The sensitivity of atmospheric Čerenkov detectors for gamma-ray astronomy-Reference-Cited by-同舟云学术

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The sensitivity of atmospheric Čerenkov detectors for gamma-ray astronomy

Published:1976-09 Issue:1 Volume:35 Page:95-109
ISSN:1826-9877
Container-title:Il Nuovo Cimento B Series 11
language:en
Short-container-title:Nuovo Cim B

Author:

Weekes T. C.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.1007/BF02726286.pdf

Reference16 articles.

1. J. V. Jelley andN. A. Porter:Quart. Journ. Roy. Astron. Soc.,4, 275 (1963).

2. V. I. Zatsepin andA. E. Chudakov:Sov. Phys. JETP,15, 1126 (1962).

3. C. D. Long: Ph. D. Thesis, National University of Ireland (1967).

4. C. Castagnoli, P. Picchi andM. A. Locci:Nuovo Cimento,9 B, 213 (1972).

5. G. H. Rieke: Smithsonian Astronomical Observatory, Special Report 310 (1969).

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1. The T[CLC]e[/CLC]V Spectrum of Markarian 501;The Astrophysical Journal;1998-07-01

2. Measurement of TeV gamma-ray spectra with the Cherenkov imaging technique;Astroparticle Physics;1998-06

3. Upper Limits on TeV Gamma-Ray Emission from Active Galactic Nuclei;The Astrophysical Journal;1995-10

4. Instrumentation for very high energy gamma-ray astronomy;Experimental Astronomy;1995

5. Gamma-ray observations of the Crab Nebula at TeV energies;The Astrophysical Journal;1991-08

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