NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Collections About News Help Login
Back to Results
Verification of the PROS timing analysis packageROSAT observations of known pulsars are used to verify the functions of timing programs. The Crab Pulsar and PSR 0540-69, with 33 and 50 millisecond periods, are used to examine the fast Fourier transform and the epoch-folding task used to search for periodic signals. These fast pulsars provide a more vigorous test of the system than those with periods of a few seconds.
Document ID
19940018035
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Manning, K. R. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Conroy, M. A. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Deponte, J. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Moran, J. F. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Primini, F. A. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Seward, F. D. (Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Aschenbach, B. (Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: NASA, Washington, Second Annual Conference on Astronomical Data Analysis Software and Systems. Abstracts
Subject Category
Computer Programming And Software
Accession Number
94N22508
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Related Records

IDRelationTitle19940017808Collected WorksA High Resolution Liquid Xenon Imaging Telescope for 0.3-10 MeV Gamma Ray Astrophysics: Construction and Initial Balloon Flights
No Preview Available