BB202

Trignometric Parallax of a Radio Star in the Pleiades

Abstract

Investigators
Name Other * Institution Email Phone
Geoff Bower PI UC Berkeley gbower@astro.berkeley.edu 510 642-4075
Jay Anderson Rice University jay@eeyore.rice.edu
* PI = Principal Investigator; CO = Contact author; T = Thesis observations; S = Student

Front Ends
Gregorian X(8.2 to 10.0 GHz)

Back Ends
VLBA recorder and DAR

Type of Observing
Monitor Very Long Baseline Interferometry

Switching Type

Processor (correlator)
Socorro

Allotted time 32.00 hours

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Updated 09/19/2007