We present the third extension to the Very Long Baseline Array (VLBI) Calibrator Survey, containing 360 new sources not previously observed with very long baseline interferometry (VLBI). The survey, based on three 24 hour VLBA observing sessions, fills the areas on the sky above declination45 where the calibrator density is less than one source within a 4 radius disk at any given direction. The positions were derived from astrometric analysis of the group delays determined at 2.3 and 8.6 GHz frequency bands using the CALC/SOLVE software package. The VCS3 catalog of source positions, plots of correlated flux density versus length of projected baseline, and contour plots and FITS files of naturally weighted CLEAN images, as well as calibrate...
The East Coast very long baseline interferometry (VLBI) group has performed about 60 experiments ove...
International audienceThe space astrometry mission Gaia will construct a dense optical QSO-based cel...
The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catal...
This paper presents the fourth extension to the Very Long Baseline Array (VLBA) Calibrator Survey, c...
Six very successful Very Long Baseline Array (VLBA) calibrator survey campaigns were run between 199...
The original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns from 1994 to 2007 in wh...
he original VLBA Calibrator (VCS) surveys were a set of 24 24-hr VLBA sessions between 1994 and 2007...
A systematic very long baseline interferometry (VLBI) sky survey, undertaken to find a suitable set ...
This paper presents the fifth extension to the Very Long Baseline Array (VLBA) Calibrator Survey (VC...
Six very successful VLBA calibrator survey campaigns were run between 1994 and 2007 to build up a la...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
Very Long Baseline Interferometry (VLBI) is a measurement technique at radio wavelengths, which is u...
For Very Long Baseline Interferometry (VLBI), the fringe spacing is extremely narrow compared to the...
Building celestial reference frames such as the International Celestial Reference Frame (ICRF) from ...
The compact extragalactic radio-emitting objects used to define the International Celestial Referenc...
The East Coast very long baseline interferometry (VLBI) group has performed about 60 experiments ove...
International audienceThe space astrometry mission Gaia will construct a dense optical QSO-based cel...
The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catal...
This paper presents the fourth extension to the Very Long Baseline Array (VLBA) Calibrator Survey, c...
Six very successful Very Long Baseline Array (VLBA) calibrator survey campaigns were run between 199...
The original VLBA Calibrator Surveys (VCS) were a series of 6 VLBA campaigns from 1994 to 2007 in wh...
he original VLBA Calibrator (VCS) surveys were a set of 24 24-hr VLBA sessions between 1994 and 2007...
A systematic very long baseline interferometry (VLBI) sky survey, undertaken to find a suitable set ...
This paper presents the fifth extension to the Very Long Baseline Array (VLBA) Calibrator Survey (VC...
Six very successful VLBA calibrator survey campaigns were run between 1994 and 2007 to build up a la...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
Very Long Baseline Interferometry (VLBI) is a measurement technique at radio wavelengths, which is u...
For Very Long Baseline Interferometry (VLBI), the fringe spacing is extremely narrow compared to the...
Building celestial reference frames such as the International Celestial Reference Frame (ICRF) from ...
The compact extragalactic radio-emitting objects used to define the International Celestial Referenc...
The East Coast very long baseline interferometry (VLBI) group has performed about 60 experiments ove...
International audienceThe space astrometry mission Gaia will construct a dense optical QSO-based cel...
The point source list of the Wilkinson Microwave Anisotropy Probe (WMAP) is a uniform, all-sky catal...