output
20042015
most citedSwift BAT Survey of AGN

301 citations

Showing 2014Show all

7 papers · 1 filter

astro-ph.HE2014

Modelling the -ray and radio light curves of the double pulsar system

A. S. Seyffert, C. Venter, A. K. Harding +1

Guillemot et al. recently reported the discovery of -ray pulsations from the 22.7ms pulsar (pulsar A) in the famous double pulsar system J0737-3039A/B. The -ray light curve (…

astro-ph.HE201416 cited

Probing large-scale wind structures in Vela X-1 using off-states with INTEGRAL

L. Sidoli, A. Paizis, F. Fuerst +4

Vela X-1 is the prototype of the class of wind-fed accreting pulsars in high mass X-ray binaries hosting a supergiant donor. We have analyzed in a systematic way ten years of INTEG…

astro-ph.HE2014150 cited

Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era

Christopher P. L. Berry, Ilya Mandel, Hannah Middleton +15

Advanced ground-based gravitational-wave (GW) detectors begin operation imminently. Their intended goal is not only to make the first direct detection of GWs, but also to make infe…

hep-ph201484 cited

Searching for Traces of Planck-Scale Physics with High Energy Neutrinos

Floyd W. Stecker, Sean T. Scully, Stefano Liberati +1

High energy cosmic neutrino observations provide a sensitive test of Lorentz invariance violation, which may be a consequence of quantum gravity theories. We consider a class of no…

astro-ph.GA2014241 cited

Clumpy Galaxies in CANDELS. I. The Definition of UV Clumps and the Fraction of Clumpy Galaxies at 0.5<z<3

Yicheng Guo, Henry C. Ferguson, Eric F. Bell +19

Although giant clumps of stars are crucial to galaxy formation and evolution, the most basic demographics of clumps are still uncertain, mainly because the definition of clumps has…

astro-ph.HE201475 cited

Discovery of a ~5 day characteristic timescale in the Kepler power spectrum of Zw 229-15

Rick Edelson, Simon Vaughan, Matt Malkan +4

We present time series analyses of the full Kepler dataset of Zw 229-15. This Kepler light curve --- with a baseline greater than three years, composed of virtually continuous, eve…