Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/117/2941 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-19
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/AJ/117/2941 Rotation periods of Orion PMS stars (Stassun+, 1999)
*================================================================================
*The rotation period distribution of pre-main-sequence stars in and around
*the Orion nebula.
* Stassun K.G., Mathieu R.D., Mazeh T., Vrba F.J.
* <Astron. J. 117, 2941 (1999)>
* =1999AJ....117.2941S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Data for rotator sample
integer*4 nr__
parameter (nr__=254) ! Number of records
character*99 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 v_SMM99_ (nr__) ! Star number
integer*4 JW (nr__) ! ? JW number (1)
character*1 n_JW (nr__) ! [k] Hillenbrand (1997, Cat. <J/AJ/113/1733>)
* identifies this star as JW466
integer*4 RAh (nr__) ! (h) Right ascension (J2000.0) (2)
integer*4 RAm (nr__) ! (min) Right ascension (J2000.0)
real*4 RAs (nr__) ! (s) Right ascension (J2000.0)
character*1 DE_ (nr__) ! Declination sign (J2000.0)
integer*4 DEd (nr__) ! (deg) Declination (J2000.0)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0)
real*4 DEs (nr__) ! (arcsec) Declination (J2000.0)
real*4 Imag (nr__) ! (mag) I magnitude
real*4 Per (nr__) ! (d) Rotation period
character*1 n_Per (nr__) ! [j] j: Detected at limit of period search
real*4 e_Per (nr__) ! (d) ? rms uncertainty on Per (3)
real*4 PerCH (nr__) ! (d) ? Rotation period from Choi & Herbst,
* 1996AJ....111..283C
real*4 EWHa (nr__) ! (0.1nm) ? H{alpha} equivalent width (4)
character*1 n_EWHa (nr__) ! [i] i: Strong H{alpha} emitter
real*4 EWLi (nr__) ! (0.1nm) ? Li equivalent width (5)
real*4 FWHMLi (nr__) ! (0.1nm) ? Li FWHM (5)
real*4 RV (nr__) ! (km/s) ? Radial velocity
integer*4 Memb (nr__) ! (%) ? Membership probability (1)
real*4 Mass (nr__) ! (solMass) ? Mass (Hillenbrand, 1997, Cat. <J/AJ/113/1733>)
real*4 Rad (nr__) ! (solRad) ? Radius (Hillenbrand, Cat. <J/AJ/113/1733>)
real*4 v_vbr (nr__) ! ? Velocity to break-up velocity ratio
real*4 D_I_K (nr__) ! ? Near-IR excess emission (Hillenbrand et al.
* 1998ApJ...492..540H)
*Note (1): Source: Jones & Walker, 1988AJ.....95.1755J
* ID numbers 3000- and 5000- correspond to ID numbers from
* Hillenbrand, 1997, Cat. <J/AJ/113/1733>
*Note (2): Coordinates referenced to USNO-A1.0 astrometric database.
*Note (3): Uncertainty computed as in text. A value of zero indicates an
* uncertainty less than 0.005 days.
*Note (4): A value of zero indicates no detected H{alpha} emission
* outside the nebular line. Values indicate emission strength.
*Note (5): A value of zero indicates no detected Li absorption.
* Values indicate absorption strength.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Data for rotators with 1%<FAP<5%
(FAP = false alarm probability)
integer*4 nr__1
parameter (nr__1=16) ! Number of records
character*99 ar__1 ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000.0
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 v_SMM99__1 (nr__1) ! Star number
integer*4 JW_1 (nr__1) ! ? JW number (1)
character*1 n_JW_1 (nr__1) ! [k] Hillenbrand (1997, Cat. <J/AJ/113/1733>)
* identifies this star as JW466
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000.0) (2)
integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000.0)
real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000.0)
character*1 DE__1 (nr__1) ! Declination sign (J2000.0)
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000.0)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000.0)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000.0)
real*4 Imag_1 (nr__1) ! (mag) I magnitude
real*4 Per_1 (nr__1) ! (d) Rotation period
character*1 n_Per_1 (nr__1) ! [j] j: Detected at limit of period search
real*4 e_Per_1 (nr__1) ! (d) ? rms uncertainty on Per (3)
real*4 PerCH_1 (nr__1) ! (d) ? Rotation period from Choi & Herbst,
* 1996AJ....111..283C
real*4 EWHa_1 (nr__1) ! (0.1nm) ? H{alpha} equivalent width (4)
character*1 n_EWHa_1 (nr__1) ! [i] i: Strong H{alpha} emitter
real*4 EWLi_1 (nr__1) ! (0.1nm) ? Li equivalent width (5)
real*4 FWHMLi_1 (nr__1) ! (0.1nm) ? Li FWHM (5)
real*4 RV_1 (nr__1) ! (km/s) ? Radial velocity
integer*4 Memb_1 (nr__1) ! (%) ? Membership probability (1)
real*4 Mass_1 (nr__1) ! (solMass) ? Mass (Hillenbrand, 1997, Cat. <J/AJ/113/1733>)
real*4 Rad_1 (nr__1) ! (solRad) ? Radius (Hillenbrand, Cat. <J/AJ/113/1733>)
real*4 v_vbr_1 (nr__1) ! ? Velocity to break-up velocity ratio
real*4 D_I_K_1 (nr__1) ! ? Near-IR excess emission (Hillenbrand et al.
