Zobrazeno 1 - 10
of 88
pro vyhledávání: '"Klaus, Todd"'
Autor:
Jenkins, James S., Díaz, Matías R., Kurtovic, Nicolás T., Espinoza, Néstor, Vines, Jose I., Rojas, Pablo A. Peña, Brahm, Rafael, Torres, Pascal, Cortés-Zuleta, Pía, Soto, Maritza G., Lopez, Eric D., King, George W., Wheatley, Peter J., Winn, Joshua N., Ciardi, David R., Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Jenkins, Jon M., Beichman, Charles A., Bieryla, Allyson, Burke, Christopher J., Christiansen, Jessie L., Henze, Christopher E., Klaus, Todd C., McCauliff, Sean, Mori, Mayuko, Narita, Norio, Nishiumi, Taku, Tamura, Motohide, de Leon, Jerome Pitogo, Quinn, Samuel N., Villaseñor, Jesus Noel, Vezie, Michael, Lissauer, Jack J., Collins, Karen A., Collins, Kevin I., Isopi, Giovanni, Mallia, Franco, Ercolino, Andrea, Petrovich, Cristobal, Jordán, Andrés, Acton, Jack S., Armstrong, David J., Bayliss, Daniel, Bouchy, François, Belardi, Claudia, Bryant, Edward M., Burleigh, Matthew R., Cabrera, Juan, Casewell, Sarah L., Chaushev, Alexander, Cooke, Benjamin F., Eigmüller, Philipp, Erikson, Anders, Foxell, Emma, Gänsicke, Boris T., Gill, Samuel, Gillen, Edward, Günther, Maximilian N., Goad, Michael R., Hooton, Matthew J., Jackman, James A. G., Louden, Tom, McCormac, James, Moyano, Maximiliano, Nielsen, Louise D., Pollacco, Don, Queloz, Didier, Rauer, Heike, Raynard, Liam, Smith, Alexis M. S., Tilbrook, Rosanna H., Titz-Weider, Ruth, Turner, Oliver, Udry, Stéphane, Walker, Simon. R., Watson, Christopher A., West, Richard G., Palle, Enric, Ziegler, Carl, Law, Nicholas, Mann, Andrew W.
About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,
Externí odkaz:
http://arxiv.org/abs/2009.12832
Autor:
Dragomir, Diana, Teske, Johanna, Gunther, Maximilian N., Ségransan, Damien, Burt, Jennifer A., Huang, Chelsea X., Vanderburg, Andrew, Matthews, Elisabeth, Dumusque, Xavier, Stassun, Keivan G., Pepper, Joshua, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Beatty, Thomas, Bouchy, François, Brown, Timothy M., Butler, R. Paul, Ciardi, David R., Crane, Jeffrey D., Eastman, Jason D., Fossati, Luca, Francis, Jim, Fulton, Benjamin J., Gaudi, B. Scott, Goeke, Robert F., James, David, Klaus, Todd C., Kuhn, Rudolf B., Lovis, Christophe, Lund, Michael B., McDermott, Scott, Paegert, Martin, Pepe, Francesco, Rodriguez, Joseph E., Sha, Lizhou, Shectman, Stephen A., Shporer, Avi, Siverd, Robert J., Soto, Aylin Garcia, Stevens, Daniel J., Twicken, Joseph D., Udry, Stéphane, Villanueva Jr., Steven, Wang, Sharon X., Wohler, Bill, Yao, Xinyu, Zhan, Zhuchang
The future of exoplanet science is bright, as TESS once again demonstrates with the discovery of its longest-period confirmed planet to date. We hereby present HD 21749b (TOI 186.01), a sub-Neptune in a 36-day orbit around a bright (V = 8.1) nearby (
Externí odkaz:
http://arxiv.org/abs/1901.00051
Autor:
Twicken, Joseph D., Catanzarite, Joseph H., Clarke, Bruce D., Girouard, Forrest, Jenkins, Jon M., Klaus, Todd C., Li, Jie, McCauliff, Sean D., Seader, Shawn E., Tenenbaum, Peter, Wohler, Bill, Bryson, Stephen T., Burke, Christopher J., Caldwell, Douglas A., Haas, Michael R., Henze, Christopher E., Sanderfer, Dwight T.
