Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/646/1009 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-18
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/646/1009 Structures of dust in Perseus molecular cloud (Kirk+, 2006)
*================================================================================
*The large- and small-scale structures of dust in the star-forming
*Perseus molecular cloud.
* Kirk H., Johnstone D., Di Francesco J.
* <Astrophys. J., 646, 1009-1023 (2006)>
* =2006ApJ...646.1009K
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Properties of Submillimeter Clumps in Perseus
integer*4 nr__
parameter (nr__=58) ! Number of records
character*85 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)
character*12 SMM ! Name from J2000 positions (HHMMSS+DDMMm)
* [KJD2006] SMM JHHMMmm+DDMMm in Simbad
integer*4 RAh ! (h) Peak flux right ascension (J2000) (1)
integer*4 RAm ! (min) Peak flux right ascension (J2000) (1)
real*4 RAs ! (s) Peak flux right ascension (J2000) (1)
character*1 DE_ ! Peak flux declination sign (J2000) (1)
integer*4 DEd ! (deg) Peak flux declination (J2000) (1)
integer*4 DEm ! (arcmin) Peak flux declination (J2000) (1)
real*4 DEs ! (arcsec) Peak flux declination (J2000) (1)
real*4 f0 ! (Jy) Peak flux at 850um (in Jy/beam)
real*4 S850um ! (Jy) Total flux at 850um (2)
real*4 Reff ! (arcsec) Radius derived from clfind (Williams et al.
* 1994, Cat. <J/ApJ/428/693>)
real*4 Mass ! (solMass) Mass derived from the total flux assuming
* Td=15K and k850=0.02cm^2^/g, d=250pc
real*4 Conc ! Concentration from Bonnor-Ebert modeling
real*4 Temp ! (K) Temperature from Bonnor-Ebert modeling
real*4 MBE ! (solMass) Mass from Bonnor-Ebert modeling
real*4 logNc ! ([cm-3]) Central number density from Bonnor-Ebert
* modeling
real*4 logP_k ! ([cm-3.K]) External pressure derived from Bonnor-Ebert
* modeling, log(P_ext_/k)
integer*4 v_HRF2005_ ! ? Best corresponding submillimeter clump in
* Hatchell et al. (2005, Cat. <J/A+A/440/151>)
* number (3)
integer*4 EC ! Closest corresponding extinction core number,
* [KJD2006] EC NN in Simbad, in table2
*Note (1): Position of peak flux within clump (accurate to 6").
*Note (2): Note a beam size of 19.9" is used for the peak flux.
*Note (3): More clumps were identified in their survey, as discussed in
* Section 4.1.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Properties of Extinction Cores in Perseus
integer*4 nr__1
parameter (nr__1=39) ! Number of records
character*59 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 EC_1 ! Identification number,
* [KJD2006] EC NN in Simbad
integer*4 RAh_1 ! (h) Peak flux right ascension (J2000) (1)
integer*4 RAm_1 ! (min) Peak flux right ascension (J2000) (1)
real*4 RAs_1 ! (s) Peak flux right ascension (J2000) (1)
character*1 DE__1 ! Peak flux declination sign (J2000) (1)
integer*4 DEd_1 ! (deg) Peak flux declination (J2000) (1)
integer*4 DEm_1 ! (arcmin) Peak flux declination (J2000) (1)
real*4 DEs_1 ! (arcsec) Peak flux declination (J2000) (1)
real*4 AVpeak ! Peak extinction (2)
real*4 AVbg ! Background extinction (2)
real*4 Mass_1 ! (solMass) Mass (2)
real*4 sigmax ! (arcsec) sigma_x_ (2)
real*4 sigmay ! (arcsec) sigma_y_ (2)
real*4 v_n_ ! (10+3cm-3) Mean number density (2)
integer*4 ESC ! Associated extinction super core,
* [KJD2006] ESC NN in Simbad, in table3
*Note (1): Position of peak extinction within core (accurate to 2.5').
