LOCNES: a solar telescope to study stellar activity in the near infrared

Autor: R., Claudi, A., Ghedina, E., Pace, M., Di Giorgio A., V., D'Orazi, L., Gallorini, F., Lanza A., J., Liu S., M., Rainer, A., Tozzi, I., Carleo, J., Maldonado Prado, G., Micela, E., Molinari, E., Poretti, D., Phillips, G., Tripodo, M., Cecconi, A., Galli, D., Gonzalez M., V., Guerra Padilla, G., Guerra Ramòn J., A., Harutyunyan, N., Hernàndez Càceres, M., Hernàndez Dìaz, M., Lodi, H., Pèrez Ventura, L., Riverol Rodrìguez A., A., Riverol Rodrìguez C., J, San Juan Gòmez

LOCNES (LOw-Cost NIR Extended Solar telescope) is a solar telescope installed at the TNG (Telescopio Nazionale Galileo). It feeds the light of the Sun into the NIR spectrograph GIANO-B through a 40-m patch of optical fibers. LOCNES has been designed

Externí odkaz: http://arxiv.org/abs/2012.11350

Three years of HARPS-N high-resolution spectroscopy and precise radial velocity data for the Sun

Autor: Alessandro Sozzetti, Luca Malavolta, M. Cecconi, Raphaëlle D. Haywood, Ennio Poretti, Damien Ségransan, Ken Rice, Lars A. Buchhave, L. Riverol, David F. Phillips, C. Riverol, Danuta Sosnowska, Stéphane Udry, Annelies Mortier, Heather M. Cegla, A. Collier Cameron, M. Gonzalez, Mercedes López-Morales, Emilio Molinari, F. Alesina, Francesco Pepe, David W. Latham, Samantha Thompson, Xavier Dumusque, Giuseppina Micela, N. Buchschacher, Adriano Ghedina, J. Burnier, T. G. Wilson, Rosario Cosentino, Matteo Pinamonti, Marcello Lodi, C. Lovis, M. Cretignier, Jesus Maldonado, J. San Juan, Ryan Cloutier, H. Perez Ventura

Publikováno v: Astronomy & Astrophysics
Dumusque, X, Cretignier, M, Sosnowska, D, Buchschacher, N, Lovis, C, Phillips, D F, Pepe, F, Alesina, F, Buchhave, L A, Burnier, J, Cecconi, M, Cegla, H M, Cloutier, R, Cameron, A C, Cosentino, R, Ghedina, A, Gonzalez, M, Haywood, R D, Latham, D W, Lodi, M, Lopez-Morales, M, Maldonado, J, Malavolta, L, Micela, G, Molinari, E, Mortier, A, Ventura, H P, Pinamonti, M, Poretti, E, Rice, K, Riverol, L, Riverol, C, Juan, J S, Segransan, D, Sozzetti, A, Thompson, S J, Udry, S & Wilson, T G 2021, ' Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun ', Astronomy and Astrophysics, vol. 648, A103 . https://doi.org/10.1051/0004-6361/202039350
Dumusque, X, Cretignier, M, Sosnowska, D, Buchschacher, N, Lovis, C, Phillips, D F, Pepe, F, Alesina, F, Buchhave, L A, Burnier, J, Cecconi, M, Cegla, H M, Cloutier, R, Cameron, A C, Cosentino, R, Ghedina, A, Gonzalez, M, Haywood, R D, Latham, D W, Lodi, M, Lopez-Morales, M, Maldonado, J, Malavolta, L, Micela, G, Molinari, E, Mortier, A, Ventura, H P, Pinamonti, M, Poretti, E, Rice, K, Riverol, L, Riverol, C, Juan, J S, Segransan, D, Sozzetti, A, Thompson, S J, Udry, S & Wilson, T G 2021, ' Three Years of HARPS-N High-Resolution Spectroscopy and Precise Radial Velocity Data for the Sun ', Astronomy and Astrophysics, vol. 648, A103, pp. 1-19 . https://doi.org/10.1051/0004-6361/202039350

The solar telescope connected to HARPS-N has been observing the Sun since the summer of 2015. Such high-cadence, long-baseline data set is crucial for understanding spurious radial-velocity signals induced by our Sun and by the instrument. On the ins

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b6d742858dde14fb8cd48362e5482b4
http://hdl.handle.net/20.500.12386/32125

LOCNES: A solar telescope to study the Sun-as-a-star activity in the near infrared

