Capaccioli, Massimo VST processing facility: first astronomical applications. In: 54th Congress SAIt, 4-7 May 2010, Napoli. (In stampa)
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| Tipologia del documento: | Contributo a Convegno o Workshop ([non definito]) |
|---|---|
| Titolo: | VST processing facility: first astronomical applications |
| Autori: | Autore Email Capaccioli, Massimo [non definito] |
| Autore/i: | Grado, Aniello; Limatola, L.; Getman, F. |
| Numero di pagine: | 6 |
| Dipartimento: | Scienze fisiche |
| Sezione di dipartimento: | UniTA |
| URL ufficiale: | http://arxiv.org/PS_cache/arxiv/pdf/1102/1102.1588... |
| Tipo di evento: | Congresso |
| Titolo dell'evento: | 54th Congress SAIt |
| Luogo dell'evento: | Napoli |
| Data dell'evento: | 4-7 May 2010 |
| Numero di pagine: | 6 |
| Parole chiave: | Image Processing; Astronomical Techniques; Astrophysical Data |
| Settori scientifico-disciplinari del MIUR: | Area 02 - Scienze fisiche > FIS/05 - Astronomia e astrofisica |
| Depositato il: | 02 Mar 2011 13:05 |
| Ultima modifica: | 30 Apr 2014 19:43 |
| URI: | http://www.fedoa.unina.it/id/eprint/7900 |
Abstract
VST–Tube is a new software package designed to process optical astronomical images. It is an automated pipeline to go from the raw exposures to fully calibrated co-added images, and to extract catalogs with aperture and PSF photometry. A set of tools allow the data administration and the quality check of the intermediate and final products. VST-Tube comes with a Graphical User Interface to facilitate the interaction between data and user. We outline here the VST–Tube architecture and show some applications enlightening some of the characteristics of the pipeline.
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