Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/642/972 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-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/642/972 IR photometry of a star-forming core in NGC 2264 (Young+, 2006) *================================================================================ *Spitzer and Magellan observations of NGC 2264: a remarkable star-forming core *near IRS 2. * Young E.T., Teixeira P.S., Lada C.J., Muzerolle J., Persson S.E., * Murphy D.C., Siegler N., Marengo M., Krause O., Mainzer A.K. * <Astrophys. J., 642, 972-978 (2006)> * =2006ApJ...642..972Y C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Sources in the IRAS 12 S1 core integer*4 nr__ parameter (nr__=110) ! Number of records character*93 ar__ ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0 real*8 DEdeg (nr__) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) integer*4 v_YTL2006_ (nr__) ! Star ID (1) character*1 n__YTL2006_(nr__) ! [d] "d" for V608 Mon (2) integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000.0) integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000.0) real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000.0) character*1 DE_ (nr__) ! Sign of the Declination (J2000.0) integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000.0) integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000.0) real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000.0) character*16 v2MASSJ (nr__) ! 2MASS name (HHMMSSss+DDMMSSs) real*4 Jmag (nr__) ! (mag) ? PANIC J band magnitude (3) real*4 Hmag (nr__) ! (mag) ? PANIC H band magnitude (3) real*4 Kmag (nr__) ! (mag) ? PANIC K band magnitude (3) real*4 v3_6mag (nr__) ! (mag) ? Magnitude at 3.6{mu}m real*4 v4_5mag (nr__) ! (mag) ? Magnitude at 4.5{mu}m real*4 v5_8mag (nr__) ! (mag) ? Magnitude at 5.8{mu}m real*4 v8_0mag (nr__) ! (mag) ? Magnitude at 8.0{mu}m real*4 v24mag (nr__) ! (mag) ? Magnitude at 24{mu}m character*1 f_24mag (nr__) ! [abce] Confusion flag on 24mag (4) *Note (1): Sources detected only in the Spitzer images have numbers>1000 *Note (2): "d" indicates that source 54 is V608 Mon. *Note (3): Sources brighter than Jmag=12 Hmag=12 and Kmag=11 are saturated * and we substitute 2MASS photometry. *Note (4): Flag on 24mag is defined as follows: * a = The 24{mu}m flux is confused and contains contributions from source 10. * b = The 24{mu}m flux is confused and contains contributions from * sources 30, 32, 34, 35, 37, 40, and 41. * c = The 24{mu}m flux is confused and contains contributions from * sources 47 and 49. * e = The 24{mu}m flux is confused and contains contributions from the * nearby source 63, which has the more steeply rising SED. C============================================================================= C Loading file 'table1.dat' ! Sources in the IRAS 12 S1 core C Format for file interpretation 1 format( + I4,A1,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A16,1X,F5.2, + 1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.2,A1) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,110 read(1,'(A93)')ar__ read(ar__,1) + v_YTL2006_(i__),n__YTL2006_(i__),RAh(i__),RAm(i__),RAs(i__), + DE_(i__),DEd(i__),DEm(i__),DEs(i__),v2MASSJ(i__),Jmag(i__), + Hmag(i__),Kmag(i__),v3_6mag(i__),v4_5mag(i__),v5_8mag(i__), + v8_0mag(i__),v24mag(i__),f_24mag(i__) if(ar__(47:51) .EQ. '') Jmag(i__) = rNULL__ if(ar__(53:57) .EQ. '') Hmag(i__) = rNULL__ if(ar__(59:63) .EQ. '') Kmag(i__) = rNULL__ if(ar__(65:69) .EQ. '') v3_6mag(i__) = rNULL__ if(ar__(71:75) .EQ. '') v4_5mag(i__) = rNULL__ if(ar__(77:81) .EQ. '') v5_8mag(i__) = rNULL__ if(ar__(83:87) .EQ. '') v8_0mag(i__) = rNULL__ if(ar__(89:92) .EQ. '') v24mag(i__) = rNULL__ 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) + v_YTL2006_(i__),n__YTL2006_(i__),RAh(i__),RAm(i__),RAs(i__), + DE_(i__),DEd(i__),DEm(i__),DEs(i__),v2MASSJ(i__),Jmag(i__), + Hmag(i__),Kmag(i__),v3_6mag(i__),v4_5mag(i__),v5_8mag(i__), + v8_0mag(i__),v24mag(i__),f_24mag(i__) write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end