Zobrazeno 1 - 9
of 9
pro vyhledávání: '"Vach, Sydney"'
Autor:
Vach, Sydney, Zhou, George, Huang, Chelsea X., Mann, Andrew W., Barber, Madyson G., Bieryla, Allyson, Latham, David W., Collins, Karen A., Rogers, James G., Bouma, Luke G., Douglas, Stephanie T., Quinn, Samuel N., Fairnington, Tyler R., Krüger, Joachim, Shporer, Avi, Collins, Kevin I., Srdoc, Gregor, Schwarz, Richard P., Relles, Howard M., Barkaoui, Khalid, McLeod, Kim K., Schneider, Alayna, Narita, Norio, Fukui, Akihiko, Sefako, Ramotholo, Fong, William, Mireles, Ismael, Torres, Guillermo, Ricker, George R., Seager, Sara, Winn, Joshua N.
Observing and characterizing young planetary systems can aid in unveiling the evolutionary mechanisms that sculpt the mature exoplanet population. As an all-sky survey, NASA's Transiting Exoplanet Survey Satellite (TESS) has expanded the known young
Externí odkaz:
http://arxiv.org/abs/2407.19680
Autor:
Vach, Sydney, Zhou, George, Huang, Chelsea X., Rogers, James G, Bouma, L. G., Douglas, Stephanie T., Kunimoto, Michelle, Mann, Andrew W., Barber, Madyson G., Quinn, Samuel N., Latham, David W., Bieryla, Allyson, Collins, Karen
Within the first few hundreds of millions of years, many physical processes sculpt the eventual properties of young planets. NASA's TESS mission has surveyed young stellar associations across the entire sky for transiting planets providing glimpses i
Externí odkaz:
http://arxiv.org/abs/2403.03261
Autor:
Clark, Jake, Addison, Brett, Okumura, Jack, Vach, Sydney, Heitzmann, Alexis, Rodriguez, Joseph, Wright, Duncan, Clerte, Mathieu, Brown, Carolyn, Fetherolf, Tara, Wittenmyer, Robert, Plavchan, Peter, Kane, Stephen, Horner, Jonathan, Kielkopf, John, Shporer, Avi, Tinney, C., Hui-Gen, Liu, Ballard, Sarah, Bowler, Brendan, Mengel, Matthew, Zhou, George, Lee, Annette, David, Avelyn, Heim, Jessica, Lee, Michele, Sevilla, Veronica, Zafar, Naqsh, Hinkel, Natalie, Allen, Bridgette, Bayliss, Daniel, Berberyan, Arthur, Berlind, Perry, Bieryla, Allyson, Bouchy, Francois, Brahm, Rafael, Bryant, Edward, Christiansen, Jessie, Ciardi, David, Ciardi, Krys, Collins, Karen, Dallant, Jules, Davis, Allen, Diaz, Matias, Dressing, Courtney, Esquerdo, Gilbert, Harre, Jan-Vincent, Howell, Steve, Jenkins, Jon, Jensen, Eric, Jones, Matias, Jordan, Andres, Latham, David, Lund, Michael, McCormac, James, Nielsen, Louise, Otegi, Jon, Quinn, Samuel, Radford, Don, Ricker, George, Schwarz, Richard, Seager, Sara, Smith, Alexis, Stockdale, Chris, Tan, Thiam-Guan, Udry, Stephane, Vanderspek, Roland, Gunther, Maximilian, Wang, Songhu, Wingham, Geof, Winn, Joshua
Publikováno v:
AJ 165 207 (2023)
NASA's Transiting Exoplanet Survey Satellite (TESS) mission, has been uncovering a growing number of exoplanets orbiting nearby, bright stars. Most exoplanets that have been discovered by TESS orbit narrow-line, slow-rotating stars, facilitating the
Externí odkaz:
http://arxiv.org/abs/2212.08242
Autor:
Vach, Sydney, Quinn, Samuel N., Vanderburg, Andrew, Kane, Stephen R., Collins, Karen A., Kraus, Adam L., Zhou, George, Medina, Amber A., Schwarz, Richard P., Collins, Kevin I., Conti, Dennis M., Stockdale, Chris, Massey, Bob, Suarez, Olga, Guillot, Tristan, Mekarnia, Djamel, Abe, Lyu, Dransfield, Georgina, Crouzet, Nicolas, Triaud, Amaury H. M. J., Schmider, François-Xavier, Agabi, Abelkrim, Buttu, Marco, Furlan, Elise, Gnilka, Crystal L., Howell, Steve B., Ziegler, Carl, Briceño, César, Law, Nicholas, Mann, Andrew W., Rudat, Alexander, Colon, Knicole D., Rose, Mark E., Kunimoto, Michelle, Günther, Maximilian N., Charbonneau, David, Ciardi, David R., Ricker, George R., Vanderspek, Roland K., Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M.
