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High Time Resolution Spectroscopy of Short Period Variable Objects

Published online by Cambridge University Press:  22 February 2018

R. Michel  and
J. L. A. Fordham
R. Michel
Affiliation:
Instituto de Astronomía, UNAM, Ensenada, México
J. L. A. Fordham
Affiliation:
Department of Physics and Astronomy, UCL, London, UK

Extract

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Photon counting detector technology allows high time resolution spectroscopy on sources such as pulsars and cataclysmic variables. Here we report on first observing trials on Cvs in a high time resolution mode undertaken with the MIC photon counting detector (Fordham et al. 2000) on the 2.1m telescope at San Pedro Martir Observatory.

Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 263
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Fordham, J. L. A., Kawakami, H., Michel, R., Much, R., & Robinson, J. R. 2000, MNRAS, 319, 414 Google Scholar