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Departamento Gestión de Conocimiento, Monitoreo y Prospección
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(Very) Fast astronomical photometry for meter-class telescopes
Indexado
WoS WOS:000469927500001
Scopus SCOPUS_ID:85067822421
DOI
Año 2019
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Our team at the INAF-Astronomical Observatory of Padova and the University of Padova is engaged in the design, construction and operations of instruments with very high time accuracy in the optical band for applications to High Time Resolution Astrophysics and Quantum Astronomy. Two instruments were built to perform photon counting with sub-nanosecond temporal accuracy, Aqueye+ and Iqueye. Aqueye+ is regularly mounted at the 1.8m Copernicus telescope in Asiago, while Iqueye was mounted at several 4m class telescopes around the world and is now attached through the Iqueye Fiber Interface to the 1.2m Galileo telescope in Asiago. They are used to perform coordinated high time resolution optical observations and, for the first time ever, experiments of optical intensity interferometry on a baseline of a few kilometers. We report on recent technological developments and scientific results obtained within the framework of this project.

Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Zampieri, L. Hombre INAF Astron Observ Padova - Italia
Osservatorio Astronomico di Padova - Italia
2 Naletto, G. Hombre Univ Padua - Italia
Università degli Studi di Padova - Italia
3 Barbieri, Cesare Hombre INAF Astron Observ Padova - Italia
Univ Padua - Italia
Osservatorio Astronomico di Padova - Italia
Università degli Studi di Padova - Italia
4 Burtovoi, A. Hombre INAF Astron Observ Padova - Italia
Univ Padua - Italia
Osservatorio Astronomico di Padova - Italia
Università degli Studi di Padova - Italia
5 Fiori, M. Mujer Univ Padua - Italia
Università degli Studi di Padova - Italia
6 Spolon, A. - Univ Padua - Italia
Università degli Studi di Padova - Italia
7 Ochner, P. Hombre Univ Padua - Italia
Università degli Studi di Padova - Italia
8 Lessio, L. Hombre INAF Astron Observ Padova - Italia
Osservatorio Astronomico di Padova - Italia
9 Umbriaco, Gabriele Mujer Univ Padua - Italia
Università degli Studi di Padova - Italia
10 Barbieri, M. Hombre Universidad de Atacama - Chile

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Financiamiento



Fuente
Fondazione Cassa di Risparmio di Padova e Rovigo
Fondazione Banca Popolare di Marostica-Volksbank
Italian Ministry of University MIUR through the programme PRIN 2006
Project of Excellence 2006 Fondazione CARIPARO
INAF-Astronomical Observatory of Padova
University of Padova under the Quantum Future Strategic Project
Università degli Studi di Padova
Italian Ministry of University MIUR
Fondazione Banca Popolare di Lodi

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Agradecimientos



Agradecimiento
We are grateful to all the staff of the Asiago observing station (Venerio Chiomento, Giancarlo Farisato, Aldo Frigo, Giorgio Martorana, Luciano Traverso, Robertino Bau', Giovanni Costa, Alessandro Siviero) for their work and support. We also thank Marco Fiaschi, Tommaso Occhipinti, Enrico Verroi and Paolo Zoccarato for their external support to the project. This wok is based on observations collected at the Copernicus telescope (Asiago, Italy) of the INAF-Osservatorio Astronomico di Padova and at the Galileo telescope (Asiago, Italy) of the University of Padova. This project is partly supported by the University of Padova under the Quantum Future Strategic Project, by the Italian Ministry of University MIUR through the programme PRIN 2006, by the Project of Excellence 2006 Fondazione CARIPARO, by INAF-Astronomical Observatory of Padova under the grant "Osservazioni con strumentazione astronomica ad elevata risoluzione temporale e modellizzazione di emissione ottica variabile", and by Fondazione Banca Popolare di Marostica-Volksbank.
tion (Venerio Chiomento, Giancarlo Farisato, Aldo Frigo, Giorgio Martorana, Luciano Traverso, Robertino Bau’, Giovanni Costa, Alessandro Siviero) for their work and support. We also thank Marco Fiaschi, Tommaso Occhipinti, Enrico Verroi and Paolo Zoccarato for their external support to the project. This wok is based on observations collected at the Copernicus telescope (Asiago, Italy) of the INAF-Osservatorio As-tronomico di Padova and at the Galileo telescope (Asiago, Italy) of the University of Padova. This project is partly supported by the University of Padova under the Quantum Future Strategic Project, by the Italian Ministry of University MIUR through the programme PRIN 2006, by the Project of Excellence 2006 Fondazione CARIPARO, by INAF-Astronomical Observatory of Padova under the grant “Osservazioni con stru-mentazione astronomica ad elevata risoluzione temporale e modellizzazione di emis-sione ottica variabile”, and by Fondazione Banca Popolare di Marostica-Volksbank.

Muestra la fuente de financiamiento declarada en la publicación.