Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/352/1439 into FORTRAN code for loading all data files into arrays.
Note that special values are assigned to unknown or unspecified
numbers (also called NULL numbers);
when necessary, the coordinate components making up the right ascension
and declination are converted into floating-point numbers
representing these angles in degrees.
program load_ReadMe
C=============================================================================
C F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-18
C=============================================================================
* This code was generated from the ReadMe file documenting a catalogue
* according to the "Standard for Documentation of Astronomical Catalogues"
* currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
* (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
* Please report problems or questions to
C=============================================================================
implicit none
* Unspecified or NULL values, generally corresponding to blank columns,
* are assigned one of the following special values:
* rNULL__ for unknown or NULL floating-point values
* iNULL__ for unknown or NULL integer values
real*4 rNULL__
integer*4 iNULL__
parameter (rNULL__=--2147483648.) ! NULL real number
parameter (iNULL__=(-2147483647-1)) ! NULL int number
integer idig ! testing NULL number
C=============================================================================
Cat. J/MNRAS/352/1439 Parkes Multi-Beam Pulsar Survey. IV. (Hobbs+, 2004)
*================================================================================
*The Parkes Multi-Beam Pulsar Survey -
*IV. Discovery of 180 pulsars and parameters for 281 previously known pulsars.
* Hobbs G., Faulkner A., Stairs I.H., Camilo F., Manchester R.N., Lyne A.G.,
* Kramer M., D'amico N., Kaspi V.M., Possenti A., Mclaughlin M.A.,
* Lorimer D.R., Burgay M., Joshi B.C., Crawford F.
* <Mon. Not. R. Astron. Soc., 352, 1439-1472 (2004)>
* =2004MNRAS.352.1439H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Positions, flux densities and pulse widths for
180 pulsars discovered in the Parkes multibeam
pulsar survey.
integer*4 nr__
parameter (nr__=180) ! Number of records
character*103 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*10 PSRJ (nr__) ! PSRJ designation
character*1 f_PSRJ (nr__) ! [AJ] Note on PSRJ (G1)
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*8 RAs (nr__) ! (s) Right ascension (J2000)
real*4 e_RAs (nr__) ! (s) rms uncertainty on right ascension
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*4 e_DEs (nr__) ! (arcsec) rms uncertainty on declination
real*4 GLON (nr__) ! (deg) Galactic longitude
real*4 GLAT (nr__) ! (deg) Galactic latitude
integer*4 Beam (nr__) ! [1/13] Beam number of the multibeam receiver
real*4 bDist (nr__) ! Radial distance, in units of beam radii
real*4 S_N (nr__) ! Signal-to-noise ratio of the pulse profile
real*4 S1_4 (nr__) ! (mJy) Flux density at 1400MHz
real*4 e_S1_4 (nr__) ! (mJy) rms uncertainty on S1400MHz
real*4 W50 (nr__) ! (ms) Pulse width at 50% of the peak
integer*4 W10 (nr__) ! (ms) ? Pulse width at 10% of the peak, only for
* high signal-to-noise ratio profiles
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Periods, period derivatives and dispersion
measures for 180 pulsars discovered in the
Parkes multibeam pulsar survey.
integer*4 nr__1
parameter (nr__1=180) ! Number of records
character*108 ar__1 ! Full-size record
character*10 PSRJ_1 (nr__1) ! PSRJ designation
character*1 f_PSRJ_1 (nr__1) ! [AJ] Note on PSRJ (G1)
character*2 n_PSRJ (nr__1) ! [G*+] Note on PSRJ (1)
real*8 Per (nr__1) ! (s) Period
integer*4 e_Per (nr__1) ! (10-16s) rms uncertainty on Per
real*8 dP_dt (nr__1) ! (10-15) Period derivative
integer*4 e_dP_dt (nr__1) ! (10-23) rms uncertainty on dP/dt
real*8 MJD (nr__1) ! (d) Epoch of the period in modified Julian date
integer*4 NTOA (nr__1) ! ? Number of pulse topocentric arrival time
* included in the timing solution
integer*4 MJD1 (nr__1) ! (d) MJD range covered the rms of the post-fit
* timing residuals
integer*4 MJD2 (nr__1) ! (d) MJD range covered the rms of the post-fit
* timing residuals
real*4 Res (nr__1) ! (ms) ? Residual
real*8 DM (nr__1) ! (pc/cm3) Pulsar dispersion measure
real*4 e_DM (nr__1) ! (pc/cm3) rms uncertainty on DM
*Note (1): Notes use the following symbols:
* G = pulsars that have glitched.
* * = pulsars which exhibit significant timing noise that has been
* removed, to first order, by the fitting of a frequency second
* derivative (even higher derivatives were included in the timing
* model if necessary).
