Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/644/990 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-Mar-28 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/644/990 Sub-mm clumps at 450 and 850{mu}m in M17 (Reid+, 2006) *================================================================================ *High-mass star formation. II. The mass function of submillimeter clumps in M17. * Reid M.A., Wilson C.D. * <Astrophys. J., 644, 990-1005 (2006)> * =2006ApJ...644..990R C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Properties of the 850um Clumps integer*4 nr__ parameter (nr__=121) ! Number of records character*95 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*7 v_RW2006b_ ! Name SNN NNN (1) character*1 m__RW2006b_ ! [ABC] Multiplicity index for clump (1) character*1 n__RW2006b_ ! [e] Note on Name (2) integer*4 RAh ! (h) Right ascension (J2000) integer*4 RAm ! (min) Right ascension (J2000) real*4 RAs ! (s) Right ascension (J2000) character*1 DE_ ! Declination sign (J2000) integer*4 DEd ! (deg) Declination (J2000) integer*4 DEm ! (arcmin) Declination (J2000) integer*4 DEs ! (arcsec) Declination (J2000) real*4 Reff ! (pc) Effective radius real*4 Speak ! (Jy) Peak flux density at 850um for table1 and * 450um for table2, in Jy/beam real*4 e_Speak ! (Jy) rms uncertainty on Speak (3) real*4 Sint ! (Jy) Integrated flux density at 850um for table1 * and 450um for table2 real*4 e_Sint ! (Jy) rms uncertainty on Sint (3) real*4 alpha ! ?=- Spectral index * (only in table1) (4) integer*4 Td ! (K) ?=- Dust temperature (only in table1) (5) real*4 M_30K ! (solMass) ?=- Mass calculated with fixed Td (Td=30K) real*4 e_M_30K ! (solMass) ? rms uncertainty on M(30K) (3) real*4 M_Td ! (solMass) ?=- Mass calculated with estimated Td * (only in table1) real*4 e_M_Td ! (solMass) ? rms uncertainty on M(Td) (3) * (only in table1) integer*4 Npsc ! Number of MSX point sources contained * within the clump's 0.5Speak contour *Note (1): Names in Simbad are [RW2006b] SMM NNN in table1 and * [RW2006b] SMM NNNA in table2. * The names of the 450um clumps have been set to reflect the names of * the 850um clumps in which their peaks appear. Thus, clumps SMM 21A-21C * are the three 450um clumps whose peaks appear within the * boundaries of 850um clump SMM 21. *Note (2): "e" denotes a clump to which corrections for free-free emission * have been applied in the calculation of the spectral index, dust * temperature, and masses. The free-free correction has not been applied * to the peak and integrated fluxes listed here. *Note (3): The uncertainties stated in this table are composed of the * uncertainties in the gain calibration, the sky opacities, and the * corrections due to the error beam. These uncertainties are typically * significantly larger than the random measurement errors associated * with the rms flux of the map. The exception is the peak flux, where * the random error of sigma=0.027Jy/beam (table1) or sigma=0.32Jy/beam * (table2) dominates the systematic error for the clumps with lower peak * fluxes. *Note (4): The systematic uncertainty in the spectral index, alpha, is 13%. * These systematic uncertainties, which are composed of the * uncertainties in the gain calibration and sky opacities, dominate the * random errors on the spectral index. *Note (5): See Sect. 3.2 for a discussion of the uncertainties in the * temperatures. Temperatures are omitted where high spectral index makes * them incalculable or where no reliable spectral index can be * calculated (see text). All of the temperatures above 40K should be * considered highly uncertain, indicating only that a clump is probably * hot. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Properties of the 450um Clumps integer*4 nr__1 parameter (nr__1=101) ! Number of records character*95 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) character*7 v_RW2006b__1 ! Name SNN NNN (1) character*1 m__RW2006b__1 ! [ABC] Multiplicity index for clump (1) character*1 n__RW2006b__1 ! [e] Note on Name (2) integer*4 RAh_1 ! (h) Right ascension (J2000) integer*4 RAm_1 ! (min) Right ascension (J2000) real*4 RAs_1 ! (s) Right ascension (J2000) character*1 DE__1 ! Declination sign (J2000) integer*4 DEd_1 ! (deg) Declination (J2000) integer*4 DEm_1 ! (arcmin) Declination (J2000) integer*4 DEs_1 ! (arcsec) Declination (J2000) real*4 Reff_1 ! (pc) Effective radius real*4 Speak_1 ! (Jy) Peak flux density at 850um for table1 and * 450um for table2, in Jy/beam real*4 e_Speak_1 ! (Jy) rms uncertainty on Speak (3) real*4 Sint_1 ! (Jy) Integrated flux density at 850um for table1 * and 450um for table2 real*4 e_Sint_1 ! (Jy) rms uncertainty on Sint (3) real*4 alpha_1 ! ?=- Spectral index * (only in table1) (4) integer*4 Td_1 ! (K) ?