PSF modelling for very wide-field CCD astronomy

PSF modelling for very wide-field CCD astronomy

Context. One of the possible approaches to detecting optical counterparts of GRBs requires monitoring large parts of the sky. This idea has gained some instrumental support in recent years, such as with the “Pi of the Sky” project. The broad sky coverage of the “Pi of the Sky” apparatus results from...

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Bibliographic Details
Main Authors: Piotrowski, L., Batsch, T., Czyrkowski, H., Cwiok, M., Dabrowski, R., Kasprowicz, G., Majcher, A., Majczyna, A., Malek, K., Mankiewicz, L., Nawrocki, K., Opiela, R., Siudek, M., Sokolowski, Marcin, Wawrzaszek, R., Wrochna, G., Zaremba, M., Zarnecki, A.
Format: Journal Article
Published: EDP Sciences 2013
Subjects:
techniques: photometric
methods: laboratory
methods: data analysis
methods: analytical
instrumentation: detectors
astroparticle physics
Online Access:http://hdl.handle.net/20.500.11937/14027

Internet

http://hdl.handle.net/20.500.11937/14027

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