Zobrazeno 1 - 10
of 455
pro vyhledávání: '"E, Covino"'
Autor:
F. Z. Majidi, J. M. Alcalá, A. Frasca, S. Desidera, C. F. Manara, G. Beccari, V. D’Orazi, A. Bayo, K. Biazzo, R. Claudi, E. Covino, G. Mantovan, M. Montalto, D. Nardiello, G. Piotto, E. Rigliaco
We characterize twelve young stellar objects (YSOs) located in the Lupus I region, spatially overlapping with the Upper Centaurus Lupus (UCL) sub-stellar association. The aim of this study is to understand whether the Lupus I cloud has more members t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::26da49b14003e5e7b318ede6243d39bd
Autor:
M. Damasso, D. Locci, S. Benatti, A. Maggio, D. Nardiello, M. Baratella, K. Biazzo, A. S. Bonomo, S. Desidera, V. D'Orazi, M. Mallonn, A. F. Lanza, A. Sozzetti, F. Marzari, F. Borsa, J. Maldonado, L. Mancini, E. Poretti, G. Scandariato, A. Bignamini, L. Borsato, R. Capuzzo Dolcetta, M. Cecconi, R. Claudi, R. Cosentino, E. Covino, A. Fiorenzano, A. Harutyunyan, A. W. Mann, G. Micela, E. Molinari, M. Molinaro, I. Pagano, M. Pedani, M. Pinamonti, G. Piotto, H. Stoev
For more than two years, we monitored with the HARPS-N spectrograph the 400 Myr-old star HD\,63433, which hosts two close-in (orbital periods $P_b\sim7.1$ and $P_c\sim20.5$ days) sub-Neptunes detected by the TESS space telescope, and it was announced
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::64044c8aaca620414ba7fe83c67d12ba
https://hdl.handle.net/2108/327643
https://hdl.handle.net/2108/327643
Autor:
L. Mancini, M. Esposito, E. Covino, J. Southworth, E. Poretti, G. Andreuzzi, D. Barbato, K. Biazzo, L. Borsato, I. Bruni, M. Damasso, L. Di Fabrizio, D. F. Evans, V. Granata, A. F. Lanza, L. Naponiello, V. Nascimbeni, M. Pinamonti, A. Sozzetti, J. Tregloan-Reed, M. Basilicata, A. Bignamini, A. S. Bonomo, R. Claudi, R. Cosentino, S. Desidera, A. F. M. Fiorenzano, P. Giacobbe, A. Harutyunyan, Th. Henning, C. Knapic, A. Maggio, G. Micela, E. Molinari, I. Pagano, M. Pedani, G. Piotto
Aim: We aim to refine the orbital and physical parameters and determine the sky-projected planet orbital obliquity of five eccentric transiting planetary systems: HAT-P-15, HAT-P-17, HAT-P-21, HAT-P-26, and HAT-P-29. Each of the systems hosts a hot J
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ae13bd58becb0aadf73ef6b4925cfdc3
https://eprints.keele.ac.uk/11462/1/v04-afterrefereereport.pdf
https://eprints.keele.ac.uk/11462/1/v04-afterrefereereport.pdf
Autor:
L. Fossati, G. Guilluy, I. F. Shaikhislamov, I. Carleo, F. Borsa, A. S. Bonomo, P. Giacobbe, M. Rainer, C. Cecchi-Pestellini, M. L. Khodachenko, M. A. Efimov, M. S. Rumenskikh, I. B. Miroshnichenko, A. G. Berezutsky, V. Nascimbeni, M. Brogi, A. F. Lanza, L. Mancini, L. Affer, S. Benatti, K. Biazzo, A. Bignamini, D. Carosati, R. Claudi, R. Cosentino, E. Covino, S. Desidera, A. Fiorenzano, A. Harutyunyan, A. Maggio, L. Malavolta, J. Maldonado, G. Micela, E. Molinari, I. Pagano, M. Pedani, G. Piotto, E. Poretti, G. Scandariato, A. Sozzetti, H. Stoev
The hot Jupiter WASP-80b has been identified as a possible excellent target for detecting and measuring HeI absorption in the upper atmosphere. We observed 4 primary transits of WASP-80b in the optical and near-IR using the HARPS-N and GIANO-B high-r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e244505d36cd197ca22ff26ac81b1566
http://wrap.warwick.ac.uk/163997/1/WRAP-The-GAPS-Programme-TNG-2022.pdf
http://wrap.warwick.ac.uk/163997/1/WRAP-The-GAPS-Programme-TNG-2022.pdf
Autor:
K. Biazzo, V. D’Orazi, S. Desidera, D. Turrini, S. Benatti, R. Gratton, L. Magrini, A. Sozzetti, M. Baratella, A. S. Bonomo, F. Borsa, R. Claudi, E. Covino, M. Damasso, M. P. Di Mauro, A. F. Lanza, A. Maggio, L. Malavolta, J. Maldonado, F. Marzari, G. Micela, E. Poretti, F. Vitello, L. Affer, A. Bignamini, I. Carleo, R. Cosentino, A. F. M. Fiorenzano, P. Giacobbe, A. Harutyunyan, G. Leto, L. Mancini, E. Molinari, M. Molinaro, D. Nardiello, V. Nascimbeni, I. Pagano, M. Pedani, G. Piotto, M. Rainer, G. Scandariato
