Zobrazeno 1 - 10
of 106
pro vyhledávání: '"Ivo Saviane"'
Autor:
Misaki Mizumoto, Hiroaki Sameshima, Naoto Kobayashi, Noriyuki Matsunaga, Sohei Kondo, Satoshi Hamano, Chikako Yasui, Kei Fukue, Akira Arai, Hideyo Kawakita, Shogo Otsubo, Giuseppe Bono, Ivo Saviane
Publikováno v:
The Astrophysical Journal, Vol 960, Iss 1, p 41 (2023)
Outflows in an active galactic nucleus (AGN) are considered to play a key role in the evolution of the host galaxy through transfer of a large amount of energy. A narrow-line region (NLR) in the AGN is composed of ionized gas extending from parsec to
Externí odkaz:
https://doaj.org/article/fb871a13c547479ea267a19f9d3bfcf1
Autor:
Pietro Fiorentin, Renata Binotto, Stefano Cavazzani, Andrea Bertolo, Sergio Ortolani, Ivo Saviane
Publikováno v:
Remote Sensing, Vol 14, Iss 22, p 5787 (2022)
A very wide-used instrument for the measurement of the Night Sky Brightness (NSB) is the Sky Quality Meter (SQM). One of its important issues is tracking NSB for long time and connecting its variations to changes in outdoor lighting. The stability of
Externí odkaz:
https://doaj.org/article/92d1b1a4b50b4dd3b029f0a2c8f21ad1
Autor:
Marina Rejkuba, J. Olivares Carvajal, J. Hartke, R. Contreras Ramos, Elena Valenti, J. A. Carballo-Bello, F. Gran, M. Zoccali, A. Rojas-Arriagada, C. Navarrete, Ivo Saviane
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 509:4962-4981
Recent wide-area surveys have enabled us to study the Milky Way with unprecedented detail. Its inner regions, hidden behind dust and gas, have been partially unveiled with the arrival of near-IR photometric and spectroscopic datasets. Among recent di
Autor:
Pietro Schipani, Sergio Campana, Riccardo Claudi, Matteo Aliverti, Andrea Baruffolo, Sagi Ben-Ami, Giulio Capasso, Rosario Cosentino, Francesco D'Alessio, Paolo D'Avanzo, Ofir Hershko, Hanindyo Kuncarayakti, Marco Landoni, Matteo Munari, Giuliano Pignata, Kalyan Radhakrishnan, Adam Rubin, Salvatore Scuderi, Fabrizio Vitali, David Young, Jani Achrén, José Antonio Araiza-Durán, Iair Arcavi, Federico Battaini, Anna Brucalassi, Rachel Bruch, Enrico Cappellaro, Mirko Colapietro, Massimo Della Valle, Rosario Di Benedetto, Sergio D'Orsi, Avishay Gal-Yam, Matteo Genoni, Marcos Hernandez Díaz, Jari Kotilainen, Gianluca Li Causi, Luigi Lessio, Laurent Marty, Seppo Mattila, Michael Rappaport, Davide Ricci, Marco Riva, Bernardo Salasnich, Salvatore Savarese, Stephen Smartt, Ricardo Zanmar Sánchez, Maximilian Stritzinger, Gabriele Umbriaco, Héctor Pérez Ventura, Luca Pasquini, Markus Schöller, Hans-Ulrich Kaüfl, Matteo Accardo, Leander Mehrgan, Emanuela Pompei, Ivo Saviane
Publikováno v:
Ground-based and Airborne Instrumentation for Astronomy IX.