The Kepler Mission was designed to identify and characterize transiting planets in the Kepler Field of View and to determine their occurrence rates. Emphasis was placed on identification of Earth-size planets orbiting in the Habitable Zone of their h
Externí odkaz:
http://arxiv.org/abs/1803.04526
Autor:
Thompson, Susan E., Coughlin, Jeffrey L., Hoffman, Kelsey, Mullally, Fergal, Christiansen, Jessie L., Burke, Christopher J., Bryson, Steve, Batalha, Natalie, Haas, Michael R., Catanzarite, Joseph, Rowe, Jason F., Barentsen, Geert, Caldwell, Douglas A., Clarke, Bruce D., Jenkins, Jon M., Li, Jie, Latham, David W., Lissauer, Jack J., Mathur, Savita, Morris, Robert L., Seader, Shawn E., Smith, Jeffrey C., Klaus, Todd C., Twicken, Joseph D., Wohler, Bill, Akeson, Rachel, Ciardi, David R., Cochran, William D., Barclay, Thomas, Campbell, Jennifer R., Chaplin, William J., Charbonneau, David, Henze, Christopher E., Howell, Steve B., Huber, Daniel, Prsa, Andrej, Ramirez, Solange V., Morton, Timothy D., Christensen-Dalsgaard, Jorgen, Dotson, Jessie L., Doyle, Laurance, Dunham, Edward W., Dupree, Andrea K., Ford, Eric B., Geary, John C., Girouard, Forrest R., Isaacson, Howard, Kjeldsen, Hans, Steffen, Jason H., Quintana, Elisa V., Ragozzine, Darin, Shabram, Megan, Shporer, Avi, Aguirre, Victor Silva, Still, Martin, Tenenbaum, Peter, Welsh, William F., Wolfgang, Angie, Zamudio, Khadeejah A., Koch, David G., Borucki, William J.
We present the Kepler Object of Interest (KOI) catalog of transiting exoplanets based on searching four years of Kepler time series photometry (Data Release 25, Q1-Q17). The catalog contains 8054 KOIs of which 4034 are planet candidates with periods
Externí odkaz:
http://arxiv.org/abs/1710.06758
Autor:
Twicken, Joseph D., Jenkins, Jon M., Seader, Shawn E., Tenenbaum, Peter, Smith, Jeffrey C., Brownston, Lee S., Burke, Christopher J., Catanzarite, Joseph H., Clarke, Bruce D., Cote, Miles T., Girouard, Forrest R., Klaus, Todd C., Li, Jie, McCauliff, Sean D., Morris, Robert L., Wohler, Bill, Campbell, Jennifer R., Uddin, Akm Kamal, Zamudio, Khadeejah A., Sabale, Anima, Bryson, Steven T., Caldwell, Douglas A., Christiansen, Jessie L., Coughlin, Jeffrey L., Haas, Michael R., Henze, Christopher E., Sanderfer, Dwight T., Thompson, Susan E.
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:
http://arxiv.org/abs/1604.06140
Autor:
Rowe, Jason F., Coughlin, Jeffrey L., Antoci, Victoria, Barclay, Thomas, Batalha, Natalie M., Borucki, William J., Burke, Christopher J., Bryson, Steven T., Caldwell, Douglas A., Campbell, Jennifer R., Catanzarite, Joseph H., Christiansen, Jessie L., Cochran, William, Gilliland, Ronald L., Girouard, Forrest R., Haas, Michael R., Helminiak, Krzysztof G., Henze, Christopher E., Hoffman, Kelsey L., Howell, Steve B., Huber, Daniel, Hunter, Roger C., Jang-Condell, Hannah, Jenkins, Jon M., Klaus, Todd C., Latham, David W., Li, Jie, Lissauer, Jack J., McCauliff, Sean D., Morris, Robert L., Mullally, F., Ofir, Aviv, Quarles, Billy, Quintana, Elisa, Sabale, Anima, Seader, Shawn, Shporer, Avi, Smith, Jeffrey C., Steffen, Jason H., Still, Martin, Tenenbaum, Peter, Thompson, Susan E., Twicken, Joseph D., Van Laerhoven, Christa, Wolfgang, Angie, Zamudio, Khadeejah A.
