output
19922026
most citedThe Sloan Digital Sky Survey: Technical Summary

10.4k citations

Showing 2010 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA2010★ 11 cited

Radio and Gamma-Ray Constraints on the Emission Geometry and Birthplace of PSR J2043+2740

A. Noutsos, A. A. Abdo, M. Ackermann +146

We report on the first year of Fermi gamma-ray observations of pulsed high-energy emission from the old PSR J2043+2740. The study of the gamma-ray efficiency of such old pulsars gi…

astro-ph.GA2010★ 35 cited

Black Holes in Bulgeless Galaxies: An XMM-Newton Investigation of NGC 3367 and NGC 4536

W. McAlpine, S. Satyapal, M. Gliozzi +3

The vast majority of optically identified active galactic nuclei (AGNs) in the local Universe reside in host galaxies with prominent bulges, supporting the hypothesis that black ho…

astro-ph.GA2010★ 17 cited

Radio Recombination Lines at Decametre Wavelengths: Prospects for the Future

W. M. Peters, T. Joseph W. Lazio, T. E. Clarke +2

This paper considers the suitability of a number of emerging and future instruments for the study of radio recombination lines (RRLs) at frequencies below 200 MHz. These lines aris…

astro-ph.GA2010★ 338 cited

Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT

LAT Collaboration

Pulsars are rapidly-rotating, highly-magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until r…

astro-ph.GA2010★ 53 cited

A survey of the Galactic center region in HCO+, H13CO+ and SiO

D. Riquelme, L. Bronfman, R. Mauersberger +2

Aims: A large scale survey of the Galactic center region in he 3 mm rotational transitions of SiO, HCO+ and H13CO+ (beamsize ~ 3. 6 arcmin) was conducted to provide an estimate of…

astro-ph.GA2010★ 162 cited

A population of gamma-ray emitting globular clusters seen with the Fermi Large Area Telescope

The Fermi LAT collaboration

Globular clusters with their large populations of millisecond pulsars (MSPs) are believed to be potential emitters of high-energy gamma-ray emission. Our goal is to constrain the m…