2012MNRAS.424..244D

Query : 2012MNRAS.424..244D

2012MNRAS.424..244D - Mon. Not. R. Astron. Soc., 424, 244-251 (2012/July-3)

Optimal interpolation and prediction in pulsar timing.

DENG X.P., COLES W., HOBBS G., KEITH M.J., MANCHESTER R.N., SHANNON R.M. and ZHENG J.H.

Abstract (from CDS):

For pulsar projects it is often necessary to predict the pulse phase in advance, for example when preparing for new observations. Interpolation of the pulse phase between existing measurements is also often required, for example when folding X-ray or gamma-ray observations according to the radio pulse phase. Until now these procedures have been done using various ad hoc methods. The purpose of this paper is to show how to interpolate or predict the pulse phase optimally using statistical models of the various noise processes and the phase measurement uncertainty.

Abstract Copyright: 2012 The Authors Monthly Notices of the Royal Astronomical Society2012 RAS

Journal keyword(s): methods: data analysis - pulsars: general

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME Vela Pulsar Psr 08 35 20.65525 -45 10 35.1545     15.10     ~ 2446 1
2 PSR J1713+0747 Psr 17 13 49.5367813 +07 47 37.450240           ~ 530 1
3 PSR B1937+21.4 Psr 19 39 38.560096 +21 34 59.13552           ~ 1142 0

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