Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Villanueva Jr, Steven"'
Autor:
Sgro, Lauren A., Dalba, Paul A., Esposito, Thomas M., Marchis, Franck, Dragomir, Diana, Villanueva Jr., Steven, Fulton, Benjamin, Billiani, Mario, Loose, Margaret, Meneghelli, Nicola, Rivett, Darren, Saibi, Fadi, Saibi, Sophie, Martin, Bryan, Lekkas, Georgios, Zaharevitz, Daniel, Zellem, Robert T., Terentev, Ivan A., Gagliano, Robert, Jacobs, Thomas Lee, Kristiansen, Martti H., LaCourse, Daryll M., Omohundro, Mark, Schwengeler, Hans M.
NASA's Transiting Exoplanet Survey Satellite (TESS) has identified over 7,000 candidate exoplanets via the transit method, with gas giants among the most readily detected due to their large radii. Even so, long intervals between TESS observations for
Externí odkaz:
http://arxiv.org/abs/2405.15021
Autor:
Dalba, Paul A., Kane, Stephen R., Isaacson, Howard, Fulton, Benjamin, Howard, Andrew W., Schwieterman, Edward W., Thorngren, Daniel P., Fortney, Jonathan, Vowell, Noah, Beard, Corey, Blunt, Sarah, Brinkman, Casey L., Chontos, Ashley, Dai, Fei, Giacalone, Steven, Hill, Michelle L., Kosiarek, Molly, Lubin, Jack, Mayo, Andrew W., Mocnik, Teo, Murphy, Joseph M. Akana, Petigura, Erik A., Rice, Malena, Rubenzahl, Ryan A., Van Zandt, Judah, Weiss, Lauren M., Dragomir, Diana, Kipping, David, Payne, Matthew J., Roy, Arpita, Teachey, Alex, Villanueva Jr, Steven
Discovering and characterizing exoplanets at the outer edge of the transit method's sensitivity has proven challenging owing to geometric biases and the practical difficulties associated with acquiring long observational baselines. Nonetheless, a sam
Externí odkaz:
http://arxiv.org/abs/2401.03021
Autor:
Mann, Christopher R., Dalba, Paul A., Lafrenière, David, Fulton, Benjamin J., Hébrard, Guillaume, Boisse, Isabelle, Dalal, Shweta, Deleuil, Magali, Delfosse, Xavier, Demangeon, Olivier, Forveille, Thierry, Heidari, Neda, Kiefer, Flavien, Martioli, Eder, Moutou, Claire, Endl, Michael, Cochran, William D., MacQueen, Phillip, Marchis, Franck, Dragomir, Diana, Gupta, Arvind F., Feliz, Dax L., Nicholson, Belinda A., Ziegler, Carl, Villanueva Jr., Steven, Rowe, Jason, Talens, Geert Jan, Thorngren, Daniel, LaCourse, Daryll, Jacobs, Tom, Howard, Andrew W., Bieryla, Allyson, Latham, David W., Rabus, Markus, Fetherolf, Tara, Hellier, Coel, Howell, Steve B., Plavchan, Peter, Reefe, Michael, Combs, Deven, Bowen, Michael, Wittrock, Justin, Ricker, George R., Seager, S., Winn, Joshua N., Jenkins, Jon M., Barclay, Thomas, Watanabe, David, Collins, Karen A., Eastman, Jason D., Ting, Eric B.
Publikováno v:
AJ, 166, 239 (2023)
Large-scale exoplanet surveys like the TESS mission are powerful tools for discovering large numbers of exoplanet candidates. Single-transit events are commonplace within the resulting candidate list due to the unavoidable limitation of observing bas
Externí odkaz:
http://arxiv.org/abs/2311.10232
Autor:
Dong, Jiayin, Wang, Songhu, Rice, Malena, Zhou, George, Huang, Chelsea X., Dawson, Rebekah I., Stefánsson, Gudmundur K., Halverson, Samuel, Kanodia, Shubham, Mahadevan, Suvrath, McElwain, Michael W., Alvarado-Montes, Jaime A., Ninan, Joe P., Robertson, Paul, Roy, Arpita, Schwab, Christian, Logsdon, Sarah E., Terrien, Ryan C., Collins, Karen A., Srdoc, Gregor, Sefako, Ramotholo, Laloum, Didier, Latham, David W., Bieryla, Allyson, Dalba, Paul A., Dragomir, Diana, Villanueva Jr., Steven, Howell, Steve B., Ricker, George R., Seager, S., Winn, Joshua N., Jenkins, Jon M., Shporer, Avi, Rapetti, David
Warm Jupiters are close-in giant planets with relatively large planet-star separations (i.e., $10< a/R_\star <100$). Given their weak tidal interactions with their host stars, measurements of stellar obliquity may be used to probe the initial obliqui
Externí odkaz:
http://arxiv.org/abs/2305.16495
Autor:
