911 citations
- Goddard Space Flight CenterUS23 papers
- University of Maryland, College ParkUS10 papers
- Max Planck Institute for Extraterrestrial PhysicsDE8 papers
- Center for Astrophysics Harvard & SmithsonianUS5 papers
- Centre National de la Recherche ScientifiqueFR5 papers
- Deleted Institution5 papers
- Astrophysique, Instrumentation et ModélisationFR4 papers
- California Institute of TechnologyUS4 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR4 papers
- Kavli Institute for Particle Astrophysics and CosmologyUS4 papers
- National Institute for AstrophysicsIT4 papers
- RIKENJP4 papers
43 papers
The absorption-dominated model for the X-ray spectra of type I active galaxies: MCG-6-30-15
L. Miller, T. J. Turner, J. N. Reeves
MCG-6-30-15 is the archetypal example of a type I active galaxy showing broad "red-wing" emission in its X-ray spectrum at energies below the 6.4 keV Fe K-alpha emission line and a…
Discovery of Pulsations from the Pulsar J0205+6449 in SNR 3C 58 with the Fermi Gamma-Ray Space Telescope
Fermi LAT collaboration, Fermi Pulsar Timing Consortium
We report the discovery of gamma-ray pulsations (> 0.1 GeV) from the young radio and X-ray pulsar PSR J0205+6449 located in the Galactic supernova remnant 3C 58. Data in the gamma-…
A Compton-thick Wind in the High Luminosity Quasar, PDS 456
J. N. Reeves, P. T. O'Brien, V. Braito +7
PDS 456 is a nearby (z=0.184), luminous (L_bol ~10^47 erg/s) type I quasar. A deep 190 ks Suzaku observation in February 2007 revealed the complex, broad band X-ray spectrum of PDS…
Observational Limits on Type 1 AGN Accretion Rate in COSMOS
Jonathan R. Trump, Chris D. Impey, Brandon C. Kelly +13
We present black hole masses and accretion rates for 182 Type 1 AGN in COSMOS. We estimate masses using the scaling relations for the broad Hb, MgII, and CIV emission lines in the…
Star Formation in the Central 400 pc of the Milky Way: Evidence for a Population of Massive YSOs
F. Yusef-Zadeh, J. W. Hewitt, R. G. Arendt +8
The central kpc of the Milky Way might be expected to differ significantly from the rest of the Galaxy with regard to gas dynamics and the formation of YSOs. We probe this possibil…
Measurement of the Cosmic Ray e+ plus e- spectrum from 20 GeV to 1 TeV with the Fermi Large Area Telescope
LAT Collaboration
Designed as a high-sensitivity gamma-ray observatory, the Fermi Large Area Telescope is also an electron detector with a large acceptance exceeding 2m^2 sr at 300 GeV. Building on…