Zobrazeno 41 - 50
of 595
pro vyhledávání: '"Gaudi, B. Scott"'
Autor:
Johnson, Samson A., Penny, Matthew T., Gaudi, B. Scott, Kerins, Eamonn, Rattenbury, Nicholas J., Robin, Annie C., Novati, Sebastiano Calchi, Henderson, Calen B.
The Nancy Grace Roman Space Telescope (Roman) will perform a Galactic Exoplanet Survey (RGES) to discover bound exoplanets with semi-major axes greater than 1 au using gravitational microlensing. Roman will even be sensitive to planetary mass objects
Externí odkaz:
http://arxiv.org/abs/2006.10760
Autor:
Ahlers, John P., Johnson, Marshall C., Stassun, Keivan G, Colon, Knicole D., Barnes, Jason W., Stevens, Daniel J., Beatty, Thomas, Gaudi, B. Scott, Collins, Karen A., Rodriguez, Joseph, Ricker, George, Vanderspek, Roland, Latham, David, Seager, Sara, Winn, Joshua, Jenkins, Jon M., Caldwell, Douglas A., Goeke, Robert F., Osborn, Hugh P., Paegert, Martin, Rowden, Pam, Tenenbaum, Peter
KELT-9 b is an ultra hot Jupiter transiting a rapidly rotating, oblate early-A-type star in a polar orbit. We model the effect of rapid stellar rotation on KELT-9 b's transit light curve using photometry from the Transiting Exoplanet Survey Satellite
Externí odkaz:
http://arxiv.org/abs/2004.14812
Autor:
Hirao, Yuki, Bennett, David P., Ryu, Yoon-Hyun, Koshimoto, Naoki, Udalski, Andrzej, Yee, Jennifer C., Sumi, Takahiro, Bond, Ian A., Shvartzvald, Yossi, Abe, Fumio, Barry, Richard K., Bhattacharya, Aparna, Donachie, Martin, Fukui, Akihiko, Itow, Yoshitaka, Kondo, Iona, Li, Man Cheung Alex, Matsubara, Yutaka, Matsuo, Taro, Miyazaki, Shota, Muraki, Yasushi, Nagakane, Masayuki, Ranc, Clement, Rattenbury, Nicholas J., Suematsu, Haruno, Shibai, Hiroshi, Suzuki, Daisuke, Tristram, Paul J., Yonehara, Atsunori, Skowron, J., Poleski, R., Mroz, P., Szymanski, M. K., Soszynski, I., Kozlowski, S., Pietrukowicz, P., Ulaczyk, K., Rybicki, K., Iwanek, P., Albrow, Michael D., Chung, Sun-Ju, Gould, Andrew, Han, Cheongho, Hwang, Kyu-Ha, Jung, Youn Kil, Shin, In-Gu, Zang, Weicheng, Cha, Sang-Mok, Kim, Dong-Jin, Kim, Hyoun-Woo, Kim, Seung-Lee, Lee, Chung-Uk, Lee, Dong-Joo, Lee, Yongseok, Park, Byeong-Gon, Pogge, Richard W., Beichman, Charles A., Bryden, Geoffery, Novati, Sebastiano Calchi, Carey, Sean, Gaudi, B. Scott, Henderson, Calen B., Zhu, Wei, Bachelet, Etienne, Bolt, Greg, Christie, Grant, Hundertmark, Markus, Natusch, Tim, Maoz, Dan, McCormick, Jennie, Street, Rachel A., Tan, Thiam-Guan, Tsapras, Yiannis, Jorgensen, U. G., Dominik, M., Bozza, V., Skottfelt, J., Snodgrass, C., Ciceri, S., Jaimes, R. Figuera, Evans, D. F., Peixinho, N., Hinse, T. C., Burgdorf, M. J., Southworth, J., Rahvar, S., Sajadian, S., Rabus, M., von Essen, C., Fujii, Y. I., Campbell-White, J., Lowry, S., Helling, C., Mancini, L., Haikala, L., Kandori, Ryo
We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the ${\it Spitzer}$ satellite in a solar orbit. At high magnification, the anomaly in the light curve was dens
Externí odkaz:
http://arxiv.org/abs/2004.09067
Autor:
Gaudi, B. Scott, Seager, Sara, Mennesson, Bertrand, Kiessling, Alina, Warfield, Keith, Cahoy, Kerri, Clarke, John T., Domagal-Goldman, Shawn, Feinberg, Lee, Guyon, Olivier, Kasdin, Jeremy, Mawet, Dimitri, Plavchan, Peter, Robinson, Tyler, Rogers, Leslie, Scowen, Paul, Somerville, Rachel, Stapelfeldt, Karl, Stark, Christopher, Stern, Daniel, Turnbull, Margaret, Amini, Rashied, Kuan, Gary, Martin, Stefan, Morgan, Rhonda, Redding, David, Stahl, H. Philip, Webb, Ryan, Alvarez-Salazar, Oscar, Arnold, William