Hinkle, Jason T., Kochanek, Christopher S., Shappee, Benjamin J., Vallely, Patrick J., Auchettl, Katie, Fausnaugh, Michael, Holoien, Thomas W. -S., Treiber, Helena P., Payne, Anna V., Gaudi, B. Scott, Prieto, Jose L., Stassun, Keivan G., Thompson, Todd A., Tonry, John L., Villanueva Jr, Steven
We analyze high-cadence data from the Transiting Exoplanet Survey Satellite (TESS) of the ambiguous nuclear transient (ANT) ASASSN-18el. The optical changing-look phenomenon in ASASSN-18el has been argued to be due to either a drastic change in the a
Externí odkaz:
http://arxiv.org/abs/2206.04071
Autor:
Dalba, Paul A., Kane, Stephen R., Dragomir, Diana, Villanueva Jr., Steven, Collins, Karen A., Jacobs, Thomas Lee, Lacourse, Daryll M., Gagliano, Robert, Kristiansen, Martti H., Omohundro, Mark, Schwengeler, Hans M., Terentev, Ivan A., Vanderburg, Andrew, Fulton, Benjamin, Isaacson, Howard, Van Zandt, Judah, Howard, Andrew W., Thorngren, Daniel P., Howell, Steve B., Batalha, Natalie M., Chontos, Ashley, Crossfield, Ian J. M., Dressing, Courtney D., Huber, Daniel, Petigura, Erik A., Robertson, Paul, Roy, Arpita, Weiss, Lauren M., Behmard, Aida, Beard, Corey, Brinkman, Casey L., Giacalone, Steven, Hill, Michelle L., Lubin, Jack, Mayo, Andrew W., Močnik, Teo, Murphy, Joseph M. Akana, Polanski, Alex S., Rice, Malena, Rosenthal, Lee J., Rubenzahl, Ryan A., Scarsdale, Nicholas, Turtelboom, Emma V., Tyler, Dakotah, Benni, Paul, Boyce, Pat, Esposito, Thomas M., Girardin, E., Laloum, Didier, Lewin, Pablo, Mann, Christopher R., Marchis, Franck, Schwarz, Richard P., Srdoc, Gregor, Steuer, Jana, Sivarani, Thirupathi, Unni, Athira, Eisner, Nora L., Fetherolf, Tara, Li, Zhexing, Yao, Xinyu, Pepper, Joshua, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Burke, Christopher J., Eastman, Jason D., Lund, Michael B., Rodriguez, David R., Rowden, Pamela, Ting, Eric B., Villaseñor, Jesus Noel
We report the discovery of TOI-2180 b, a 2.8 $M_{\rm J}$ giant planet orbiting a slightly evolved G5 host star. This planet transited only once in Cycle 2 of the primary Transiting Exoplanet Survey Satellite (TESS) mission. Citizen scientists identif
Externí odkaz:
http://arxiv.org/abs/2201.04146
Autor:
Guerrero, Natalia M., Seager, S., Huang, Chelsea X., Vanderburg, Andrew, Soto, Aylin Garcia, Mireles, Ismael, Hesse, Katharine, Fong, William, Glidden, Ana, Shporer, Avi, Latham, David W., Collins, Karen A., Quinn, Samuel N., Burt, Jennifer, Dragomir, Diana, Crossfield, Ian, Vanderspek, Roland, Fausnaugh, Michael, Burke, Christopher J., Ricker, George, Daylan, Tansu, Essack, Zahra, Günther, Maximilian N., Osborn, Hugh P., Pepper, Joshua, Rowden, Pamela, Sha, Lizhou, Villanueva Jr., Steven, Yahalomi, Daniel A., Yu, Liang, Ballard, Sarah, Batalha, Natalie M., Berardo, David, Chontos, Ashley, Dittmann, Jason A., Esquerdo, Gilbert A., Mikal-Evans, Thomas, Jayaraman, Rahul, Krishnamurthy, Akshata, Louie, Dana R., Mehrle, Nicholas, Niraula, Prajwal, Rackham, Benjamin V., Rodriguez, Joseph E., Rowden, Stephen J. L., Sousa-Silva, Clara, Watanabe, David, Wong, Ian, Zhan, Zhuchang, Zivanovic, Goran, Christiansen, Jessie L., Ciardi, David R., Swain, Melanie A., Lund, Michael B., Mullally, Susan E., Fleming, Scott W., Rodriguez, David R., Boyd, Patricia T., Quintana, Elisa V., Barclay, Thomas, Colón, Knicole D., Rinehart, S. A., Schlieder, Joshua E., Clampin, Mark, Jenkins, Jon M., Twicken, Joseph D., Caldwell, Douglas A., Coughlin, Jeffrey L., Henze, Chris, Lissauer, Jack J., Morris, Robert L., Rose, Mark E., Smith, Jeffrey C., Tenenbaum, Peter, Ting, Eric B., Wohler, Bill, Bakos, G. Á., Bean, Jacob L., Berta-Thompson, Zachory K., Bieryla, Allyson, Bouma, Luke G., Buchhave, Lars A., Butler, Nathaniel, Charbonneau, David, Doty, John P., Ge, Jian, Holman, Matthew J., Howard, Andrew W., Kaltenegger, Lisa, Kane, Stephen R., Kjeldsen, Hans, Kreidberg, Laura, Lin, Douglas N. C., Minsky, Charlotte, Narita, Norio, Paegert, Martin, Pál, András, Palle, Enric, Sasselov, Dimitar D., Spencer, Alton, Sozzetti, Alessandro, Stassun, Keivan G., Torres, Guillermo, Udry, Stephane, Winn, Joshua N.