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:
http://arxiv.org/abs/1501.07286
Autor:
Seader, Shawn, Jenkins, Jon M., Tenenbaum, Peter, Twicken, Joseph D., Smith, Jeffrey C., Morris, Rob, Catanzarite, Joseph, Clarke, Bruce D., Li, Jie, Cote, Miles T., Burke, Christopher J., McCauliff, Sean, Girouard, Forrest R., Campbell, Jennifer R., Uddin, Akm Kamal, Zamudio, Khadeejah A., Sabale, Anima, Henze, Christopher E., Thompson, Susan E., Klaus, Todd C.
Publikováno v:
ApJS 217 18 (2015)
We present the results of a search for potential transit signals in the full 17-quarter data set collected during Kepler's primary mission that ended on May 11, 2013, due to the on-board failure of a second reaction wheel needed to maintain high prec
Externí odkaz:
http://arxiv.org/abs/1501.03586
Autor:
Tenenbaum, Peter, Jenkins, Jon M., Seader, Shawn, Burke, Christopher J., Christiansen, Jessie L., Rowe, Jason F., Caldwell, Douglas A., Clarke, Bruce D., Coughlin, Jeffrey L., Li, Jie, Quintana, Elisa V., Smith, Jeffrey C., Thompson, Susan E., Twicken, Joseph D., Haas, Michael R., Henze, Christopher E., Hunter, Roger C., Sanderfer, Dwight T., Campbell, Jennifer R., Girouard, Forrest R., Klaus, Todd C., McCauliff, Sean D., Middour, Christopher K., Sabale, Anima, Uddin, Akm Kamal, Wohler, Bill, Barclay, Thomas, Still, Martin
We present the results of a search for potential transit signals in four years of photometry data acquired by the Kepler Mission. The targets of the search include 111,800 stars which were observed for the entire interval and 85,522 stars which were
Externí odkaz:
http://arxiv.org/abs/1311.0248
Autor:
Barclay, Thomas, Rowe, Jason F., Lissauer, Jack J., Huber, Daniel, Fressin, Francois, Howell, Steve B., Bryson, Stephen T., Chaplin, William J., Désert, Jean-Michel, Lopez, Eric D., Marcy, Geoffrey W., Mullally, Fergal, Ragozzine, Darin, Torres, Guillermo, Adams, Elisabeth R., Agol, Eric, Barrado, David, Basu, Sarbani, Bedding, Timothy R., Buchhave, Lars A., Charbonneau, David, Christiansen, Jessie L., Christensen-Dalsgaard, Jørgen, Ciardi, David, Cochran, William D., Dupree, Andrea K., Elsworth, Yvonne, Everett, Mark, Fischer, Debra A., Ford, Eric B., Fortney, Jonathan J., Geary, John C., Haas, Michael R., Handberg, Rasmus, Hekker, Saskia, Henze, Christopher E., Horch, Elliott, Howard, Andrew W., Hunter, Roger C., Isaacson, Howard, Jenkins, Jon M., Karoff, Christoffer, Kawaler, Steven D., Kjeldsen, Hans, Klaus, Todd C., Latham, David W., Li, Jie, Lillo-Box, Jorge, Lund, Mikkel N., Lundkvist, Mia, Metcalfe, Travis S., Miglio, Andrea, Morris, Robert L., Quintana, Elisa V., Stello, Dennis, Smith, Jeffrey C., Still, Martin, Thompson, Susan E.
Publikováno v:
Nature, Volume 494, pp. 452-454 (2013)
Since the discovery of the first exoplanet we have known that other planetary systems can look quite unlike our own. However, until recently we have only been able to probe the upper range of the planet size distribution. The high precision of the Ke
Externí odkaz:
http://arxiv.org/abs/1305.5587
Autor:
Quintana, Elisa V., Rowe, Jason F., Barclay, Thomas, Howell, Steve B., Ciardi, David R., Demory, Brice-Olivier, Caldwell, Douglas A., Borucki, William J., Christiansen, Jessie L., Jenkins, Jon M., Klaus, Todd C., Fulton, Benjamin J., Morris, Robert L., Sanderfer, Dwight T., Shporer, Avi, Smith, Jeffrey C., Still, Martin, Thompson, Susan E.
We present high precision photometry of Kepler-41, a giant planet in a 1.86 day orbit around a G6V star that was recently confirmed through radial velocity measurements. We have developed a new method to confirm giant planets solely from the photomet
Externí odkaz:
http://arxiv.org/abs/1303.0858