Zobrazeno 1 - 10
of 52
pro vyhledávání: '"Luca Fini"'
Publikováno v:
Adaptive Optics Systems VIII.
Autor:
Marcello Lodi, A. F. Lanza, Andrea Bignamini, M. Sozzi, Gaetano Scandariato, C. Riverol, Jesus Maldonado, Luca Malavolta, Giuseppe Leto, R. G. Gratton, Massimo Cecconi, Katia Biazzo, Carlo Baffa, Riccardo Claudi, G. Falcini, N. Buchschacher, Marco Pedani, Elisabetta Giani, Silvano Desidera, Concepción Iglesias González, H. Perez Ventura, Luigi Mancini, Daniela Fantinel, Antonio Maggio, Salvo Scuderi, Ennio Poretti, Ulf Seemann, Andrea Tozzi, Matthias Mallonn, José Guerra, A. Galli, Giuseppina Micela, E. Alei, Valerio Nascimbeni, Avet Harutyunyan, Matteo Pinamonti, G. Frustagli, Aldo S. Bonomo, Monica Rainer, Alfio Puglisi, Aldo F. M. Fiorenzano, Livia Origlia, Serena Benatti, Alessandro Sozzetti, Isabella Pagano, Andrea Baruffolo, Adriano Ghedina, Paolo Giacobbe, M. Gonzalez, Ernesto Oliva, Ilaria Carleo, Francesca Ghinassi, Rosario Cosentino, Elvira Covino, M. Esposito, N. Hernandez, Giampaolo Piotto, M. Hernandez Diaz, Luca Fini, J. San Juan, Seth Redfield, M. Iuzzolino, Nicoletta Sanna, L. Riverol, Laura Affer, Francesco Borsa, Emilio Molinari, Mario Damasso, E. González-Álvarez, V. Billotti
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
instname
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Context. The existence of hot Jupiters is still not well understood. Two main channels are thought to be responsible for their current location: a smooth planet migration through the protoplanetary disk or the circularization of an initial highly ecc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7afd36d2b01747b9a280585ac928276
http://hdl.handle.net/2108/250712
http://hdl.handle.net/2108/250712
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:520-539
One of the main goals of the feasibility study MOSE (MOdellig ESO Sites) is to evaluate the performances of a method conceived to forecast the optical turbulence above the ESO sites of the Very Large Telescope and the European-Extremely Large Telesco
(35-words maximum) In this talk I present the scientific drivers related to the optical turbulence forecast applied to the ground-based astronomy supported by Adaptive Optics, the state of the art of the achieved results and the most relevant challen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7aed30ad5f9c7ceb805ff8909cef77aa
http://arxiv.org/abs/1902.07989
http://arxiv.org/abs/1902.07989
Autor:
Andrea Baruffolo, Alessandro Sozzetti, E. González-Álvarez, Raffaele Gratton, M. Cecconi, Luca Malavolta, Alfio Puglisi, G. Falcini, Livia Origlia, Andrea Bignamini, M. Iuzzolino, C. Riverol, Daniela Fantinel, Adriano Ghedina, Salvatore Scuderi, Riccardo Claudi, A. Galli, Ilaria Carleo, S. Messina, Rosario Cosentino, Jesus Maldonado, Carlo Baffa, N. Buchschacher, Silvano Desidera, Ulf Seemann, Emilio Molinari, Kimberly R. Sokal, J. San Juan, Andrea Tozzi, Giuseppina Micela, Kyle F. Kaplan, Avet Harutyunyan, Benjamin Kidder, Monica Rainer, Gregory N. Mace, M. Sozzi, Serena Benatti, Juan Carlos Guerra, F. Ghinassi, M. Gonzalez, Nicoletta Sanna, Antonino F. Lanza, L. Riverol, M. Endl, Concepción Iglesias González, H. Perez Ventura, D. Fugazza, N. Hernandez, Elisabetta Giani, Ernesto Oliva, Marcello Lodi, E. Sissa, M. Hernandez Diaz, Luca Fini
Context. Stellar activity is currently challenging the detection of young planets via the radial velocity (RV) technique. Aims. We attempt to definitively discriminate the nature of the RV variations for the young active K5 star BD+20 1790, for which
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2376dfadd80b0093ceaeb3fca74179a
http://arxiv.org/abs/1805.01281
http://arxiv.org/abs/1805.01281
Autor:
Serena Benatti, Alessandro Sozzetti, Luca Fini, G. Falcini, Jesus Maldonado, J. San Juan Gómez, Livia Origlia, Andrea Baruffolo, M. Sozzi, Nicoletta Sanna, Daniela Fantinel, Massimo Cecconi, Carlo Baffa, M. Hernandez Diaz, Adriano Ghedina, C. Riverol, Luca Malavolta, José Guerra, Ulf Seemann, Ernesto Oliva, E. Gonzalez-Alvarez, Valdemaro Biliotti, L. Riverol, Monica Rainer, H. Perez Ventura, M. Gonzalez, Salvo Scuderi, A. Galli, C. Gonzalez, Giuseppina Micela, Rosario Cosentino, N. Buchschacher, Emilio Molinari, Riccardo Claudi, Elisabetta Giani, Marcello Lodi, R. G. Gratton, Francesca Ghinassi, Andrea Tozzi, Avet Harutyunyan, M. Iuzzolino, I. Carleo, N. Hernandez, Alfio Puglisi
