Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/732/101 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/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 ! (deg) Right Ascension J2000 real*8 DEdeg ! (deg) Declination J2000 C ---------------------------------- ! (position vector(s) in degrees) integer*4 Seq ! Running sequence number integer*4 RAh ! (h) Hour of right ascension (J2000) integer*4 RAm ! (min) Minute of right ascension (J2000) integer*4 RAs ! (s) Second of right ascension (J2000) character*1 DE_ ! Sign of declination (J2000) integer*4 DEd ! (deg) Degree of declination (J2000) integer*4 DEm ! (arcmin) Arcminute of declination (J2000) integer*4 DEs ! (arcsec) Arcsecond of declination (J2000) real*4 Vlsr ! (km/s) LSR velocity real*4 TA ! (K) Antenna peak temperature real*4 Rad ! (arcsec) Beam-deconvolved radius R_core_ in arcsec real*4 Rc ! (pc) Beam-deconvolved radius R_core_ in parsec (1) real*4 dv_c ! (km/s) Velocity width in FWHM corrected for the * spectrometer resolution (dv_core_) (2) real*4 Mc ! (Msun) LTE mass M_core_ (3) real*4 Mv ! (Msun) Virial mass M_vir_ (3) real*4 Mv_Mc ! Ratio virial mass/LTE mass (3) real*4 n ! (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,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vlsr,TA,Rad,Rc,dv_c,Mc,Mv, + Mv_Mc,n 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) + Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vlsr,TA,Rad,Rc,dv_c,Mc,Mv, + Mv_Mc,n write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg c .......End.of.Just test output........... end do close(1) C============================================================================= stop end