Capaccioli, Massimo VST processing facility: first astronomical applications. In: 54th Congress SAIt, 4-7 May 2010, Napoli. (In press)
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Item Type: | Conference or Workshop Item (UNSPECIFIED) | ||||
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Title: | VST processing facility: first astronomical applications | ||||
Creators: |
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Autore/i: | Grado, Aniello; Limatola, L.; Getman, F. | ||||
Number of Pages: | 6 | ||||
Department: | Scienze fisiche | ||||
Sezione di dipartimento: | UniTA | ||||
Original publication URL: | http://arxiv.org/PS_cache/arxiv/pdf/1102/1102.1588... | ||||
Event Type: | Congresso | ||||
Event Title: | 54th Congress SAIt | ||||
Event Location: | Napoli | ||||
Event Dates: | 4-7 May 2010 | ||||
Number of Pages: | 6 | ||||
Keywords: | Image Processing; Astronomical Techniques; Astrophysical Data | ||||
Settori scientifico-disciplinari del MIUR: | Area 02 - Scienze fisiche > FIS/05 - Astronomia e astrofisica | ||||
Date Deposited: | 02 Mar 2011 13:05 | ||||
Last Modified: | 30 Apr 2014 19:43 | ||||
URI: | http://www.fedoa.unina.it/id/eprint/7900 |
Collection description
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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