Context. Exoplanetary properties strongly depend on stellar properties: to know the planet with accuracy and precision it is necessary to know the star as accurately and precisely as possible. Aims. Our immediate aim is to characterize in a homogeneo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::39a9212cc5d693cdd5f98c525632f359
https://hdl.handle.net/11577/3454816
https://hdl.handle.net/11577/3454816
Autor:
J. Maldonado, S. Colombo, A. Petralia, S. Benatti, S. Desidera, L. Malavolta, A. F. Lanza, M. Damasso, G. Micela, M. Mallonn, S. Messina, A. Sozzetti, B. Stelzer, K. Biazzo, R. Gratton, A. Maggio, D. Nardiello, G. Scandariato, L. Affer, M. Baratella, R. Claudi, E. Molinari, A. Bignamini, E. Covino, I. Pagano, G. Piotto, E. Poretti, R. Cosentino, I. Carleo
Active region evolution plays an important role in the generation and variability of magnetic fields on the surface of lower main-sequence stars. However, determining the lifetime of active region growth and decay as well as their evolution is a comp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::483ea166e8b0d1b3c324d748803631db
http://hdl.handle.net/11577/3454811
http://hdl.handle.net/11577/3454811
Autor:
G. Guilluy, P. Giacobbe, I. Carleo, P. E. Cubillos, A. Sozzetti, A. S. Bonomo, M. Brogi, S. Gandhi, L. Fossati, V. Nascimbeni, D. Turrini, E. Schisano, F. Borsa, A. F. Lanza, L. Mancini, A. Maggio, L. Malavolta, G. Micela, L. Pino, M. Rainer, A. Bignamini, R. Claudi, R. Cosentino, E. Covino, S. Desidera, A. Fiorenzano, A. Harutyunyan, V. Lorenzi, C. Knapic, E. Molinari, E. Pacetti, I. Pagano, M. Pedani, G. Piotto, E. Poretti
Publikováno v:
Astronomy & Astrophysics, 665, A104
The field of exo-atmospheric characterisation is progressing at an extraordinary pace. Atmospheric observations are now available for tens of exoplanets, mainly hot and warm inflated gas giants, and new molecular species continue to be detected revea
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::102d5d621647e8fc7a512a99bce5d6ca
https://hdl.handle.net/2108/316746
https://hdl.handle.net/2108/316746
Autor:
L. Pino, M. Brogi, J. M. Désert, V. Nascimbeni, A. S. Bonomo, E. Rauscher, M. Basilicata, K. Biazzo, A. Bignamini, F. Borsa, R. Claudi, E. Covino, M. P. Di Mauro, G. Guilluy, A. Maggio, L. Malavolta, G. Micela, E. Molinari, M. Molinaro, M. Montalto, D. Nardiello, M. Pedani, G. Piotto, E. Poretti, M. Rainer, G. Scandariato, D. Sicilia, A. Sozzetti
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 668, ⟨10.1051/0004-6361/202244593⟩
Astronomy and Astrophysics-A&A, 2022, 668, ⟨10.1051/0004-6361/202244593⟩
[Abridged] We present a novel method to study the thermal emission of exoplanets as a function of orbital phase at very high spectral resolution, and apply it to investigate the climate of the ultra-hot Jupiter KELT-9b. We combine 3 nights of HARPS-N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a09a880d995ebba13d7c8704b36c5c06
Akademický článek
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Autor:
J. Maldonado, A. Petralia, M. Damasso, M. Pinamonti, G. Scandariato, E. González-Álvarez, L. Affer, G. Micela, A. F. Lanza, G. Leto, E. Poretti, A. Sozzetti, M. Perger, P. Giacobbe, R. Zanmar Sánchez, A. Maggio, J. I. González Hernández, R. Rebolo, I. Ribas, A. Suárez-Mascareño, B. Toledo-Padrón, A. Bignamini, E. Molinari, E. Covino, R. Claudi, S. Desidera, E. Herrero, J. C. Morales, I. Pagano, G. Piotto
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
[Context] It is now well-established that small, rocky planets are common around low-mass stars. However, the detection of such planets is challenged by the short-term activity of host stars. [Aims] The HARPS-N red Dwarf Exoplanet Survey programme is
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0ea2df49d489cf0491a8aad9b24c109f
http://hdl.handle.net/10261/257811
http://hdl.handle.net/10261/257811