Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/399/1709 into FORTRAN code for reading data files line by line.
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 2026-Jun-08
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/399/1709 Near-infrared survey of Miras (Matsunaga+, 2009)
*================================================================================
*A near-infrared survey of Miras and the distance to the Galactic Centre.
* Matsunaga N., Kawadu T., Nishiyama S., Nagayama T., Hatano H., Tamura M.,
* Glass I.S., Nagata T.
* <Mon. Not. R. Astron. Soc., 399, 1709-1729 (2009)>
* =2009MNRAS.399.1709M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Catalogue of variable stars
integer*4 nr__
parameter (nr__=1364) ! Number of records
character*80 ar__ ! Full-size record
integer*4 Seq ! Sequential number
character*16 Name ! Name (HHMMSSss+DDMMSSs)
real*4 Jmag ! (mag) ?=99.99 J mean magnitude
real*4 Jamp ! (mag) ?=0.00 Peak-to-peak amplitude for J magnitude
real*4 Hmag ! (mag) ?=99.99 H mean magnitude
real*4 Hamp ! (mag) ?=0.00 Peak-to-peak amplitude for H magnitude
real*4 Ksmag ! (mag) ?=99.99 Ks mean magnitude
real*4 Kamp ! (mag) ?=0.00 Peak-to-peak amplitude for Ks magnitude
integer*4 f_Jmag ! [0/6] Problem on Jmag when non-zero (1)
integer*4 f_Hmag ! [0/6] Problem on Hmag when non-zero (1)
integer*4 f_Ksmag ! [0/6] Problem on Ksmag when non-zero (1)
integer*4 SSTGC ! ? Ramirez et al. (2008, Cat. <II/295>)
* counterpart
character*7 v_GMC2001_ ! Glass et al. (G01, 2001. Cat. <J/MNRAS/321/77>)
* counterpart
integer*4 Per ! (d) ? Period
integer*4 f_Per ! [0/5] Flag on period (0=OK) (2)
*Note (1): Flags on magnitudes as follows:
* 0 = The magnitude was obtained without any clear problems
* 1 = We did not obtain the magnitude because the object often falls
* out of the field of view
* 2 = We did not obtain the magnitude because the object is too bright
* 3 = We did not obtain the magnitude because the object is too faint
* 4 = We obtained the mean magnitude, but it is affected by its
* location around the edge of the images
* 5 = We obtained the mean magnitude, but it is affected by saturation
* or deviation from the linear response
* 6 = We obtained the mean magnitude, but it is affected by the fact that
* the object was not detected in some cases because of its faintness
*Note (2): Flag on period as follows:
* 0 = P_G01_ and P_IRSF_ agree with each other to within 0.075dex.
* We adopt PIRSF
* 1 = P_G01_ and P_IRSF_ disagree and we adopt P_IRSF_
* 2 = P_G01_ is not given and we adopt P_IRSF_
* 3 = P_G01_ fit our light curve but P_IRSF_ is not properly obtained.
* We adopt P_G01_
* 4 = P_G01_ does not fit the IRSF light curve. No periodicity is found
* 5 = P_G01_ is not given and no clear periodicity is found with the
* IRSF data
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Extinctions A_Ks_ and distance moduli mu0
estimated for Miras
integer*4 nr__1
parameter (nr__1=175) ! Number of records
character*40 ar__1 ! Full-size record
integer*4 Seq_1 ! Sequential number of star
real*4 AHK_Ks ! (mag) ?=99.99 Extinction A_Ks_ from HK pair of
* filter bands (1)
real*4 muJK0 ! (mag) ?=99.99 Distance moduli from JK pair of
* filter bands (2)
real*4 AJK_Ks ! (mag) ?=99.99 Extinction A_Ks_ from JK pair of
* filter bands (1)
real*4 muHK0 ! (mag) ?=99.99 Distance moduli from HK pair of
* filter bands (2)
real*4 AJH_Ks ! (mag) ?=99.99 Extinction A_Ks_ from JH pair of
* filter bands (1)
real*4 muJH0 ! (mag) ?=99.99 Distance moduli from JH pair of
* filter bands (2)
*Note (1): For example, AHH,Ks= (H-Ks)/(r_H_-1)-(M_H_-M_Ks_)/(r_H_-1),
* r_H_=1.731
*Note (2): For example, muHK0=(r_H_Ks-H)/(r_H_-1)-(r_H_M_Ks_-M_H_)/(r_H_-1),
* r_H_=1.731
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Light variations
integer*4 nr__2
parameter (nr__2=116887) ! Number of records
character*33 ar__2 ! Full-size record
integer*4 Seq_2 ! Sequential number of star
real*8 MJD ! (d) Modified Julian date
real*4 Jmag_1 ! (mag) ?=99.99 J mean magnitude
real*4 Hmag_1 ! (mag) ?=99.99 H mean magnitude
real*4 Ksmag_1 ! (mag) ?=99.99 Ks mean magnitude
C=============================================================================
C Loading file 'table6.dat' ! Catalogue of variable stars
C Format for file interpretation
1 format(
+ I4,1X,A16,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,
+ I1,I1,I1,1X,I7,1X,A7,1X,I3,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,1364
read(1,'(A80)')ar__
read(ar__,1)
+ Seq,Name,Jmag,Jamp,Hmag,Hamp,Ksmag,Kamp,f_Jmag,f_Hmag,f_Ksmag,
+ SSTGC,v_GMC2001_,Per,f_Per
if(ar__(60:66) .EQ. '') SSTGC = iNULL__
if(ar__(76:78) .EQ. '') Per = iNULL__
c ..............Just test output...........
write(6,1)
+ Seq,Name,Jmag,Jamp,Hmag,Hamp,Ksmag,Kamp,f_Jmag,f_Hmag,f_Ksmag,
+ SSTGC,v_GMC2001_,Per,f_Per
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Extinctions A_Ks_ and distance moduli mu0
* estimated for Miras
C Format for file interpretation
2 format(I4,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,175
read(1,'(A40)')ar__1
read(ar__1,2)Seq_1,AHK_Ks,muJK0,AJK_Ks,muHK0,AJH_Ks,muJH0
c ..............Just test output...........
write(6,2)Seq_1,AHK_Ks,muJK0,AJK_Ks,muHK0,AJH_Ks,muJH0
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Light variations
C Format for file interpretation
3 format(I4,1X,F10.4,1X,F5.2,1X,F5.2,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,116887
read(1,'(A33)')ar__2
read(ar__2,3)Seq_2,MJD,Jmag_1,Hmag_1,Ksmag_1
c ..............Just test output...........
write(6,3)Seq_2,MJD,Jmag_1,Hmag_1,Ksmag_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end