L., Arya, Manan, Balasubramanian, Bala, Baysinger, Mike, Bell, Ray, Below, Chris, Benson, Jonathan, Blais, Lindsey, Booth, Jeff, Bourgeois, Robert, Bradford, Case, Brewer, Alden, Brooks, Thomas, Cady, Eric, Caldwell, Mary, Calvet, Rob, Carr, Steven, Chan, Derek, Cormarkovic, Velibor, Coste, Keith, Cox, Charlie, Danner, Rolf, Davis, Jacqueline, Dewell, Larry, Dorsett, Lisa, Dunn, Daniel, East, Matthew, Effinger, Michael, Eng, Ron, Freebury, Greg, Garcia, Jay, Gaskin, Jonathan, Greene, Suzan, Hennessy, John, Hilgemann, Evan, Hood, Brad, Holota, Wolfgang, Howe, Scott, Huang, Pei, Hull, Tony, Hunt, Ron, Hurd, Kevin, Johnson, Sandra, Kissil, Andrew, Knight, Brent, Kolenz, Daniel, Kraus, Oliver, Krist, John, Li, Mary, Lisman, Doug, Mandic, Milan, Mann, John, Marchen, Luis, Marrese-Reading, Colleen, McCready, Jonathan, McGown, Jim, Missun, Jessica, Miyaguchi, Andrew, Moore, Bradley, Nemati, Bijan, Nikzad, Shouleh, Nissen, Joel, Novicki, Megan, Perrine, Todd, Pineda, Claudia, Polanco, Otto, Putnam, Dustin, Qureshi, Atif, Richards, Michael, Riggs, A. J. Eldorado, Rodgers, Michael, Rud, Mike, Saini, Navtej, Scalisi, Dan, Scharf, Dan, Schulz, Kevin, Serabyn, Gene, Sigrist, Norbert, Sikkia, Glory, Singleton, Andrew, Shaklan, Stuart, Smith, Scott, Southerd, Bart, Stahl, Mark, Steeves, John, Sturges, Brian, Sullivan, Chris, Tang, Hao, Taras, Neil, Tesch, Jonathan, Therrell, Melissa, Tseng, Howard, Valente, Marty, Van Buren, David, Villalvazo, Juan, Warwick, Steve, Webb, David, Westerhoff, Thomas, Wofford, Rush, Wu, Gordon, Woo, Jahning, Wood, Milana, Ziemer, John, Arney, Giada, Anderson, Jay, Maíz-Apellániz, Jesús, Bartlett, James, Belikov, Ruslan, Bendek, Eduardo, Cenko, Brad, Douglas, Ewan, Dulz, Shannon, Evans, Chris, Faramaz, Virginie, Feng, Y. Katherina, Ferguson, Harry, Follette, Kate, Ford, Saavik, García, Miriam, Geha, Marla, Gelino, Dawn, Götberg, Ylva, Hildebrandt, Sergi, Hu, Renyu, Jahnke, Knud, Kennedy, Grant, Kreidberg, Laura, Isella, Andrea, Lopez, Eric, Marchis, Franck, Macri, Lucas, Marley, Mark, Matzko, William, Mazoyer, Johan, McCandliss, Stephan, Meshkat, Tiffany, Mordasini, Christoph, Morris, Patrick, Nielsen, Eric, Newman, Patrick, Petigura, Erik, Postman, Marc, Reines, Amy, Roberge, Aki, Roederer, Ian, Ruane, Garreth, Schwieterman, Edouard, Sirbu, Dan, Spalding, Christopher, Teplitz, Harry, Tumlinson, Jason, Turner, Neal, Werk, Jessica, Wofford, Aida, Wyatt, Mark, Young, Amber, Zellem, Rob
The Habitable Exoplanet Observatory, or HabEx, has been designed to be the Great Observatory of the 2030s. For the first time in human history, technologies have matured sufficiently to enable an affordable space-based telescope mission capable of di
Externí odkaz:
http://arxiv.org/abs/2001.06683
Autor:
Martínez, Romy Rodríguez, Gaudi, B. Scott, Rodriguez, Joseph E., Zhou, George, Labadie-Bartz, Jonathan, Quinn, Samuel N., Penev, Kaloyan Minev, Tan, Thiam-Guan, Latham, David W., Paredes, Leonardo A., Kielkopf, John, Addison, Brett C., Wright, Duncan J., Teske, Johanna K., Howell, Steve B., Ciardi, David R., Ziegler, Carl, Stassun, Keivan G., Johnson, Marshall C., Eastman, Jason D., Siverd, Robert J., Beatty, Thomas G., Bouma, Luke G., Pepper, Joshua, Lund, Michael B., Villanueva, Steven, Stevens, Daniel J., Jensen, Eric L. N., Kilby, Coleman, Cohen, David H., Bayliss, Daniel, Bieryla, Allyson, Cargile, Phillip A., Collins, Karen A., Conti, Dennis M., Colon, Knicole D., Curtis, Ivan A., DePoy, Darren L., Evans, Phil A., Feliz, Dax, Gregorio, Joao, Rothenberg, Jason, James, David J., Penny, Matthew T., Reed, Phillip A., Relles, Howard M., Stephens, Denise C., Joner, Michael D., Kuhn, Rudolf B., Stockdale, Chris, Trueblood, Mark, Trueblood, Patricia, Yao, Xinyu, Zambelli, Roberto, Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Henry, Todd J., James, Hodari-Sadiki, Jao, Wei-Chun, Wang, Sharon X., Butler, R. Paul, Crane, Jeffrey D., Thompson, Ian B., Schectman, Stephen, Wittenmyer, Robert A., Bedding, Timothy R., Okumura, Jack, Plavchan, Peter, Bowler, Brendan P., Horner, Jonathan, Kane, Stephen R., Mengel, Matthew W., Morton, Timothy D., Tinney, C. G., Zhang, Hui, Scott, Nicholas J., Matson, Rachel A., Everett, Mark E., Tokovinin, Andrei, Mann, Andrew W., Dragomir, Diana, Guenther, Maximilian N., Ting, Eric B., Fausnaugh, Michael, Glidden, Ana, Quintana, Elisa V., Manner, Mark, Marshall, Jennifer L., McLeod, Kim K., Khakpash, Somayeh
