activity
19972024
most citedThe Large Area Telescope on the Fermi Gamma-ray Space Telescope Mission

4.1k citations · 40.1k across the 247 of their papers we have counts for

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Showing 1997Show all

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astro-ph1997★ 172 cited

Discovery of >350 GeV Gamma Rays from the BL Lacertae Object 1ES 2344+514

M. Catanese, C. W. Akerlof, H. M. Badran +31

We present the discovery of >350 GeV gamma-ray emission from the BL Lacertae object 1ES 2344+514 with the Whipple Observatory 10m gamma-ray telescope. This is the third BL Lac obje…

astro-ph1997★ 200 cited

Multiwavelength Observations of a Flare from Markarian 501

M. Catanese, S. M. Bradbury, A. C. Breslin +23

We present multiwavelength observations of the BL Lacertae object Markarian 501 (Mrk 501) in 1997 between April 8 and April 19. Evidence of correlated variability is seen in very h…

astro-ph1997

A Search for TeV Emission from Unidentified Sources in the Galactic Plane

J. H. Buckley, P. J. Boyle, S. M. Bradbury +24

The ~70 unidentified sources of the EGRET sky survey may be one of its most important legacies. The identification of these sources at other wavelengths is critical to understandin…

astro-ph1997

First Results from a Search for TeV Emission from BL Lacs

M. Catanese, P. J. Boyle, J. H. Buckley +22

Two active galactic nuclei have been detected at TeV energies using the atmospheric Cherenkov imaging technique. The Whipple Observatory gamma-ray telescope has been used to observ…

astro-ph1997★ 2 cited

Constraints on Cosmic-Ray Origin Theories from TeV Gamma-Ray Observations

R. W. Lessard, P. J. Boyle, S. M. Bradbury +23

If supernova remnants (SNRs) are the sites of cosmic-ray acceleration, the associated nuclear interactions should result in observable fluxes of TeV gamma-rays from the nearest SNR…

astro-ph1997★ 4 cited

A search for correlations of TeV gamma-rays with ultra-high energy cosmic rays

C. W. Akerlof, S. Biller, P. Boyle +25

A search was conducted for TeV gamma-rays emitted from the direction of the ultra-high energy cosmic ray detected by the Fly's Eye Experiment with E ~ 3 x 10**20 eV. No enhancement…