Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/703/736 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/703/736 Clump properties in the LMC 30 Dor region (Pineda+, 2009) *================================================================================ *The influence of far-ultraviolet radiation on the properties of molecular clouds *in the 30 Dor region of the Large Magellanic Cloud. * Pineda J.L., Ott J., Klein U., Wong T., Muller E., Hughes A. * <Astrophys. J., 703, 736-751 (2009)> * =2009ApJ...703..736P C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Clump properties in the 30 Dor molecular ridge integer*4 nr__ parameter (nr__=67) ! Number of records character*84 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 ! [1/67] Clump number * (<[POK2009] NN> in Simbad) integer*4 RAh ! (h) Hour of right ascension (J2000) integer*4 RAm ! (min) Minute of right ascension (J2000) real*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) real*4 DEs ! (arcsec) Arcsecond of declination (J2000) real*4 Vlsr ! (km/s) LSR velocity real*4 DelV ! (km/s) FWHM of the observed line profile * ({Delta}{nu}'); deconvolved by the * instrumental resolution real*4 e_DelV ! (km/s) DelV uncertainty real*4 Rad ! (pc) Clump radius; deconvolved by the * instrumental resolution real*4 e_Rad ! (pc) Rad uncertainty real*4 Tmb ! (K) Brightness temperature real*4 e_Tmb ! (K) Tmb uncertainty real*4 log_LCO ! (K.km/s) CO luminosity (1) real*4 log_Mvir ! (Msun) Virial mass (1) real*4 XCO ! (10+20cm-2/(K.km/s)) CO-to-H2 conversion factor (X_CO_) (2) real*4 e_XCO ! (10+20cm-2/(K.km/s)) XCO uncertainty real*4 Chi ! ([-]) Strength of the FUV radiation field (3) *Note (1): The CO luminosities and virial masses have typically errors of 50%. *Note (2): We estimate the value of X_CO_ for clumps in the 30 Dor molecular * ridge assuming that they are in virial equilibrium. In this case, * X_CO_ is calculated dividing the clump's virial mass -which we assume * is an accurate measure of the total mass of H2 present- by its CO * luminosity (see section 3.1 for further details). *Note (3): Strength of the FUV radiation field in units of the Draine * (1978ApJS...36..595D) field ({chi}_0_). They have typical errors of * 20%, as this is the accuracy of the HIRES/IRAS images used to derive * this quantity (see section 3.2). C============================================================================= C Loading file 'table1.dat' ! Clump properties in the 30 Dor molecular ridge C Format for file interpretation 1 format( + I2,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.1,1X,F4.1, + 1X,F3.1,1X,F4.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X,F3.1,1X, + F4.1,1X,F4.1,1X,F5.1) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,67 read(1,'(A84)')ar__ read(ar__,1) + Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Vlsr,DelV,e_DelV,Rad,e_Rad, + Tmb,e_Tmb,log_LCO,log_Mvir,XCO,e_XCO,Chi 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,DelV,e_DelV,Rad,e_Rad, + Tmb,e_Tmb,log_LCO,log_Mvir,XCO,e_XCO,Chi write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg c .......End.of.Just test output........... end do close(1) C============================================================================= stop end