2002A&A...385..733V


Query : 2002A&A...385..733V

2002A&A...385..733V - Astronomy and Astrophysics, volume 385, 733-742 (2002/4-2)

PuMa, a digital Pulsar Machine.

VOUTE J.L.L., KOUWENHOVEN M.L.A., VAN HAREN P.C., LANGERAK J.J., STAPPERS B.W., DRIESENS D., RAMACHANDRAN R. and BEIJAARD T.D.

Abstract (from CDS):

We have designed and constructed PuMa, a pulsar machine that has both a baseband recording and a digital filterbank mode. Its design is based on the use of digital signal processors (DSPs). Their operation is controlled by software, which makes PuMa reconfigurable, flexible and easy to operate. The maximum number of channels in the digital filterbank mode is 32768 over a bandwidth of 80MHz. This makes PuMa suitable for pulsar observations at low sky frequencies. The maximum bandwidth in baseband recording mode is two times 10MHz. The machine was installed at the Westerbork Synthesis Radio Telescope in The Netherlands in 1998. We discuss in some detail PuMa's technical properties and capabilities. Recent observations, a sample of which are presented here, demonstrate its capabilities and that it is performing up to its specifications.

Abstract Copyright:

Journal keyword(s): instrumentation: detectors - instrumentation: miscellaneous - pulsars: general

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2023
#notes
1 PSR B0329+54 Psr 03 32 59.3370698592 +54 34 45.028206408           ~ 622 1
2 M 1 SNR 05 34 30.9 +22 00 53           ~ 6056 1
3 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5136 0
4 PSR B1937+21 Psr 19 39 39.6 +21 37 22           ~ 1038 2

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2023.06.04-09:42:51

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