Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Guadalupe Tovar Mendoza"'
Autor:
Tobin M. Wainer, James R. A. Davenport, Guadalupe Tovar Mendoza, Adina D. Feinstein, Tom Wagg
Publikováno v:
The Astronomical Journal, Vol 168, Iss 6, p 232 (2024)
We examine 4 yr of Kepler 30 minutes data, and five sectors of Transiting Exoplanet Survey Satellite 2 minutes data for the dM3 star KIC-8507979/TIC-272272592. This rapidly rotating ( P = 1.2 day) star has previously been identified as flare active,
Externí odkaz:
https://doaj.org/article/b24b520ac4284d9b9867716c036fb7a0
Autor:
Lynnae C. Quick, Aki Roberge, Guadalupe Tovar Mendoza, Elisa V. Quintana, Allison A. Youngblood
Publikováno v:
The Astrophysical Journal, Vol 956, Iss 1, p 29 (2023)
We have estimated total internal heating rates and depths to possible subsurface oceans for 17 planets that may be cold ocean planets, low-mass exoplanets with equilibrium surface temperatures and/or densities that are consistent with icy surfaces an
Externí odkaz:
https://doaj.org/article/d0d398713efd48a69c5a56e60b0a2782
Publikováno v:
The Astronomical Journal. 164:17
Stellar variability is a limiting factor for planet detection and characterization, particularly around active M-type stars. Here we revisit one of the most active stars from the Kepler mission, the M4 star GJ 1243, and use a sample of 414 flare even
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1a5a05aec4659a9d7124846abfb06a87
https://doi.org/10.3847/1538-3881/ac6fe6
https://doi.org/10.3847/1538-3881/ac6fe6
The flaring M4 dwarf GJ 1243 has become a benchmark for studying stellar flare and starspot activity thanks to the exceptional photometric monitoring archive from the Kepler mission. New light curves from the TESS mission for this star allow precise
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1940cf26d8e37407c02baac6ab482595
Autor:
Jacob Lustig-Yaeger, Edward W. Schwieterman, Guadalupe Tovar Mendoza, Yuka Fujii, Rodrigo Luger, Victoria S. Meadows, Tyler D. Robinson
Publikováno v:
The Astronomical Journal, vol 156, iss 6
Rotational mapping and glint are two proposed methods to directly detect liquid water on the surface of habitable exoplanets. However, false positives for both methods may prevent the unambiguous detection of exoplanet oceans. We use simulations of E
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4f2c569be8595cea1b01bb2a6e8649f4
http://arxiv.org/abs/1901.05011
http://arxiv.org/abs/1901.05011
Autor:
Jacob Lustig-Yaeger, Victoria S. Meadows, Guadalupe Tovar Mendoza, Edward W. Schwieterman, Yuka Fujii, Rodrigo Luger, Tyler D. Robinson
Publikováno v:
Astronomical Journal; Dec2018, Vol. 156 Issue 6, p1-1, 1p