Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/413/2218 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_1.5, on 2013-May-22
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__=-1.e37) ! NULL real number
parameter (iNULL__=-2147483647) ! NULL int number
C=============================================================================
Cat. J/MNRAS/413/2218 Stellar rotation in Hyades and Praesepe (Delorme+, 2011)
*================================================================================
*Stellar rotation in the Hyades and Praesepe: gyrochronology and braking
*time-scale.
* Delorme P., Cameron A.C., Hebb L., Rostron J., Lister T.A., Norton A.J.,
* Pollacco D., West R.G.
* <Mon. Not. R. Astron. Soc., 413, 2218-2234 (2011)>
* =2011MNRAS.413.2218D
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Hyades SuperWASP fields used in this survey
integer*4 nr__
parameter (nr__=21) ! Number of records
character*35 ar__ ! Full-size record
real*8 RA_ (nr__) ! (deg) Right Ascension J2000
real*8 Dec (nr__) ! (deg) Declination J2000
integer*4 RAh (nr__) ! (h) Field centre right ascension (J2000)
integer*4 RAm (nr__) ! (min) Field centre right ascension (J2000)
character*1 DE_ (nr__) ! Field centre declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Field centre declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Field centre declination (J2000)
integer*4 Nimg (nr__) ! Number of images
integer*4 Nnig (nr__) ! Usable nights
character*10 Date (nr__) ! ("YYYY-MM-DD") First night date
integer*4 Nb (nr__) ! Baseline (nights)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Hyades members with SuperWASP rotation periods
integer*4 nr__1
parameter (nr__1=62) ! Number of records
character*113 ar__1 ! Full-size record
character*19 SWASP (nr__1) ! Swasp designation (JHHMMSS.ss+DDMMSS.s)
character*12 USNO (nr__1) ! USNO B-1.0 designation
character*3 X (nr__1) ! [Yes/No ] X-ray activity? (table2 only) (1)
real*4 Per (nr__1) ! (d) Rotation (spin) period (2)
real*4 dPer (nr__1) ! (d) ? Difference between the two period
* determinations (2)
real*4 J_Ks (nr__1) ! (mag) 2MASS J-Ks colour index
real*4 Ksmag (nr__1) ! (mag) 2MASS Ks magnitude
real*4 Vmag (nr__1) ! (mag) ?=- V magnitude
real*4 Dist (nr__1) ! (deg) Distance to the cluster centre
real*4 pmRA (nr__1) ! (mas) Proper motion along RA
real*4 e_pmRA (nr__1) ! (mas) rms uncertainty on pmRA
real*4 pmDE (nr__1) ! (mas) Proper motion along DE
real*4 e_pmDE (nr__1) ! (mas) rms uncertainty on pmDE
real*4 plx (nr__1) ! (mas) ?=- Parallax (table2 only)
real*4 Mmb (nr__1) ! Membership probability
*Note (1): traces whether or not Stern, Schmitt & Kahabka (1995,
* Cat. J/ApJ/448/683) reported X-ray activity.
*Note (2): if the object has been identified on two different seasons, the
* period given is the average of the two periods whose difference is
* indicated in dPer.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Praesepe members with SuperWASP rotation periods
integer*4 nr__2
parameter (nr__2=52) ! Number of records
character*113 ar__2 ! Full-size record
character*19 SWASP_1 (nr__2) ! Swasp designation (JHHMMSS.ss+DDMMSS.s)
character*12 USNO_1 (nr__2) ! USNO B-1.0 designation
character*3 X_1 (nr__2) ! [Yes/No ] X-ray activity? (table2 only) (1)
real*4 Per_1 (nr__2) ! (d) Rotation (spin) period (2)
real*4 dPer_1 (nr__2) ! (d) ? Difference between the two period
* determinations (2)
real*4 J_Ks_1 (nr__2) ! (mag) 2MASS J-Ks colour index
real*4 Ksmag_1 (nr__2) ! (mag) 2MASS Ks magnitude
real*4 Vmag_1 (nr__2) ! (mag) ?=- V magnitude
real*4 Dist_1 (nr__2) ! (deg) Distance to the cluster centre
real*4 pmRA_1 (nr__2) ! (mas) Proper motion along RA
real*4 e_pmRA_1 (nr__2) ! (mas) rms uncertainty on pmRA
real*4 pmDE_1 (nr__2) ! (mas) Proper motion along DE
real*4 e_pmDE_1 (nr__2) ! (mas) rms uncertainty on pmDE
real*4 plx_1 (nr__2) ! (mas) ?=- Parallax (table2 only)
real*4 Mmb_1 (nr__2) ! Membership probability
*Note (1): traces whether or not Stern, Schmitt & Kahabka (1995,
* Cat. J/ApJ/448/683) reported X-ray activity.
