output
20042011
most citedSwift BAT Survey of AGN

301 citations

Showing 2006Show all

15 papers · 1 filter

astro-ph200642 cited

Multi-frequency monitoring of gamma-ray loud blazars: I. Light curves and spectral energy distributions

U. Bach, C. M. Raiteri, M. Villata +23

Context: Being dominated by non-thermal emission from aligned relativistic jets, blazars allow us to elucidate the physics of extragalactic jets, and, ltimately, how the energy is…

astro-ph200636 cited

Redshift Filtering by Swift Apparent X-ray Column Density

Dirk Grupe, John A. Nousek, Daniel E. vanden Berk +5

We remark on the utility of an observational relation between the absorption column density in excess of the Galactic absorption column density, $ΔN_{\rm H} = N_{\rm H, fit} - N_{\…

astro-ph20061 cited

The "Supercritical Pile" GRB Model: Afterglows and GRB, XRR, XRF Unification

Demosthenes Kazanas, Apostolos Mastichiadis, Markos Georganopoulos

We present the general notions and observational consequences of the "Supercritical Pile" GRB model; the fundamental feature of this model is a detailed process for the conversion…

astro-ph2006109 cited

The variable X-ray spectrum of Markarian 766 - I. Principal components analysis

L. Miller, T. J. Turner, J. N. Reeves +3

Aims: We analyse a long XMM-Newton spectrum of the narrow-line Seyfert 1 galaxy Mrk 766, using the marked spectral variability on timescales >20ks to separate components in the X-r…

astro-ph2006208 cited

Relativistic Beaming and the Intrinsic Properties of Extragalactic Radio Jets

M. H. Cohen, M. L. Lister, D. C. Homan +4

Relations between the observed quantities for a beamed radio jet, apparent transverse speed and apparent luminosity (beta_app,L), and the intrinsic quantities, Lorentz factor and i…

astro-ph200630 cited

A Stellar-mass Black Hole in the Ultra-luminous X-ray Source M82 X-1?

Takashi Okajima, Ken Ebisawa, Toshihiro Kawaguchi

We have analyzed the archival XMM-Newton data of the bright Ultra-Luminous X-ray Source (ULX) M82 X-1 with an 105 ksec exposure when the source was in the steady state. Thanks to t…