Table 3
Radio sources used for the OOF holography imaging and calibration of the data.
| Name | RA | Dec | S34 GHz | Q |
|---|---|---|---|---|
| 3C286 | l3h31m08.3s | +30°30′03.0″ | 1.72 Jy | С |
| NGC7027 | 21h07m01.6s | +42° 14′10.0″ | 5.25 Jy | С |
| 3C84 | 03h19m48.2s | +41°30′42.1″ | 2l.80Jy | T |
| 3C273 | 12h29m06.7s | +02°03′08.6″ | 11.50Jy | T |
| 3C454.3 | 22h53m57.8s | + 16°08′53.6″ | 11.30Jy | T |
Notes. The flux densities of the target sources are typical flux densities from 2020. Given are the source name, right ascension, and declination coordinates in J2000 (RA/Dec), flux density (Sv) at 34GHz (S34 GHz), and a qualifier (Q) for target (T) and calibrator (C). Sources are variable AGN, but are usually bright and the long-term variability does not affect the OOF holography observations.
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