Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/131/2089 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/131/2089 Planetary nebulae in NGC 3379 and NGC 3384 (Sluis+, 2006)
*================================================================================
*Uncovering planetary nebulae in early-type galaxies using the Rutgers
*Fabry-Perot.
* Sluis A.P.N., Williams T.B.
* <Astron. J., 131, 2089-2104 (2006)>
* =2006AJ....131.2089S
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! NGC 3379 planetary nebulae
integer*4 nr__
parameter (nr__=54) ! Number of records
character*85 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*3 ID (nr__) ! Source identification (1)
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000) (2)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000) (2)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000) (2)
character*1 DE_ (nr__) ! Sign of the Declination (J2000) (2)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000) (2)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) (2)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) (2)
real*4 lambda (nr__) ! (0.1nm) Peak wavelength in Angstroms
integer*4 HRV (nr__) ! (km/s) Heliocentric line-of-sight velocity
integer*4 e_HRV (nr__) ! (km/s) Uncertainty in HRV
real*4 Flux (nr__) ! (10-19W/m2) Emission line flux in units
* of 10^-16^erg/s/cm^2^
real*4 v5007mag (nr__) ! (mag) Emission line magnitude (3)
real*4 e_5007mag (nr__) ! (mag) Uncertainty in 5007mag
real*4 S (nr__) ! The likelihood ratio test statistic (4)
integer*4 Num (nr__) ! ? Number of data points in spectrum
real*4 S_N (nr__) ! Signal-to-noise ratio
integer*4 C89ID (nr__) ! ? Ciardullo et al. (1989, J/ApJ/344/715)
* identification
real*4 C89mag (nr__) ! (mag) ? Ciardullo et al. (1989, J/ApJ/344/715)
* emission line magnitude
integer*4 C89HRV (nr__) ! (km/s) ? Ciardullo et al. (1989, J/ApJ/344/715)
* heliocentric line-of-sight velocity
*Note (1): E and W denote PNe found in the East and West fields, respectively.
* Nomenclature in Simbad:
* Table 5: [SW2006] NGC 3379 WNN
* Table 6: [SW2006] NGC 3384 WNN
*Note (2): Where the uncertainty in each coordinate is 0.4" (includes random and
* systematic uncertainty);
*Note (3): 5007mag=-2.5log(Flux)+13.74 (no extinction correction was made).
*Note (4): The spectra have a wide range in their number of data points and we
* determine S_c_({alpha}) for regions with one, two, or three pointings
* separately. Hence, the values of S listed in Table 6 are not always
* directly comparable.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! NGC 3384 planetary nebulae
integer*4 nr__1
parameter (nr__1=50) ! Number of records
character*85 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*3 ID_1 (nr__1) ! Source identification (1)
integer*4 RAh_1 (nr__1) ! (h) Hour of Right Ascension (J2000) (2)
integer*4 RAm_1 (nr__1) ! (min) Minute of Right Ascension (J2000) (2)
real*4 RAs_1 (nr__1) ! (s) Second of Right Ascension (J2000) (2)
character*1 DE__1 (nr__1) ! Sign of the Declination (J2000) (2)
integer*4 DEd_1 (nr__1) ! (deg) Degree of Declination (J2000) (2)
integer*4 DEm_1 (nr__1) ! (arcmin) Arcminute of Declination (J2000) (2)
real*4 DEs_1 (nr__1) ! (arcsec) Arcsecond of Declination (J2000) (2)
real*4 lambda_1 (nr__1) ! (0.1nm) Peak wavelength in Angstroms
integer*4 HRV_1 (nr__1) ! (km/s) Heliocentric line-of-sight velocity
integer*4 e_HRV_1 (nr__1) ! (km/s) Uncertainty in HRV
real*4 Flux_1 (nr__1) ! (10-19W/m2) Emission line flux in units
* of 10^-16^erg/s/cm^2^
real*4 v5007mag_1 (nr__1) ! (mag) Emission line magnitude (3)
real*4 e_5007mag_1(nr__1) ! (mag) Uncertainty in 5007mag
real*4 S_1 (nr__1) ! The likelihood ratio test statistic (4)
integer*4 Num_1 (nr__1) ! ? Number of data points in spectrum
real*4 S_N_1 (nr__1) ! Signal-to-noise ratio
integer*4 C89ID_1 (nr__1) ! ? Ciardullo et al. (1989, J/ApJ/344/715)
* identification
real*4 C89mag_1 (nr__1) ! (mag) ? Ciardullo et al. (1989, J/ApJ/344/715)
* emission line magnitude
integer*4 C89HRV_1 (nr__1) ! (km/s) ? Ciardullo et al. (1989, J/ApJ/344/715)
* heliocentric line-of-sight velocity
*Note (1): E and W denote PNe found in the East and West fields, respectively.
