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J/MNRAS/386/1881    New pulsar rotation measures             (Noutsos+, 2008)

New pulsar rotation measures and the Galactic magnetic field. Noutsos A., Johnston S., Kramer M., Karastergiou A. <Mon. Not. R. Astron. Soc., 386, 1881-1896 (2008)> =2008MNRAS.386.1881N
ADC_Keywords: Pulsars ; Magnetic fields Keywords: techniques: polarimetric - pulsars: general - Galaxy: structure - galaxies: magnetic fields Abstract: We measured a sample of 150 pulsar rotation measures (RMs) using the 20-cm receiver of the Parkes 64-m radio telescope. 46 of the pulsars in our sample have not had their RM values previously published, whereas 104 pulsar RMs have been revised. We used a novel quadratic fitting algorithm to obtain an accurate RM from the calibrated polarization profiles recorded across 256MHz of receiver bandwidth. The new data are used in conjunction with previously known dispersion measures and the NE2001 electron-density model to study models of the direction and magnitude of the Galactic magnetic field. Description: We observed a sample of 239 pulsars with the 20-cm H-OH receiver of the Parkes 64-m radio telescope in order to obtain a polarization data base at high time resolution for all these objects. The observing session was carried out from 2006 August 24 to 27. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 83 150 The results from the analysis, including the combined statistical and systematic error
See also: VII/189 : Catalog of Pulsars (Taylor+ 1995) http://www.atnf.csiro.au/research/pulsar/psrcat : ATNF pulsar catalog Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 10 A10 --- PSR Pulsar name (JHHMM+DDMM) 12- 14 I3 --- Num ? Pulsar number in Fig. 2 17- 22 F6.2 deg GLON Galactic longitude 25- 30 F6.2 deg GLAT Galactic latitude 32- 37 F6.2 pc/cm3 DM Column-density integral to the pulsar 39- 43 F5.2 kpc Dist Distance 45- 51 F7.2 rad/m2 RMp ?=- Published rotation measure 52 A1 --- r_RMp Reference for published RM (1) 54- 58 F5.2 rad/m2 e_RMp ?=- rms uncertainty on RMp 61- 66 F6.1 rad/m2 RM New rotation measure 68- 71 F4.1 rad/m2 e_RM rms uncertainty on RM 73- 77 F5.2 10-10T Bpar Parallel component of the magnetic field (uG) 79 A1 --- leBpar Limit flag on e_Bpar 80- 83 F4.2 10-10T e_Bpar rms uncertainty on Bpar
Note (1): References as follows: a = Hamilton & Lyne (1987MNRAS.224.1073H) b = Han et al. (2006, Cat. <J/ApJ/642/868) c = Han et al. (1999MNRAS.306..371H) d = Qiao et al. (1995MNRAS.274..572Q) e = Manchester (1974ApJ...188..637M) f = Johnston et al. (2005MNRAS.364.1397J) g = van Ommen et al. (1997MNRAS.287..307V) h = Hamilton et al. (1977Natur.265..224H) i = Taylor, Manchester & Lyne (1993ApJS...88..529T, Cat. VII/156) j = Costa et al. (1991MNRAS.252...13C) k = Rand & Lyne (1994MNRAS.268..497R)
History: From electronic version of the journal
(End) Patricia Vannier [CDS] 15-Jun-2009
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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