Accurate astrometry of 22 southern hemisphere radio sources

被引:15
作者
Fey, AL
Ojha, R
Jauncey, DL
Johnston, KJ
Reynolds, JE
Lovell, JEJ
Tzioumis, AK
Quick, JFH
Nicolson, GD
Ellingsen, SP
McCulloch, PM
Koyama, Y
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] Kashima Space Res Ctr, Commun Res Lab, Kashima, Ibaraki 3148501, Japan
关键词
astrometry; catalogs; quasars : general; radio continuum : galaxies; reference systems; techniques : interferometric;
D O I
10.1086/381957
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Milliarcsecond-accurate radio positions for 22 southern hemisphere extragalactic sources are reported. These positions are derived from Mark III very long baseline interferometry observations made between 2003 February and 2003 August. The results presented here 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. The positions for all 22 sources are south of delta = - 30degrees (positions for 10 of the sources are south of delta = - 60degrees) and represent the largest group of new milliarcsecond-accurate astrometric positions for sources in this declination range since the initial definition of the International Celestial Reference Frame. The reported positions have average formal uncertainties of 0.5 mas in right ascension and 0.6 mas in declination.
引用
收藏
页码:1791 / 1795
页数:5
相关论文
共 21 条
[1]  
ARIAS EF, 1995, ASTRON ASTROPHYS, V303, P604
[2]   Emission line AGNs from the REX survey - Results from optical spectroscopy [J].
Caccianiga, A ;
Maccacaro, T ;
Wolter, A ;
Della Ceca, R ;
Gioia, IM .
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, 2000, 144 (02) :247-269
[3]  
CANNON WH, 1997, VISTAS ASTRON, V41, P297
[4]  
CAPRETTE DS, 1990, 100765 NASA GSFC
[5]   PRECISION GEODESY USING THE MARK-III VERY-LONG-BASELINE INTERFEROMETER SYSTEM [J].
CLARK, TA ;
COREY, BE ;
DAVIS, JL ;
ELGERED, G ;
HERRING, TA ;
HINTEREGGER, HF ;
KNIGHT, CA ;
LEVINE, JI ;
LUNDQVIST, G ;
MA, C ;
NESMAN, EF ;
PHILLIPS, RB ;
ROGERS, AEE ;
RONNANG, BO ;
RYAN, JW ;
SCHUPLER, BR ;
SHAFFER, DB ;
SHAPIRO, II ;
VANDENBERG, NR ;
WEBBER, JC ;
WHITNEY, AR .
IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 1985, 23 (04) :438-449
[6]   The Parkes half-jansky flat-spectrum sample [J].
Drinkwater, MJ ;
Webster, RL ;
Francis, PJ ;
Condon, JJ ;
Ellison, SL ;
Jauncey, DL ;
Lovell, J ;
Peterson, BA ;
Savage, A .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 284 (01) :85-125
[7]  
FEY AL, 2004, UNPUB AJ
[8]   The second VLBA Calibrator Survey: VCS2 [J].
Fomalont, EB ;
Petrov, L ;
MacMillan, DS ;
Gordon, D ;
Ma, C .
ASTRONOMICAL JOURNAL, 2003, 126 (05) :2562-2566
[9]  
KINGHAM KA, 2003, 211619 NASA GSFC, P201
[10]   The Deep X-ray Radio Blazar Survey (DXRBS) - II. New identifications [J].
Landt, H ;
Padovani, P ;
Perlman, ES ;
Giommi, P ;
Bignall, H ;
Tzioumis, A .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2001, 323 (03) :757-784