Autor: David F. Phillips, V. Guerra Padilla, I. Carleo, Adriano Ghedina, Emanuele Pace, J. Maldonado Prado, C. A. Riverol Rodríguez, Emilio Molinari, L. Gallorini, H. Perez Ventura, Riccardo Claudi, M. Hernandez Diaz, J. San Juan Gómez, Valentina D'Orazi, Massimo Cecconi, A. M. di Giorgio, N. Hernández Cáceres, Andrea Tozzi, M. Gonzalez, Avet Harutyunyan, J. G. Guerra Ramón, Giuseppina Micela, Marcello Lodi, A. F. Lanza, A. Galli, Monica Rainer, G. Tripodo, A. L. Riverol Rodriguez, S. J. Liu, Ennio Poretti

Publikováno v: Ground-based and Airborne Telescopes VIII.

LOCNES (LOw-Cost NIR Extended Solar telescope) is a solar telescope installed at the TNG (Telescopio Nazionale Galileo). It feeds the light of the Sun into the NIR spectrograph GIANO-B through a 40-m patch of optical fibers. LOCNES has been designed

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::79faef23c97ad78ed610925682c93bc8
https://doi.org/10.1117/12.2562231

The GAPS Programme at TNG: XXI. A GIARPS case study of known young planetary candidates: confirmation of HD 285507 b and refutation of AD Leonis b

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)

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

SOXS End-to-End simulator: development and applications for pipeline design

Autor: Sagi Ben-Ami, Giorgio Pariani, M. Hernandez Diaz, A. Brucalassi, G. Li Causi, Jari Kotilainen, Hanindyo Kuncarayakti, Matteo Aliverti, Sergio Campana, J. A. Araiza-Duran, Iair Arcavi, O. Hershko, Andrea Baruffolo, Seppo Mattila, J. Achrén, Marco Landoni, P. D'Avanzo, Stephen Smartt, M. De Pascale, Rosario Cosentino, Kalyan Radhakrishnan, Federico Biondi, Marco Riva, Maximilian Stritzinger, M. Della Valle, Rachel Bruch, Avishay Gal-Yam, Sergio D'Orsi, D. R. Young, Fabrizio Vitali, Francesco D'Alessio, Bernardo Salasnich, Giuliano Pignata, Adam Rubin, Davide Ricci, R. Di Benedetto, Giulio Capasso, Enrico Cappellaro, P. Schipani, H. Perez Ventura, Matteo Munari, R. Zanmar Sanchez, Matteo Genoni, Michael Rappaport, Riccardo Claudi, Mirko Colapietro, Salvatore Scuderi

Publikováno v: Genoni, M, Landoni, M, Li Causi, G, Pariani, G, Alierti, M, Campana, S, Schipani, P, Claudi, R, Munari, M, Rubin, A, D'Avanzo, P, Riva, M, Baruffolo, A, Biondi, F, Capasso, G, Cosentino, R, D'Alessio, F, Hershko, O, Kuncarayakti, H, Pignata, G, Scuderi, S, Radhakrishnan, K, Ben-Ami, S, Vitali, F, Young, D, Brucalass, A, Achrén, J, Araiza-Duran, J A, Arcavi, I, Bruch, R, Cappellaro, E, Colapietro, M, Della Valle, M, De Pascale, M, Di Benedetto, R, D'Orsi, S, Gal-Yam, A, Hernandez Diaz, M, Kotilainen, J, Mattila, S, Rappaport, M, Ricci, D, Salasnich, B, Smartt, S, Zanmar Sanchez, R, Stritzinger, M & Ventura, H 2020, SOXS end-to-end simulator : Development and applications for pipeline design . in G Z Angeli & P Dierickx (eds), Modeling, Systems Engineering, and Project Management for Astronomy IX ., 114501B, SPIE-International Society for Optical Engineering, Proceedings of SPIE-The International Society for Optical Engineering, vol. 11450, Modeling, Systems Engineering, and Project Management for Astronomy IX 2020, Virtual, Online, United States, 14/12/2020 . https://doi.org/10.1117/12.2560640

We present the development of the End-to-End simulator for the SOXS instrument at the ESO-NTT 3.5-m telescope. SOXS will be a spectroscopic facility, made by two arms high efficiency spectrographs, able to cover the spectral range 350-2000 nm with re

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71dd45bd5fe0c1ff2d8fcc8b76d77309