*Note (2): if the object has been identified on two different seasons, the
* period given is the average of the two periods whose difference is
* indicated in dPer.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! Cross-identifications and B, V photometry from
the literature of rotational variables with
Hyades membership probabilities greater than 0.5
integer*4 nr__3
parameter (nr__3=62) ! Number of records
character*77 ar__3 ! Full-size record
character*19 SWASP_2 (nr__3) ! Swasp designation (JHHMMSS.ss+DDMMSS.s)
character*12 USNO_2 (nr__3) ! USNO B-1.0 designation
character*18 OName (nr__3) ! Cluster member ID
character*4 SpType (nr__3) ! MK spectral type
real*4 Vmagl (nr__3) ! (mag) ? Literature V magnitude
real*4 B_Vl (nr__3) ! (mag) ? Literature B-V colour index
integer*4 Ref (nr__3) ! ? Reference for photometry (1)
*Note (1): References as follows:
* 1 = Upgren, Weis & Deluca (1979AJ.....84.1586U)
* 2 = Weis (1983PASP...95...29W)
* 3 = Upgren, Weis & Hanson (1985AJ.....90.2039U)
* 4 = Weis & Hanson (1988AJ.....96..148W)
* 5 = Stauffer (1982AJ.....87..899S)
* 11 = Klein Wassink (1927PGro...41....1K)
* 12 = Jones & Stauffer (1991AJ....102.1080J)
* 13 = Johnson (1952ApJ...116..640J)
* 14 = Upgren et al. (1979AJ.....84.1586U)
* 15 = Weis (1981PASP...93..437W)
* 16 = Mermilliod et al. (1990A&A...235..114M)
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! Cross-identifications and B, V photometry from
the literature of rotational variables with
Praesepe membership probabilities greater than 0.5
integer*4 nr__4
parameter (nr__4=52) ! Number of records
character*77 ar__4 ! Full-size record
character*19 SWASP_3 (nr__4) ! Swasp designation (JHHMMSS.ss+DDMMSS.s)
character*12 USNO_3 (nr__4) ! USNO B-1.0 designation
character*18 OName_1 (nr__4) ! Cluster member ID
character*4 SpType_1 (nr__4) ! MK spectral type
real*4 Vmagl_1 (nr__4) ! (mag) ? Literature V magnitude
real*4 B_Vl_1 (nr__4) ! (mag) ? Literature B-V colour index
integer*4 Ref_1 (nr__4) ! ? Reference for photometry (1)
*Note (1): References as follows:
* 1 = Upgren, Weis & Deluca (1979AJ.....84.1586U)
* 2 = Weis (1983PASP...95...29W)
* 3 = Upgren, Weis & Hanson (1985AJ.....90.2039U)
* 4 = Weis & Hanson (1988AJ.....96..148W)
* 5 = Stauffer (1982AJ.....87..899S)
* 11 = Klein Wassink (1927PGro...41....1K)
* 12 = Jones & Stauffer (1991AJ....102.1080J)
* 13 = Johnson (1952ApJ...116..640J)
* 14 = Upgren et al. (1979AJ.....84.1586U)
* 15 = Weis (1981PASP...93..437W)
* 16 = Mermilliod et al. (1990A&A...235..114M)
C=============================================================================
C Loading file 'table1.dat' ! Hyades SuperWASP fields used in this survey
C Format for file interpretation
1 format(I2,1X,I2,1X,A1,I2,1X,I2,1X,I4,1X,I2,1X,A10,1X,I3)
C Effective file loading
open(unit=1,file='table1.dat', status='old')
write(6,*) '....Loading file: table1.dat'
do i__=1,21
read(1,'(A35)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),Nimg(i__),
+ Nnig(i__),Date(i__),Nb(i__)
c Derive coordinates RA_ and Dec from input data
c (RA_ and Dec are set to rNULL_ when unknown)
RA_(i__) = RAh(i__)
if(RAh(i__) .GE. 0) RA_(i__)=RAh(i__)*15.
if(RAm(i__) .GE. 0) RA_(i__)=RA_(i__)+RAm(i__)/4.
Dec(i__) = DEd(i__)
if(DEm(i__) .GE. 0) Dec(i__)=Dec(i__)+DEm(i__)/60.
if(DE_(i__).EQ.'-'.AND.Dec(i__).GE.0) Dec(i__)=-Dec(i__)
c ..............Just test output...........