* + = timing solutions already published
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Derived parameters for 180 pulsars discovered in
the Parkes multibeam pulsar survey
integer*4 nr__2
parameter (nr__2=180) ! Number of records
character*45 ar__2 ! Full-size record
character*10 PSRJ_2 (nr__2) ! PSRJ designation
real*4 logAge (nr__2) ! ([yr]) log of chararteristic age
real*4 logBs (nr__2) ! ([gauss]) log of surface dipole magnetic field strength
real*4 log_dE_dt (nr__2) ! ([10-7W]) log of loss in rotational energy
real*4 Dist (nr__2) ! (kpc) Distance derived from DM and Taylor & Cordes
* (1993ApJ...411..674T) model
real*4 Z (nr__2) ! (kpc) Inferred z-height
real*4 Lum (nr__2) ! (mJy/kpc2) Corresponding radio luminosity at 1400MHz
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Intermediate-mass binary pulsars (IMBPs) known
integer*4 nr__3
parameter (nr__3=14) ! Number of records
character*34 ar__3 ! Full-size record
character*10 PSR (nr__3) ! PSR designation
real*4 PerRot (nr__3) ! (ms) Rotational period
real*4 PerOrb (nr__3) ! (d) Orbital period
real*4 e (nr__3) ! (10-3) Orbital eccentricity
character*1 l_MWD (nr__3) ! Limit flag on MWD
real*4 MWD (nr__3) ! (solMass) Lower limit on the companion mass assuming a
* neutron-star mass of 1.35M_{sun}_
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Results for 281 previously known pulsars
integer*4 nr__4
parameter (nr__4=281) ! Number of records
character*116 ar__4 ! Full-size record
C Position composed of: GLON GLAT
character*10 PSRJ_3 (nr__4) ! PSRJ designation
character*1 m_PSRJ (nr__4) ! [A] Multiplicity index on PSRJ
character*1 f_PSRJ_2 (nr__4) ! [*] *: pulsars that saturated the
* digitizer (1)
character*1 n_PSRJ_1 (nr__4) ! [N] N: pulsar discoved during the Parkes
* high-latitude survey
* (Burgay et al., in prep.)
character*9 PSRB (nr__4) ! PSRB designation
real*4 GLON_1 (nr__4) ! (deg) Galactic longitude
real*4 GLAT_1 (nr__4) ! (deg) Galactic latitude
integer*4 Beam_1 (nr__4) ! Beam number
real*4 bDist_1 (nr__4) ! Radial distance, in units of beam radii
real*4 S_N_1 (nr__4) ! Signal-to-noise ratio
real*8 DMcat (nr__4) ! (pc/cm3) Catalog pulsar dispersion measure
real*8 e_DMcat (nr__4) ! (pc/cm3) rms uncertainty on DMcat
real*8 DM_1 (nr__4) ! (pc/cm3) New pulsar dispersion measure
real*4 e_DM_1 (nr__4) ! (pc/cm3) rms uncertainty on DM
real*4 S1_4cat (nr__4) ! (mJy) ? Catalog 1400MHz flux density
real*4 S1_4_1 (nr__4) ! (mJy) ? New 1400MHz flux density
real*4 e_S1_4_1 (nr__4) ! (mJy) ? rms uncertainty on S1.4
real*4 W50_1 (nr__4) ! (ms) ? Pulse width at 50% of the peak
real*4 W10_1 (nr__4) ! (ms) ? Pulse width at 10% of the peak
*Note (1): For pulsars that saturated the digitizer, flux densities or pulse
* widths were measured.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Flux density measurements at 1400MHz for those
pulsars with no previously catalogued value at
this observing frequency, but do have an
earlier flux measurement at 400MHz.
integer*4 nr__5
parameter (nr__5=38) ! Number of records
character*67 ar__5 ! Full-size record
character*10 PSRJ_4 (nr__5) ! PSRJ designation
character*9 PSRB_1 (nr__5) ! PSRB designation
real*4 DM_2 (nr__5) ! (pc/cm3) Pulsar dispersion measure
real*4 e_DM_2 (nr__5) ! (pc/cm3) rms uncertainty on DM
real*4 S1400MHz (nr__5) ! (mJy) Flux density at 1400MHz
real*4 e_S1400MHz (nr__5) ! (mJy) rms uncertainty on 1400MHz
real*4 S400MHz (nr__5) ! (mJy) ? Flux density at 400MHz
real*4 S600MHz (nr__5) ! (mJy) ? Flux density at 600MHz
real*4 SI (nr__5) ! Spectral index between 1400 and 400MHz (1)
integer*4 r_S400MHz (nr__5) ! ? Reference of S400MHz
integer*4 r_S600MHz (nr__5) ! ? Reference of S600MHz
*Note (1): Unfortunately, not all the S400MHz measurements have been published
* with corresponding uncertainties. Taking a typical uncertainty of 10%
* leads to an error in the spectral index determination of ~0.3.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'refs.dat' ! References
integer*4 nr__6
parameter (nr__6=10) ! Number of records
character*77 ar__6 ! Full-size record
integer*4 Ref (nr__6) ! Reference code
character*19 BibCode (nr__6) ! BibCode
character*27 Aut (nr__6) ! Author's name
character*25 Com (nr__6) ! Comments
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Dispersion measure values that have been
measured more than an order-of-magnitude more
precisely than in earlier studies.