* 1998ApJ...492..540H)
*Note (1): Source: Jones & Walker, 1988AJ.....95.1755J
* ID numbers 3000- and 5000- correspond to ID numbers from
* Hillenbrand, 1997, Cat. <J/AJ/113/1733>
*Note (2): Coordinates referenced to USNO-A1.0 astrometric database.
*Note (3): Uncertainty computed as in text. A value of zero indicates an
* uncertainty less than 0.005 days.
*Note (4): A value of zero indicates no detected H{alpha} emission
* outside the nebular line. Values indicate emission strength.
*Note (5): A value of zero indicates no detected Li absorption.
* Values indicate absorption strength.
C=============================================================================
C Loading file 'table1.dat' ! Data for rotator sample
C Format for file interpretation
1 format(
+ I4,1X,I4,A1,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,
+ 1X,F5.2,A1,F4.2,1X,F5.2,1X,F4.1,A1,F4.2,1X,F3.1,1X,F4.1,1X,I2,
+ 1X,F5.2,1X,F4.2,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,254
read(1,'(A99)')ar__
read(ar__,1)
+ v_SMM99_(i__),JW(i__),n_JW(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Imag(i__),Per(i__),
+ n_Per(i__),e_Per(i__),PerCH(i__),EWHa(i__),n_EWHa(i__),
+ EWLi(i__),FWHMLi(i__),RV(i__),Memb(i__),Mass(i__),Rad(i__),
+ v_vbr(i__),D_I_K(i__)
if(ar__(6:9) .EQ. '') JW(i__) = iNULL__
if(ar__(46:49) .EQ. '') e_Per(i__) = rNULL__
if(ar__(51:55) .EQ. '') PerCH(i__) = rNULL__
if(ar__(57:60) .EQ. '') EWHa(i__) = rNULL__
if(ar__(62:65) .EQ. '') EWLi(i__) = rNULL__
if(ar__(67:69) .EQ. '') FWHMLi(i__) = rNULL__
if(ar__(71:74) .EQ. '') RV(i__) = rNULL__
if(ar__(76:77) .EQ. '') Memb(i__) = iNULL__
if(ar__(79:83) .EQ. '') Mass(i__) = rNULL__
if(ar__(85:88) .EQ. '') Rad(i__) = rNULL__
if(ar__(90:93) .EQ. '') v_vbr(i__) = rNULL__
if(ar__(95:99) .EQ. '') D_I_K(i__) = rNULL__
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)
+ v_SMM99_(i__),JW(i__),n_JW(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Imag(i__),Per(i__),
+ n_Per(i__),e_Per(i__),PerCH(i__),EWHa(i__),n_EWHa(i__),
+ EWLi(i__),FWHMLi(i__),RV(i__),Memb(i__),Mass(i__),Rad(i__),
+ v_vbr(i__),D_I_K(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' ! Data for rotators with 1%<FAP<5%
* (FAP = false alarm probability)
C Format for file interpretation
2 format(
+ I4,1X,I4,A1,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,
+ 1X,F5.2,A1,F4.2,1X,F5.2,1X,F4.1,A1,F4.2,1X,F3.1,1X,F4.1,1X,I2,
+ 1X,F5.2,1X,F4.2,1X,F4.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,16
read(1,'(A99)')ar__1
read(ar__1,2)
+ v_SMM99__1(i__),JW_1(i__),n_JW_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ Imag_1(i__),Per_1(i__),n_Per_1(i__),e_Per_1(i__),PerCH_1(i__),
+ EWHa_1(i__),n_EWHa_1(i__),EWLi_1(i__),FWHMLi_1(i__),RV_1(i__),
+ Memb_1(i__),Mass_1(i__),Rad_1(i__),v_vbr_1(i__),D_I_K_1(i__)
if(ar__1(6:9) .EQ. '') JW_1(i__) = iNULL__
if(ar__1(46:49) .EQ. '') e_Per_1(i__) = rNULL__
if(ar__1(51:55) .EQ. '') PerCH_1(i__) = rNULL__
if(ar__1(57:60) .EQ. '') EWHa_1(i__) = rNULL__
if(ar__1(62:65) .EQ. '') EWLi_1(i__) = rNULL__
if(ar__1(67:69) .EQ. '') FWHMLi_1(i__) = rNULL__
if(ar__1(71:74) .EQ. '') RV_1(i__) = rNULL__
if(ar__1(76:77) .EQ. '') Memb_1(i__) = iNULL__
if(ar__1(79:83) .EQ. '') Mass_1(i__) = rNULL__
if(ar__1(85:88) .EQ. '') Rad_1(i__) = rNULL__
if(ar__1(90:93) .EQ. '') v_vbr_1(i__) = rNULL__
if(ar__1(95:99) .EQ. '') D_I_K_1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ v_SMM99__1(i__),JW_1(i__),n_JW_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ Imag_1(i__),Per_1(i__),n_Per_1(i__),e_Per_1(i__),PerCH_1(i__),
+ EWHa_1(i__),n_EWHa_1(i__),EWLi_1(i__),FWHMLi_1(i__),RV_1(i__),
+ Memb_1(i__),Mass_1(i__),Rad_1(i__),v_vbr_1(i__),D_I_K_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end