We present 2,241 exoplanet candidates identified with data from the Transiting Exoplanet Survey Satellite (TESS) during its two-year prime mission. We list these candidates in the TESS Objects of Interest (TOI) Catalog, which includes both new planet
Externí odkaz:
http://arxiv.org/abs/2103.12538
Autor:
Yao, Xinyu, Pepper, Joshua, Gaudi, B. Scott, Dalba, Paul A., Burt, Jennifer A., Wittenmyer, Robert A., Dragomir, Diana, Rodriguez, Joseph E., Villanueva, Jr., Steven, Stevens, Daniel J., Stassun, Keivan G., James, David J.
NASA's Transiting Exoplanet Survey Satellite (TESS) mission is expected to discover hundreds of planets via single transits first identified in their light curves. Determining the orbital period of these single transit candidates typically requires a
Externí odkaz:
http://arxiv.org/abs/2101.07964
Autor:
Mann, Andrew W., Johnson, Marshall C., Vanderburg, Andrew, Kraus, Adam L., Rizzuto, Aaron C., Wood, Mackenna L., Bush, Jonathan L., Rockcliffe, Keighley, Newton, Elisabeth R., Latham, David W., Mamajek, Eric E., Zhou, George, Quinn, Samuel N., Thao, Pa Chia, Benatti, Serena, Cosentino, Rosario, Desidera, Silvano, Harutyunyan, Avet, Lovis, Christophe, Mortier, Annelies, Pepe, Francesco A., Poretti, Ennio, Wilson, Thomas G., Kristiansen, Martti H., Gagliano, Robert, Jacobs, Thomas, LaCourse, Daryll M., Omohundro, Mark, Schwengeler, Hans Martin, Terentev, Ivan A., Kane, Stephen R., Hill, Michelle L., Rabus, Markus, Esquerdo, Gilbert A., Berlind, Perry, Collins, Karen A., Murawski, Gabriel, Sallam, Nezar Hazam, Aitken, Michael M., Massey, Bob, Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Barclay, Thomas, Caldwell, Douglas A., Dragomir, Diana, Doty, John P., Glidden, Ana, Tenenbaum, Peter, Torres, Guillermo, Twicken, Joseph D., Villanueva Jr, Steven
Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. Young planets ($<$1 Gyr) offer an opportunity to probe the critical early stages of this evolution, where pl
Externí odkaz:
http://arxiv.org/abs/2005.00047
Autor:
Dalba, Paul A., Gupta, Arvind F., Rodriguez, Joseph E., Dragomir, Diana, Huang, Chelsea X., Kane, Stephen R., Quinn, Samuel N., Bieryla, Allyson, Esquerdo, Gilbert A., Fulton, Benjamin J., Scarsdale, Nicholas, Batalha, Natalie M., Beard, Corey, Behmard, Aida, Chontos, Ashley, Crossfield, Ian J. M., Dressing, Courtney D., Giacalone, Steven, Hill, Michelle L., Hirsch, Lea A., Howard, Andrew W., Huber, Daniel, Isaacson, Howard, Kosiarek, Molly, Lubin, Jack, Mayo, Andrew W., Mocnik, Teo, Murphy, Joseph M. Akana, Petigura, Erik A., Robertson, Paul, Rosenthal, Lee J., Roy, Arpita, Rubenzahl, Ryan A., Van Zandt, Judah, Weiss, Lauren M., Knudstrup, Emil, Andersen, Mads F., Grundahl, Frank, Yao, Xinyu, Pepper, Joshua, Villanueva Jr., Steven, Ciardi, David R., Cloutier, Ryan, Jacobs, Thomas Lee, Kristiansen, Martti H., LaCourse, Daryll M., Lendl, Monika, Osborn, Hugh P., Palle, Enric, Stassun, Keivan G., Stevens, Daniel J., Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M., Caldwell, Douglas A., Daylan, Tansu, Fong, William, Goeke, Robert F., Rose, Mark E., Rowden, Pamela, Schlieder, Joshua E., Smith, Jeffrey C., Vanderburg, Andrew
We report the detection of a Saturn-size exoplanet orbiting HD 332231 (TOI 1456) in light curves from the Transiting Exoplanet Survey Satellite (TESS). HD 332231, an F8 dwarf star with a V-band magnitude of 8.56, was observed by TESS in Sectors 14 an
Externí odkaz:
http://arxiv.org/abs/2003.10451