activity
19982026
most citedA low-magnetic-field Soft Gamma Repeater

320 citations · 4.5k across the 121 of their papers we have counts for

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Showing 2011 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2011

High-Energy Gamma-ray Emission Properties of an Anomalous X-ray Pulsar, 4U 0142+61

Sinem Sasmaz Mus, Ersin Gogus

Anomalous X-ray Pulsars (AXPs) are bright X-ray sources. Few AXPs emit highly pulsed emission in hard X-rays. Using data collected with the Large Area Telescope on board Fermi Gamm…

astro-ph.HE2011★ 45 cited

Burst and Persistent Emission Properties during the Recent Active Episode of the Anomalous X-ray Pulsar 1E 1841-045

Lin Lin, Chryssa Kouveliotou, Ersin Gogus +19

Swift/BAT detected the first burst from 1E 1841-045 in May 2010 with intermittent burst activity recorded through at least July 2011. Here we present Swift and Fermi/GBM observatio…

astro-ph.HE2011★ 19 cited

Extended Tails from SGR 1806-20 Bursts

Ersin Gogus, Peter Woods, Chryssa Kouveliotou +6

In 2004, SGR 1806-20 underwent a period of intense and long-lasting burst activity that included the giant flare of 27 December 2004 -- the most intense extra-solar transient event…

astro-ph.HE2011★ 56 cited

Fermi/GBM Observations of SGR J0501+4516 Bursts

Lin Lin, Chryssa Kouveliotou, Matthew G. Baring +27

We present our temporal and spectral analyses of 29 bursts from SGR J0501+4516, detected with the Gamma-ray Burst Monitor onboard the Fermi Gamma-ray Space Telescope during the 13…

astro-ph.HE2011★ 1 cited

SGR 0418+5729: a low-magnetic-field magnetar

P. Esposito, N. Rea, R. Turolla +8

Soft gamma-ray repeaters and anomalous X-ray pulsars are a small (but growing) group of X-ray sources characterized by the emission of short bursts and by a large variability in th…

astro-ph.HE2011★ 12 cited

Long Term Radiative Behavior of SGR 1900+14

Ersin Gogus, Tolga Guver, Feryal Ozel +2

The prolific magnetar SGR 1900+14 showed two outbursts in the last decade and has been closely monitored in the X-rays to track the changes in its radiative properties. We use arch…