Ma, "The VLBA Calibrator Survey-VCS1," Astrophys. J., Supp., vol. 141, p.13-21, 2002. http://www.iop.org/EJ/abstract/0067-0049/141/1/13/A.J. Beasley, D. Gordon, A.B. Peck, L. Petrov, D.S. MacMillan, E.B. Fomalont, and C. Ma, The VLBA Calibrator Survey - VCS1, ...
Three sources are clearly detected (>7 σ) within the inner 2 arcmin of the GBT primary beam, including two sub-mJy sources and the 'in-beam' calibrator. In addition, by tapering the data, we map out a much larger area of sky, reaching well beyond the half-power point of the GBT ...
The Third VLBA Calibrator Survey: VCS3 We present the third extension to the Very Long Baseline Array (VLBI) Calibrator Survey, containing 360 new sources not previously observed with very long ... L Petrov,YY Kovalev,E Fomalont,... - 《Astronomical Journal》...
This paper presents the third extension to the Very Large Baseline Array\n(VLBA) Calibrator Survey, containing 360 new sources not previously observed\nwith very long baseline interferometry (VLBI). The survey, based on three 24\nhour VLBA observing sessions, fills the areas on the sky above ...
Gordon, "The Fifth VLBA Calibrator Survey - VCS5," AJ, vol. 133, pp. 1236-1242, April 2007. http://www.iop.org/EJ/abstract/1538-3881/133/4/1236/Kovalev, Y.Y., L. Petrov, E.B. Fomalont, D. Gordon, The Fifth VLBA Calibrator Survey - VCS5, AJ, 133, 1236-1242, 2007....
ICRFVLBISix campaigns with a total of twenty-four Very Long Baseline Array Calibrator Survey (VCS) observing sessions were carried out with ten radio telescopes located on U.S. territory from 1994 to 2007. The aim of those astrometric sessions was to estimate source positions and to make snap...
VLBA+GBT 1.4 GHz observations of a region within NOAO-N, reach an r.m.s. noise level of 9 microJy per beam. Three sources are clearly detected (>7 蟽) within the inner 2 arcmin of the GBT primary beam, including two sub-mJy sources and the 'in-beam' calibrator. In addition, by...
[International Association of Geodesy Symposia] || Analysis Strategies for the Densification of the ICRF with VLBA Calibrator Survey Sourcesdoi:10.1007/1345_2016_244KrásnáHana
We have identified 9 new CSOs from radio continuum observations for the VLBA Calibrator Survey, increasing the number of known CSOs by almost 50%.doi:10.1016/S1387-6473(01)00197-XA.B. PeckG.B. TaylorElsevier B.V.New Astronomy Reviews...