output
19972026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations

Showing 2000 · astro-phShow all

6 papers · 2 filters

astro-ph2000★ 34 cited

3EG J2016+3657: Confirming an EGRET Blazar Behind the Galactic Plane

J. P. Halpern, M. Eracleous, R. Mukherjee +1

We recently identified the blazar-like radio source G74.87+1.22 (B2013+370) as the counterpart of the high-energy gamma-ray source 3EG J2016+3657 in the Galactic plane. However, si…

astro-ph2000

Performance of the STACEE Atmospheric Cherenkov Telescope

STACEE Collaboration, D. A. Williams, D. Bhattacharya +20

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is located at the National Solar Thermal Test Facility of Sandia National Laboratories in Albuquerque, New Mexico,…

astro-ph2000

High Energy Gamma Rays

R. Mukherjee

This article reviews the present status of high energy gamma-ray astronomy at energies above 30 MeV. Observations in the past decade using both space- and ground-based experiments…

astro-ph2000★ 140 cited

The Frequency of Polarized Broad Emission Lines in Type 2 Seyfert Galaxies

E. C. Moran, A. J. Barth, L. E. Kay +1

We have discovered polarized broad emission lines in five type 2 Seyfert galaxies (NGC 424, NGC 591, NGC 2273, NGC 3081, and NGC 4507), establishing that these objects are type 1 S…

astro-ph2000★ 30 cited

High Energy Gamma-Ray Observations of the Crab Nebula and Pulsar with the Solar Tower Atmospheric Cherenkov Effect Experiment

STACEE Collaboration, S. Oser, D. Bhattacharya +17

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a new ground-based atmospheric Cherenkov telescope for gamma-ray astronomy. STACEE uses the large mirror area of…

astro-ph2000★ 42 cited

Multiwavelength Examination of the COS-B Field 2CG 075+00 Yields a Blazar Identification for 3EG J2016+3657

R. Mukherjee, E. V. Gotthelf, J. Halpern +1

We present a high-energy study of the intriguing COS-B gamma-ray field, 2CG 075+00, in order to search for possible counterparts. New EGRET data show that the COS-B emission probab…