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PuMa, the new Dutch PulsarMachine

Published online by Cambridge University Press:  12 April 2016

M.L.A. Kouwenhoven ,
P.C. van Haren ,
D. Driesens ,
J.J. Langerak ,
T.D. Beijaard ,
J.L.L. Voûte ,
B.W. Stappers  and
R. Ramachandran
M.L.A. Kouwenhoven
Affiliation:
Sterrenkundig Instituut, Utrecht University, Postbox 80000, 3508 TA Utrecht, The Netherlands
P.C. van Haren
Affiliation:
Instrumentele Groep Fysica, Utrecht University, Postbox 80000, 3508 TA Utrecht, The Netherlands
D. Driesens
Affiliation:
Instrumentele Groep Fysica, Utrecht University, Postbox 80000, 3508 TA Utrecht, The Netherlands
J.J. Langerak
Affiliation:
Instrumentele Groep Fysica, Utrecht University, Postbox 80000, 3508 TA Utrecht, The Netherlands
T.D. Beijaard
Affiliation:
Instrumentele Groep Fysica, Utrecht University, Postbox 80000, 3508 TA Utrecht, The Netherlands
J.L.L. Voûte
Affiliation:
Anton Pannekoek Instituut, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
B.W. Stappers
Affiliation:
Anton Pannekoek Instituut, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
R. Ramachandran
Affiliation:
Anton Pannekoek Instituut, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands

Abstract

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PuMa is a fully digital PulsarMachine the operation at the Westerbork Synthesis Radio Telescope (WSRT). Its design is based on the use of Digital Signal Processors. It has two modes of operation: a baseband recording mode and a digital filterbank mode.

Type
Part 3. Studies of Radio Emission
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 279 - 280
Copyright
Copyright © Astronomical Society of the Pacific 2000