Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/732/101 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-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/ApJ/732/101 C^18^O cores in the S140 cloud (Ikeda+, 2011)
*================================================================================
*Similarity between the C^18^O (J = 1-0) core mass function and the initial mass
*function (IMF) in the S140 region.
* Ikeda N., Kitamura Y.
* <Astrophys. J., 732, 101 (2011)>
* =2011ApJ...732..101I
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Physical properties of the C^18^O cores in the
S140 cloud
integer*4 nr__
parameter (nr__=123) ! Number of records
character*69 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Seq (nr__) ! Running sequence number
integer*4 RAh (nr__) ! (h) Hour of right ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of right ascension (J2000)
integer*4 RAs (nr__) ! (s) Second of right ascension (J2000)
character*1 DE_ (nr__) ! Sign of declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of declination (J2000)
integer*4 DEs (nr__) ! (arcsec) Arcsecond of declination (J2000)
real*4 Vlsr (nr__) ! (km/s) LSR velocity
real*4 TA (nr__) ! (K) Antenna peak temperature
real*4 Rad (nr__) ! (arcsec) Beam-deconvolved radius R_core_ in arcsec
real*4 Rc (nr__) ! (pc) Beam-deconvolved radius R_core_ in parsec (1)
real*4 dv_c (nr__) ! (km/s) Velocity width in FWHM corrected for the
* spectrometer resolution (dv_core_) (2)
real*4 Mc (nr__) ! (Msun) LTE mass M_core_ (3)
real*4 Mv (nr__) ! (Msun) Virial mass M_vir_ (3)
real*4 Mv_Mc (nr__) ! Ratio virial mass/LTE mass (3)
real*4 n (nr__) ! (10+3cm-3) Mean density of the C^18^O core (3)
*Note (1): The typical uncertainty for R_core_ is 0.04pc, derived from the
* uncertainty in the estimation of the core projected area.
*Note (2): The typical uncertainty for dv_core_ is 0.13km/s, corresponding
* to the velocity resolution.
*Note (3): The typical uncertainty for M_core_ is a factor of three (see
* text). For M_vir_, a factor of three, derived from the uncertainties
* in R_core_ and dv_core_. For M_vir_/M_core_, a factor of four, derived
* from the uncertainties in M_core_ and M_vir_. For n, a factor of four,
* derived from the uncertainties in R_core_ and M_core_.
C=============================================================================
C Loading file 'table1.dat' ! Physical properties of the C^18^O cores in the
* S140 cloud
C Format for file interpretation
1 format(
+ I3,1X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,3X,F4.1,1X,F4.2,1X,
+ F5.1,1X,F4.2,1X,F4.2,1X,F5.1,1X,F4.1,1X,F3.1,1X,F3.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,123
read(1,'(A69)')ar__
read(ar__,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vlsr(i__),TA(i__),Rad(i__),Rc(i__),
+ dv_c(i__),Mc(i__),Mv(i__),Mv_Mc(i__),n(i__)
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)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vlsr(i__),TA(i__),Rad(i__),Rc(i__),
+ dv_c(i__),Mc(i__),Mv(i__),Mv_Mc(i__),n(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end