911 citations
- Stanford UniversityUS14 papers
- University of California, Santa CruzUS12 papers
- Goddard Space Flight CenterUS11 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS11 papers
- University of Maryland, College ParkUS11 papers
- Centre National de la Recherche ScientifiqueFR10 papers
- Max Planck Institute for Extraterrestrial PhysicsDE10 papers
- SLAC National Accelerator LaboratoryUS10 papers
- AlbaNovaSE9 papers
- Istituto Nazionale di Fisica Nucleare, Roma Tor VergataIT9 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BariIT9 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di PadovaIT9 papers
13 papers · 1 filter
Fermi LAT Observations of the Vela Pulsar
A. A. Abdo
The Vela pulsar is the brightest persistent source in the GeV sky and thus is the traditional first target for new gamma-ray observatories. We report here on initial Fermi Large Ar…
Cometary Astropause of Mira Revealed in the Far-Infrared
Toshiya Ueta
Evolved mass-losing stars such as Mira enrich the interstellar medium (ISM) significantly by their dust-rich molecular wind. When these stars move fast enough relative to the ISM,…
Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
E. A. Baltz, B. Berenji, G. Bertone +25
We investigate the sensitivity of the Gamma-ray Large Area Space Telescope (GLAST) to indirectly detect weakly interacting massive particles (WIMPs) through the -ray signal that…
Measurement of cosmic-ray low-energy antiproton spectrum with the first BESS-Polar Antarctic flight
K. Abe, H. Fuke, S. Haino +27
The BESS-Polar spectrometer had its first successful balloon flight over Antarctica in December 2004. During the 8.5-day long-duration flight, almost 0.9 billion events were record…
Kinematics and H_2 morphology of the multipolar Post-AGB star IRAS 16594-4656
G. C. Van de Steene, T. Ueta, P. A. M. van Hoof +2
context: The spectrum of IRAS 16594-4656 shows shock excited H_2 emission and collisionally excited emission lines such as[O I],[C I],and [Fe II]. aim: The goal is to determine the…
A celestial gamma-ray foreground due to the albedo of small solar system bodies and a remote probe of the interstellar cosmic ray spectrum
Igor V. Moskalenko, Troy A. Porter, Seth W. Digel +2
We calculate the gamma-ray albedo flux from cosmic-ray (CR) interactions with the solid rock and ice in Main Belt asteroids (MBAs), Jovian and Neptunian Trojan asteroids, and Kuipe…