Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Hayley Wu"'
Autor:
Jun Sawada, Filipp Akopyan, Andrew S. Cassidy, Brian Taba, Michael V. Debole, Pallab Datta, Rodrigo Alvarez-Icaza, Arnon Amir, John V. Arthur, Alexander Andreopoulos, Rathinakumar Appuswamy, Heinz Baier, Davis Barch, David J. Berg, Carmelo Di Nolfo, Steven K. Esser, Myron Flickner, Thomas A. Horvath, Bryan L. Jackson, Jeff Kusnitz, Scott Lekuch, Michael Mastro, Timothy Melano, Paul A. Merolla, Steven E. Millman, Tapan K. Nayak, Norm Pass, Hartmut E. Penner, William P. Risk, Kai Schleupen, Benjamin Shaw, Hayley Wu, Brian Giera, Adam T. Moody, Nathan Mundhenk, Brian C. Van Essen, Eric X. Wang, David P. Widemann, Qing Wu, William E. Murphy, Jamie K. Infantolino, James A. Ross, Dale R. Shires, Manuel M. Vindiola, Raju Namburu, Dharmendra S. Modha
Publikováno v:
SC16: International Conference for High Performance Computing, Networking, Storage and Analysis.
Autor:
Peter Tenenbaum, Jon M. Jenkins, Hayley Wu, Forrest R. Girouard, Bruce D. Clarke, Todd C. Klaus, Stephen T. Bryson, Joseph D. Twicken
Publikováno v:
SPIE Proceedings.
We describe the Photometric Analysis (PA) software component and its context in the Kepler Science Operations Center (SOC) pipeline. The primary tasks of this module are to compute the photometric flux and photocenters (centroids) for over 160,000 lo
Autor:
Forrest R. Girouard, Bruce D. Clarke, Bill Wohler, Jon M. Jenkins, Peter Tenenbaum, Christopher Allen, Elisa V. Quintana, Sean McCauliff, Douglas A. Caldwell, Joseph D. Twicken, Hema Chandrasekaran, Miles T. Cote, Hayley Wu, Todd C Klaus, Jie Li
Publikováno v:
SPIE Proceedings.
We present an overview of the Data Validation (DV) software component and its context within the Kepler Science Operations Center (SOC) pipeline and overall Kepler Science mission. The SOC pipeline performs a transiting planet search on the corrected
Autor:
Stephen T. Bryson, Bruce D. Clarke, Christopher Allen, Douglas A. Caldwell, Joseph D. Twicken, Todd C. Klaus, Jie Li, Bill Wohler, Jay P. Gunter, Peter Tenenbaum, Hema Chandrasekaran, Jon M. Jenkins, Hayley Wu, Elisa V. Quintana
Publikováno v:
SPIE Proceedings.
This paper describes the algorithms of the Photometer Performance Assessment (PPA) software component in the science data processing pipeline of the Kepler mission. The PPA performs two tasks: One is to analyze the health and performance of the Keple
Autor:
Jon M. Jenkins, William J. Borucki, David G. Koch, Geoffrey W. Marcy, William D. Cochran, William F. Welsh, Gibor Basri, Natalie M. Batalha, Lars A. Buchhave, Timothy M. Brown, Douglas A. Caldwell, Edward W. Dunham, Michael Endl, Debra A. Fischer, Thomas N. Gautier, John C. Geary, Ronald L. Gilliland, Steve B. Howell, Howard Isaacson, John Asher Johnson, David W. Latham, Jack J. Lissauer, David G. Monet, Jason F. Rowe, Dimitar D. Sasselov, Andrew W. Howard, Phillip MacQueen, Jerome A. Orosz, Hema Chandrasekaran, Joseph D. Twicken, Stephen T. Bryson, Elisa V. Quintana, Bruce D. Clarke, Jie Li, Christopher Allen, Peter Tenenbaum, Hayley Wu, Søren Meibom, Todd C. Klaus, Christopher K. Middour, Miles T. Cote, Sean McCauliff, Forrest R. Girouard, Jay P. Gunter, Bill Wohler, Jennifer R. Hall, Khadeejah Ibrahim, AKM Kamal Uddin, Michael S. Wu, Paresh A. Bhavsar, Jeffrey Van Cleve, David L. Pletcher, Jessie L. Dotson, Michael R. Haas
We report the discovery and the Rossiter-McLaughlin effect of Kepler-8b, a transiting planet identified by the NASA Kepler Mission. Kepler photometry and Keck-HIRES radial velocities yield the radius and mass of the planet around this F8IV subgiant h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::eb6741527650942aa1aadcf5cbf25f63
http://arxiv.org/abs/1001.0416
http://arxiv.org/abs/1001.0416
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
Autor:
Jie Li, Hema Chandrasekaran, Ronald L. Gilliland, Todd C. Klaus, Michael R. Haas, William J. Borucki, David G. Koch, Bruce D. Clarke, Stephen T. Bryson, Douglas A. Caldwell, Jeffrey Van Cleve, Joseph D. Twicken, Jon M. Jenkins, Elisa V. Quintana, Peter Tenenbaum, Christopher C. R. Allen, Hayley Wu, J. Dotson
