Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/138/1380 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 2024-Apr-16
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/138/1380 Dust clumps in the Galactic Plane (Matthews+, 2009)
*================================================================================
*Looking through the Galactic Plane: imaging cold dust toward l = 44{deg}.
* Matthews H., Kirk H., Johnstone D., Weferling B., Cohen M., Jenness T.,
* Evans A., Davis G., Dent W.R.F., Fuller G., Jackson J.M., Rathborne J.,
* Richer J., Simon R.
* <Astron. J., 138, 1380-1402 (2009)>
* =2009AJ....138.1380M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Clumps identified in the 850um image
integer*4 nr__
parameter (nr__=132) ! Number of records
character*69 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq ! Clump number (<[MKJ2009] NNN> in Simbad)
character*13 v_MKJ2009_ ! Name (GLL.lll+B.bbb) (1)
integer*4 RAh ! (h) Hour of right ascension (J2000) (2)
integer*4 RAm ! (min) Minute of right ascension (J2000) (2)
real*4 RAs ! (s) Second of right ascension (J2000) (2)
character*1 DE_ ! Sign of declination (J2000) (2)
integer*4 DEd ! (deg) Degree of declination (J2000) (2)
integer*4 DEm ! (arcmin) Arcminute of declination (J2000) (2)
integer*4 DEs ! (arcsec) Arcsecond of declination (J2000) (2)
real*4 P850 ! (Jy) 850um peak flux of the clump in Jy/beam unit (3)
real*4 S850 ! (Jy) SCUBA/JCMT 850um total flux of the clump (3)
real*4 Reff ! (arcsec) Effective radius of the clump (3)
real*4 P1200 ! (Jy) Peak flux at 1200um in Jy/beam unit (4)
real*4 S1200 ! (Jy) SIMBA/SEST total flux at 1200um (4)
*Note (1): Name formed from equivalent Galactic coordinates, accurate to
* approximately 4".
*Note (2): Position of peak surface brightness within the clump at 850um
* (positional accuracy about 4").
*Note (3): Peak flux, total flux, and effective radius of the clumps as
* determined by clfind (Williams et al. 1994, Cat. J/ApJ/428/693). The
* absolute flux calibration is uncertain at a level of about 20%. The
* effective radius has not been deconvolved from the telescope beam.
*Note (4): Peak flux and total flux at 1200um determined using the 850um
* clump locations.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Distance determinations obtained from
^13^CO(1-0) and HI data
integer*4 nr__1
parameter (nr__1=132) ! Number of records
character*36 ar__1 ! Full-size record
integer*4 Seq_1 ! Clump number (as in table 2)
real*4 Pk ! (K) Peak ^13^CO(1-0) intensity
real*4 Vlsr ! (km/s) Local standard of rest velocity
character*1 n_Dist ! [N/F] Near/Far clump distance resolution
real*4 Dist ! (kpc) Clump distance based on clump velocity
integer*4 HI ! ?=0 HI catalogue cloud number (maintained locally
* at Boston University)
character*1 n_Dist1 ! [N/F/0] Near/Far distance resolution based on HI
* cloud data
real*4 Dist1 ! (kpc) ?=0 Cloud distance derived from HI cloud data
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Clump masses based on clump and cloud distance
determinations
integer*4 nr__2
parameter (nr__2=132) ! Number of records
character*21 ar__2 ! Full-size record
integer*4 Seq_2 ! Clump number
real*8 Mclp ! (Msun) Clump mass derived from the clump distance (5)
real*8 Mcld ! (Msun) ? Clump mass derived from the cloud distance (6)
*Note (5): Clump mass derived from the clump distance as listed in Table 6.
*Note (6): Clump mass derived from the cloud distance as listed in Table 6.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table8.dat' ! Sources of emission probably associated with
dust clumps
integer*4 nr__3
parameter (nr__3=132) ! Number of records
character*68 ar__3 ! Full-size record
integer*4 Seq_3 ! Clump number
character*64 Assoc ! Association(s) (7)
*Note (7): Other sources of emission probably associated with this dust clump,
* within a radius of 1 arcmin from the dust clump position.
C=============================================================================
C Loading file 'table2.dat' ! Clumps identified in the 850um image
C Format for file interpretation
1 format(
+ I3,1X,A13,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F5.2,1X,
+ F6.2,1X,F4.1,1X,F5.2,1X,F6.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,132
read(1,'(A69)')ar__
read(ar__,1)
+ Seq,v_MKJ2009_,RAh,RAm,RAs,DE_,DEd,DEm,DEs,P850,S850,Reff,
+ P1200,S1200
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Seq,v_MKJ2009_,RAh,RAm,RAs,DE_,DEd,DEm,DEs,P850,S850,Reff,
+ P1200,S1200
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table6.dat' ! Distance determinations obtained from
* ^13^CO(1-0) and HI data
C Format for file interpretation
2 format(I3,1X,F5.3,1X,F6.2,1X,A1,1X,F5.2,1X,I3,1X,A1,1X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,132
read(1,'(A36)')ar__1
read(ar__1,2)Seq_1,Pk,Vlsr,n_Dist,Dist,HI,n_Dist1,Dist1
c ..............Just test output...........
write(6,2)Seq_1,Pk,Vlsr,n_Dist,Dist,HI,n_Dist1,Dist1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Clump masses based on clump and cloud distance
* determinations
C Format for file interpretation
3 format(I3,1X,F8.1,1X,F8.1)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,132
read(1,'(A21)')ar__2
read(ar__2,3)Seq_2,Mclp,Mcld
if(ar__2(14:21) .EQ. '') Mcld = rNULL__
c ..............Just test output...........
write(6,3)Seq_2,Mclp,Mcld
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table8.dat' ! Sources of emission probably associated with
* dust clumps
C Format for file interpretation
4 format(I3,1X,A64)
C Effective file loading
open(unit=1,status='old',file=
+'table8.dat')
write(6,*) '....Loading file: table8.dat'
do i__=1,132
read(1,'(A68)')ar__3
read(ar__3,4)Seq_3,Assoc
c ..............Just test output...........
write(6,4)Seq_3,Assoc
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end