Zobrazeno 1 - 10
of 11
pro vyhledávání: '"Schlecker, Martin"'
Autor:
Dietrich, Jeremy, Apai, Dániel, Schlecker, Martin, Hardegree-Ullman, Kevin K., Rackham, Benjamin V., Kurtovic, Nicolas, Molaverdikhani, Karan, Gabor, Paul, Henning, Thomas, Chen, Wen-Ping, Mancini, Luigi, Bixel, Alex, Gibbs, Aidan, Boyle, Richard P., Brown-Sevilla, Samantha, Burn, Remo, Delage, Timmy N., Flores-Rivera, Lizxandra, Franceschi, Riccardo, Pichierri, Gabriele, Savvidou, Sofia, Syed, Jonas, Bruni, Ivan, Ip, Wing-Huen, Ngeow, Chow-Choong, Tsai, An-Li, Lin, Chia-Lung, Hou, Wei-Jie, Hsiao, Hsiang-Yao, Lin, Chi-Sheng, Lin, Hung-Chin, Basant, Ritvik
Earth-sized exoplanets that transit nearby, late spectral type red dwarfs will be prime targets for atmospheric characterization in the coming decade. Such systems, however, are difficult to find via wide-field transit surveys like Kepler or TESS. Co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::feef65448baec996c6a423e85ab29191
http://arxiv.org/abs/2302.04138
http://arxiv.org/abs/2302.04138
Autor:
Schlecker, Martin, Burn, Remo, Sabotta, Silvia, Seifert, Antonia, Henning, Thomas, Emsenhuber, Alexandre, Mordasini, Christoph, Reffert, Sabine, Shan, Yu Tong, Klahr, Hubert
Planet formation is sensitive to the environment in protoplanetary disks, for which scaling laws as a function of stellar mass are known. Can the observed population of planets around low-mass stars be explained by these trends or is there evidence f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0d50b895c16c85ff190dffccb5b9066c
Autor:
Kemmer, Jonas, Stock, Stephan, Kossakowski, Diana, Dreizler, Stefan, Kaminski, Adrian, Molaverdikhani, Karan, Schlecker, Martin, Caballero, Jose A.
We present two small transiting planets with mass measurements orbiting bright mid M dwarfs (GJ 3473, GJ 3929). GJ 3473 b (Kemmer et al. 2020) is a hot, presumably rocky, planet (P = 1.198 d, Mb = 1.86 ± 0.30 Me, and radius, Rb = 1.264 ± 0.050 Re),
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0409459a58469450e6c8f2748921757b
Autor:
Hobson, Melissa J, Brahm, Rafael, Jordan, Andres, Henning, Thomas, Espinoza, Nestor, Rojas, Felipe, Trifonov, Trifon, Schlecker, Martin, Sarkis, Paula, Kossakowski, Diana, Tala, Marcelo
Giant, long-period exoplanets are vital to unveiling the underlying physics of planet formation and evolution. They are true relics of the planet formation process, maintaining their orbital and compositional properties, and their radii evolve withou
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fc61650419e18832b79bea0136f4d1d
Autor:
Schlecker, Martin
Advancing our understanding of planet formation is a prime motivation for the search for exoplanets. While it is now widely recognized that multiple planets per system are common, their mutual relationships are still largely unexplored. This thesis i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ab2859b73f25a9dcf79ba0d0271771b
Autor:
Espinoza, Néstor, Brahm, Rafael, Henning, Thomas, Jordán, Andrés, Dorn, Caroline, Rojas, Felipe, Sarkis, Paula, Kossakowski, Diana, Schlecker, Martin, Díaz, Matías R, Jenkins, James S, Aguilera-Gomez, Claudia, Jenkins, Jon M, Twicken, Joseph D, Collins, Karen A, Lissauer, Jack, Armstrong, David J, Adibekyan, Vardan, Barrado, David, Barros, Susana C C, Battley, Matthew, Bayliss, Daniel, Bouchy, François, Bryant, Edward M, Cooke, Benjamin F, Demangeon, Olivier D S, Dumusque, Xavier, Figueira, Pedro, Giles, Helen, Lillo-Box, Jorge, et al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b3250e07853142341228b85a1c7e248e
https://doi.org/10.5167/uzh-193880
https://doi.org/10.5167/uzh-193880
Autor:
Brahm, Rafael, Nielsen, Louise D., Wittenmyer, Robert A., Wang, Songhu, Rodriguez, Joseph E., Espinoza, N��stor, Jones, Mat��as I., Jord��n, Andr��s, Henning, Thomas, Hobson, Melissa, Kossakowski, Diana, Rojas, Felipe, Sarkis, Paula, Schlecker, Martin, Trifonov, Trifon, Shahaf, Sahar, Ricker, George, Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Addison, Brett C., Bakos, G��sp��r ��., Bhatti, Waqas, Bayliss, Daniel, Berlind, Perry, Bieryla, Allyson, Bouchy, Francois, Bowler, Brendan P., Brice��o, C��sar, Brown, Timothy M., Bryant, Edward M., Caldwell, Douglas A., Charbonneau, David, Collins, Karen A., Davis, Allen B., Esquerdo, Gilbert A., Fulton, Benjamin J., Guerrero, Natalia M., Henze, Christopher E., Hogan, Aleisha, Horner, Jonathan, Huang, Chelsea X., Irwin, Jonathan, Kane, Stephen R., Kielkopf, John, Mann, Andrew W., Mazeh, Tsevi, McCormac, James, McCully, Curtis, Mengel, Matthew W., Mireles, Ismael, Okumura, Jack, Plavchan, Peter, Quinn, Samuel N., Rabus, Markus, Saesen, Sophie, Schlieder, Joshua E., Segransan, Damien, Shiao, Bernie, Shporer, Avi, Siverd, Robert J., Stassun, Keivan G., Suc, Vincent, Tan, Thiam-Guan, Torres, Pascal, Tinney, Chris G., Udry, Stephane, Vanzi, Leonardo, Vezie, Michael, Vines, Jose I., Vuckovic, Maja, Wright, Duncan J., Yahalomi, Daniel A., Zapata, Abner, Zhang, Hui, Ziegler, Carl
We present the discovery of two new 10-day period giant planets from the Transiting Exoplanet Survey Satellite ($TESS$) mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have si
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::d205eeb60f0d17009f043763c28e50e7
Publikováno v:
European Planetary Science Congress
The, so far, unique and well constrained TRAPPIST-1 system can be exploited for testing planet formation theories. Because of observational biases, terrestrial planet formation models will, for the next decade, only be testable around low mass stars,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3a75b7cdbdfde8bf7d08ee98080a187b
https://hdl.handle.net/21.11116/0000-0005-CEA0-E
https://hdl.handle.net/21.11116/0000-0005-CEA0-E
Autor:
Schlecker, Martin
The transit method is the most successful tool for exoplanet discovery to date. With more than half of all known exoplanets discovered by \emph{Kepler} using this method, the mission also revealed a number of objects with dimming events that defy the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d96966ef8e04d92a30e473e12db6385
Autor:
Paul Mollière, Tamara Molyarova, Bertram Bitsch, Thomas Henning, Aaron Schneider, Laura Kreidberg, Christian Eistrup, Remo Burn, Evert Nasedkin, Dmitry Semenov, Christoph Mordasini, Martin Schlecker, Kamber R. Schwarz, Sylvestre Lacour, Mathias Nowak, Matthäus Schulik
Publikováno v:
Mollière, Paul; Molyarova, Tamara; Bitsch, Bertram; Henning, Thomas; Schneider, Aaron; Kreidberg, Laura; Eistrup, Christian; Burn, Remo; Nasedkin, Evert; Semenov, Dmitry; Mordasini, Christoph; Schlecker, Martin; Schwarz, Kamber R.; Lacour, Sylvestre; Nowak, Mathias; Schulik, Matthäus (2022). Interpreting the Atmospheric Composition of Exoplanets: Sensitivity to Planet Formation Assumptions. Astrophysical journal, 934(1), p. 74. Institute of Physics Publishing IOP 10.3847/1538-4357/ac6a56
The Astrophysical Journal
Molliere, P, Molyarova, T, Bitsch, B, Henning, T, Schneider, A, Kreidberg, L, Eistrup, C, Burn, R, Nasedkin, E, Semenov, D, Mordasini, C, Schlecker, M, Schwarz, K R, Lacour, S, Nowak, M & Schulik, M 2022, ' Interpreting the Atmospheric Composition of Exoplanets : Sensitivity to Planet Formation Assumptions ', Astrophysical Journal, vol. 934, no. 1, 74 . https://doi.org/10.3847/1538-4357/ac6a56
The Astrophysical Journal
Molliere, P, Molyarova, T, Bitsch, B, Henning, T, Schneider, A, Kreidberg, L, Eistrup, C, Burn, R, Nasedkin, E, Semenov, D, Mordasini, C, Schlecker, M, Schwarz, K R, Lacour, S, Nowak, M & Schulik, M 2022, ' Interpreting the Atmospheric Composition of Exoplanets : Sensitivity to Planet Formation Assumptions ', Astrophysical Journal, vol. 934, no. 1, 74 . https://doi.org/10.3847/1538-4357/ac6a56
Constraining planet formation based on the atmospheric composition of exoplanets is a fundamental goal of the exoplanet community. Existing studies commonly try to constrain atmospheric abundances, or to analyze what abundance patterns a given descri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4afca889cbb86b1336eb92fd27f3bbc4