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High Time-Resolution Astronomy on the 10-m SALT

Published online by Cambridge University Press:  20 April 2012

Barry Welsh
Affiliation:
Experimental Astrophysics Group, Space Sciences Laboratory, UC Berkeley, CA 94720, USA email: bwelsh@ssl.berkeley.edu
David Anderson
Affiliation:
Experimental Astrophysics Group, Space Sciences Laboratory, UC Berkeley, CA 94720, USA email: bwelsh@ssl.berkeley.edu
Jason McPhate
Affiliation:
Experimental Astrophysics Group, Space Sciences Laboratory, UC Berkeley, CA 94720, USA email: bwelsh@ssl.berkeley.edu
John Vallerga
Affiliation:
Experimental Astrophysics Group, Space Sciences Laboratory, UC Berkeley, CA 94720, USA email: bwelsh@ssl.berkeley.edu
Oswald H. W. Siegmund
Affiliation:
Experimental Astrophysics Group, Space Sciences Laboratory, UC Berkeley, CA 94720, USA email: bwelsh@ssl.berkeley.edu
David Buckley
Affiliation:
SALT, South African Astronomical Observatory, Cape Town, South Africa
Amanda Gulbis
Affiliation:
SALT, South African Astronomical Observatory, Cape Town, South Africa
Marissa Kotze
Affiliation:
SALT, South African Astronomical Observatory, Cape Town, South Africa
Stephen Potter
Affiliation:
SALT, South African Astronomical Observatory, Cape Town, South Africa
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Abstract

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We present a brief description of the Berkeley Visible Imaging Tube (BVIT) detector system, which is a user instrument on the 10-m Southern African Large Telescope (SALT), and include some preliminary observational results gained in mid-2011. The data show that BVIT is capable of revealing emission features occurring on time-scales of < 0.1 sec, thus opening up for the general user a window of high time-resolution astronomy at visible wavelengths.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2012

References

Allred, J., et al. 2006, ApJ, 644, 484CrossRefGoogle Scholar
Barnes, A., et al. 2007, MNRAS, 380, 1182Google Scholar
Beskin, G., et al. 1990, BCrAO 79, 67Google Scholar
Buckley, D., et al. 2010, Proc. SPIE, 7735, 174Google Scholar
Dhillon, V. & Marsh, T. 2001, New. Astron. Revs, 45, 91CrossRefGoogle Scholar
Fuhrmeister, B., Liefke, C., Schmitt, J., & Reiners, A. 2008, A&A, 487, 293Google Scholar
Hawley, S., et al. 1995, ApJ, 453, 464CrossRefGoogle Scholar
Kotze, M., et al. 2012 MNRAS, in preparationGoogle Scholar
McLaughlin, M., et al. 2006, Nature, 439, 817CrossRefGoogle Scholar
Shih, I., Charles, P., & Cornelisse, R. 2011, MNRAS, 412, 120Google Scholar
Siegmund, O. H. W., et al. 2008, in: Phelan, D., Ryan, O. & Shearer, A. (eds.), High Time Resolution Astrophysics. AIP Conf. Ser. Vol. 984, (AIP), p. 103Google Scholar
Zhilyaev, B., et al. 2007, A&A, 465, 235Google Scholar