activity
19962026
most citedThe Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

2.3k citations · 12.3k across the 177 of their papers we have counts for

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8 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★ 49 cited

Detection of a Compact X-ray Source in the Supernova Remnant G29.6+0.1: A Variable Anomalous X-ray Pulsar?

G. Vasisht, E. V. Gotthelf, K. Torii +1

We present follow-up observations of the serendipitously discovered 7-s X-ray pulsar AX J1845-0258, which displays characteristics similar to those observed in the anomalous X-ray…

astro-ph2000★ 131 cited

A 700 year-old Pulsar in the Supernova Remnant Kes 75

E. V. Gotthelf, G. Vasisht, M. Boylan-Kolchin +1

Since their discovery 30 years ago, pulsars have been understood to be neutron stars (NSs) born rotating rapidly (~ 10-100 ms). These neutron stars are thought to be created in sup…

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★ 56 cited

A Possible X-ray and Radio Counterpart of the High-Energy Gamma-ray Source 3EG J2227+6122

J. P. Halpern, E. V. Gotthelf, K. M. Leighly +1

The identity of the persistent EGRET sources in the Galactic plane is largely a mystery. For one of these, 3EG J2227+6122, our complete census of X-ray and radio sources in its err…

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…