1 citations · 3 across the 11 of their papers we have counts for
17 papers
Discovering the microJy Radio VLBI Sky via "Full-beam" Self-calibration
M. A. Garrett, J. M. Wrobel, R. Morganti
We demonstrate that at 1.4 GHz the combined response of sources detected serendipitously in deep, wide-field VLBI images is sufficient to permit self-calibration techniques to be e…
Spitzer 24 micron imaging of Faint Radio Sources in the FLSv: a new radio-loud, Mid-IR/optically obscured population?
M. Orienti, M. A. Garrett, C. Reynolds +1
Data from the Spitzer Space Telescope (the First Look Survey - FLS) have recently been made public. We have compared the 24 micron images with very deep WSRT 1.4 GHz observations (…
High output data rates with PCInt on the EVN MkIV data processor
H. J. van Langevelde, H. Verkouter, S. Parsley +3
The EVN MkIV data processor is being equipped with a high data output capability, called PCInt. In its next phase it will allow very high data output rates, up to 160 Mb/s. This fu…
The nature of the Mid-IR faint radio sources from the Spitzer First Look Survey
M. Orienti, M. A. Garrett, C. Reynolds +1
Data from the Spitzer Space Telescope (the First Look Survey - FLS) have recently been made public. We have compared the 24 micron images with very deep WSRT 1.4 GHz observations,…
e-VLBI... a Wide-field Imaging Instrument with milliarcsecond Resolution & microJy Sensitivity
M. A. Garrett
The European VLBI Network (EVN) is in the process of establishing an e-VLBI array in which the radio telescopes and the EVN correlator at JIVE are connected in real-time, via high-…
21st Century VLBI: Deep Wide-Field Surveys
M. A. Garrett, J. M. Wrobel, R. Morganti
A 20-hour VLBI observation with the NRAO VLBA and GBT in the NOAO Bootes field reaches an rms noise of 9 microJy per beam at 1.4 GHz. Three sources were detected at 10-milliarcseco…