*Note (2): From results of Gaussian fitting
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Properties of Extinction Super Cores in Perseus
integer*4 nr__2
parameter (nr__2=11) ! Number of records
character*49 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 ! (deg) Right Ascension J2000
real*8 DEdeg_2 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 ESC_1 ! Identification number,
* [KJD2006] ESC NN in Simbad
integer*4 RAh_2 ! (h) Peak flux right ascension (J2000) (1)
integer*4 RAm_2 ! (min) Peak flux right ascension (J2000) (1)
real*4 RAs_2 ! (s) Peak flux right ascension (J2000) (1)
character*1 DE__2 ! Peak flux declination sign (J2000) (1)
integer*4 DEd_2 ! (deg) Peak flux declination (J2000) (1)
integer*4 DEm_2 ! (arcmin) Peak flux declination (J2000) (1)
real*4 DEs_2 ! (arcsec) Peak flux declination (J2000) (1)
real*4 AVpeak_1 ! Peak extinction (2)
real*4 Mass_2 ! (solMass) Mass from results (2)
real*4 Reff_1 ! (arcsec) Effective radius (2)
real*4 v_n__1 ! (10+3cm-3) Mean number density (2)
*Note (1): Position of peak extinction within core (accurate to 2.5').
*Note (2): Derived from Clumpfind (Williams et al. 1994, Cat. J/ApJ/428/693)
* with several clumps further separated.
C=============================================================================
C Loading file 'table1.dat' ! Properties of Submillimeter Clumps in Perseus
C Format for file interpretation
1 format(
+ A12,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,
+ F5.2,1X,F4.1,1X,F3.1,1X,F4.2,1X,F4.1,1X,F4.2,1X,F3.1,1X,F3.1,
+ 1X,I2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,58
read(1,'(A85)')ar__
read(ar__,1)
+ SMM,RAh,RAm,RAs,DE_,DEd,DEm,DEs,f0,S850um,Reff,Mass,Conc,Temp,
+ MBE,logNc,logP_k,v_HRF2005_,EC
if(ar__(81:82) .EQ. '') v_HRF2005_ = iNULL__
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)
+ SMM,RAh,RAm,RAs,DE_,DEd,DEm,DEs,f0,S850um,Reff,Mass,Conc,Temp,
+ MBE,logNc,logP_k,v_HRF2005_,EC
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Properties of Extinction Cores in Perseus
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F3.1,1X,F3.1,
+ 1X,F5.1,1X,F5.1,1X,F5.1,1X,F4.1,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,39
read(1,'(A59)')ar__1
read(ar__1,2)
+ EC_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,AVpeak,AVbg,
+ Mass_1,sigmax,sigmay,v_n_,ESC
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)
+ EC_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,AVpeak,AVbg,
+ Mass_1,sigmax,sigmay,v_n_,ESC
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Properties of Extinction Super Cores in Perseus
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,1X,F6.1,
+ 1X,F6.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,11
read(1,'(A49)')ar__2
read(ar__2,3)
+ ESC_1,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,AVpeak_1,
+ Mass_2,Reff_1,v_n__1
RAdeg_2 = rNULL__
DEdeg_2 = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2 .GT. -180) RAdeg_2=RAh_2*15.
if(RAm_2 .GT. -180) RAdeg_2=RAdeg_2+RAm_2/4.
if(RAs_2 .GT. -180) RAdeg_2=RAdeg_2+RAs_2/240.
if(DEd_2 .GE. 0) DEdeg_2=DEd_2
if(DEm_2 .GE. 0) DEdeg_2=DEdeg_2+DEm_2/60.
if(DEs_2 .GE. 0) DEdeg_2=DEdeg_2+DEs_2/3600.
if(DE__2.EQ.'-'.AND.DEdeg_2.GE.0) DEdeg_2=-DEdeg_2
c ..............Just test output...........
write(6,3)
+ ESC_1,RAh_2,RAm_2,RAs_2,DE__2,DEd_2,DEm_2,DEs_2,AVpeak_1,
+ Mass_2,Reff_1,v_n__1
write(6,'(6H Pos: 2F8.4)') RAdeg_2,DEdeg_2
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end