Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/670/428 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-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/670/428 Bubbles in the galactic disk. II. (Churchwell+, 2007) *================================================================================ *The bubbling galactic disk. II. The inner 20{deg}. * Churchwell E., Watson D.F., Povich M.S., Taylor M.G., Babler B.L., * Meade M.R., Benjamin R.A., Indebetouw R., Whitney B.A. * <Astrophys. J., 670, 428-441 (2007)> * =2007ApJ...670..428C C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Northern Bubble parameters integer*4 nr__ parameter (nr__=151) ! Number of records character*73 ar__ ! Full-size record C Position composed of: GLON GLAT character*6 v_CWP2007_ (nr__) ! Catalog name, CN NNN or CS NNN (1) real*8 GLON (nr__) ! (deg) Galactic longitude of center position real*4 GLAT (nr__) ! (deg) Galactic latitude center position real*4 Rin (nr__) ! (arcmin) Semimajor axis of the inner ellipse real*4 rin_1 (nr__) ! (arcmin) Semiminor axis of the inner ellipse real*4 Rout (nr__) ! (arcmin) Semimajor axis of the outer ellipse real*4 rout_1 (nr__) ! (arcmin) Semiminor axis of the outer ellipse real*4 Ecc (nr__) ! Eccentricity of the ellipses (2) real*4 v_R_ (nr__) ! (arcmin) Average radius of the bubble real*4 v_T_ (nr__) ! (arcmin) Average thickness of the shell character*15 MFlags (nr__) ! Morphology flags (3) *Note (1): Catalog number preceded by CN if longitude is between 10{deg} and * 0{deg}, and CS if longitude is between 360{deg} and 350{deg}. *Note (2): The centers and eccentricities of the inner and outer ellipses * are constrained to be the same. *Note (3): Morphology flags as follows: * C = complete or closed ring * B = broken or incomplete ring * CC = probable enclosed central star cluster, meaning that the stellar * density inside the ring appears to be greater than the average * stellar density outside the ring * BC = complex of two or more bubbles, that may or may not be * physically associated * MB = Bubbles that have at least one secondary bubble projected * within or on its periphery * MBm = Bubbles subsidiary to MB bubbles are labeled m(catalog number) * according to the MB bubble they are associated with * Y = Bubbles that have possible YSO(s) projected within or on its * periphery but have not formed a secondary bubble * CS = the central star(s) responsible for driving the * bubble is/are probably apparent * Fl = a flocculent or clumpy bubble structure * PN = Two bubbles that are probable planetary nebulae c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Southern Bubble parameters integer*4 nr__1 parameter (nr__1=118) ! Number of records character*73 ar__1 ! Full-size record C Position composed of: GLON GLAT character*6 v_CWP2007__1(nr__1) ! Catalog name, CN NNN or CS NNN (1) real*8 GLON_1 (nr__1) ! (deg) Galactic longitude of center position real*4 GLAT_1 (nr__1) ! (deg) Galactic latitude center position real*4 Rin_2 (nr__1) ! (arcmin) Semimajor axis of the inner ellipse real*4 rin_3 (nr__1) ! (arcmin) Semiminor axis of the inner ellipse real*4 Rout_2 (nr__1) ! (arcmin) Semimajor axis of the outer ellipse real*4 rout_3 (nr__1) ! (arcmin) Semiminor axis of the outer ellipse real*4 Ecc_1 (nr__1) ! Eccentricity of the ellipses (2) real*4 v_R__1 (nr__1) ! (arcmin) Average radius of the bubble real*4 v_T__1 (nr__1) ! (arcmin) Average thickness of the shell character*15 MFlags_1 (nr__1) ! Morphology flags (3) *Note (1): Catalog number preceded by CN if longitude is between 10{deg} and * 0{deg}, and CS if longitude is between 360{deg} and 350{deg}. *Note (2): The centers and eccentricities of the inner and outer ellipses * are constrained to be the same. *Note (3): Morphology flags as follows: * C = complete or closed ring * B = broken or incomplete ring * CC = probable enclosed central star cluster, meaning that the stellar * density inside the ring appears to be greater than the average * stellar density outside the ring * BC = complex of two or more bubbles, that may or may not be * physically associated * MB = Bubbles that have at least one secondary bubble projected * within or on its periphery * MBm = Bubbles subsidiary to MB bubbles are labeled m(catalog number) * according to the MB bubble they are associated with * Y = Bubbles that have possible YSO(s) projected within or on its * periphery but have not formed a secondary bubble * CS = the central star(s) responsible for driving the * bubble is/are probably apparent * Fl = a flocculent or clumpy bubble structure * PN = Two bubbles that are probable planetary nebulae C============================================================================= C Loading file 'table1.dat' ! Northern Bubble parameters C Format for file interpretation 1 format( + A6,1X,F7.3,1X,F6.3,1X,F4.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X, + F4.2,1X,F4.2,1X,A15) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,151 read(1,'(A73)')ar__ read(ar__,1) + v_CWP2007_(i__),GLON(i__),GLAT(i__),Rin(i__),rin_1(i__), + Rout(i__),rout_1(i__),Ecc(i__),v_R_(i__),v_T_(i__),MFlags(i__) c ..............Just test output........... write(6,1) + v_CWP2007_(i__),GLON(i__),GLAT(i__),Rin(i__),rin_1(i__), + Rout(i__),rout_1(i__),Ecc(i__),v_R_(i__),v_T_(i__),MFlags(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table2.dat' ! Southern Bubble parameters C Format for file interpretation 2 format( + A6,1X,F7.3,1X,F6.3,1X,F4.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F4.2,1X, + F4.2,1X,F4.2,1X,A15) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,118 read(1,'(A73)')ar__1 read(ar__1,2) + v_CWP2007__1(i__),GLON_1(i__),GLAT_1(i__),Rin_2(i__), + rin_3(i__),Rout_2(i__),rout_3(i__),Ecc_1(i__),v_R__1(i__), + v_T__1(i__),MFlags_1(i__) c ..............Just test output........... write(6,2) + v_CWP2007__1(i__),GLON_1(i__),GLAT_1(i__),Rin_2(i__), + rin_3(i__),Rout_2(i__),rout_3(i__),Ecc_1(i__),v_R__1(i__), + v_T__1(i__),MFlags_1(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end