Wide-field imaging
Arecibo’s Existing VLBI Capability Arecibo’s Existing VLBI Capability DAR - VLBA4 MK5A Max 1-GHz IF The Big Dish (Gain~10k/Jy,SEFD~3-5 Jy) Correlator.
The jet of Mrk 501 from millions of Schwarzschild radii down to a few hundreds
01.pdf
Neutrinos: At the Heart of the Matter?
SKADS Simulations (DS2 team)
SPIDAR: VLF Astronomy on the Moon Jodi Y. Enomoto University of Southern California ASTE 527: Space Exploration Architectures Concept Synthesis Studio.
Copyright, 1996 © Dale Carnegie & Associates, Inc. Tim Cornwell Kumar Golap Sanjay Bhatnagar W projection A new algorithm for wide field imaging with radio.
T he ICRF, ITRF and VLBA
