Zobrazeno 1 - 10
of 43
pro vyhledávání: '"Francesco Borsa"'
Autor:
Riccardo Spinelli, Elena Gallo, Francesco Haardt, Andrea Caldiroli, Federico Biassoni, Francesco Borsa, Emily Rauscher
Publikováno v:
The Astronomical Journal, Vol 165, Iss 5, p 200 (2023)
We leverage Gaia DR2 parallactic distances to deliver new or revised estimates of planetary parameters and X-ray irradiation for a distance-limited (≲100 pc) sample of 27 gaseous planets (from super-Earths to hot Jupiters) with publicly available C
Externí odkaz:
https://doaj.org/article/8cd6f3b804fe4eae8e68cccaa82fa41b
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
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
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instname
Oxygen is a constituent of many of the most abundant molecules detected in exoplanetary atmospheres and a key ingredient for tracking how and where a planet formed1. In particular, the O I 777.4 nm triplet is used to probe airglow and aurora on the E
Autor:
Simonetta Chinellato, Natalia Auricchio, Giovanni Postiglione, Joseph Huesler, Timothy Bandy, Enrico Battistelli, Guido Buonanno, Francesco Borsa, Alexis Brandeker, Daniele Brienza, Flavia Calderone, Virginie Cessa, Giacomo Dinuzzi, Jacopo Farinato, Mauro Ferrero, Riccardo Liaci, Demetrio Magrin, Luca Marafatto, Matteo Munari, Marco Nebiolo, Andrea Novi, Isabella Pagano, Daniele Piazza, Roberto Ragazzoni, Mario Salatti, Francesco Santoli, Antonio Saverino, Madine Simoncini, Valentina Viotto, Donata Valletti
Publikováno v:
Modeling, Systems Engineering, and Project Management for Astronomy X.
Autor:
Francesco Borsa, Andrea Cottinelli, Nicolas Gorius, Claudio Arena, Bart Vandenbussche, Sara Regibo, Rik Huygen, Pierre Royer, Martin Pertenais, Cesar Martin, Thierry Appourchaux, Jose Lorenzo Alvarez, Tim A. van Kempen, Wouter Laauwen, Isabella Pagano, Roberto Ragazzoni
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1a6ef17994b3a7f8d5958b8b4df7e9bc
https://doi.org/10.1117/12.2630118
https://doi.org/10.1117/12.2630118
Autor:
Ilaria Carleo, Paolo Giacobbe, Gloria Guilluy, Patricio E. Cubillos, Aldo S. Bonomo, Alessandro Sozzetti, Matteo Brogi, Siddharth Gandhi, Luca Fossati, Diego Turrini, Katia Biazzo, Francesco Borsa, Antonino F. Lanza, Luca Malavolta, Antonio Maggio, Luigi Mancini, Giusi Micela, Lorenzo Pino, Ennio Poretti, Monica Rainer, Gaetano Scandariato, Eugenio Schisano, Gloria Andreuzzi, Andrea Bignamini, Rosario Cosentino, Aldo Fiorenzano, Avet Harutyunyan, Emilio Molinari, Marco Pedani, Seth Redfield, Hristo Stoev
Publikováno v:
The Astronomical Journal, 164(3):101
Detections of molecules in the atmosphere of gas giant exoplanets allow us to investigate the physico-chemical properties of the atmospheres. Their inferred chemical composition is used as tracer of planet formation and evolution mechanisms. Currentl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::355e5b56ec37a05e20e09ac57376fd4d
https://hdl.handle.net/1887/3514767
https://hdl.handle.net/1887/3514767
Autor:
Vardan Adibekyan, M. R. Zapatero Osorio, Yann Alibert, P. Di Marcantonio, François Bouchy, Cristina Martins, N. Casasayas-Barris, Francesco Borsa, Andrea Mehner, Giuseppina Micela, Paolo Molaro, S. Cristiani, Francesco Pepe, Nuno C. Santos, J. Lillo-Box, C. Lovis, Enric Palle, Vincent Bourrier, G. Lo Curto, Gang Chen, Rafael Rebolo, Fei Yan, O. D. S. Demangeon, J. I. González Hernández, V. D Odorico, Stéphane Udry, M. Stangret, S. G. Sousa, Mahmoudreza Oshagh, C. Allende Prieto, B. Lavie, A. Suárez Mascareño, P. Figueira, Alessandro Sozzetti, David Ehrenreich, R. Génova Santos, Romain Allart, Nelson J. Nunes, Hugo M. Tabernero, E. Poretti
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
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Astronomy & Astrophysics
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Astronomy & Astrophysics
We observed two transits of the iconic gas giant HD 209458b between 380 and 780 nm, using the high-resolution ESPRESSO spectrograph. The derived planetary transmission spectrum exhibits features at all wavelengths where the parent star shows strong a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39f645fd45640324ba97c6618215299a