* Nomenclature in Simbad:
* Table 5: [SW2006] NGC 3379 WNN
* Table 6: [SW2006] NGC 3384 WNN
*Note (2): Where the uncertainty in each coordinate is 0.4" (includes random and
* systematic uncertainty);
*Note (3): 5007mag=-2.5log(Flux)+13.74 (no extinction correction was made).
*Note (4): The spectra have a wide range in their number of data points and we
* determine S_c_({alpha}) for regions with one, two, or three pointings
* separately. Hence, the values of S listed in Table 6 are not always
* directly comparable.
C=============================================================================
C Loading file 'table5.dat' ! NGC 3379 planetary nebulae
C Format for file interpretation
1 format(
+ A3,1X,I2,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,F6.1,1X,I4,1X,
+ I2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.1,1X,I2,1X,F4.1,1X,I2,1X,
+ F5.2,1X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,54
read(1,'(A85)')ar__
read(ar__,1)
+ ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),lambda(i__),HRV(i__),e_HRV(i__),Flux(i__),
+ v5007mag(i__),e_5007mag(i__),S(i__),Num(i__),S_N(i__),
+ C89ID(i__),C89mag(i__),C89HRV(i__)
if(ar__(65:66) .EQ. '') Num(i__) = iNULL__
if(ar__(73:74) .EQ. '') C89ID(i__) = iNULL__
if(ar__(76:80) .EQ. '') C89mag(i__) = rNULL__
if(ar__(82:85) .EQ. '') C89HRV(i__) = iNULL__
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)
+ ID(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),lambda(i__),HRV(i__),e_HRV(i__),Flux(i__),
+ v5007mag(i__),e_5007mag(i__),S(i__),Num(i__),S_N(i__),
+ C89ID(i__),C89mag(i__),C89HRV(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 'table6.dat' ! NGC 3384 planetary nebulae
C Format for file interpretation
2 format(
+ A3,1X,I2,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,F6.1,1X,I4,1X,
+ I2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.1,1X,I2,1X,F4.1,1X,I2,1X,
+ F5.2,1X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,50
read(1,'(A85)')ar__1
read(ar__1,2)
+ ID_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),lambda_1(i__),HRV_1(i__),
+ e_HRV_1(i__),Flux_1(i__),v5007mag_1(i__),e_5007mag_1(i__),
+ S_1(i__),Num_1(i__),S_N_1(i__),C89ID_1(i__),C89mag_1(i__),
+ C89HRV_1(i__)
if(ar__1(65:66) .EQ. '') Num_1(i__) = iNULL__
if(ar__1(73:74) .EQ. '') C89ID_1(i__) = iNULL__
if(ar__1(76:80) .EQ. '') C89mag_1(i__) = rNULL__
if(ar__1(82:85) .EQ. '') C89HRV_1(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)
+ ID_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),lambda_1(i__),HRV_1(i__),
+ e_HRV_1(i__),Flux_1(i__),v5007mag_1(i__),e_5007mag_1(i__),
+ S_1(i__),Num_1(i__),S_N_1(i__),C89ID_1(i__),C89mag_1(i__),
+ C89HRV_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