Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/230/17 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-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/ApJS/230/17 CO obs. of MCs in the Extreme Outer Galaxy region (Sun+, 2017)
*================================================================================
*Molecular clouds in the Extreme Outer Galaxy between l=34.75{deg} to 45.25{deg}.
* Sun Y., Su Y., Zhang S.-B., Xu Y., Chen X.-P., Yang J., Jiang Z.-B.,
* Fang M.
* <Astrophys. J. Suppl. Ser., 230, 17-17 (2017)>
* =2017ApJS..230...17S (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Parameters of molecular clouds (MCs) derived
by ^12^CO(1-0)
integer*4 nr__
parameter (nr__=174) ! Number of records
character*83 ar__ ! Full-size record
character*13 MWISP ! Cloud identifier (GLL.lll+B.bbb) (1)
character*2 f_MWISP ! Flag on MWISP (2)
real*4 VLSR ! (km/s) [-74/-45] Local Standard of Rest
* velocity (3)
real*4 DelV ! (km/s) [0.5/5.3] Line width Full-Width
* at Half-Maximum (3)
real*4 Int ! (K.km/s) [1/21] Integrated ^12^CO intensity (3)
real*4 Tpk ! (K) [1/7] Peak intensity (3)
real*4 Area ! (arcmin2) [0.9/27] Angular area defined by
* 3{sigma} limits
real*4 Dist ! (kpc) [16.6/20] Heliocentric distance (4)
real*4 R ! (kpc) [11.6/14.1] Galactocentric distance (4)
real*4 Z ! (kpc) [-0.5/1.5] Vertical scale height (5)
real*4 Rad ! (pc) [1/15] Cloud radius after
* beam deconvolution
real*4 Mass ! (10+2Msun) [1/139] Cloud mass (6)
real*4 Mvir ! (10+2Msun) [1/691] Virial mass
real*4 Sigma ! (Msun/pc2) [5.5/29.2] Molecular gas surface density
*Note (1): Designated as MWISP (for CO survey project name: Milky Way Imaging
* Scroll Painting) followed by the Galactic longitude and latitude
* coordinates of the peak of the emission in degrees.
*Note (2): Flag as follows:
* * = Also listed in Su et al. (2016, J/ApJ/828/59).
* d = Sources with V_LSR_>-1.6l+13.2km/s probably lie in the Outer arm.
*Note (3): For the single Gaussian fitting results of the brightest
* CO spectrum of the MCs.
*Note (4): Assuming the rotation curve and Galactic parameters obtained
* by Reid et al. (2014, J/ApJ/783/130).
*Note (5): Defined by Z=Dist*sin(b) where b is the Galactic latitude.
*Note (6): Calculated using X=2.0x10^20^cm^-2^ (K.km/s)^-1^
* (Bolatto et al. 2013ARA&A..51..207B).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Molecular clouds marginally detected by this study
integer*4 nr__1
parameter (nr__1=23) ! Number of records
character*19 ar__1 ! Full-size record
character*13 Name ! Cloud identifier
real*4 VLSR_1 ! (km/s) [-69/-48] Local Standard of Rest velocity
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Parameters of molecular clouds derived by ^13^CO(1-0)
integer*4 nr__2
parameter (nr__2=35) ! Number of records
character*64 ar__2 ! Full-size record
character*13 MWISP_1 ! Cloud identifier (GLL.lll+B.bbb)
character*1 f_MWISP_1 ! [t] t: sources belong to the same
* cloud MWISP G37.175+0.792
real*4 VLSR_2 ! (km/s) [-64/-45] Local Standard of Rest velocity (1)
real*4 e_VLSR ! (km/s) [0.04/0.2] VLSR uncertainty
real*4 DelV_1 ! (km/s) [0.5/4.5] Line width Full-Width
* at Half-Maximum (1)
real*4 e_DelV ! (km/s) [0.1/0.7] DelV uncertainty
real*4 Int_1 ! (K.km/s) [0.3/2.8] Integrated ^13^CO intensity (1)
real*4 e_Int ! (K.km/s) [0.06/0.4] Int uncertainty
real*4 Tpk_1 ! (K) [0.3/1.3] Peak intensity (1)
real*4 v12CO_13CO ! [2.8/14.3]? Integrated intensity ratio of
* ^12^C0 and ^13^CO
real*4 rms ! (K) [0.1/0.3] rms level of each detection with a
* velocity resolution of 0.166km/s (2)
*Note (1): The single Gaussian fitting results of the brightest ^13^CO spectrum
* of the molecular clouds.
*Note (2): Those with values larger than 0.2K are the rms values of a single
* pixel; otherwise, the rms was averaged over nine pixels.
C=============================================================================
C Loading file 'table1.dat' ! Parameters of molecular clouds (MCs) derived
* by ^12^CO(1-0)
C Format for file interpretation
1 format(
+ 6X,A13,1X,A2,1X,F5.1,1X,F3.1,1X,F4.1,1X,F3.1,1X,F4.1,1X,F4.1,
+ 1X,F4.1,1X,F4.1,1X,F4.1,1X,F5.1,1X,F5.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,174
read(1,'(A83)')ar__
read(ar__,1)
+ MWISP,f_MWISP,VLSR,DelV,Int,Tpk,Area,Dist,R,Z,Rad,Mass,Mvir,
+ Sigma
c ..............Just test output...........
write(6,1)
+ MWISP,f_MWISP,VLSR,DelV,Int,Tpk,Area,Dist,R,Z,Rad,Mass,Mvir,
+ Sigma
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Molecular clouds marginally detected by this study
C Format for file interpretation
2 format(A13,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,23
read(1,'(A19)')ar__1
read(ar__1,2)Name,VLSR_1
c ..............Just test output...........
write(6,2)Name,VLSR_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Parameters of molecular clouds derived by ^13^CO(1-0)
C Format for file interpretation
3 format(
+ 6X,A13,1X,A1,1X,F5.1,1X,F4.2,1X,F3.1,1X,F4.2,1X,F3.1,1X,F4.2,
+ 1X,F3.1,1X,F4.1,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,35
read(1,'(A64)')ar__2
read(ar__2,3)
+ MWISP_1,f_MWISP_1,VLSR_2,e_VLSR,DelV_1,e_DelV,Int_1,e_Int,
+ Tpk_1,v12CO_13CO,rms
if(ar__2(56:59) .EQ. '') v12CO_13CO = rNULL__
c ..............Just test output...........
write(6,3)
+ MWISP_1,f_MWISP_1,VLSR_2,e_VLSR,DelV_1,e_DelV,Int_1,e_Int,
+ Tpk_1,v12CO_13CO,rms
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end