Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/123/269 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-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/AJ/123/269 New SMC planetary nebulae (Jacoby+, 2002)
*================================================================================
*A survey for very faint planetary nebulae in the SMC.
*I. Identification, confirmation, and preliminary analysis.
* Jacoby G.H., De Marco O.
* <Astron. J., 123, 269-278 (2002)>
* =2002AJ....123..269J
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Field centers for the SMC survey
integer*4 nr__
parameter (nr__=11) ! Number of records
character*64 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 Field (nr__) ! Field number
integer*4 RAh (nr__) ! (h) Right ascension (J2000.0)
integer*4 RAm (nr__) ! (min) Right ascension (J2000.0)
real*4 RAs (nr__) ! (s) Right ascension (J2000.0)
character*1 DE_ (nr__) ! Declination sign (J2000.0)
integer*4 DEd (nr__) ! (deg) Declination (J2000.0)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0)
integer*4 DEs (nr__) ! (arcsec) Declination (J2000.0)
real*4 Seeing (nr__) ! (arcsec) Seeing
character*36 Comm (nr__) ! Comments
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! SMC planetary nebulae candidates: new in this survey
integer*4 nr__1
parameter (nr__1=25) ! Number of records
character*57 ar__1 ! Full-size record
C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000.0
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000.0
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 v_JD2002_ (nr__1) ! Sequential number
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000.0)
integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000.0)
real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000.0)
character*1 DE__1 (nr__1) ! Declination sign (J2000.0)
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000.0)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000.0)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000.0)
real*4 m5007 (nr__1) ! (mag) m5007 magnitude (-2.5logF(5007)-13.74) (1)
integer*4 DiamI (nr__1) ! (arcsec) ? Image diameter (2)
integer*4 DiamS (nr__1) ! (arcsec) Spectroscopic diameter (2)
integer*4 Field_1 (nr__1) ! Field number
character*1 l__NII__Ha (nr__1) ! Limit flag on [NII]/Ha
real*4 v_NII__Ha (nr__1) ! Intensity ratio [NII]/Ha
character*9 Comm_1 (nr__1) ! Comments
*Note (1): The magnitudes have uncertainties of 0.1mag in their zero points.
* In addition, the magnitudes have measurement accuracies that are no
* better than 0.05mag. The number of significant figures in the
* magnitude values reflects the accuracy of the estimate.
*Note (2): The image diameter is the approximate PN diameter measured
* from the [O III] difference image, while the spectroscopic diameter
* is the diameter of the PN measured from the brightest line in the
* spectrum - often [O III]{lambda}5007, along the slit length from the
* CTIO 4m spectroscopy. The lack of a value in this column indicates
* that the PN diameter was smaller than the seeing.
C=============================================================================
C Loading file 'table2.dat' ! Field centers for the SMC survey
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F3.1,1X,A36)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,11
read(1,'(A64)')ar__
read(ar__,1)
+ Field(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Seeing(i__),Comm(i__)
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)
+ Field(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Seeing(i__),Comm(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! SMC planetary nebulae candidates: new in this survey
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,2X,I2,
+ 1X,I2,2X,I1,1X,A1,F4.2,1X,A9)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,25
read(1,'(A57)')ar__1
read(ar__1,2)
+ v_JD2002_(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),m5007(i__),DiamI(i__),
+ DiamS(i__),Field_1(i__),l__NII__Ha(i__),v_NII__Ha(i__),
+ Comm_1(i__)
if(ar__1(34:35) .EQ. '') DiamI(i__) = iNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = 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(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ v_JD2002_(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),m5007(i__),DiamI(i__),
+ DiamS(i__),Field_1(i__),l__NII__Ha(i__),v_NII__Ha(i__),
+ Comm_1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end