We present the discoveries of KELT-25b (TIC 65412605, TOI-626.01) and KELT-26b (TIC 160708862, TOI-1337.01), two transiting companions orbiting relatively bright, early A-stars. The transit signals were initially detected by the KELT survey, and subs
Externí odkaz:
http://arxiv.org/abs/1912.01017
Autor:
Pepper, Joshua, Kane, Stephen R., Rodriguez, Joseph E., Hinkel, Natalie R., Eastman, Jason D., Daylan, Tansu, Mocnik, Teo, Dalba, Paul A., Fetherolf, Tara, Stassun, Keivan G., Campante, Tiago L., Vanderburg, Andrew, Huber, Daniel, Gaudi, B. Scott, Bossini, Diego, Crossfield, Ian, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Twicken, Joseph D., Rose, Mark, Smith, Jeffrey C., Glidden, Ana, Levine, Alan M., Rinehart, Stephen, Collins, Karen A., Mann, Andrew W., Burt, Jennifer A., James, David J., Siverd, Robert J.
The exoplanet HD 118203 b, orbiting a bright (V = 8.05) host star, was discovered using the radial velocity method by da Silva et al. (2006), but was not previously known to transit. TESS photometry has revealed that this planet transits its host sta
Externí odkaz:
http://arxiv.org/abs/1911.05150
Autor:
Stevens, Daniel J., Zhou, George, Johnson, Marshall C., Rizzuto, Aaron C., Rodriguez, Joseph E., Bieryla, Allyson, Villanueva, Jr., Steven, Wright, Jason T., Gaudi, B. Scott, Latham, David W., Beatty, Thomas G., Lund, Michael B., Siverd, Robert J., Kraus, Adam L., Berlind, Perry, Calkins, Michael L., Esquerdo, Gilbert A., Kuhn, Rudolf B., Pepper, Joshua
We present the discovery of \thisstar\ (HD 58730), a very low mass ratio ($q \equiv M_2/M_1 \approx 0.07$) eclipsing binary (EB) identified by the Kilodegree Extremely Little Telescope (KELT) survey. We present the discovery light curve and perform a
Externí odkaz:
http://arxiv.org/abs/1910.06212
Autor:
Mansfield, Megan, Bean, Jacob L., Stevenson, Kevin B., Komacek, Thaddeus D., Bell, Taylor J., Tan, Xianyu, Malik, Matej, Beatty, Thomas G., Wong, Ian, Cowan, Nicolas B., Dang, Lisa, Désert, Jean-Michel, Fortney, Jonathan J., Gaudi, B. Scott, Keating, Dylan, Kempton, Eliza M. -R., Kreidberg, Laura, Line, Michael R., Parmentier, Vivien, Stassun, Keivan G., Swain, Mark R., Zellem, Robert T.
Publikováno v:
Astrophysical Journal Letters, 888, L15 (2020)
Phase curve observations provide an opportunity to study the full energy budgets of exoplanets by quantifying the amount of heat redistributed from their daysides to their nightsides. Theories explaining the properties of phase curves for hot Jupiter
Externí odkaz:
http://arxiv.org/abs/1910.01567
Exoplanets have been observed around stars at all stages of stellar evolution, in many cases orbiting in configurations that will eventually lead to the planets being engulfed or consumed by their host stars, such as Hot Jupiters or ultra-short perio
Externí odkaz:
http://arxiv.org/abs/1909.05259
Autor:
Gaudi, B. Scott, Clarke, John C., Domagal-Goldman, Shawn, Fischer, Debra, Kiessling, Alina, Mennesson, Bertrand, Peterson, Bradley M., Roberge, Aki, Stern, Dan, Warfield, Keith
The Hubble Space Telescope (HST) has been the most impactful science-driven mission ever flown by NASA. However, when HST reaches the end of its life, there will be a void due to the loss of some of the science capabilities afforded by HST to astrono
Externí odkaz:
http://arxiv.org/abs/1908.03277