Fast Photometry - New Facilities at La-Silla

Details Fast Photometry - New Facilities at La-Silla Fast Photometry - New Facilities at La-Silla

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980msngr..22...16p&link_type=abstract

The Messenger, No.22, P. 16, 1980

Physics

Scientific paper

The standard photometric equipment at La Silla has 1 second of time as the shortest integration time. This is fully sufficient for most observing programmes. There are, however, several kinds of phenomena which have timescales of about a second or shorter. Among the fastest phenomena, one could mention the optical outbursts of the X-ray bursters (see The Messenger No. 18,34) or occultations of stars by objects in the solar system.

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