activity
19962026
most citedShapiro delay measurement of a two solar mass neutron star

3.9k citations · 48.4k across the 396 of their papers we have counts for

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Showing 2009Show all

9 papers · 1 filter

astro-ph.GA2009★ 264 cited

The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge

F. R. Ferraro, E. Dalessandro, A. Mucciarelli +9

Globular star clusters are compact and massive stellar systems old enough to have witnessed the entire history of our Galaxy, the Milky Way. Although recent results suggest that th…

astro-ph.SR2009★ 65 cited

Gamma-ray and Radio Properties of Six Pulsars Detected by the Fermi Large Area Telescope

The Fermi LAT collaboration, the Fermi Pulsar Timing Consortium

We report the detection of pulsed gamma-rays for PSRs J0631+1036, J0659+1414, J0742-2822, J1420-6048, J1509-5850 and J1718-3825 using the Large Area Telescope (LAT) on board the Fe…

astro-ph.HE2009★ 463 cited

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

A. A. Abdo

The dramatic increase in the number of known gamma-ray pulsars since the launch of the Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a popu…

astro-ph.GA2009★ 144 cited

Radio detection of LAT PSRs J1741-2054 and J2032+4127: no longer just gamma-ray pulsars

F. Camilo, P. S. Ray, S. M. Ransom +24

Sixteen pulsars have been discovered so far in blind searches of photons collected with the Large Area Telescope on the Fermi Gamma-ray Space Telescope. We here report the discover…

astro-ph.GA2009★ 23 cited

Out of the frying pan: a young pulsar with a long radio trail emerging from SNR G315.9-0.0

F. Camilo, C. -Y. Ng, B. M. Gaensler +4

The faint radio supernova remnant SNR G315.9-0.0 is notable for a long and thin trail that extends outward perpendicular from the edge of its approximately circular shell. In a sea…

astro-ph.GA2009★ 37 cited

Discovery of the energetic pulsar J1747-2809 in the supernova remnant G0.9+0.1

F. Camilo, S. M. Ransom, B. M. Gaensler +1

The supernova remnant G0.9+0.1 has long been inferred to contain a central energetic pulsar. In observations with the NRAO Green Bank Telescope at 2 GHz, we have detected radio pul…