853 citations
- California Institute of TechnologyUS8 papers
- University of CopenhagenDK8 papers
- Johns Hopkins UniversityUS7 papers
- Max Planck SocietyDE7 papers
- University of MichiganUS7 papers
- Max Planck Institute for Extraterrestrial PhysicsDE5 papers
- National Radio Astronomy ObservatoryUS5 papers
- Universities Space Research AssociationUS5 papers
- University of LeicesterGB5 papers
- University of Maryland, Baltimore CountyUS5 papers
- University of Maryland, College ParkUS5 papers
- Deleted Institution4 papers
6 papers · 2 filters
Prospecting for Heavy Elements with Future Far-IR/Submillimeter Observatories
D. Leisawitz, D. J. Benford, A. Kashlinsky +6
To understand the cosmic history of element synthesis it will be important to obtain extinction-free measures of the heavy element contents of high-redshift objects and to chart tw…
Konus catalog of short GRBs
E. P. Mazets, R. L. Aptekar, D. D. Frederiks +5
Observational data on the short GRBs obtained with the GGS-Wind Konus experiment in the period from 1994 to 2002 are presented. The catalog currently includes 130 events, detailing…
Gamma Rays From Rotation-Powered Pulsars
Alice K. Harding
The seven known gamma-ray pulsars represent a very small fraction of the more than 1000 presently known radio pulsars, yet they can give us valuable information about pulsar partic…
Implications of Ultrahigh Energy Air Showers for Physics and Astrophysics
F. W. Stecker
The primary ultrahigh energy particles which produce giant extensive air showers in the Earth's atmosphere present an intriguing mystery from two points of view: (1) How are these…
Astrophysics at the Highest Energy Frontiers
F. W. Stecker
I discuss recent advances being made in the physics and astrophysics of cosmic rays and cosmic gamma-rays at the highest observed energies as well as the related physics and astrop…
Spectral and Timing Properties of the Low-mass X-ray Binary 4U 0614+09 with XMM-Newton
M. Mendez, Jean Cottam, F. Paerels
4U 0614+09 is a low-mass X-ray binary with a weakly magnetized neutron star primary. It shows variability on time scales that range from years down to ~0.8 milliseconds. Before the…