http://arxiv.org/abs/2101.04094
http://arxiv.org/abs/2101.04094
Autor:
S. Hojjatpanah, L. Genolet, Matteo Genoni, Paolo Molaro, Edoardo Maria Alberto Redaelli, T. Bandy, A. Segovia, Jorge Lillo-Box, Diogo Alves, A. Suárez Mascareño, Olivier Demangeon, Vincent Bourrier, João P. Faria, Julia V. Seidel, F. Tenegi, P. Figueira, Yann Alibert, Danuta Sosnowska, Giorgio Pariani, Matteo Aliverti, Antonino Bianco, M. Moschetti, J. Knudstrup, B. Delabre, M. Amate, Romain Allart, Olaf Iwert, Valentina D'Odorico, Francesco Borsa, Hugo M. Tabernero, J. L. Lizon, M. R. Zapatero Osorio, G. Avila, Paolo Conconi, Vardan Adibekyan, Alexandre Cabral, Ennio Poretti, Mário J. P. F. G. Monteiro, J. L. Rasilla, Andrea Mehner, Antonio Gouveia Oliveira, Filippo Maria Zerbi, Alessandro Sozzetti, François Bouchy, Luca Pasquini, Baptiste Lavie, Marco Landoni, E. Mueller, S. Deiries, Luca Oggioni, Nelson J. Nunes, R. Génova Santos, Claudio Cumani, João Coelho, S. C. C. Barros, Denis Mégevand, J. I. González Hernández, S. Santana-Tschudi, Paolo Santin, M. Affolter, Giuseppina Micela, Alessio Zanutta, G. Lo Curto, A. Fragoso, C. Allende Prieto, Pedro Santos, J. H. C. Martins, Antonio Manescau, Florian Kerber, Willy Benz, Hans Dekker, David Ehrenreich, Paolo Spanò, Rafael Rebolo, Xavier Dumusque, Cristina Martins, Núria Casasayas-Barris, Francesco Pepe, S. G. Sousa, Stefano Cristiani, C. Broeg, C. Maire, Andrea Modigliani, Stéphane Udry, Nuno C. Santos, Marco Riva, C. Lovis, Enric Palle, I. Hughes, P. Di Marcantonio
Publikováno v:
Astronomy & Astrophysics
Aims. We report on ESPRESSO high-resolution transmission spectroscopic observations of two primary transits of the highly-irradiated, ultra-hot Jupiter-size planet WASP-76b. We investigate the presence of several key atomic and molecular features of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::985b4f6fe42ce630a8d9440dcf886fb9
Autor:
Grzegorz Nowak, V. Nascimbeni, João M. Mendonça, Daniela Sicilia, Rafael Luque, Lars A. Buchhave, Brett C. Addison, Mahmoudreza Oshagh, Avet Harutyunyan, M. Stangret, Enric Palle, Massimo Cecconi, A. S. Bonomo, Hannu Parviainen, A. Bello-Arufe, Francesco Borsa, Luca Malavolta, René Tronsgaard, Debra A. Fischer, Alessandro Sozzetti, Fei Yan, Núria Casasayas-Barris, J. Orell-Miquel, Samuel H. C. Cabot
Publikováno v:
Stangret, M, Pallé, E, Casasayas-Barris, N, Oshagh, M, Bello-Arufe, A, Luque, R, Nascimbeni, V, Yan, F, Orell-Miquel, J, Sicilia, D, Malavolta, L, Addison, B C, Buchhave, L A, Bonomo, A S, Borsa, F, Cabot, S H C, Cecconi, M, Fischer, D A, Harutyunyan, A, Mendonça, J M, Nowak, G, Parviainen, H, Sozzetti, A & Tronsgaard, R 2021, ' The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b) : A misaligned orbit and no signs of atomic or molecular absorptions ', Astronomy and Astrophysics, vol. 654, A73 . https://doi.org/10.1051/0004-6361/202040100
Ultra-hot Jupiters are defined as giant planets with equilibrium temperatures larger than 2000 K. Most of them are found orbiting bright A-F type stars, making them extremely suitable objects to study their atmospheres using high-resolution spectrosc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8115d2a77c1ab240b4ffd6077369e337
http://hdl.handle.net/20.500.12386/32119
http://hdl.handle.net/20.500.12386/32119
Autor:
Francesco Borsa, Silvano Desidera, Ignazio Pillitteri, Darius Modirrousta-Galian, Riccardo Claudi, Giuseppina Micela, S. Benatti, A. Maggio, D. Locci, L. Malavolta, Scott J. Wolk, Mario Damasso
We performed a radial velocity (RV) monitoring of the 40 Myr old star DS Tuc A with HARPS at the ESO-3.6m to determine the planetary mass of its 8.14-days planet, first revealed by TESS. We also observed two planetary transits with HARPS and ESPRESSO
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e234a8191fc76b97a63e717f296e63e3
http://hdl.handle.net/11577/3415744
http://hdl.handle.net/11577/3415744