Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Julian Alvarado-Gomez"'
Autor:
Engin Keles, Matthias Mallonn, Daniel Kitzmann, Katja Poppenhaeger, H Jens Hoeijmakers, Ilya Ilyin, Xanthippi Alexoudi, Thorsten A Carroll, Julian Alvarado-Gomez, Laura Ketzer, Aldo S Bonomo, Francesco Borsa, B Scott Gaudi, Thomas Henning, Luca Malavolta, Karan Molaverdikhani, Valerio Nascimbeni, Jennifer Patience, Lorenzo Pino, Gaetano Scandariato, Everett Schlawin, Evgenya Shkolnik, Daniela Sicilia, Alessandro Sozzetti, Mary G Foster, Christian Veillet, Ji Wang, Fei Yan, Klaus G Strassmeier
Publikováno v:
Keles, Engin; Mallonn, Matthias; Kitzmann, Daniel; Poppenhaeger, Katja; Hoeijmakers, Herman; Ilyin, Ilya; Alexoudi, Xanthippi; Carroll, Thorsten A; Alvarado-Gomez, Julian; Ketzer, Laura; Bonomo, Aldo S; Borsa, Francesco; Gaudi, B Scott; Henning, Thomas; Malavolta, Luca; Molaverdikhani, Karan; Nascimbeni, Valerio; Patience, Jennifer; Pino, Lorenzo; Scandariato, Gaetano; ... (2022). The PEPSI exoplanet transit survey (PETS) I: investigating the presence of a silicate atmosphere on the super-earth 55 Cnc e. Monthly notices of the Royal Astronomical Society, 513(1), pp. 1544-1556. Oxford University Press 10.1093/mnras/stac810
The study of exoplanets and especially their atmospheres can reveal key insights on their evolution by identifying specific atmospheric species. For such atmospheric investigations, high-resolution transmission spectroscopy has shown great success, e
Autor:
Jeremy J. Drake, Peter N. Cheimets, Cecilia Garraffo, Bradford Wargelin, Allison Youngblood, Vinay L. Kashyap, Paola Testa, David Caldwell, James Mason, Brian T. Fleming, Kevin France, Scott Wolk, Oswald Siegmund, Tommi Koskinen, Julian Alvarado-Gomez, Maria Mercedes Lopez-Morales, Guillaume Gronoff, Jay Bookbinder, Martin Barstow, David Windt, Randy Gladstone, Chris Loghry, Rix Yarbrough
Publikováno v:
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII.
The Normal-incidence Extreme Ultraviolet Photometer (NExtUP) is a smallsat mission concept designed to measure the EUV radiation conditions of exoplanet host stars, and F-M type stars in general. EUV radiation is absorbed at high altitude in a planet