. H. Cornett, Jeffrey L. Linsky, R. Reed, H. Garner, H. D. Vitagliano, J. B. Hutchings, Edward B. Jenkins
Publikováno v:
The Astrophysical Journal. 492:L83-L93
The Space Telescope Imaging Spectrograph (STIS) was successfully installed into the Hubble Space Telescope (HST) in 1997 February, during the second HST servicing mission, STS-82. STIS is a versatile spectrograph, covering the 115-1000 nm wavelength
Autor:
Jeffrey Kolodziejczak, J. VanCleve, D. Ebbets, J. Stober, Vic S. Argabright, Douglas A. Caldwell
Publikováno v:
SPIE Proceedings.
Kepler is NASAs first space mission dedicated to the study of exoplanets. The primary scientific goal is statistical to estimate the frequency of planetary systems associated with sun-like stars. Kepler was launched into an Earth-trailing helioc
Publikováno v:
SPIE Proceedings.
A small fraction of Kepler telescope exposures are rejected because of transient, excess background in the field. The patterns of illumination vary from broad streaks to diffuse patches, sometimes filling the focal plane. Examination of such images a
Autor:
Lucianne M. Walkowicz, Andrea Miglio, Douglas A. Caldwell, Jeffrey Kolodziejczak, William J. Borucki, Vic S. Argabright, Stephen T. Bryson, William F. Welsh, Jon M. Jenkins, William J. Chaplin, Ronald L. Gilliland, Edward W. Dunham, Jeffrey Van Cleve, David G. Koch, Derek Buzasi, Yvonne Elsworth, Gibor Basri
Kepler Mission results are rapidly contributing to fundamentally new discoveries in both the exoplanet and asteroseismology fields. The data returned from Kepler are unique in terms of the number of stars observed, precision of photometry for time se
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c8aeb074bc82dcb4beb52537741643b0
http://arxiv.org/abs/1107.5207
http://arxiv.org/abs/1107.5207
Autor:
M. T. Cote, Jeffery J. Kolodziejczak, Douglas A. Caldwell, Todd C. Klaus, Vic S. Argabright, Jon M. Jenkins, Jeffery Van Cleve, Bruce D. Clarke
Publikováno v:
SPIE Proceedings.
In order for Kepler to achieve its required less than 20 PPM photometric precision for magnitude 12 and brighter stars, instrument-induced variations in the CCD readout bias pattern (our "2D black image"), which are either fixed or slowly varying in
Autor:
William J. Borucki, Jon M. Jenkins, Peter Tenenbaum, Hayley Wu, Jessie L. Dotson, Douglas A. Caldwell, Stephen T. Bryson, Edward W. Dunham, P. R. Gazis, Jeffrey Van Cleve, John C. Geary, Eric Bachtell, David G. Koch, Michael R. Haas, Vic S. Argabright, Jeffery J. Kolodziejczak, Jie Li, Hema Chandrasekaran, Ronald L. Gilliland
The Kepler Mission relies on precise differential photometry to detect the 80 parts per million (ppm) signal from an Earth-Sun equivalent transit. Such precision requires superb instrument stability on time scales up to ~2 days and systematic error r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bd79056669020e25e8c1df0a63e88513
http://arxiv.org/abs/1001.0216
http://arxiv.org/abs/1001.0216