Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/606/929 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-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 (nr__) ! (deg) Right Ascension J2000.0
real*8 DEdeg (nr__) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
character*8 Source (nr__) ! Source name (1)
integer*4 RAh (nr__) ! (h) ? Right ascension (J2000.0)
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)
integer*4 DEs (nr__) ! (arcsec) ? Declination (J2000.0)
integer*4 S350um (nr__) ! (Jy) Flux density at 350{mu}m, within 22" aperture
integer*4 e_S350um (nr__) ! (Jy) rms uncertainty on S350um
character*1 l_S2_7mm (nr__) ! Limit flag on S2.7mm
* (upper limits are 3{sigma})
real*4 S2_7mm (nr__) ! (Jy) Flux density at 2.7mm, within 22" aperture
real*4 e_S2_7mm (nr__) ! (Jy) ? rms uncertainty on S2.7mm
integer*4 Mass (nr__) ! (solMass) Mass (2)
integer*4 e_Mass (nr__) ! (solMass) rms uncertainty on Mass
real*4 logNH (nr__) ! ([cm-2]) ? Hydrogen column density (3)
real*4 e_logNH (nr__) ! ([cm-2]) ? rms uncertainty on logNH
integer*4 AV (nr__) ! [52/144]? Extinction in V band, in magnitudes,
* AV=NH/(4*10^21^) (4)
real*4 AK (nr__) ! (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 (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 C18O (nr__1) ! Sequential number, [HZS2004] C18O NN
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000.0)
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 Emi (nr__1) ! (Jy.km/s) Emission
real*4 logN_C18O (nr__1) ! ([cm-2]) C^18^O column density
real*4 AK_1 (nr__1) ! (mag) Extinction in K band
integer*4 MH2 (nr__1) ! (solMass) H_2_ mass
real*4 Vel (nr__1) ! (km/s) Velocity
real*4 e_Vel (nr__1) ! (km/s) rms uncertainty on Vel
real*4 PFlux (nr__1) ! (Jy) Peak flux, in Jy/beam
real*4 e_PFlux (nr__1) ! (Jy) rms uncertainty on PFlux, in Jy/beam
real*4 Width (nr__1) ! (km/s) Line width
real*4 e_Width (nr__1) ! (km/s) rms uncertainty on Width
integer*4 Mvirial (nr__1) ! (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 (nr__2) ! Star number given in Figure 12 and 13,
* [HZS2004] Star NNN
character*1 f_Star (nr__2) ! [a] Flag on Star (1)
character*16 v2MASS (nr__2) ! 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(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),S350um(i__),e_S350um(i__),l_S2_7mm(i__),
+ S2_7mm(i__),e_S2_7mm(i__),Mass(i__),e_Mass(i__),logNH(i__),
+ e_logNH(i__),AV(i__),AK(i__)
if(ar__(10:11) .EQ. '') RAh(i__) = iNULL__
if(ar__(13:14) .EQ. '') RAm(i__) = iNULL__
if(ar__(16:19) .EQ. '') RAs(i__) = rNULL__
if(ar__(22:23) .EQ. '') DEd(i__) = iNULL__
if(ar__(25:26) .EQ. '') DEm(i__) = iNULL__
if(ar__(28:29) .EQ. '') DEs(i__) = iNULL__
if(ar__(45:48) .EQ. '') e_S2_7mm(i__) = rNULL__
if(ar__(59:63) .EQ. '') logNH(i__) = rNULL__
if(ar__(65:68) .EQ. '') e_logNH(i__) = rNULL__
if(ar__(70:72) .EQ. '') AV(i__) = iNULL__
if(ar__(74:77) .EQ. '') AK(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)
+ Source(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),S350um(i__),e_S350um(i__),l_S2_7mm(i__),
+ S2_7mm(i__),e_S2_7mm(i__),Mass(i__),e_Mass(i__),logNH(i__),
+ e_logNH(i__),AV(i__),AK(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 '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(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Emi(i__),logN_C18O(i__),
+ AK_1(i__),MH2(i__),Vel(i__),e_Vel(i__),PFlux(i__),
+ e_PFlux(i__),Width(i__),e_Width(i__),Mvirial(i__)
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)
+ C18O(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),Emi(i__),logN_C18O(i__),
+ AK_1(i__),MH2(i__),Vel(i__),e_Vel(i__),PFlux(i__),
+ e_PFlux(i__),Width(i__),e_Width(i__),Mvirial(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
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(i__),f_Star(i__),v2MASS(i__)
c ..............Just test output...........
write(6,3)Star(i__),f_Star(i__),v2MASS(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end