Zobrazeno 1 - 10
of 189
pro vyhledávání: '"Bakos , Gaspar"'
Autor:
Pinto, Marcelo Tala, Jordán, Andrés, Acuña, Lorena, Jones, Matías, Brahm, Rafael, Reinarz, Yared, Eberhardt, Jan, Espinoza, Néstor, Henning, Thomas, Hobson, Melissa, Rojas, Felipe, Schlecker, Martin, Trifonov, Trifon, Bakos, Gaspar, Boyle, Gavin, Csubry, Zoltan, Hartmann, Joel, Knepper, Benjamin, Kreidberg, Laura, Suc, Vincent, Teske, Johanna, Butler, R. Paul, Crane, Jeffrey, Schectman, Steve, Thompson, Ian, Osip, Dave, Ricker, George, Collins, Karen A., Watkins, Cristilyn N., Bieryla, Allyson, Stockdale, Chris, Wang, Gavin, Zambelli, Roberto, Seager, Sara, Winn, Joshua, Rose, Mark E., Rice, Malena, Essack, Zahra
We report the discovery and characterization of three new transiting giant planets orbiting TOI-6628, TOI-3837 and TOI-5027, and one new warm sub-Saturn orbiting TOI-2328, whose transits events were detected in the lightcurves of the Transiting Exopl
Externí odkaz:
http://arxiv.org/abs/2412.02069
Autor:
Bryant, Edward M., Bayliss, Daniel, Hartman, Joel D., Sedaghati, Elyar, Hobson, Melissa J., Jordán, Andrés, Brahm, Rafael, Bakos, Gaspar Á., Almenara, Jose Manuel, Barkaoui, Khalid, Bonfils, Xavier, Cointepas, Marion, Collins, Karen A., Dransfield, Georgina, Evans, Phil, Gillon, Michaël, Jehin, Emmanuël, Murgas, Felipe, Pozuelos, Francisco J., Schwarz, Richard P., Timmermans, Mathilde, Watkins, Cristilyn N., Wünsche, Anaël, Butler, R. Paul, Crane, Jeffrey D., Shectman, Steve, Teske, Johanna K., Charbonneau, David, Essack, Zahra, Jenkins, Jon M., Lewis, Hannah M., Seager, Sara, Ting, Eric B., Winn, Joshua N.
Short-period gas giant planets have been shown to be significantly rarer for host stars less massive than the Sun. We report the discovery of two transiting giant planets - TOI-2379 b and TOI-2384 b - with low-mass (early M) host stars. Both planets
Externí odkaz:
http://arxiv.org/abs/2409.01239
Autor:
Hartman, Joel D., Bayliss, Daniel, Brahm, Rafael, Bryant, Edward M., Jordán, Andrés, Bakos, Gáspár Á., Hobson, Melissa J., Sedaghati, Elyar, Bonfils, Xavier, Cointepas, Marion, Almenara, Jose Manuel, Barkaoui, Khalid, Timmermans, Mathilde, Dransfield, George, Ducrot, Elsa, Zúñiga-Fernández, Sebastián, Hooton, Matthew J., Pedersen, Peter Pihlmann, Pozuelos, Francisco J., Triaud, Amaury H. M. J., Gillon, Michaël, Jehin, Emmanuel, Waalkes, William C., Berta-Thompson, Zachory K., Howell, Steve B., Furlan, Elise, Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Rapetti, David, Collins, Karen A., Charbonneau, David, Burke, Christopher J., Rodriguez, David R.
We present the discovery of TOI 762 A b and TIC 46432937 b, two giant planets transiting M dwarf stars. Transits of both systems were first detected from observations by the NASA TESS mission, and the transiting objects are confirmed as planets throu
Externí odkaz:
http://arxiv.org/abs/2407.07187
Autor:
Bouma, Luke G., Jayaraman, Rahul, Rappaport, Saul, Rebull, Luisa M., Hillenbrand, Lynne A., Winn, Joshua N., David-Uraz, Alexandre, Bakos, Gáspár Á.
Complex periodic variables (CPVs) are stars that exhibit highly structured and periodic optical light curves. Previous studies have indicated that these stars are typically disk-free pre-main-sequence M dwarfs with rotation periods ranging from 0.2 t
Externí odkaz:
http://arxiv.org/abs/2309.06471
Autor:
Pribulla, Theodor, Borkovits, Tamás, Jayaraman, Rahul, Rappaport, Saul, Mitnyan, Tibor, Zasche, Petr, Komžík, Richard, Pál, András, Uhlař, Robert, Mašek, Martin, Henzl, Zbyněk, Bíró, Imre Barna, Csányi, István, Stuik, Remko, Kristiansen, Martti H., Schwengeler, Hans M., Gagliano, Robert, Jacobs, Thomas L., Omohundro, Mark, Kostov, Veselin, Powell, Brian P., Terentev, Ivan A., Vanderburg, Andrew, LaCourse, Daryll, Rodriguez, Joseph E., Bakos, Gáspár, Csubry, Zoltán, Hartman, Joel
We have found that the 2+2 quadruple star system BU CMi is currently the most compact quadruple system known, with an extremely short outer period of only 121 days. The previous record holder was TIC 219006972 (Kostov et al. 2023), with a period of 1
Externí odkaz:
http://arxiv.org/abs/2307.01521
Autor:
Trifonov, Trifon, Brahm, Rafael, Espinoza, Nestor, Henning, Thomas, Jordán, Andrés, Nesvorny, David, Dawson, Rebekah I., Lissauer, Jack J., Lee, Man Hoi, Kossakowski, Diana, Rojas, Felipe I., Hobson, Melissa J., Sarkis, Paula, Schlecker, Martin, Bitsch, Bertram, Bakos, Gaspar Á., Barbieri, Mauro, Bhatti, Waqas, Butler, R. Paul, Crane, Jeffrey D., Nandakumar, Sangeetha, Díaz, Matías R., Shectman, Stephen, Teske, Johanna, Torres, Pascal, Suc, Vincent, Vines, Jose I., Wang, Sharon X., Ricker, George R., Shporer, Avi, Vanderburg, Andrew, Dragomir, Diana, Vanderspek, Roland, Burke, Christopher J., Daylan, Tansu, Shiao, Bernie, Jenkins, Jon M., Wohler, Bill, Seager, Sara, Winn, Joshua N.
