D. Anish Roshi, Marty Bloss, Patrick Brandt, Srikanth Bussa, Hong Chen, Paul Demorest, Gregory Desvignes, Terry Filiba, Richard J. Fisher, John Ford, David Frayer, Robert Garwood, Suraj Gowda, Glenn Jones, Billy Mallard, Joseph Masters, Randy McCullough, Guifre Molera, Karen O'Neil, Jason Ray, Simon Scott, Amy Shelton, Andrew Siemion, Mark Wagner, Galen Watts, Dan Werthimer, Mark Whitehead
A new spectrometer for the Green Bank Telescope (GBT) is being built jointly
by the NRAO and the CASPER, University of California, Berkeley. The
spectrometer uses 8 bit ADCs and will be capable of processing up to 1.25 GHz
bandwidth from 8 dual polarized beams. This mode will be used to process data
from focal plane arrays. The spectrometer supports observing mode with 8
tunable digital sub-bands within the 1.25 GHz bandwidth. The spectrometer can
also be configured to process a bandwidth of up to 10 GHz with 64 tunable
sub-bands from a dual polarized beam. The vastly enhanced backend capabilities
will support several new science projects with the GBT.
View original:
http://arxiv.org/abs/1202.0938
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