Milliarcsecond-accurate astrometry of 34 southern hemisphere radio sources

被引:7
|
作者
Fey, Alan L.
Ojha, Roopesh
Quick, Jonathan F. H.
Nicolson, George D.
Lovell, James E. J.
Reynolds, John E.
Ellingsen, Simon P.
McCulloch, Peter M.
Johnston, Kenneth J.
Jauncey, David L.
Tzioumis, Anastasios K.
机构
[1] USN Observ, Washington, DC 20392 USA
[2] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[3] Hartebeesthoek Radio Astron Observ, ZA-1740 Krugersdorp, South Africa
[4] Univ Tasmania, Sch Math & Phys, Hobart, Tas 7001, Australia
[5] USN Observ, Washington, DC 20392 USA
来源
ASTRONOMICAL JOURNAL | 2006年 / 132卷 / 05期
关键词
astrometry; catalogs; quasars : general; radio continuum : galaxies; reference systems; techniques : interferometric;
D O I
10.1086/507991
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Milliarcsecond-accurate radio positions in the International Celestial Reference Frame for 34 southern hemisphere extragalactic sources are reported. The positions are derived from Mark III/IV very long baseline interferometry observations made between 2004 August and 2006 April using radio telescopes located in Australia, South Africa, and Hawaii. Positions for 7 of the 34 sources have been reported previously by us but are reported here with significantly improved accuracy. These results supplement an ongoing project to increase the sky density of southern hemisphere sources in order to better define the International Celestial Reference Frame and to provide additional phase reference sources with accurate positions for use in astrophysical observations. Positions for all 34 sources are south of delta = -20 degrees (positions for nine of the sources are south of delta = -60 degrees) and have average formal uncertainties of 0.23 mas in alpha cos delta and 0.35 mas in delta.
引用
收藏
页码:1944 / 1949
页数:6
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