=- Dust temperature (only in table1) (5) real*4 M_30K_1 ! (solMass) ?=- Mass calculated with fixed Td (Td=30K) real*4 e_M_30K_1 ! (solMass) ? rms uncertainty on M(30K) (3) real*4 M_Td_1 ! (solMass) ?=- Mass calculated with estimated Td * (only in table1) real*4 e_M_Td_1 ! (solMass) ? rms uncertainty on M(Td) (3) * (only in table1) integer*4 Npsc_1 ! Number of MSX point sources contained * within the clump's 0.5Speak contour *Note (1): Names in Simbad are [RW2006b] SMM NNN in table1 and * [RW2006b] SMM NNNA in table2. * The names of the 450um clumps have been set to reflect the names of * the 850um clumps in which their peaks appear. Thus, clumps SMM 21A-21C * are the three 450um clumps whose peaks appear within the * boundaries of 850um clump SMM 21. *Note (2): "e" denotes a clump to which corrections for free-free emission * have been applied in the calculation of the spectral index, dust * temperature, and masses. The free-free correction has not been applied * to the peak and integrated fluxes listed here. *Note (3): The uncertainties stated in this table are composed of the * uncertainties in the gain calibration, the sky opacities, and the * corrections due to the error beam. These uncertainties are typically * significantly larger than the random measurement errors associated * with the rms flux of the map. The exception is the peak flux, where * the random error of sigma=0.027Jy/beam (table1) or sigma=0.32Jy/beam * (table2) dominates the systematic error for the clumps with lower peak * fluxes. *Note (4): The systematic uncertainty in the spectral index, alpha, is 13%. * These systematic uncertainties, which are composed of the * uncertainties in the gain calibration and sky opacities, dominate the * random errors on the spectral index. *Note (5): See Sect. 3.2 for a discussion of the uncertainties in the * temperatures. Temperatures are omitted where high spectral index makes * them incalculable or where no reliable spectral index can be * calculated (see text). All of the temperatures above 40K should be * considered highly uncertain, indicating only that a clump is probably * hot. C============================================================================= C Loading file 'table1.dat' ! Properties of the 850um Clumps C Format for file interpretation 1 format( + A7,A1,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F4.2,1X, + F5.2,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,I3,1X,F6.2,1X,F5.2,1X, + F6.2,1X,F5.2,1X,I1) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,121 read(1,'(A95)')ar__ read(ar__,1) + v_RW2006b_,m__RW2006b_,n__RW2006b_,RAh,RAm,RAs,DE_,DEd,DEm, + DEs,Reff,Speak,e_Speak,Sint,e_Sint,alpha,Td,M_30K,e_M_30K, + M_Td,e_M_Td,Npsc if (idig(ar__(60:63)).EQ.0) alpha = rNULL__ if (Td .EQ. 45) Td = iNULL__ if (idig(ar__(69:74)).EQ.0) M_30K = rNULL__ if(ar__(76:80) .EQ. '') e_M_30K = rNULL__ if (idig(ar__(82:87)).EQ.0) M_Td = rNULL__ if(ar__(89:93) .EQ. '') e_M_Td = rNULL__ 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) + v_RW2006b_,m__RW2006b_,n__RW2006b_,RAh,RAm,RAs,DE_,DEd,DEm, + DEs,Reff,Speak,e_Speak,Sint,e_Sint,alpha,Td,M_30K,e_M_30K, + M_Td,e_M_Td,Npsc 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 the 450um Clumps C Format for file interpretation 2 format( + A7,A1,A1,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F4.2,1X, + F5.2,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,I3,1X,F6.2,1X,F5.2,1X, + F6.2,1X,F5.2,1X,I1) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,101 read(1,'(A95)')ar__1 read(ar__1,2) + v_RW2006b__1,m__RW2006b__1,n__RW2006b__1,RAh_1,RAm_1,RAs_1, + DE__1,DEd_1,DEm_1,DEs_1,Reff_1,Speak_1,e_Speak_1,Sint_1, + e_Sint_1,alpha_1,Td_1,M_30K_1,e_M_30K_1,M_Td_1,e_M_Td_1,Npsc_1 if (idig(ar__1(60:63)).EQ.0) alpha_1 = rNULL__ if (Td_1 .EQ. 45) Td_1 = iNULL__ if (idig(ar__1(69:74)).EQ.0) M_30K_1 = rNULL__ if(ar__1(76:80) .EQ. '') e_M_30K_1 = rNULL__ if (idig(ar__1(82:87)).EQ.0) M_Td_1 = rNULL__ if(ar__1(89:93) .EQ. '') e_M_Td_1 = rNULL__ 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) + v_RW2006b__1,m__RW2006b__1,n__RW2006b__1,RAh_1,RAm_1,RAs_1, + DE__1,DEd_1,DEm_1,DEs_1,Reff_1,Speak_1,e_Speak_1,Sint_1, + e_Sint_1,alpha_1,Td_1,M_30K_1,e_M_30K_1,M_Td_1,e_M_Td_1,Npsc_1 write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1 c .......End.of.Just test output........... end do close(1) C============================================================================= stop end C Locate position of first digit in string; or return 0 integer function idig(c) character*(*) c character*1 c1 integer lc,i lc=len(c) idig=0 do i=1,lc if(c(i:i).ne.' ') go to 1 end do 1 if(i.gt.lc) return c1=c(i:i) if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1 if(i.gt.lc) return c1=c(i:i) if(c1.ge.'0'.and.c1.le.'9') idig=i return end