J/MNRAS/335/275 Parkes Multi-Beam Pulsar Survey new PSR (Morris+, 2002)
The Parkes Multi-Beam Pulsar Survey - II. Discovery and timing of 120 pulsars. Morris D.J., Hobbs G., Lyne A.G., Stairs I.H., Camilo F., Manchester R.N., Possenti A., Bell J.F., Kaspi V.M., D'Amico N., McKay N.P.F., Crawford F., Kramer M. <Mon. Not. R. Astron. Soc. 335, 275 (2002)> =2002MNRAS.335..275M
ADC_Keywords: Pulsars ; Radio sources Keywords: methods: observational - pulsars: general - pulsar: individual: PSR J1734-3333, PSR J1830-1135 Abstract: The Parkes Multibeam Pulsar Survey is a sensitive survey of a strip of the Galactic plane with |b|<5° and 260°<l<50° at 1374MHz. Here we report the discovery of 120 new pulsars and subsequent timing observations, primarily using the 76-m Lovell radio telescope at Jodrell Bank. The main features of the sample of 370 published pulsars discovered during the multibeam survey are described. Furthermore, we highlight two pulsars: PSR J1734-3333, a young pulsar with the second highest surface magnetic field strength among the known radio pulsars, BS=5.4x1013G, and PSR J1830-1135, he second slowest radio pulsar known, with a 6-s period. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1.dat 96 120 Positions, flux densities and pulse widths for 120 higher declination pulsars discovered in the Parkes Multibeam Pulsar Survey. table2.dat 99 120 Rotational parameters and dispersion measures for 120 pulsars discovered in the Parkes Multibeam Pulsar Survey.
See also: J/MNRAS/328/17 : Parkes Multi-Beam Pulsar Survey. I. (Manchester+, 2001) J/MNRAS/342/1299 : Parkes Multi-Beam Pulsar Survey. III. (Kramer+, 2003) J/MNRAS/352/1439 : Parkes Multi-Beam Pulsar Survey. IV. (Hobbs+, 2004) J/MNRAS/372/777 : Parkes Multibeam Pulsar Survey. VI. (Lorimer+, 2006) Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 10 A10 --- PSRJ PSR J designation (1) 11- 12 A2 --- n_PSRJ [AP ] Note on PSRJ (2) 14- 15 I2 h RAh Right ascension (J2000.0) 17- 18 I2 min RAm Right ascension (J2000.0) 20- 25 F6.3 s RAs Right ascension (J2000.0) 27- 30 F4.3 s e_RAs rms uncertainty on right ascension 32 A1 --- DE- Declination sign (J2000.0) 33- 34 I2 deg DEd Declination (J2000.0) 36- 37 I2 arcmin DEm Declination (J2000.0) 39- 43 F5.2 arcsec DEs ? Declination (J2000.0) 45- 50 F6.2 arcsec e_DEs rms uncertainty on declination 52- 57 F6.2 deg GLON Galactic longitude 59- 63 F5.2 deg GLAT Galactic latitude 65- 66 I2 --- Beam [1/13] Beam number of the multi-beam receiver 68- 71 F4.2 --- Dist Radial distance in units of beam radii 73- 77 F5.1 --- S/N Signal-to-noise ratio of the pulse profile in the discovery observation 79- 82 F4.2 mJy S1400MHz Median flux density at 1400MHz averaged over all the observations included in the timing solution 84- 86 F3.2 mJy e_S1400MHz rms uncertainty on S1400MHz 88- 92 F5.1 ms W50 Pulse widths at 50% of the mean pulse profile 94- 96 I3 ms W10 ? Pulse widths at 10% of the mean pulse profile for pulsars with high S/N
Note (1): PSRs J1841-0348, J1842-0415 and J1844-0310 were discovered independently by Lorimer et al. (2000A&A...358..169L). Note (2): Note on PPSRJ as follows: A = pulsars that have been timed at Arecibo P = pulsars timed using the Parkes telescope All other pulsars were timed using the Lovell telescope at Jodrell Bank.
Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1- 10 A10 --- PSRJ PSR J designation 11 A1 --- f_PSRJ [* ] Note on PSRJ (1) 13- 28 F16.14 s Per Solar-system barycentric pulse period 30- 35 E6.2 s e_Per rms uncertainty on Per 37- 47 F11.6 10-15 dP/dt Period derivative 49- 53 E5.2 10-15 e_dP/dt rms uncertainty on dP/dt 56- 62 F7.1 d Epoch MJD epoch of which the period refers to 64- 67 I4 --- NTOA Number of times-of-arrival used in the timing solution 70- 74 I5 d DataSpan1 MJD range covered by the timing observations 75 A1 --- --- [-] 76- 80 I5 d DataSpan2 MJD range covered by the timing observations 82- 86 F5.1 ms RMS rms value for the timing residual 88- 93 F6.1 pc/cm3 DM Pulsar's dispersion measure 95- 98 F4.1 pc/cm3 e_DM rms uncertainty on DM
Note (1): Asterisks indicate those pulsars the timing residuals of which contain significant timing noise that has been removed, to first order, by the fitting of a period double derivative.
History: From electronic version of the journal References Manchester et al., Paper I 2001MNRAS.328...17M, Cat. J/MNRAS/328/17 Kramer et al., Paper III 2003MNRAS.342.1299K, Cat. J/MNRAS/342/1299 Hobbs et al., Paper IV 2004MNRAS.352.1439H, Cat. J/MNRAS/352/1439 Faulkner et al., Paper V 2004MNRAS.355..147F Lorimer et al., Paper VI 2006MNRAS.372..777L, Cat. J/MNRAS/372/777
(End) Patricia Bauer [CDS] 12-Nov-2002
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