TOI-2202 b is a transiting warm Jovian-mass planet with an orbital period of P=11.91 days identified from the Full Frame Images data of five different sectors of the TESS mission. Ten TESS transits of TOI-2202 b combined with three follow-up light cu
Externí odkaz:
http://arxiv.org/abs/2108.05323
Astrophysical time series often contain periodic signals. The large and growing volume of time series data from photometric surveys demands computationally efficient methods for detecting and characterizing such signals. The most efficient algorithms
Externí odkaz:
http://arxiv.org/abs/2101.12348
Autor:
Lindor, Bethlee M., Hartman, Joel D., Bakos, Gáspár Á., Bhatti, Waqas, Csubry, Zoltan, Penev, Kaloyan, Bieryla, Allyson, Latham, David W., Torres, Guillermo, Buchhave, Lars A., Kovács, Géza, de Val-Borro, Miguel, Howard, Andrew W., Isaacson, Howard, Fulton, Benjamin J., Boisse, Isabelle, Santerne, Alexandre, Hébrard, Guillaume, Kovács, Támás, Huang, Chelsea X., Dembicky, Jack, Falco, Emilio, Everett, Mark E., Horch, Elliott P., Lázár, József, Papp, István, Sári, Pál
Publikováno v:
AJ 161 64 (2021)
We report the discovery by the ground-based HATNet survey of the transiting exoplanet HAT-P-68b, which has a mass of 0.724 $\pm$ 0.043 $M_{Jup}$, and radius of 1.072 $\pm$ 0.012 $R_{Jup}$. The planet is in a circular P = 2.2984-day orbit around a mod
Externí odkaz:
http://arxiv.org/abs/2010.16026
Autor:
Sha, Lizhou, Huang, Chelsea X., Shporer, Avi, Rodriguez, Joseph E., Vanderburg, Andrew, Brahm, Rafael, Hagelberg, Janis, Matthews, Elisabeth C., Ziegler, Carl, Livingston, John H., Stassun, Keivan G., Wright, Duncan J., Crane, Jeffrey D., Espinoza, Néstor, Bouchy, François, Bakos, Gáspár Á., Collins, Karen A., Zhou, George, Bieryla, Allyson, Hartman, Joel D., Wittenmyer, Robert A., Nielsen, Louise D., Plavchan, Peter, Bayliss, Daniel, Sarkis, Paula, Tan, Thiam-Guan, Cloutier, Ryan, Mancini, Luigi, Jordán, Andrés, Wang, Sharon, Henning, Thomas, Narita, Norio, Penev, Kaloyan, Teske, Johanna K., Kane, Stephen R., Mann, Andrew W., Addison, Brett C., Tamura, Motohide, Horner, Jonathan, Barbieri, Mauro, Burt, Jennifer A., Díaz, Matías R., Crossfield, Ian J. M., Dragomir, Diana, Drass, Holger, Feinstein, Adina D., Zhang, Hui, Hart, Rhodes, Kielkopf, John F., Jensen, Eric L. N., Montet, Benjamin T., Ottoni, Gaël, Schwarz, Richard P., Rojas, Felipe, Nespral, David Lopez Fdez, Torres, Pascal, Mengel, Matthew W., Udry, Stéphane, Zapata, Abner, Snoddy, Erin, Okumura, Jack, Ricker, George R., Vanderspek, Roland K., Latham, David W., Winn, Joshua N., Seager, Sara, Jenkins, Jon M., Colón, Knicole D., Henze, Christopher E., Krishnamurthy, Akshata, Ting, Eric B., Vezie, Michael, Villanueva, Steven
Publikováno v:
AJ 161 (2021) 82
We report the discovery of two short-period Saturn-mass planets, one transiting the G subgiant TOI-954 (TIC 44792534, $ V = 10.343 $, $ T = 9.78 $) observed in TESS sectors 4 and 5, and one transiting the G dwarf K2-329 (EPIC 246193072, $ V = 12.70 $
Externí odkaz:
http://arxiv.org/abs/2010.14436
Autor:
Schlecker, Martin, Kossakowski, Diana, Brahm, Rafael, Espinoza, Néstor, Henning, Thomas, Carone, Ludmila, Molaverdikhani, Karan, Trifonov, Trifon, Mollière, Paul, Hobson, Melissa J., Jordán, Andrés, Rojas, Felipe I., Klahr, Hubert, Sarkis, Paula, Bakos, Gáspár Á., Bhatti, Waqas, Osip, David, Suc, Vincent, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Vezie, Michael, Villaseñor, Jesus Noel, Rose, Mark E., Rodriguez, David R., Rodriguez, Joseph E., Quinn, Samuel N., Shporer, Avi
The orbital parameters of warm Jupiters serve as a record of their formation history, providing constraints on formation scenarios for giant planets on close and intermediate orbits. Here, we report the discovery of TIC 237913194b, detected in full f
Externí odkaz:
http://arxiv.org/abs/2010.03570