Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Amy Louca"'
Autor:
Caroline Piaulet-Ghorayeb, Björn Benneke, Michael Radica, Eshan Raul, Louis-Philippe Coulombe, Eva-Maria Ahrer, Daria Kubyshkina, Ward S. Howard, Joshua Krissansen-Totton, Ryan J. MacDonald, Pierre-Alexis Roy, Amy Louca, Duncan Christie, Marylou Fournier-Tondreau, Romain Allart, Yamila Miguel, Hilke E. Schlichting, Luis Welbanks, Charles Cadieux, Caroline Dorn, Thomas M. Evans-Soma, Jonathan J. Fortney, Raymond Pierrehumbert, David Lafrenière, Lorena Acuña, Thaddeus Komacek, Hamish Innes, Thomas G. Beatty, Ryan Cloutier, René Doyon, Anna Gagnebin, Cyril Gapp, Heather A. Knutson
Publikováno v:
The Astrophysical Journal Letters, Vol 974, Iss 1, p L10 (2024)
With sizable volatile envelopes but smaller radii than the solar system ice giants, sub-Neptunes have been revealed as one of the most common types of planet in the galaxy. While the spectroscopic characterization of larger sub-Neptunes (2.5–4 R _
Externí odkaz:
https://doaj.org/article/bafb1eec668c4c80b09ceaf693c9125e
Autor:
Frank Rensen, Yamila Miguel, Mantas Zilinskas, Amy Louca, Peter Woitke, Christiane Helling, Oliver Herbort
Publikováno v:
Remote Sensing, Vol 15, Iss 3, p 841 (2023)
The deep atmosphere of Jupiter is obscured beneath thick clouds. This causes direct observations to be difficult, and thermochemical equilibrium models fill in the observational gaps. This research uses Galileo and Juno data together with the Gibbs f
Externí odkaz:
https://doaj.org/article/3f09f5d30c6a4ed8861d360de8584e44
Autor:
Siddharth Gandhi, Aurora Kesseli, Yapeng Zhang, Amy Louca, Ignas Snellen, Matteo Brogi, Yamila Miguel, Núria Casasayas-Barris, Stefan Pelletier, Rico Landman, Cathal Maguire, Neale P. Gibson
Publikováno v:
The Astronomical Journal, Vol 165, Iss 6, p 242 (2023)
Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical species and atmospheric dynamics in exoplanets, most notably ultrahot Jupiters (UHJs). However, quantitative estimates on abundances have been challenging but are essentia
Externí odkaz:
https://doaj.org/article/93c13a440c484949ba9723c9cbed8680
Autor:
Amy Louca, Yamila Miguel
The evolution of stars on grand time-scales affect their surroundings in many ways. Due to their intrinsic rotation, causing strong magnetic activity, they vary greatly in radiative activity in X-ray and ultraviolet (XUV) throughout their lifetime. P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4c84263cbebbbf8870fbb67cba844c20
This study is focused on the implementation of neural networks to replace mathematical frameworks in the one-dimensional chemical kinetics code, VULCAN (Tsai et al. 2017; 2021). The underlying time-dependent ordinary differential equations are very t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b2827f40b558472290e6400b06cd8f56
Autor:
Zafar Rustamkulov, David Sing, Michael Line, E. May, Everett Schlawin, Kevin Stevenson, Jayesh Goyal, Sagnick Mukherjee, Sarah Moran, Hannah Wakeford, Joshua Lothringer, Aarynn Carter, Ryan MacDonald, Nestor Espinoza, Mercedes López-Morales, Jacob Bean, Caroline Piaulet, Quentin Changeat, Natalie Batalha, L. Kreidberg, Pierre-Alexis Roy, Nikolay Nikolov, Natasha Batalha, Peter Wheatley, Karan Molaverdikhani, Viven Parmentier, Björn Benneke, Jeremy Leconte, Jake Taylor, Neale Gibson, William Waalkes, Yamila Miguel, Jean-Michel Désert, Patricio Cubillos, Nicolas Iro, Tansu Daylan, Eva-Maria Ahrer, Amy Louca, Jacob Lustig-Yaeger, RENYU HU, Luis Welbanks, Jasmina Blecic, Benjamin Rackham, Michael Radica, Peter Gao, Giuseppe Morello, Enric Palle, Olivia Venot, Xi Zhang, Natalie Allen, Eliza Kempton, Katy Chubb, Jonathan Fortney, Pascal Tremblin, Taylor Bell, Thomas Mikal-Evans, Megan Mansfield, Ian Crossfield, Keshav Aggarwal, Joseph Harrington, Sarah Casewell, Monika Lendl, Agnibha Banerjee, Seth Redfield, Joanna Barstow, Adina Feinstein, Sebastian Zieba, Jake Turner, Kevin Heng, Munazza Alam, Lili Alderson, Evgenya Shkolnik, Diana Powell, Lakeisha Ramos-Rosado, Dominique Petit dit de la Roche, John Southworth, Saugata Barat, Luigi Mancini, Tiffany Kataria, Kazumasa Ohno, Nathan Mayne, Yucian Hong, Laura Rogers, Jorge Lillo-box, Johanna Teske, David Barrado, Gregory Tucker, Eric Agol
Transmission spectroscopy of exoplanets has revealed signatures of water vapor, aerosols, and alkali metals in a few dozen exoplanet atmospheres. However, these previous inferences with the Hubble and Spitzer Space Telescopes were hindered by the obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::92ae022bc89f7cd230c45d13910c3ac3
https://doi.org/10.21203/rs.3.rs-2092302/v1
https://doi.org/10.21203/rs.3.rs-2092302/v1
Strongly irradiated rocky planets will have sufficiently high surface temperatures to sustain dayside magma lakes and oceans that will outgas low-pressure days-side silicate atmospheres. The surface magma will preferentially outgas its most volatile
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ee06a69b926a99c27d03a05a2fdac963
https://doi.org/10.5194/epsc2021-781
https://doi.org/10.5194/epsc2021-781
Publikováno v:
European Planetary Science Congress, EPSC2021-222. Europlanet Society
STARTPAGE=EPSC2021;ENDPAGE=222;TITLE=European Planetary Science Congress
STARTPAGE=EPSC2021;ENDPAGE=222;TITLE=European Planetary Science Congress
Ultra-hot Jupiters have dayside temperatures similar to those of M-dwarfs. While molecular absorption from the hydroxyl radical (OH) is easily observed in near-infrared spectra of M-dwarfs, it is often not considered when studying the atmospheres of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::851e8a4481c12965f2200d5a218c1998
https://doi.org/10.5194/epsc2021-222
https://doi.org/10.5194/epsc2021-222