As an all-sky survey, NASA's $TESS$ mission is able to detect the brightest and rarest types of transiting planetary systems, including young planets that enable study of the evolutionary processes that occur within the first billion years. Here, we
Externí odkaz:
http://arxiv.org/abs/2111.02416
Autor:
Rodriguez, Joseph E., Quinn, Samuel N., Zhou, George, Vanderburg, Andrew, Nielsen, Louise D., Wittenmyer, Robert A., Brahm, Rafael, Reed, Phillip A., Huang, Chelsea X., Vach, Sydney, Ciardi, David R., Oelkers, Ryan J., Stassun, Keivan G., Hellier, Coel, Gaudi, B. Scott, Eastman, Jason D., Collins, Karen A., Bieryla, Allyson, Christian, Sam, Latham, David W., Carleo, Ilaria, Wright, Duncan J., Matthews, Elisabeth, Gonzales, Erica J., Ziegler, Carl, Dressing, Courtney D., Howell, Steve B., Tan, Thiam-Guan, Wittrock, Justin, Plavchan, Peter, McLeod, Kim K., Baker, David, Wang, Gavin, Radford, Don, Schwarz, Richard P., Esposito, Massimiliano, Ricker, George R., Vanderspek, Roland K., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Addison, Brett, Anderson, D. R., Barclay, Thomas, Beatty, Thomas G., Berlind, Perry, Bouchy, Francois, Bowen, Michael, Bowler, Brendan P., Brasseur, C. E., Briceño, César, Caldwell, Douglas A., Calkins, Michael L., Chaturvedi, Priyanka, Chaverot, Guillaume, Chimaladinne, Sudhish, Christiansen, Jessie L., Collins, Kevin, Crossfield, Ian J. M., Eastridge, Kevin, Espinoza, N'estor, Esquerdo, Gilbert A., Feliz, Dax, Fenske, Tyler, Fong, William, Gan, Tianjun, Giacalone, Steven, Gill, Holden, Gordon, Lindsey, Granados, Alex, Grieves, Nolan, Guenther, Eike W., Guerrero, Natalia, Henning, Thomas, Henze, Christopher E., Hesse, Katharine, Hobson, Melissa J., Horner, Jonathan, James, David J., Jensen, Eric L. N., Jimenez, Mary, Jordán, Andrés, Kane, Stephen R., Kielkopf, John, Kim, Kingsley, Kuhn, Rudolf B., Latouf, Natasha, Law, Nicholas M., Levine, Alan M., Lund, Michael B., Mann, Andrew W., Mao, Shude, Matson, Rachel A., McDermott, Scott, Mengel, Matthew W., Mink, Jessica, Newman, Patrick, O'Dwyer, Tanner, Okumura, Jack, Palle, Enric, Pepper, Joshua, Quintana, Elisa V., Sarkis, Paula, Savel, Arjun, Schlieder, Joshua E., Schnaible, Chloe, Shporer, Avi, Sefako, Ramotholo, Seidel, Julia, Siverd, Robert J., Skinner, Brett, Stalport, Manu, Stevens, Daniel J., Stibbards, Caitlin, Tinney, C. G., West, R. G., Yahalomi, Daniel A., Zhang, Hui
We present the discovery and characterization of five hot and warm Jupiters -- TOI-628 b (TIC 281408474; HD 288842), TOI-640 b (TIC 147977348), TOI-1333 b (TIC 395171208, BD+47 3521A), TOI-1478 b (TIC 409794137), and TOI-1601 b (TIC 139375960) -- bas
Externí odkaz:
http://arxiv.org/abs/2101.01726
Akademický článek
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Akademický článek
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Autor:
Vach, Sydney, Quinn, Samuel N, Vanderburg, Andrew, Kane, Stephen A., Collins, Karen A., Kraus, Adam L., Zhou, George
Most of the significant changes in planetary evolution occur within the first billion years. Observing young planetary systems allows us to understand the physical mechanisms driving these changes in ways that observations of mature planets cannot. T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::56baa54e8b602258a0c7cd7486d13bdd
Autor:
Vach, Sydney
We report the discovery of TOI-640b from NASA’s Transiting Exoplanet Survey Satellite (TESS) mission, a hot Jupiter orbiting a newly evolved sub-giant star with a period of 5.0039 0:0003 days. Using photometric data collected from TESS, we extracte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4d86767acd5667f2de6292d3f020ef58