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20022009
most citedTEMPO2, a new pulsar timing package. I: Overview

1.2k citations

Showing 2006Show all

70 papers · 1 filter

astro-ph200637 cited

Longitude-resolved imaging of Jupiter at lambda = 2 cm

R. J. Sault, C. Engel, Imke de Pater

We present a technique for creating a longitude-resolved image of Jupiter's thermal radio emission. The technique has been applied to VLA data taken on 25 January 1996 at a wavelen…

astro-ph200617 cited

Radio Observations of the Hubble Deep Field South Region III: The 2.5, 5.2 and 8.7 GHz Catalogues and Radio Source Properties

Minh T. Huynh, Carole A. Jackson, Ray P. Norris

Deep radio observations of a wide region centred on the Hubble Deep Field South have been performed, providing one of the most sensitive set of radio observations acquired on the A…

astro-ph2006189 cited

H.E.S.S. observations of the supernova remnant RX J0852.0-4622: shell-type morphology and spectrum of a widely extended VHE gamma-ray source

HESS Collaboration, F. A. Aharonian

The shell-type supernova remnant RX J0852.0-4622 was observed with the High Energy Stereoscopic System (H.E.S.S.) of Atmospheric Cherenkov Telescopes between December 2004 and May…

astro-ph2006235 cited

The 2dF-SDSS LRG and QSO Survey: QSO clustering and the L-z degeneracy

J. da Angela, T. Shanks, S. M. Croom +12

We combine the QSO samples from the 2dF QSO Redshift Survey (2QZ) and the 2dF-SDSS LRG and QSO Survey (2SLAQ) in order to investigate the clustering of z~1.4 QSOs and measure the c…

astro-ph200660 cited

Field Deployment of Prototype Antenna Tiles for the Mileura Widefield Array--Low Frequency Demonstrator

Judd D. Bowman, David G. Barnes, Frank H. Briggs +22

Experiments were performed with prototype antenna tiles for the Mileura Widefield Array--Low Frequency Demonstrator (MWA-LFD) to better understand the widefield, wideband propertie…

astro-ph200631 cited

Non-thermal radio emission from O-type stars. II. HD 167971

R. Blomme, M. De Becker, M. C. Runacres +2

HD 167971 is a triple system consisting of a 3.3-day eclipsing binary (O5-8 V + O5-8 V) and an O8 supergiant. It is also a well known non-thermal radio emitter. We observed the rad…