SOXS (Son Of X-Shooter) is a single object spectrograph offering a simultaneous spectral coverage from U- to H-band, built by an international consortium for the 3.58-m ESO New Technology Telescope at the La Silla Observatory. It is designed to obser
Recent wide-area surveys have enabled us to study the Galaxy with unprecedented detail. Even its inner regions, hidden behind dust and gas, have been partially unveiled by the current surveys. However, there is a population of low-mass globular clust
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::108ab20e56e8608c209537fff692d7de
Autor:
Satoshi Hamano, Naoto Kobayashi, Hideyo Kawakita, Keiichi Takenaka, Yuji Ikeda, Noriyuki Matsunaga, Sohei Kondo, Hiroaki Sameshima, Kei Fukue, Shogo Otsubo, Akira Arai, Chikako Yasui, Hitomi Kobayashi, Giuseppe Bono, Ivo Saviane
Publikováno v:
The Astrophysical Journal Supplement Series. 262:2
We searched for diffuse interstellar bands (DIBs) in the 0.91$
Comment: 23 pages, 12 figures, 4 tables. Accepted for publication in The Astrophysical Journal Supplement
Comment: 23 pages, 12 figures, 4 tables. Accepted for publication in The Astrophysical Journal Supplement
Autor:
Dante Minniti, Kaike Pan, Roger E. Cohen, R. Contreras Ramos, J. Olivares Carvajal, Rachael L. Beaton, Ivo Saviane, D. A. García-Hernández, C. Moni Bidin, Richard R. Lane, José G. Fernández-Trincado, M. Zoccali, Doug Geisler, F. Gran, D. V. Bizyaev, Sandro Villanova, A. Rojas-Arriagada, Christian Nitschelm, F. Rojas
The second phase of the APOGEE survey is providing near-infrared, high-resolution, high signal-to-noise spectra of stars in the halo, disk, bar and bulge of the Milky Way. The near-infrared spectral window is especially important in the study of the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::22ac0603680732f3a14def2ca328c750
Autor:
Gabriele Bruni, Francesca Panessa, Ivo Saviane, Loredana Bassani, Francesco Ursini, Lorenzo Monaco, Angela Malizia, P. Ubertini, Angela Bazzano, Daniele Dallacasa, N. Masetti, Tiziana Venturi
We present an update on the sample of soft gamma-ray selected giant radio galaxies (GRGs) extracted from INTEGRAL/IBIS and Swift/BAT surveys; it includes 8 new sources and one candidate object. In the new sample all, but one source, display FR II rad
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc0696a63fcfdfe3e6e5263754270b5f
http://arxiv.org/abs/2010.06427
http://arxiv.org/abs/2010.06427
Sky Quality Meter and satellite correlation for the night cloud cover analysis at astronomical sites
Autor:
Pietro Fiorentin, Ivo Saviane, Sergio Ortolani, S. Cavazzani, A Bertolo, Giovanni Carraro, Zitelli, R Binotto
The analysis of night cloud cover is very important for astronomical observations in real time, considering a typical observation time of about 15 minutes, and to provide statistics. In this article, we use the Sky Quality Meter (SQM) for high-resolu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51e893cd2cdfeab6e36aabc66ab11368
Autor:
Vardan Adibekyan, Piercarlo Bonifacio, Giuseppina Micela, J. I. González Hernández, Alessandro Sozzetti, M. R. Zapatero-Osorio, Paolo Molaro, Nelson J. Nunes, Ivo Saviane, P. Figueira, Yann Alibert, A. Suarez-Mascareno, Andrea Mehner, Sérgio F. Sousa, Elisabetta Caffau, V. D'Odorico, R. Genova, Lorenzo Monaco, Stéphane Udry, Ennio Poretti, David Ehrenreich, Nuno C. Santos, C. Lovis, C. Allende Prieto, Francesco Pepe, Cristina Martins, David Aguado, S. Cristiani, G. Cupani, P. Di Marcantonio, G. Lo Curto, Rafael Rebolo
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Universidad de Alicante (UA)
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A129. ⟨10.1051/0004-6361/201935833⟩
Universidad de Alicante (UA)
Astronomy & Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 633, pp.A129. ⟨10.1051/0004-6361/201935833⟩
Context. The vast majority of the known stars of ultra low metallicity ([Fe=H] >-4:5) are known to be enhanced in carbon, and belong to the 'low-carbon band' (A(C) = log(C=H) + 12 7:6). It is generally, although not universally, accepted that this pe
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5683840d4f28b2c6500cec69c463681
http://hdl.handle.net/10261/234011
http://hdl.handle.net/10261/234011