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The status of the Whipple 10m GRANITE III upgrade program.

Authors :
Finley, J. P.
Bond, I. H.
Bradbury, S. M.
Breslin, A. C.
Buckley, J. H.
Burdett, A. M.
Carson, M.
Carter-Lewis, D. A.
Catanese, M.
Cawley, M. F.
Dunlea, S.
D’Vali, M.
Fegan, D. J.
Fegan, S. J.
Gaidos, J. A.
Hall, T. A.
Hillas, A. M.
Horan, D.
Knapp, J.
Krennrich, F.
Source :
AIP Conference Proceedings; 2000, Vol. 515 Issue 1, p301, 7p, 7 Graphs
Publication Year :
2000

Abstract

The Whipple Collaboration has been carrying out an upgrade program, GRANITE III, on the 10m telescope atop Mt. Hopkins. The 3 year program, 1996 through 1999, has involved a large field-of-view camera, a hardware pattern recognition trigger, and finally a small pixel camera. Results of the first and second stage of the program indicate that a large field-of-view yield an increased collection area for cosmic-ray triggers and the hardware pattern trigger reduces the energy threshold of the telescope by greatly suppressing night sky accidental triggers over a simple multiplicity coincidence trigger. The final phase of the program, being completed during the summer and fall of 1999, will be the installation of a small pixel camera. The pixel size of ∼0°.12 will yield the lowest threshold energy at which the 10 m Whipple telescope has ever operated. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR]

Subjects

Subjects :
TELESCOPES
COSMIC rays

Details

Language :
English
ISSN :
0094243X
Volume :
515
Issue :
1
Database :
Complementary Index
Journal :
AIP Conference Proceedings
Publication Type :
Conference
Accession number :
6028247