Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/606/929 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-20
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/ApJ/606/929 IR to mm observations of IRAS 18317-0757 (Hunter+, 2004)
*================================================================================
*IRAS 18317-0757: a cluster of embedded massive stars and protostars.
* Hunter T.R., Zhang Q., Sridharan T.K.
* <Astrophys. J., 606, 929-942 (2004)>
* =2004ApJ...606..929H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Observed emission properties of submillimeter
clumps
integer*4 nr__
parameter (nr__=7) ! Number of records
character*88 ar__ ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000.0
real*8 DEdeg ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*8 Source ! Source name (1)
integer*4 RAh ! (h) ? Right ascension (J2000.0)
integer*4 RAm ! (min) ? Right ascension (J2000.0)
real*4 RAs ! (s) ? Right ascension (J2000.0)
character*1 DE_ ! Declination sign (J2000.0)
integer*4 DEd ! (deg) ? Declination (J2000.0)
integer*4 DEm ! (arcmin) ? Declination (J2000.0)
integer*4 DEs ! (arcsec) ? Declination (J2000.0)
integer*4 S350um ! (Jy) Flux density at 350{mu}m, within 22" aperture
integer*4 e_S350um ! (Jy) rms uncertainty on S350um
character*1 l_S2_7mm ! Limit flag on S2.7mm
* (upper limits are 3{sigma})
real*4 S2_7mm ! (Jy) Flux density at 2.7mm, within 22" aperture
real*4 e_S2_7mm ! (Jy) ? rms uncertainty on S2.7mm
integer*4 Mass ! (solMass) Mass (2)
integer*4 e_Mass ! (solMass) rms uncertainty on Mass
real*4 logNH ! ([cm-2]) ? Hydrogen column density (3)
real*4 e_logNH ! ([cm-2]) ? rms uncertainty on logNH
integer*4 AV ! [52/144]? Extinction in V band, in magnitudes,
* AV=NH/(4*10^21^) (4)
real*4 AK ! (mag) ? Extinction in K band, AK=0.112*AV (4)
*Note (1): Clumps are identified as [HCW2000] IRAS 18317-0757 SMM N in Simbad.
* "Total" represents the total flux including extended emission within
* dotted region of Fig.2.
*Note (2): Mass, Assuming T=25K and grain emissivity Q=1.0x10^-4^ at 350um
* (Hildebrand, 1983QJRAS..24..267H)
*Note (3): Hydrogen column density Assuming uniform emission of diameter 11"
* (0.25pc).
*Note (4): Extinction to a star at the center of the dust core, i.e.,
* half the column density, reduced by a factor of 2 to more accurately
* estimate the extinction toward a young star at the center of the
* clump, rather than behind it.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Position and mass of C^18^O (1-0) clumps
integer*4 nr__1
parameter (nr__1=26) ! Number of records
character*77 ar__1 ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000.0
real*8 DEdeg_1 ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 C18O ! Sequential number, [HZS2004] C18O NN
integer*4 RAh_1 ! (h) Right ascension (J2000.0)
integer*4 RAm_1 ! (min) Right ascension (J2000.0)
real*4 RAs_1 ! (s) Right ascension (J2000.0)
character*1 DE__1 ! Declination sign (J2000.0)
integer*4 DEd_1 ! (deg) Declination (J2000.0)
integer*4 DEm_1 ! (arcmin) Declination (J2000.0)
real*4 DEs_1 ! (arcsec) Declination (J2000.0)
real*4 Emi ! (Jy.km/s) Emission
real*4 logN_C18O ! ([cm-2]) C^18^O column density
real*4 AK_1 ! (mag) Extinction in K band
integer*4 MH2 ! (solMass) H_2_ mass
real*4 Vel ! (km/s) Velocity
real*4 e_Vel ! (km/s) rms uncertainty on Vel
real*4 PFlux ! (Jy) Peak flux, in Jy/beam
real*4 e_PFlux ! (Jy) rms uncertainty on PFlux, in Jy/beam
real*4 Width ! (km/s) Line width
real*4 e_Width ! (km/s) rms uncertainty on Width
integer*4 Mvirial ! (solMass) Virial mass (1)
*Note (1):
* ---------------------------
* Emission MH2 Mvirial
* ---------------------------
* Total clump component 352 2930 2915
* Extended component 527 4410
* Total emission 879 7340
* ---------------------------
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! Stars detected in all three 2MASS bands
integer*4 nr__2
parameter (nr__2=44) ! Number of records
character*23 ar__2 ! Full-size record
integer*4 Star ! Star number given in Figure 12 and 13,
* [HZS2004] Star NNN
character*1 f_Star ! [a] Flag on Star (1)
character*16 v2MASS ! The 2MASS PSC name
*Note (1): a: Stars with A_V_>10, according to the color-color diagram
* shown in Figure 12.
C=============================================================================
C Loading file 'table1.dat' ! Observed emission properties of submillimeter
* clumps
C Format for file interpretation
1 format(
+ A8,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,I3,1X,I2,1X,A1,
+ F5.3,1X,F4.2,1X,I4,1X,I3,1X,F5.2,1X,F4.2,1X,I3,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,7
read(1,'(A88)')ar__
read(ar__,1)
+ Source,RAh,RAm,RAs,DE_,DEd,DEm,DEs,S350um,e_S350um,l_S2_7mm,
+ S2_7mm,e_S2_7mm,Mass,e_Mass,logNH,e_logNH,AV,AK
if(ar__(10:11) .EQ. '') RAh = iNULL__
if(ar__(13:14) .EQ. '') RAm = iNULL__
if(ar__(16:19) .EQ. '') RAs = rNULL__
if(ar__(22:23) .EQ. '') DEd = iNULL__
if(ar__(25:26) .EQ. '') DEm = iNULL__
if(ar__(28:29) .EQ. '') DEs = iNULL__
if(ar__(45:48) .EQ. '') e_S2_7mm = rNULL__
if(ar__(59:63) .EQ. '') logNH = rNULL__
if(ar__(65:68) .EQ. '') e_logNH = rNULL__
if(ar__(70:72) .EQ. '') AV = iNULL__
if(ar__(74:77) .EQ. '') AK = rNULL__
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)
+ Source,RAh,RAm,RAs,DE_,DEd,DEm,DEs,S350um,e_S350um,l_S2_7mm,
+ S2_7mm,e_S2_7mm,Mass,e_Mass,logNH,e_logNH,AV,AK
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table5.dat' ! Position and mass of C^18^O (1-0) clumps
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.1,1X,F5.2,
+ 1X,F4.1,1X,I3,1X,F4.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,
+ 1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,26
read(1,'(A77)')ar__1
read(ar__1,2)
+ C18O,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Emi,logN_C18O,
+ AK_1,MH2,Vel,e_Vel,PFlux,e_PFlux,Width,e_Width,Mvirial
RAdeg_1 = rNULL__
DEdeg_1 = 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 .GT. -180) RAdeg_1=RAh_1*15.
if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
if(DEd_1 .GE. 0) DEdeg_1=DEd_1
if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ C18O,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Emi,logN_C18O,
+ AK_1,MH2,Vel,e_Vel,PFlux,e_PFlux,Width,e_Width,Mvirial
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table7.dat' ! Stars detected in all three 2MASS bands
C Format for file interpretation
3 format(I3,1X,A1,1X,A16)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,44
read(1,'(A23)')ar__2
read(ar__2,3)Star,f_Star,v2MASS
c ..............Just test output...........
write(6,3)Star,f_Star,v2MASS
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end