write(6,1)
+ RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),Nimg(i__),
+ Nnig(i__),Date(i__),Nb(i__)
write(6,'(6H Pos: 2F8.4)') RA_(i__),Dec(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Hyades members with SuperWASP rotation periods
C Format for file interpretation
2 format(
+ 6X,A19,1X,A12,1X,A3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F5.2,2X,F5.2,
+ 1X,F4.1,1X,F5.1,1X,F4.1,1X,F5.1,1X,F4.1,1X,F5.2,1X,F5.3)
C Effective file loading
open(unit=1,file='table2.dat', status='old')
write(6,*) '....Loading file: table2.dat'
do i__=1,62
read(1,'(A113)')ar__1
read(ar__1,2)
+ SWASP(i__),USNO(i__),X(i__),Per(i__),dPer(i__),J_Ks(i__),
+ Ksmag(i__),Vmag(i__),Dist(i__),pmRA(i__),e_pmRA(i__),
+ pmDE(i__),e_pmDE(i__),plx(i__),Mmb(i__)
if(ar__1(51:55) .EQ. '') dPer(i__) = rNULL__
if (Vmag(i__) .EQ. 2.2233e-322) Vmag(i__) = rNULL__
if (plx(i__) .EQ. 2.2233e-322) plx(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ SWASP(i__),USNO(i__),X(i__),Per(i__),dPer(i__),J_Ks(i__),
+ Ksmag(i__),Vmag(i__),Dist(i__),pmRA(i__),e_pmRA(i__),
+ pmDE(i__),e_pmDE(i__),plx(i__),Mmb(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Praesepe members with SuperWASP rotation periods
C Format for file interpretation
3 format(
+ 6X,A19,1X,A12,1X,A3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F5.2,2X,F5.2,
+ 1X,F4.1,1X,F5.1,1X,F4.1,1X,F5.1,1X,F4.1,1X,F5.2,1X,F5.3)
C Effective file loading
open(unit=1,file='table4.dat', status='old')
write(6,*) '....Loading file: table4.dat'
do i__=1,52
read(1,'(A113)')ar__2
read(ar__2,3)
+ SWASP_1(i__),USNO_1(i__),X_1(i__),Per_1(i__),dPer_1(i__),
+ J_Ks_1(i__),Ksmag_1(i__),Vmag_1(i__),Dist_1(i__),pmRA_1(i__),
+ e_pmRA_1(i__),pmDE_1(i__),e_pmDE_1(i__),plx_1(i__),Mmb_1(i__)
if(ar__2(51:55) .EQ. '') dPer_1(i__) = rNULL__
if (Vmag_1(i__) .EQ. 2.2233e-322) Vmag_1(i__) = rNULL__
if (plx_1(i__) .EQ. 2.2233e-322) plx_1(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ SWASP_1(i__),USNO_1(i__),X_1(i__),Per_1(i__),dPer_1(i__),
+ J_Ks_1(i__),Ksmag_1(i__),Vmag_1(i__),Dist_1(i__),pmRA_1(i__),
+ e_pmRA_1(i__),pmDE_1(i__),e_pmDE_1(i__),plx_1(i__),Mmb_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea1.dat' ! Cross-identifications and B, V photometry from
* the literature of rotational variables with
* Hyades membership probabilities greater than 0.5
C Format for file interpretation
4 format(6X,A19,1X,A12,1X,A18,1X,A4,2X,F5.2,1X,F4.2,1X,I2)
C Effective file loading
open(unit=1,file='tablea1.dat', status='old')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,62
read(1,'(A77)')ar__3
read(ar__3,4)
+ SWASP_2(i__),USNO_2(i__),OName(i__),SpType(i__),Vmagl(i__),
+ B_Vl(i__),Ref(i__)
if(ar__3(65:69) .EQ. '') Vmagl(i__) = rNULL__
if(ar__3(71:74) .EQ. '') B_Vl(i__) = rNULL__
if(ar__3(76:77) .EQ. '') Ref(i__) = iNULL__
c ..............Just test output...........
write(6,4)
+ SWASP_2(i__),USNO_2(i__),OName(i__),SpType(i__),Vmagl(i__),
+ B_Vl(i__),Ref(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea2.dat' ! Cross-identifications and B, V photometry from
* the literature of rotational variables with
* Praesepe membership probabilities greater than 0.5
C Format for file interpretation
5 format(6X,A19,1X,A12,1X,A18,1X,A4,2X,F5.2,1X,F4.2,1X,I2)
C Effective file loading
open(unit=1,file='tablea2.dat', status='old')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,52
read(1,'(A77)')ar__4
read(ar__4,5)
+ SWASP_3(i__),USNO_3(i__),OName_1(i__),SpType_1(i__),
+ Vmagl_1(i__),B_Vl_1(i__),Ref_1(i__)
if(ar__4(65:69) .EQ. '') Vmagl_1(i__) = rNULL__
if(ar__4(71:74) .EQ. '') B_Vl_1(i__) = rNULL__
if(ar__4(76:77) .EQ. '') Ref_1(i__) = iNULL__
c ..............Just test output...........
write(6,5)
+ SWASP_3(i__),USNO_3(i__),OName_1(i__),SpType_1(i__),
+ Vmagl_1(i__),B_Vl_1(i__),Ref_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end