Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Thea Kozakis"'
Autor:
Geronimo L. Villanueva, Thomas J. Fauchez, Vincent Kofman, Eleonora Alei, Elspeth K. H. Lee, Estelle Janin, Michael D. Himes, Jérémy Leconte, Michaela Leung, Sara Faggi, Mei Ting Mak, Denis E. Sergeev, Thea Kozakis, James Manners, Nathan Mayne, Edward W. Schwieterman, Alex R. Howe, Natasha Batalha
Publikováno v:
The Planetary Science Journal, Vol 5, Iss 3, p 64 (2024)
Radiative transfer (RT) models are critical in the interpretation of exoplanetary spectra, in simulating exoplanet climates, and when designing the specifications of future flagship observatories. However, most models differ in methodologies and inpu
Externí odkaz:
https://doaj.org/article/6dfceb321dbc48bda6b36ef11af2ded8
Molecular oxygen (O2) paired with a reducing gas is regarded as a promising biosignature pair for atmospheric characterization of terrestrial exoplanets. In circumstances when O2 may not be detectable in a planetary atmosphere (for instance, at mid-I
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::261ffcb3b4faffc2dad8c3f696dc0fa9
https://doi.org/10.5194/epsc2022-1267
https://doi.org/10.5194/epsc2022-1267
Publikováno v:
Lin, Z, Seager, S, Ranjan, S, Kozakis, T & Kaltenegger, L 2022, ' H 2-dominated Atmosphere as an Indicator of Second-generation Rocky White Dwarf Exoplanets ', The Astrophysical Journal Letters, vol. 925, no. 1, L10 . https://doi.org/10.3847/2041-8213/ac4788
Following the discovery of the first exoplanet candidate transiting a white dwarf (WD), a "white dwarf opportunity" for characterizing the atmospheres of terrestrial exoplanets around WDs is emerging. Large planet-to-star size ratios and hence large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2dd0b7ed8b32a6f4ede06662676ea6f0
Publikováno v:
Kozakis, T, Mendonça, J M & Buchhave, L A 2022, ' Is ozone a reliable proxy for molecular oxygen? I. The O 2-O 3 relationship for Earth-like atmospheres ', Astronomy and Astrophysics, vol. 665, A156 . https://doi.org/10.1051/0004-6361/202244164
Molecular oxygen (O2) paired with a reducing gas is regarded as a promising biosignature pair for the atmospheric characterization of terrestrial exoplanets. In circumstances when O2 may not be detectable in a planetary atmosphere (e.g., at mid-IR wa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7add55755ad80a895f634613b79d1921
https://orbit.dtu.dk/en/publications/5a9b3648-7ed2-4fc1-acb9-4e0d6fd0ba38
https://orbit.dtu.dk/en/publications/5a9b3648-7ed2-4fc1-acb9-4e0d6fd0ba38
Autor:
Eric E. Mamajek, Thea Kozakis, Lisa Kaltenegger, Ryan J. MacDonald, Nikole K. Lewis, Jonathan C. McDowell, Andrew Vanderburg
The near-term search for life beyond the solar system currently focuses on transiting planets orbiting small M dwarfs, and the challenges of detecting signs of life in their atmospheres. However, planets orbiting white dwarfs (WDs) would provide a un
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f83f2941b1ad4caea372d90ca49b93de
Autor:
Lisa Kaltenegger, Thea Kozakis
In the near future we will have ground- and space-based telescopes that are designed to observe and characterize Earth-like planets. While attention is focused on exoplanets orbiting main sequence stars, more than 150 exoplanets have already been det
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::37e0d6f47cd2a7ce0a8a4784cd70720c
With the first observations of debris disks as well as proposed planets around white dwarfs, the question of how rocky planets around such stellar remnants can be characterized and probed for signs of life becomes tangible. White dwarfs are similar i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ca0178fea5a08738df2f11b2a10837c
http://arxiv.org/abs/2001.00049
http://arxiv.org/abs/2001.00049
An Earth-like exoplanet orbiting a white dwarf would be exposed to different UV environments than Earth, influencing both its atmospheric photochemistry and UV surface environment. Using a coupled 1D climate-photochemistry code we model atmospheres o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f2310452cf39c9ba451db4274a7e909e
Autor:
Thea Kozakis, Lisa Kaltenegger
Publikováno v:
The Astrophysical Journal. 875:99
During the post-main sequence phase of stellar evolution the orbital distance of the habitable zone, which allows for liquid surface water on terrestrial planets, moves out past the system's original frost line, providing an opportunity for outer pla
Publikováno v:
Astrophysical Journal; 7/20/2018, Vol. 862 Issue 1, p1-1, 1p