Zobrazeno 1 - 10
of 272
pro vyhledávání: '"Mullally, F."'
Autor:
Specht, D., Poleski, R., Penny, M. T., Kerins, E., McDonald, I., Lee, Chung-Uk, Udalski, A., Bond, I. A., Shvartzvald, Y., Zang, Weicheng, 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, Michael D., Chung, Sun-Ju, Jung, Youn Kil, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Ryu, Yoon-Hyun, Shin, In-Gu, Yang, Hongjing, Yee, Jennifer C., Cha, Sang-Mok, Kim, Dong-Jin, Kim, Seung-Lee, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Szymański, M. K., Soszyński, I., Ulaczyk, K., Pietrukowicz, P., Kozlowski, Sz., Skowron, J., Mróz, P., Mao, Shude, Fouqué, Pascal, Zhu, Wei, 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. Calchi
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:
http://arxiv.org/abs/2203.16959
Autor:
Burke, Christopher J., Mullally, F., Thompson, Susan E., Coughlin, Jeffrey L., Rowe, Jason F.
We re-examine the statistical confirmation of small long-period Kepler planet candidates in light of recent improvements in our understanding of the occurrence of systematic false alarms in this regime. Using the final Data Release 25 (DR25) Kepler p
Externí odkaz:
http://arxiv.org/abs/1901.00506
Autor:
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., Pápics, 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., Doğan, 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-Żakowicz, J., Mosser, B., Murphy, S. J., Régulo, C., Ripepi, V., Salabert, D., Sousa, S. G., Stello, D., Uytterhoeven, K.
$\theta$ 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
Externí odkaz:
http://arxiv.org/abs/1607.01035
Autor:
Mullally, F., Coughlin, Jeffery L., Thompson, Susan E., Christiansen, Jessie, Burke, Christopher, Clarke, Bruce D., Haas, Michael R.
We present a new automated method to identify instrumental features masquerading as small, long period planets in the \kepler\ planet candidate catalog. These systematics, mistakenly identified as planet transits, can have a strong impact on occurren
Externí odkaz:
http://arxiv.org/abs/1602.03204
Autor:
Henderson, Calen B., Poleski, Radosław, Penny, Matthew, Street, Rachel A., Bennett, David P., Hogg, David W., Gaudi, B. Scott, Zhu, W., Barclay, T., Barentsen, G., Howell, S. B., Mullally, F., Udalski, A., Szymański, M. K., Skowron, J., Mróz, P., Kozłowski, S., Wyrzykowski, Ł., Pietrukowicz, P., Soszyński, I., Ulaczyk, K., Pawlak, M., Sumi, T., Abe, F., Asakura, Y., Barry, R. K., Bhattacharya, A., Bond, I. A., Donachie, M., Freeman, M., Fukui, A., Hirao, Y., Itow, Y., Koshimoto, N., Li, M. C. A., Ling, C. H., Masuda, K., Matsubara, Y., Muraki, Y., Nagakane, M., Ohnishi, K., Oyokawa, H., Rattenbury, N., Saito, To., Sharan, A., Sullivan, D. J., Tristram, P. J., Yonehara, A., Bachelet, E., Bramich, D. M., Cassan, A., Dominik, M., Jaimes, R. Figuera, Horne, K., Hundertmark, M., Mao, S., Ranc, C., Schmidt, R., Snodgrass, C., Steele, I. A., Tsapras, Y., Wambsganss, J., Bozza, V., Burgdorf, M. J., Jørgensen, U. G., Novati, S. Calchi, Ciceri, S., D'Ago, G., Evans, D. F., Hessman, F. V., Hinse, T. C., Husser, T. -O., Mancini, L., Popovas, A., Rabus, M., Rahvar, S., Scarpetta, G., Skottfelt, J., Southworth, J., Unda-Sanzana, E., Bryson, S. T., Caldwell, D. A., Haas, M. R., Larson, K., McCalmont, K., Packard, M., Peterson, C., Putnam, D., Reedy, L., Ross, S., Van Cleve, J. E., Akeson, R., Batista, V., Beaulieu, J. -P., Beichman, C. A., Bryden, G., Ciardi, D., Cole, A., Coutures, C., Foreman-Mackey, D., Fouqué, P., Friedmann, M., Gelino, C., Kaspi, S., Kerins, E., Korhonen, H., Lang, D., Lee, C. -H., Lineweaver, C. H., Maoz, D., Marquette, J. -B., Mogavero, F., Morales, J. C., Nataf, D., Pogge, R. W., Santerne, A., Shvartzvald, Y., Suzuki, D., Tamura, M., Tisserand, P., Wang, D.