integer*4 nr__7
parameter (nr__7=30) ! Number of records
character*47 ar__7 ! Full-size record
character*10 PSRJ_5 (nr__7) ! PSRJ designation
character*9 PSRB_2 (nr__7) ! PSRB designation
real*4 DMc (nr__7) ! (pc/cm3) Earlier pulsar dispersion measure (from table7)
real*4 e_DMc (nr__7) ! (pc/cm3) rms uncertainty on DMc
real*8 DM_3 (nr__7) ! (pc/cm3) New pulsar dispersion measure (from table7)
real*4 e_DM_3 (nr__7) ! (pc/cm3) rms uncertainty on DM
C=============================================================================
C Loading file 'table1.dat' ! Positions, flux densities and pulse widths for
* 180 pulsars discovered in the Parkes multibeam
* pulsar survey.
C Format for file interpretation
1 format(
+ A10,A1,2X,I2,1X,I2,1X,F8.5,1X,F6.5,1X,A1,I2,1X,I2,1X,F6.3,1X,
+ F6.3,1X,F6.2,1X,F5.2,1X,I2,1X,F4.2,1X,F5.1,1X,F5.3,1X,F4.3,1X,
+ F5.1,1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,180
read(1,'(A103)')ar__
read(ar__,1)
+ PSRJ(i__),f_PSRJ(i__),RAh(i__),RAm(i__),RAs(i__),e_RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),e_DEs(i__),GLON(i__),
+ GLAT(i__),Beam(i__),bDist(i__),S_N(i__),S1_4(i__),e_S1_4(i__),
+ W50(i__),W10(i__)
if(ar__(101:103) .EQ. '') W10(i__) = iNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ PSRJ(i__),f_PSRJ(i__),RAh(i__),RAm(i__),RAs(i__),e_RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),e_DEs(i__),GLON(i__),
+ GLAT(i__),Beam(i__),bDist(i__),S_N(i__),S1_4(i__),e_S1_4(i__),
+ W50(i__),W10(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Periods, period derivatives and dispersion
* measures for 180 pulsars discovered in the
* Parkes multibeam pulsar survey.
C Format for file interpretation
2 format(
+ A10,A1,A2,1X,F18.16,1X,I8,1X,F13.8,1X,I8,1X,F7.1,1X,I3,1X,I5,
+ 1X,I5,1X,F5.2,1X,F7.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,180
read(1,'(A108)')ar__1
read(ar__1,2)
+ PSRJ_1(i__),f_PSRJ_1(i__),n_PSRJ(i__),Per(i__),e_Per(i__),
+ dP_dt(i__),e_dP_dt(i__),MJD(i__),NTOA(i__),MJD1(i__),
+ MJD2(i__),Res(i__),DM(i__),e_DM(i__)
if(ar__1(74:76) .EQ. '') NTOA(i__) = iNULL__
if(ar__1(90:94) .EQ. '') Res(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ PSRJ_1(i__),f_PSRJ_1(i__),n_PSRJ(i__),Per(i__),e_Per(i__),
+ dP_dt(i__),e_dP_dt(i__),MJD(i__),NTOA(i__),MJD1(i__),
+ MJD2(i__),Res(i__),DM(i__),e_DM(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Derived parameters for 180 pulsars discovered in
* the Parkes multibeam pulsar survey
C Format for file interpretation
3 format(A10,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F5.2,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,180
read(1,'(A45)')ar__2
read(ar__2,3)
+ PSRJ_2(i__),logAge(i__),logBs(i__),log_dE_dt(i__),Dist(i__),
+ Z(i__),Lum(i__)
c ..............Just test output...........
write(6,3)
+ PSRJ_2(i__),logAge(i__),logBs(i__),log_dE_dt(i__),Dist(i__),
+ Z(i__),Lum(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Intermediate-mass binary pulsars (IMBPs) known
C Format for file interpretation
4 format(A10,1X,F5.1,1X,F4.1,1X,F6.4,1X,A1,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,14
read(1,'(A34)')ar__3
read(ar__3,4)
+ PSR(i__),PerRot(i__),PerOrb(i__),e(i__),l_MWD(i__),MWD(i__)
c ..............Just test output...........