GIARPS (GIAno and haRPS) is a project devoted to have on the same focal station of the Telescopio Nazionale Galileo (TNG) both high resolution spectrographs, HARPS-N (VIS) and GIANO-B (NIR), working simultaneously. This could be considered the first
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c97a39777b8af30f58a3e2bb8f9f7365
http://hdl.handle.net/11577/3285759
http://hdl.handle.net/11577/3285759
Autor:
N. Buchschacher, Marcello Lodi, José Guerra, Francesca Ghinassi, Ennio Poretti, N. Hernandez, L. Riverol, Manuel Gonzalez, C. Riverol, Andrea Tozzi, Luca Fini, Daniela Fantinel, G. Falcini, Carlo Baffa, Avet Harutyunyan, Hector Ventura, Ernesto Oliva, Livia Origlia, Marcos Hernandez Diaz, Valdemaro Biliotti, Nicoletta Sanna, Jose San Juan, Andrea Bignamini, Serena Benatti, Alessandro Sozzetti, Luca Malavolta, M. Iuzzolino, Raffaele Gratton, Ulf Seeman, E. Gonzalez-Alvarez, Alfio Puglisi, Andrea Baruffolo, I. Carleo, Monica Rainer, Carlos Gonzalez, Rosario Cosentino, A. Galli, Elisabetta Giani, Jesus Maldonado, Massimo Cecconi, Adriano Ghedina, Salvatore Scuderi, M. Sozzi, Giuseppina Micela, Emilio Molinari, Riccardo Claudi
GIANO-B is the high resolution near-infrared (NIR) spectrograph of the Telescopio Nazionale Galileo (TNG), which started its regular operations in October 2017. Here we present GIANO-B Online Data Reduction Software (DRS) operating at the Telescope.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::775283507b89352b087ef771ef58371b
http://hdl.handle.net/11577/3285758
http://hdl.handle.net/11577/3285758
Autor:
Andrea Tozzi, Avet Harutyunyan, Jose San Juan, Luca Malavolta, Luca Fini, Francesca Ghinassi, C. Riverol, Marcos Hernandez Diaz, M. Iuzzolino, Elisabetta Giani, Carlos Gonzalez, Marcello Lodi, Giuseppina Micela, Livia Origlia, M. Sozzi, A. Galli, Andrea Bignamini, Monica Rainer, Nicoletta Sanna, L. Riverol, José Guerra, Raffaele Gratton, N. Hernandez, I. Carleo, G. Falcini, Adriano Ghedina, Jesus Maldonado, Carlo Baffa, Rosario Cosentino, Massimo Cecconi, Salvo Scuderi, Serena Benatti, Alessandro Sozzetti, Emilio Molinari, Riccardo Claudi, Alfio Puglisi, N. Buchschacher, Andrea Baruffolo, Daniela Fantinel, Manuel Gonzalez, Hector Ventura, Ernesto Oliva, Ulf Seeman, E. Gonzalez-Alvarez
The NIR echelle spectrograph GIANO-B at the Telescopio Nazionale Galileo is equipped with a fully automated online DRS: part of this pipeline is the GOFIO reduction software, that processes all the observed data, from the calibrations to the nodding
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5a76b69b3e5c9d3d1fc51aee4496db7c
http://hdl.handle.net/11577/3285760
http://hdl.handle.net/11577/3285760
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 449:1664-1678
This article aims at proving the feasibility of the forecast of all the most relevant classical atmospherical parameters for astronomical applications (wind speed and direction, temperature) above the ESO ground-base site of Cerro Paranal with a meso
Autor:
Elena Suárez González, Luca Malavolta, Nicoletta Sanna, Giuseppina Micela, Carlo Baffa, M. Hernandez Diaz, C. Riverol, Luca Fini, I. Carleo, Andrea Tozzi, Adriano Ghedina, Avet Harutyunyan, Ulf Seemann, José Guerra, Salvo Scuderi, Serena Benatti, Alessandro Sozzetti, Rosario Cosentino, Emilio Molinari, Riccardo Claudi, Monica Rainer, Livia Origlia, Francesca Ghinassi, A. Galli, Daniela Fantinel, Jesus Maldonado, Massimo Cecconi, Concepción Iglesias González, M. Gonzalez, Elisabetta Giani, Marcello Lodi, N. Hernandez, R. G. Gratton, Andrea Baruffolo, J. Sanjuan, H. Perez Ventura, Ernesto Oliva, N. Buchschacher, L. Riverol
Publikováno v:
The European Physical Journal Plus. 132
Since 2012, thanks to the installation of the high-resolution echelle spectrograph in the optical range HARPS-N, the Italian telescope TNG (La Palma) became one of the key facilities for the study of the extrasolar planets. In 2014 TNG also offered G