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 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:
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FileName Lrecl Records Explanations
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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.
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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
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Bytes Format Units Label Explanations
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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
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Note (1): PSRs J1841-0348, J1842-0415 and J1844-0310 were discovered
independently by Lorimer et al. (2000A&A...358..169L 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.
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Byte-by-byte Description of file: table2.dat
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Bytes Format Units Label Explanations
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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
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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.
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History:
From electronic version of the journal
References
Manchester et al., Paper I 2001MNRAS.328...17M 2001MNRAS.328...17M, Cat. J/MNRAS/328/17
Kramer et al., Paper III 2003MNRAS.342.1299K 2003MNRAS.342.1299K, Cat. J/MNRAS/342/1299
Hobbs et al., Paper IV 2004MNRAS.352.1439H 2004MNRAS.352.1439H, Cat. J/MNRAS/352/1439
Faulkner et al., Paper V 2004MNRAS.355..147F 2004MNRAS.355..147F
Lorimer et al., Paper VI 2006MNRAS.372..777L 2006MNRAS.372..777L, Cat. J/MNRAS/372/777
(End) Patricia Bauer [CDS] 12-Nov-2002