output
20042011
most citedSwift BAT Survey of AGN

301 citations

Showing 2009 · astro-ph.HEShow all

7 papers · 2 filters

astro-ph.HE200966 cited

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…

astro-ph.HE200966 cited

Searching for New Physics with Ultrahigh Energy Cosmic Rays

Floyd W. Stecker, Sean T. Scully

Ultrahigh energy cosmic rays that produce giant extensive showers of charged particles and photons when they interact in the Earth's atmosphere provide a unique tool to search for…

astro-ph.HE200936 cited

A Chandra view of NGC 3621: a bulgeless galaxy hosting an AGN in its early phase?

M. Gliozzi, S. Satyapal, M. Eracleous +2

We report the detection of a weak X-ray point source coincident with the nucleus of the bulgeless disk galaxy NGC 3621, recently discovered by Spitzer to display high ionization mi…

astro-ph.HE200910 cited

The Supercritical Pile GRB Model: The Prompt to Afterglow Evolution

A. Mastichiadis, D. Kazanas

The "Supercritical Pile" is a very economical GRB model that provides for the efficient conversion of the energy stored in the protons of a Relativistic Blast Wave (RBW) into radia…

astro-ph.HE200990 cited

A decade of timing an accretion-powered millisecond pulsar: The continuing spin down and orbital evolution of SAX J1808.4-3658

J. M. Hartman, A. Patruno, D. Chakrabarty +4

The Rossi X-ray Timing Explorer has observed five outbursts from the transient 2.5 ms accretion-powered pulsar SAX J1808.4-3658 during 1998-2008. We present a pulse timing study of…

astro-ph.HE2009144 cited

A statistical study of gamma-ray burst afterglows measured by the Swift Ultra-violet Optical Telescope

S. R. Oates, M. J. Page, P. Schady +14

We present the first statistical analysis of 27 UVOT optical/ultra-violet lightcurves of GRB afterglows. We have found, through analysis of the lightcurves in the observer's frame,…