High time resolution astrophysics and ELTs: Which wavelength?

Details High time resolution astrophysics and ELTs: Which wavelength? High time resolution astrophysics and ELTs: Which wavelength?

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008spie.6986e..10s&link_type=abstract

Extremely Large Telescopes: Which Wavelengths? Retirement Symposium for Arne Ardeberg. Edited by Andersen, Torben E. Proceed

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Observational High Time Resolution Astrophysics differs from conventional astrophysics in regard to the detectors employed which have a time resolution less than that obtainable through CCD with a normal readout τ < a few minutes. This paper looks at the implications for HTRA from extremely large telescopes and specifically, as an exemplar its possible impact on pulsar astrophysics. We demonstrate, by using the derived point-spread-function from models of the Euro50 telescope, the possible effects active and adaptive mirrors have on observing rapidly varying astronomical objects.

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