509 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Purdue University West LafayetteUS138 papers
- University of UtahUS136 papers
- Iowa State UniversityUS135 papers
- University of California, Los AngelesUS135 papers
- Center for Astrophysics Harvard & SmithsonianUS133 papers
- Ollscoil na Gaillimhe – University of GalwayIE133 papers
- Washington University in St. LouisUS133 papers
- McGill UniversityCA129 papers
- Munster Technological UniversityIE129 papers
- University of California, Santa CruzUS124 papers
- University College DublinIE123 papers
- Columbia UniversityUS122 papers
5 papers · 2 filters
Detection of TeV Gamma Rays from the BL Lac Object 1ES1959+650 with the Whipple 10m Telescope
J. Holder, VERITAS collaboration
We present the first strong detection of very high energy gamma-rays from the close (z=0.048) X-ray selected BL Lacertae object 1ES1959+650. Observations were made with the Whipple…
The TeV spectrum of H1426+428
D. Petry, I. H. Bond, S. M. Bradbury +45
The BL Lac object H1426+428 was recently detected as a high energy gamma-ray source by the VERITAS collaboration (Horan et al. 2002). We have reanalyzed the 2001 portion of the dat…
Discovery of Spectral Variability of Markarian 421 at TeV Energies
F. Krennrich, I. H. Bond, S. M. Bradbury +38
The detection of spectral variability of the gamma-ray blazar Mrk 421 at TeV energies is reported. Observations with the Whipple Observatory 10m gamma-ray telescope taken in 2000/2…
RR Lyrae Stars and Anomalous Cepheids in the Draco Dwarf Spheroidal Galaxy
K. Kinemuchi, H. A. Smith, A. LaCluyze +4
We present new results on RR Lyrae stars and anomalous Cepheids in the Draco dwarf spheroidal galaxy. We have increased the number of double-mode RR Lyrae stars and found three new…
Detection of the BL Lac Object H1426+428 at TeV Gamma Ray Energies
D. Horan
A very high energy (VHE) gamma-ray signal has been detected at the 5.4 sigma level from H1426+428, an x-ray selected BL Lacertae object at a redshift of 0.129. The object was monit…