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19992026
most citedA sample of low-redshift BL Lacertae objects. II. EVN and MERLIN data and multi-wavelength analysis

70 citations · 306 across the 23 of their papers we have counts for

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astro-ph2008★ 63 cited

Giant cavities, cooling and metallicity substructure in Abell 2204

J. S. Sanders, A. C. Fabian, G. B. Taylor

We present results from deep Chandra and XMM-Newton observations of the relaxed X-ray luminous galaxy cluster Abell 2204. We detect metallicity inhomogeneities in the intracluster…

astro-ph2008★ 19 cited

Spatial and Temporal Variations in Interstellar Absorption toward HD 72127AB

Daniel E. Welty, Thuso Simon, L. M. Hobbs

New optical spectra of Ca II and Na I toward HD 72127AB provide additional evidence for both spatial and temporal variations in the complex interstellar absorption along the two si…

astro-ph2006★ 70 cited

A sample of low-redshift BL Lacertae objects. II. EVN and MERLIN data and multi-wavelength analysis

M. Giroletti, G. Giovannini, G. B. Taylor +1

We present new radio observations of 9 members of a sample of 29 nearby (z < 0.2) BL Lac objects. The new data have been obtained with the European VLBI Network and/or the MERLIN a…

astro-ph2004★ 42 cited

The HI Parkes Zone of Avoidance Survey: the Northern Extension

J. L. Donley, L. Staveley-Smith, R. C. Kraan-Korteweg +6

We present the results of the northern extension of the HI Parkes Zone of Avoidance Survey, a blind HI survey utilizing the multibeam receiver on the Parkes 64-m telescope. In the…

astro-ph2003

Pierre Auger Atmosphere-Monitoring Lidar System

A. Filipcic, M. Horvat, D. Veberic +7

The fluorescence-detection techniques of cosmic-ray air-shower experiments require precise knowledge of atmospheric properties to reconstruct air-shower energies. Up to now, the at…

astro-ph2001

HI deficiency in the galaxy cluster ACO 3627. ATCA observations in the Great Attractor region

B. Vollmer, V. Cayatte, W. van Driel +5

ATCA 21 cm HI observations of the rich galaxy cluster ACO 3627 in the Great Attractor region are presented. Three fields of 30' diameter located within one Abell radius of ACO 3627…