We report on a recent 90 cm wide-field VLBI survey of two 3.1 deg^2 fields using the VLBA, Westerbork and Jodrell Bank telescopes. In-beam calibration was used to calibrate each field, the process was simplified by imaging the calibrators in DIFMAP and transferring the calibration solutions to AIPS using the newly developed DIFMAP task - cordump. We detected and imaged 13 out of the 141 sources originally detected by the low resolution (54") WENSS survey of the same two fields. The sources were detected at 7-12 sigma levels above the image noise, had total flux densities ranging between 85-1640 mJy and were between 16'-58' from the phase centre of each field. This is the first systematic (and non-biased), deep, high resolution survey of the...
29 pages, 27 figures, accepted for publication in MNRASWe present the first wide area (19 deg$^2$), ...
Received... Context. Wide-field surveys are a commonly-used method for studying thousands of objects...
Two large VLBI surveys are currently underway which utilise the snapshot technique pioneered on the ...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
The past decade has seen significant advances in wide-field cm-wave very long baseline interferometr...
We present the first wide area (19 deg(2)), deep (a parts per thousand 120-150 mu Jy beam(-1)), high...
Very Long Baseline Interferometry (VLBI) has significant advantages in disentangling active galactic...
We present the first results from the first Caltech-Jodrell Bank VLBI survey (the CJ1 survey). The C...
We report λ-18 cm VLBI observations made in 1991 September of a further 25 objects from the first Ca...
We present the first wide area (19 deg2), deep (≈120-150 μJy beam-1), high-resolution (5.6 × 7.4 arc...
Context. Wide-field surveys are a commonly-used method for studying thousands of objects simultaneou...
We present results from a large global VLBI(Very Long Baseline Interferometry) survey of compact rad...
International audienceWe present the first sub-mJy (≈0.7 mJy beam−1) survey to be completed below 10...
We present the first wide area (19 deg2), deep (≈120-150 μJy beam-1), high-resolution (5.6 × 7.4 arc...
29 pages, 27 figures, accepted for publication in MNRASWe present the first wide area (19 deg$^2$), ...
Received... Context. Wide-field surveys are a commonly-used method for studying thousands of objects...
Two large VLBI surveys are currently underway which utilise the snapshot technique pioneered on the ...
We report on the first wide-field, very long baseline interferometry (VLBI) survey at 90 cm. The sur...
The past decade has seen significant advances in wide-field cm-wave very long baseline interferometr...
We present the first wide area (19 deg(2)), deep (a parts per thousand 120-150 mu Jy beam(-1)), high...
Very Long Baseline Interferometry (VLBI) has significant advantages in disentangling active galactic...
We present the first results from the first Caltech-Jodrell Bank VLBI survey (the CJ1 survey). The C...
We report λ-18 cm VLBI observations made in 1991 September of a further 25 objects from the first Ca...
We present the first wide area (19 deg2), deep (≈120-150 μJy beam-1), high-resolution (5.6 × 7.4 arc...
Context. Wide-field surveys are a commonly-used method for studying thousands of objects simultaneou...
We present results from a large global VLBI(Very Long Baseline Interferometry) survey of compact rad...
International audienceWe present the first sub-mJy (≈0.7 mJy beam−1) survey to be completed below 10...
We present the first wide area (19 deg2), deep (≈120-150 μJy beam-1), high-resolution (5.6 × 7.4 arc...
29 pages, 27 figures, accepted for publication in MNRASWe present the first wide area (19 deg$^2$), ...
Received... Context. Wide-field surveys are a commonly-used method for studying thousands of objects...
Two large VLBI surveys are currently underway which utilise the snapshot technique pioneered on the ...