write(6,4)
+ PSR(i__),PerRot(i__),PerOrb(i__),e(i__),l_MWD(i__),MWD(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Results for 281 previously known pulsars
C Format for file interpretation
5 format(
+ A10,A1,A1,A1,1X,A9,1X,F6.2,1X,F5.2,1X,I2,1X,F3.1,1X,F6.1,1X,
+ F9.4,1X,F7.4,1X,F8.3,1X,F6.3,2X,F6.1,1X,F5.2,1X,F4.2,1X,F6.2,
+ 1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,281
read(1,'(A116)')ar__4
read(ar__4,5)
+ PSRJ_3(i__),m_PSRJ(i__),f_PSRJ_2(i__),n_PSRJ_1(i__),PSRB(i__),
+ GLON_1(i__),GLAT_1(i__),Beam_1(i__),bDist_1(i__),S_N_1(i__),
+ DMcat(i__),e_DMcat(i__),DM_1(i__),e_DM_1(i__),S1_4cat(i__),
+ S1_4_1(i__),e_S1_4_1(i__),W50_1(i__),W10_1(i__)
if(ar__4(87:92) .EQ. '') S1_4cat(i__) = rNULL__
if(ar__4(94:98) .EQ. '') S1_4_1(i__) = rNULL__
if(ar__4(100:103) .EQ. '') e_S1_4_1(i__) = rNULL__
if(ar__4(105:110) .EQ. '') W50_1(i__) = rNULL__
if(ar__4(112:116) .EQ. '') W10_1(i__) = rNULL__
c ..............Just test output...........
write(6,5)
+ PSRJ_3(i__),m_PSRJ(i__),f_PSRJ_2(i__),n_PSRJ_1(i__),PSRB(i__),
+ GLON_1(i__),GLAT_1(i__),Beam_1(i__),bDist_1(i__),S_N_1(i__),
+ DMcat(i__),e_DMcat(i__),DM_1(i__),e_DM_1(i__),S1_4cat(i__),
+ S1_4_1(i__),e_S1_4_1(i__),W50_1(i__),W10_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Flux density measurements at 1400MHz for those
* pulsars with no previously catalogued value at
* this observing frequency, but do have an
* earlier flux measurement at 400MHz.
C Format for file interpretation
6 format(
+ A10,3X,A9,2X,F6.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F4.1,1X,F4.1,1X,
+ F5.2,I1,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,38
read(1,'(A67)')ar__5
read(ar__5,6)
+ PSRJ_4(i__),PSRB_1(i__),DM_2(i__),e_DM_2(i__),S1400MHz(i__),
+ e_S1400MHz(i__),S400MHz(i__),S600MHz(i__),SI(i__),
+ r_S400MHz(i__),r_S600MHz(i__)
if(ar__5(49:52) .EQ. '') S400MHz(i__) = rNULL__
if(ar__5(54:57) .EQ. '') S600MHz(i__) = rNULL__
if(ar__5(64:64) .EQ. '') r_S400MHz(i__) = iNULL__
if(ar__5(66:67) .EQ. '') r_S600MHz(i__) = iNULL__
c ..............Just test output...........
write(6,6)
+ PSRJ_4(i__),PSRB_1(i__),DM_2(i__),e_DM_2(i__),S1400MHz(i__),
+ e_S1400MHz(i__),S400MHz(i__),S600MHz(i__),SI(i__),
+ r_S400MHz(i__),r_S600MHz(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'refs.dat' ! References
C Format for file interpretation
7 format(I2,1X,A19,1X,A27,2X,A25)
C Effective file loading
open(unit=1,status='old',file=
+'refs.dat')
write(6,*) '....Loading file: refs.dat'
do i__=1,10
read(1,'(A77)')ar__6
read(ar__6,7)Ref(i__),BibCode(i__),Aut(i__),Com(i__)
c ..............Just test output...........
write(6,7)Ref(i__),BibCode(i__),Aut(i__),Com(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Dispersion measure values that have been
* measured more than an order-of-magnitude more
* precisely than in earlier studies.
C Format for file interpretation
8 format(A10,2X,A9,1X,F5.1,1X,F4.1,2X,F7.3,1X,F5.3)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,30
read(1,'(A47)')ar__7
read(ar__7,8)
+ PSRJ_5(i__),PSRB_2(i__),DMc(i__),e_DMc(i__),DM_3(i__),
+ e_DM_3(i__)
c ..............Just test output...........
write(6,8)
+ PSRJ_5(i__),PSRB_2(i__),DMc(i__),e_DMc(i__),DM_3(i__),
+ e_DM_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end