activity
19992013
most citedAn expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20

191 citations · 801 across the 10 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2013★ 27 cited

VLBI observations of the shortest orbital period black hole binary, MAXI J1659-152

Z. Paragi, A. J. van der Horst, T. Belloni +9

The X-ray transient MAXI J1659-152 was discovered by Swift/BAT and it was initially identified as a GRB. Soon its Galactic origin and binary nature were established. There exists a…

astro-ph2008★ 25 cited

SN 2001em: Not so Fast

F. K. Schinzel, G. B. Taylor, C. J. Stockdale +2

SN 2001em is a peculiar supernova, originally classified as Type Ib/c. About two years after the SN it was detected in the radio, showing a rising radio flux with an optically thin…

astro-ph2005★ 15 cited

Structure in the radio counterpart to the 2004 Dec 27 giant flare from SGR 1806-20

R. P. Fender, T. W. B. Muxlow, M. A. Garrett +7

On Dec 27, 2004, the magnetar SGR 1806-20 underwent an enormous outburst resulting in the formation of an expanding, moving, and fading radio source. We report observations of this…

astro-ph2005★ 73 cited

A Re-brightening of the Radio Nebula associated with the 2004 December 27 giant flare from SGR 1806--20

J. D. Gelfand, Y. E. Lyubarsky, D. Eichler +7

The 2004 Dec. 27 giant Gamma-ray flare detected from the magnetar SGR 1806-20 created an expanding radio nebula which we have monitored with the Australia Telescope Compact Array a…

astro-ph2005★ 98 cited

Diagnosing the outflow from the SGR 1806-20 Giant Flare with Radio Observations

J. Granot, E. Ramirez-Ruiz, G. B. Taylor +6

On 2004 Dec. 27, the soft gamma repeater (SGR) 1806-20 emitted the brightest giant flare (GF) ever detected from an SGR, with an (isotropic) energy release times greater…

astro-ph2005★ 191 cited

An expanding radio nebula produced by a giant flare from the magnetar SGR 1806-20

B. M. Gaensler, C. Kouveliotou, J. D. Gelfand +16

Soft gamma repeaters (SGRs) are "magnetars", a small class of slowly spinning neutron stars with extreme surface magnetic fields, ~10^15 gauss. On 2004 December 27, a giant flare w…