activity
20022015
most citedFermi Large Area Telescope Second Source Catalog

1.3k citations · 5.1k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2015★ 42 cited

Radio-quiet and radio-loud pulsars: similar in Gamma-rays but different in X-rays

M. Marelli, R. P. Mignani, A. De Luca +4

We present new Chandra and XMM-Newton observations of a sample of eight radio-quiet Gamma-ray pulsars detected by the Fermi Large Area Telescope. For all eight pulsars we identify…

astro-ph.HE2014★ 42 cited

Phase-resolved X-ray spectra of magnetars and the coronal outflow model

R. Hascoet, A. M. Beloborodov, P. R. den Hartog

We test a model recently proposed for the persistent hard X-ray emission from magnetars. In the model, hard X-rays are produced by a decelerating electron-positron flow in the clos…

astro-ph.HE2013★ 47 cited

Associating long-term gamma-ray variability with the superorbital period of LS I 61 303

LAT Collaboration

Gamma-ray binaries are stellar systems for which the spectral energy distribution (discounting the thermal stellar emission) peaks at high energies. Detected from radio to TeV gamm…

astro-ph.HE2013★ 837 cited

The Second Fermi Large Area Telescope Catalog of Gamma-ray Pulsars

LAT collaboration

This catalog summarizes 117 high-confidence > 0.1 GeV gamma-ray pulsar detections using three years of data acquired by the Large Area Telescope (LAT) on the Fermi satellite. Half…

astro-ph.HE2013★ 69 cited

GMRT discovery of PSR J1544+4937, an eclipsing black-widow pulsar identified with a Fermi LAT source

B. Bhattacharyya, J. Roy, P. S. Ray +17

Using the Giant Metrewave Radio Telescope (GMRT) we performed deep observations to search for radio pulsations in the directions of unidentified Fermi Large Area Telescope (LAT) ga…

astro-ph.HE2012★ 115 cited

Binary Millisecond Pulsar Discovery via Gamma-Ray Pulsations

H. J. Pletsch, L. Guillemot, H. Fehrmann +150

Millisecond pulsars, old neutron stars spun-up by accreting matter from a companion star, can reach high rotation rates of hundreds of revolutions per second. Until now, all such "…