The Kepler Mission seeks to detect Earth-size planets transiting solar-like stars in its ~115 deg^2 field of view over the course of its 3.5 year primary mission by monitoring the brightness of each of ~156,000 Long Cadence stellar targets with a tim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::918c0c11959e10d3dcecc3b543ff63bb
http://arxiv.org/abs/1001.0256
http://arxiv.org/abs/1001.0256
Autor:
Kamal Uddin, Stephen T. Bryson, Forrest R. Girouard, Bill Wohler, Jay P. Gunter, Jon M. Jenkins, Peter Tenenbaum, Douglas A. Caldwell, Joseph D. Twicken, Todd C. Klaus, Jie Li, David G. Koch, Christopher K. Middour, Michael R. Haas, Sean McCauliff, Jeneen Sommers, Jennifer R. Hall, Hema Chandrasekaran, D. Pletcher, Ronald L. Gilliland, Michael S. Wu, Bruce D. Clarke, Paresh A. Bhavsar, William J. Borucki, Miles T. Cote, Hayley Wu, Christopher Allen, Jeffrey Van Cleve, J. Dotson, Elisa V. Quintana
The Kepler Mission Science Operations Center (SOC) performs several critical functions including managing the ~156,000 target stars, associated target tables, science data compression tables and parameters, as well as processing the raw photometric d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4ddf1a8c8c1b1806d09b53332eb3fad3
http://arxiv.org/abs/1001.0258
http://arxiv.org/abs/1001.0258
Autor:
William J. Borucki, David G. Koch, Gibor Basri, Natalie Batalha, Alan Boss, Timothy M. Brown, Douglas Caldwell, Jørgen Christensen-Dalsgaard, William D. Cochran, Edna DeVore, Edward W. Dunham, Andrea K. Dupree, Thomas N. Gautier III, John C. Geary, Ronald Gilliland, Alan Gould, Steve B. Howell, Jon M. Jenkins, Hans Kjeldsen, David W. Latham, Jack J. Lissauer, Geoffrey W. Marcy, David G. Monet, Dimitar Sasselov, Jill Tarter, David Charbonneau, Laurance Doyle, Eric B. Ford, Jonathan Fortney, Matthew J. Holman, Sara Seager, Jason H. Steffen, William F. Welsh, Christopher Allen, Stephen T. Bryson, Lars Buchhave, Hema Chandrasekaran, Jessie L. Christiansen, David Ciardi, Bruce D. Clarke, Jessie L. Dotson, Michael Endl, Debra Fischer, Francois Fressin, Michael Haas, Elliott Horch, Andrew Howard, Howard Isaacson, Jeffery Kolodziejczak, Jie Li, Phillip MacQueen, Søren Meibom, Andrej Prsa, Elisa V. Quintana, Jason Rowe, William Sherry, Peter Tenenbaum, Guillermo Torres, Joseph D. Twicken, Jeffrey Van Cleve, Lucianne Walkowicz, Hayley Wu
Publikováno v:
Borucki, W J, Koch, D G, Basri, G, Batalha, N, Boss, A, Brown, T M, Caldwell, D, Christensen-Dalsgaard, J, Cochran, W D, DeVore, E, Dunham, E W, Dupree, A K, Gautier III, T N, Geary, J C, Gilliland, R, Gould, A, Howell, S B, Jenkins, J M, Kjeldsen, H, Latham, D W, Lissauer, J J, Marcy, G W, Monet, D G, Sasselov, D, Tarter, J, Charbonneau, D, Doyle, L, Ford, E B, Fortney, J, Holman, M J, Seager, S, Steffen, J H, Welsh, W F, Allen, C, Bryson, S T, Buchhave, L, Chandrasekaran, H, Christiansen, J L, Ciardi, D, Clarke, B D, Dotson, J L, Endl, M, Fischer, D, Fressin, F, Haas, M, Horch, E, Howard, A, Isaacson, H, Kolodziejczak, J, Li, J, MacQueen, P, Meibom, S, Prsa, A, Quintana, E V, Rowe, J, Sherry, W, Tenenbaum, P, Torres, G, Twicken, J D, Van Cleve, J, Walkowicz, L & Wu, H 2011, ' Characteristics of Kepler Planetary Candidates Based on the First Data Set ', Astrophysical Journal, vol. 728, no. 2/article id. 117 . https://doi.org/10.1088/0004-637X/728/2/117
In the spring of 2009, the Kepler Mission commenced high-precision photometry on nearly 156,000 stars to determine the frequency and characteristics of small exoplanets, conduct a guest observer program, and obtain asteroseismic data on a wide variet
Autor:
Jenkins, Jon M., Caldwell, Douglas A., Chandrasekaran, Hema, Twicken, Joseph D., Bryson, Stephen T., Quintana, Elisa V., Clarke, Bruce D., Jie Li, Allen, Christopher, Tenenbaum, Peter, Hayley Wu, Klaus, Todd C., Van Cleve, Jeffrey, Dotson, Jessie A., Haas, Michael R., Gilliland, Ronald L., Koch, David G., Borucki, William J.
Publikováno v:
Astrophysical Journal Letters; 4/20/2010, Vol. 713 Issue 2, pL120-L125, 6p