$K2$'s Campaign 9 ($K2$C9) will conduct a $\sim$3.7 deg$^{2}$ survey toward the Galactic bulge from 7/April through 1/July of 2016 that will leverage the spatial separation between $K2$ and the Earth to facilitate measurement of the microlens paralla
Externí odkaz:
http://arxiv.org/abs/1512.09142
Autor:
Coughlin, Jeffrey L., Mullally, F., Thompson, Susan E., Rowe, Jason F., Burke, Christopher J., Latham, David W., Batalha, Natalie M., Ofir, Aviv, Quarles, Billy L., Henze, Christopher E., Wolfgang, Angie, Caldwell, Douglas A., Bryson, Stephen T., Shporer, Avi, Catanzarite, Joseph, Akeson, Rachel, Barclay, Thomas, Borucki, William J., Boyajian, Tabetha S., Campbell, Jennifer R., Christiansen, Jessie L., Girouard, Forrest R., Haas, Michael R., Howell, Steve B., Huber, Daniel, Jenkins, Jon M., Li, Jie, Patil-Sabale, Anima, Quintana, Elisa V., Ramirez, Solange, Seader, Shawn, Smith, Jeffrey C., Tenenbaum, Peter, Twicken, Joseph D., Zamudio, Khadeejah A.
We present the seventh Kepler planet candidate catalog, which is the first to be based on the entire, uniformly processed, 48 month Kepler dataset. This is the first fully automated catalog, employing robotic vetting procedures to uniformly evaluate
Externí odkaz:
http://arxiv.org/abs/1512.06149
Autor:
Hallakoun, N., Maoz, D., Kilic, M., Mazeh, T., Gianninas, A., Agol, E., Bell, K. J., Bloemen, S., Brown, W. R., Debes, J., Faigler, S., Kull, I., Kupfer, T., Loeb, A., Morris, B. M., Mullally, F.
We report the discovery of the sixth known eclipsing double white dwarf (WD) system, SDSS J1152+0248, with a 2.3968 +/- 0.0003 h orbital period, in data from the Kepler Mission's K2 continuation. Analysing and modelling the K2 data together with grou
Externí odkaz:
http://arxiv.org/abs/1507.06311
Autor:
Burke, Christopher J., Christiansen, Jessie L., Mullally, F., Seader, Shawn, Huber, Daniel, Rowe, Jason F., Coughlin, Jeffrey L., Thompson, Susan E., Catanzarite, Joseph, Clarke, Bruce D., Morton, Timothy D., Caldwell, Douglas A., Bryson, Stephen T., Haas, Michael R., Batalha, Natalie M., Jenkins, Jon M., Tenenbaum, Peter, Twicken, Joseph D., Li, Jie, Quintana, Elisa, Barclay, Thomas, Henze, Christopher E., Borucki, William J., Howell, Steve B., Still, Martin
We measure planet occurrence rates using the planet candidates discovered by the Q1-Q16 Kepler pipeline search. This study examines planet occurrence rates for the Kepler GK dwarf target sample for planet radii, 0.75
Externí odkaz:
http://arxiv.org/abs/1506.04175
Autor:
Bours, M. C. P., Marsh, T. R., Gaensicke, B. T., Tauris, T. M., Istrate, A. G., Badenes, C., Dhillon, V. S., Gal-Yam, A., Hermes, J. J., Kengkriangkrai, S., Kilic, M., Koester, D., Mullally, F., Prasert, N., Steeghs, D., Thompson, S. E., Thorstensen, J. R.
We present Hubble Space Telescope UV spectra of the 4.6 h period double white dwarf SDSS J125733.63+542850.5. Combined with Sloan Digital Sky Survey optical data, these reveal that the massive white dwarf (secondary) has an effective temperature T2 =
Externí odkaz:
http://arxiv.org/abs/1505.05144
Autor:
Mullally, F., Coughlin, Jeffrey L., Thompson, Susan E., Rowe, Jason, Burke, Christopher, Latham, David W., Batalha, Natalie M., Bryson, Stephen T., Christiansen, Jessie, Henze, Christopher E., Ofir, Aviv, Quarles, Billy, Shporer, Avi, Van Eylen, Vincent, Van Laerhoven, Christa, Shah, Yash, Wolfgang, Angie, Chaplin, W. J., Xie, Ji-Wei, Akeson, Rachel, Argabright, Vic, Bachtell, Eric, Borucki, Thomas Barclay William J., Caldwell, Douglas A., Campbell, Jennifer R., Catanzarite, Joseph H., Cochran, William D., Duren, Riley M., Fleming, Scott W., Fraquelli, Dorothy, Girouard, Forrest R., Haas, Michael R., Hełminiak, Krzysztof G., Howell, Steve B., Huber, Daniel, Larson, Kipp, Gautier III, Thomas N., Jenkins, Jon, Li, Jie, Lissauer, Jack J., McArthur, Scot, Miller, Chris, Morris, Robert L., Patil-Sabale, Anima, Plavchan, Peter, Putnam, Dustin, Quintana, Elisa V., Ramirez, Solange, Aguirre, V. Silva, Seader, Shawn, Smith, Jeffrey C., Steffen, Jason H., Stewart, Chris, Stober, Jeremy, Still, Martin, Tenenbaum, Peter, Troeltzsch, John, Twicken, Joseph D., Zamudio, Khadeejah A.
\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:
http://arxiv.org/abs/1502.02038