Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- P. Canfield4 profiles506 · h 82
- S. Bud’ko4 profiles421 · h 52
- J. Vary220 · h 49
- R. Prozorov4 profiles187 · h 54
- C. Soukoulis121 · h 111
- D. Johnston2 profiles118 · h 47
- R. McQueeney117 · h 45
- M. Tanatar113 · h 44
- P. Maris2 profiles93 · h 41
- A. Kreyssig2 profiles87 · h 37
- N. Ni2 profiles82 · h 51
- C. Struck79 · h 27
- Centre National de la Recherche ScientifiqueFR2.2k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR2.1k papers
- Brookhaven National LaboratoryUS2k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR2k papers
- University of ManchesterGB2k papers
- Lawrence Berkeley National LaboratoryUS1.9k papers
- McGill UniversityCA1.9k papers
- Columbia UniversityUS1.9k papers
- Stony Brook UniversityUS1.8k papers
- National Institute for Subatomic PhysicsNL1.8k papers
- University of California, IrvineUS1.8k papers
- Charles UniversityCZ1.8k papers
19 papers · 2 filters
Search for Pulsed TeV Gamma-ray Emission from the Crab Pulsar
R. W. Lessard, I. H. Bond, S. M. Bradbury +23
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10 m gamma-ray telescope. The direction of the Crab pulsar was obser…
Smoke in the "Smoke Rings": ISO Observations of Dust in Collisional Ring Galaxies
P. N. Appleton, V. Charmandaris, C. Horellou +2
Collisional ring galaxies probably result from a head-on collision between a compact companion galaxy and a gas-rich disk system. We present a review of the discovery of warm dust…
Ground-Based Gamma-Ray Astronomy
Michael Catanese
Ground-based gamma-ray astronomy has become an active astrophysical discipline with four confirmed sources of TeV gamma rays, two plerionic supernova remnants (SNRs) and two BL Lac…
DQ Herculis in Profile: Whole Earth Telescope Observations and Smoothed Particle Hydrodynamics Simulations
M. A. Wood, the XCov 15 Team
DQ Herculis was the Summer 1997 WET northern-hemisphere primary target. The O-C phase diagram of the 71-s signal reveals out-of-eclipse phase variations resulting from the self ecl…
Detection Techniques of Microsecond Gamma-Ray Bursts using Ground-Based Telescopes
F. Krennrich, S. Le Bohec, T. C. Weekes
Gamma-ray observations above 200 MeV are conventionally made by satellite-based detectors. The EGRET detector on the Compton Gamma Ray Observatory (CGRO) has provided good sensitiv…
Galaxy Collisions
Curtis Struck
Theories of how galaxies, the fundamental constituents of large-scale structure, form and evolve have undergone a dramatic paradigm shift in the last few decades. Earlier views wer…
VERITAS: Performance characteristics (baseline design)
V. V. Vassiliev, D. A. Carter-Lewis, A. M. Hillas +6
VERITAS is a proposed major ground-based gamma-ray observatory to be built at the Whipple Observatory in southern Arizona, USA. It will consist of an array of seven 10m imaging Che…
Simple Models for Turbulent Self-Regulation in Galaxy Disks
Curtis Struck, Daniel C. Smith
We propose that turbulent heating, wave pressure and gas exchanges between different regions of disks play a dominant role in determining the preferred, quasi-equilibrium, self-sim…
The Very Energetic Radiation Imaging Telescope Array System (VERITAS)
S. M. Bradbury, I. H. Bond, A. C. Breslin +32
We give an overview of the current status and scientific goals of VERITAS, a proposed hexagonal array of seven 10 m aperture imaging Cherenkov telescopes. The selected site is Mont…
Plasma and Warm Dust in the Collisional Ring Galaxy VIIZw466 from VLA and ISO Observations
P. N. Appleton, V. Charmandaris, C. Horellou +3
We present the first mid-infrared (Mid-IR) (m) and radio continuum (20,~6 and 3.6 cm) observations of the star-forming collisional ring galaxy VII Zw 466 and its…
Very High Energy Gamma-Ray Astronomy
Michael Catanese, Trevor C. Weekes
We present a review of the current status of very high energy gamma-ray astronomy. The development of the atmospheric Cherenkov imaging technique for ground-based gamma-ray astrono…
A Search for Pulsed TeV Gamma Ray Emission from the Crab Pulsar
A. M. Burdett, I. H. Bond, P. J. Boyle +28
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10m gamma-ray telescope. The direction of the Crab pulsar was observ…
Search for TeV Gamma-Rays from Shell-Type Supernova Remnants
Whipple Collaboration, R. W. Lessard, I. H. Bond +26
If cosmic rays with energies <100 TeV originate in the galaxy and are accelerated in shock waves in shell-type supernova remnants (SNRs), gamma-rays will be produced as the result…
The HI and Ionized Gas Disk of the Seyfert Galaxy NGC 1144 = Arp 118: A Violently Interacting Galaxy with Peculiar Kinematics
M. A. Bransford, P. N. Appleton, C. F. McCain +1
We present observations of the distribution and kinematics of neutral and ionized gas in NGC 1144, a galaxy that forms part of the Arp 118 system. Ionized gas is present over a hug…
On the gravitational stability of a compressed slab of gas in the background of weakly interacting massive particles
David Tsiklauri
Linear stability of an isothermal, pressure-bounded, self-gravitating gas slab which is gravitationally coupled with the background weakly interacting massive particles (WIMPs) is…
The Future of Cherenkov Astronomy
Michael Catanese
In the last ten years, the field of Cherenkov astronomy has become an important contributor to high energy astrophysics with the detection of eight objects at energies above 300 Ge…
The Flux Variability of Markarian 501 in Very High Energy Gamma Rays
J. Quinn, I. H. Bond, P. J. Boyle +26
The BL Lacertae object Markarian 501 was identified as a source of gamma-ray emission at the Whipple Observatory in March 1995. Here we present a flux variability analysis on sever…
Correlated variability of Mkn 421 at X-ray and TeV wavelengths on timescales of hours
L. Maraschi, G. Fossati, F. Tavecchio +26
Mkn 421 was observed for about two days with BeppoSAX, prior to and partly overlapping the start of a 1 week continuous exposure with ASCA in April 1998, as part of a world-wide mu…
New Generation Atmospheric Cherenkov Detectors
Frank Krennrich
High energy gamma-ray astronomy has been established during the last decade through the launch of the Compton Gamma Ray Observatory (CGRO) and the success of its ground-based count…