activity
19962023
most citedTransient pulsed radio emission from a magnetar

449 citations · 8.8k across the 143 of their papers we have counts for

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7 papers · 1 filter

astro-ph2000★ 34 cited

3EG J2016+3657: Confirming an EGRET Blazar Behind the Galactic Plane

J. P. Halpern, M. Eracleous, R. Mukherjee +1

We recently identified the blazar-like radio source G74.87+1.22 (B2013+370) as the counterpart of the high-energy gamma-ray source 3EG J2016+3657 in the Galactic plane. However, si…

astro-ph2000★ 250 cited

Observation of X-ray lines from a Gamma-Ray Burst (GRB991216): Evidence of Moving Ejecta from the Progenitor

L. Piro, G. Garmire, M. Garcia +18

We report on the discovery of two emission features observed in the X-ray spectrum of the afterglow of the gamma-ray burst (GRB) of 16 Dec. 1999 by the Chandra X-Ray Observatory. T…

astro-ph2000★ 304 cited

The Vela Pulsar and its Synchrotron Nebula

D. J. Helfand, E. V. Gotthelf, J. P. Halpern

(Abridged) We present high-resolution Chandra X-ray observations of PSR B0833-45, the 89 ms pulsar associated with the Vela supernova remnant. We have acquired two observations sep…

astro-ph2000

The transient X-ray source SAX J2239.3+6116 and its optical counterpart

J. J. M. in 't Zand, J. Halpern, M. Eracleous +4

We have discovered with the Wide Field Cameras on board BeppoSAX the weak transient X-ray source SAXJ2239.3+6116 whose position coincides with that of 4U2238+60/3A2237+608 and is c…

astro-ph2000★ 82 cited

GRB 991216 Joins the Jet Set: Discovery and Monitoring of its Optical Afterglow

J. P. Halpern, R. Uglesich, N. Mirabal +8

The optical light curve of the energetic gamma-ray burst GRB 991216 is consistent with jet-like behavior in which a power-law decay steepens from t**(-1.22 +/- 0.04) at early times…

astro-ph2000★ 42 cited

Multiwavelength Examination of the COS-B Field 2CG 075+00 Yields a Blazar Identification for 3EG J2016+3657

R. Mukherjee, E. V. Gotthelf, J. Halpern +1

We present a high-energy study of the intriguing COS-B gamma-ray field, 2CG 075+00, in order to search for possible counterparts. New EGRET data show that the COS-B emission probab…