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Proposal Identification No.: P1924 Date Received: 2004­Feb­02 15:30:11
Technical Page
Proposal Type: Regular
General Category: Pulsars
Observation Category:
Total Time Requested: 55 Hours
Proposal Title: Polarisation Calibration for the Arecibo Signal Processor
ABSTRACT:
We propose an extension of the high quality, full Stokes Parameter calibration procedures developed by Heiles and
others for spectroscopy to a new backend based on realtime voltage processing in a PC array. Our initial scientific
goals are improved precision timing of pulsars and new pulsar studies aimed at deeper understanding of the
emission mechanism, although a number of other scientific projects will also greatly benifit from our backend. The
PC array backend will provide a general purpose platform for new approaches in signal processing for many
astronomical and atmospheric goals. We propose to have 55 hours of Arecibo observing time for this.
Name Institution E­mail Phone Student
Rajagopalan Ramachandran UC Berkeley ramach@astron.berkeley.edu 510­642­2529 no
Service Observing Request Remot e Observing Request
X None No
All of the observing run. X Maybe
Part of the observing run. Yes
Queue Observing
Instrument Setup
L­wide S­low 327
Atmospheric Observation Instruments:
Special Equipment or setup: none
RFI Considerations
Frequency Ranges Planned
1