Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJS/203/8 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-Apr-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/ApJS/203/8 Optical SNR candidates in M83 (Blair+, 2012)
*================================================================================
*The Magellan/IMACS catalog of optical supernova remnant candidates in M83.
* Blair W.P., Winkler P.F., Long K.S.
* <Astrophys. J. Suppl. Ser., 203, 8 (2012)>
* =2012ApJS..203....8B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! ISM-dominated supernova remnants and candidates;
updated version from the erratum published in
2017, ApJS, 229, 43
integer*4 nr__
parameter (nr__=225) ! Number of records
character*90 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)
integer*4 Seq ! [1/346] Object running sequence number (1)
character*1 f_Seq ! Flag on Seq (2)
integer*4 RAh ! (h) [13] Hour of Right Ascension (J2000)
integer*4 RAm ! (min) [36/37] Minute of Right Ascension (J2000)
real*4 RAs ! (s) Second of Right Ascension (J2000)
character*1 DE_ ! [-] Sign of the Declination (J2000)
integer*4 DEd ! (deg) [29] Degree of Declination (J2000)
integer*4 DEm ! (arcmin) [46/59] Arcminute of Declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of Declination (J2000)
real*4 Rad ! (kpc) [0.1/12] Galactic radius
real*4 Diam ! (arcsec) [0.8/6] Diameter of circular regions used
* for flux extractions (3)
real*4 F_Ha ! (10-19W/m2) [0.3/236] H{alpha} flux (4)
real*4 F__SII_ ! (10-19W/m2) [0/83] Flux of [SII] (4)
real*4 F__OIII_ ! (10-19W/m2) [0/185] Flux of [OIII] (4)
real*4 v_SII__Ha ! [0/2] Ratio of [SII] to H{alpha}
real*4 v_OIII__Ha ! [0/6] Ratio of [OIII] to H{alpha}
character*1 X ! [y/n] X-ray? (5)
character*22 OName ! Other names (6)
*Note (1): Numbering in table 3 begins at 301 to separate this group from the
* ISM SNR sample (table 2).
*Note (2):
* x = Position and size for object 014 has been slightly revised since
* the original paper (J/ApJS/203/8).
*Note (3): Diameter of the circular regions used for flux extractions; these
* are effectively upper limits for the object sizes.
*Note (4): In units of 10^-16^erg/cm2/s; a correction factor of 1.45 has been
* applied to H{alpha} (see the text).
*Note (5): A "y" indicates a likely X-ray detection in deep Chandra data
* (Long+ 2014, J/ApJS/212/21).
*Note (6): Other Name abbreviations:
* BL = Blair & Long (2004ApJS..155..101B; <[BL2004b] SNR NN> in Simbad);
* SW = Soria & Wu (2003, Cat. J/A+A/410/53; <[SW2003] NNN> in Simbad);
* H = Hadfield et al. (2005, Cat. J/A+A/439/265; <[HCS2005] NNN> for Simbad);
* D10 = Dopita et al. (2010ApJ...710..964D)
* D10-T4 = Table 4, Dopita et al. (2010ApJ...710..964D);
* L = Long el al. (2014, J/ApJS/212/21).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! [OIII]-selected objects and supernova remnant
candidates; updated version from the erratum
(2017, ApJS, 229, 43)
integer*4 nr__1
parameter (nr__1=46) ! Number of records
character*90 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)
integer*4 Seq_1 ! [1/346] Object running sequence number (1)
character*1 f_Seq_1 ! Flag on Seq (2)
integer*4 RAh_1 ! (h) [13] Hour of Right Ascension (J2000)
integer*4 RAm_1 ! (min) [36/37] Minute of Right Ascension (J2000)
real*4 RAs_1 ! (s) Second of Right Ascension (J2000)
character*1 DE__1 ! [-] Sign of the Declination (J2000)
integer*4 DEd_1 ! (deg) [29] Degree of Declination (J2000)
integer*4 DEm_1 ! (arcmin) [46/59] Arcminute of Declination (J2000)
real*4 DEs_1 ! (arcsec) Arcsecond of Declination (J2000)
real*4 Rad_1 ! (kpc) [0.1/12] Galactic radius
real*4 Diam_1 ! (arcsec) [0.8/6] Diameter of circular regions used
* for flux extractions (3)
real*4 F_Ha_1 ! (10-19W/m2) [0.3/236] H{alpha} flux (4)
real*4 F__SII__1 ! (10-19W/m2) [0/83] Flux of [SII] (4)
real*4 F__OIII__1 ! (10-19W/m2) [0/185] Flux of [OIII] (4)
real*4 v_SII__Ha_1 ! [0/2] Ratio of [SII] to H{alpha}
real*4 v_OIII__Ha_1 ! [0/6] Ratio of [OIII] to H{alpha}
character*1 X_1 ! [y/n] X-ray? (5)
character*22 OName_1 ! Other names (6)
*Note (1): Numbering in table 3 begins at 301 to separate this group from the
* ISM SNR sample (table 2).
*Note (2):
* x = Position and size for object 014 has been slightly revised since
* the original paper (J/ApJS/203/8).
*Note (3): Diameter of the circular regions used for flux extractions; these
* are effectively upper limits for the object sizes.
*Note (4): In units of 10^-16^erg/cm2/s; a correction factor of 1.45 has been
* applied to H{alpha} (see the text).
*Note (5): A "y" indicates a likely X-ray detection in deep Chandra data
* (Long+ 2014, J/ApJS/212/21).
*Note (6): Other Name abbreviations:
* BL = Blair & Long (2004ApJS..155..101B; <[BL2004b] SNR NN> in Simbad);
* SW = Soria & Wu (2003, Cat. J/A+A/410/53; <[SW2003] NNN> in Simbad);
* H = Hadfield et al. (2005, Cat. J/A+A/439/265; <[HCS2005] NNN> for Simbad);
* D10 = Dopita et al. (2010ApJ...710..964D)
* D10-T4 = Table 4, Dopita et al. (2010ApJ...710..964D);
* L = Long el al. (2014, J/ApJS/212/21).
C=============================================================================
C Loading file 'table2.dat' ! ISM-dominated supernova remnants and candidates;
* updated version from the erratum published in
* 2017, ApJS, 229, 43
C Format for file interpretation
1 format(
+ I3,1X,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,
+ 1X,F3.1,1X,F5.1,1X,F4.1,1X,F5.1,1X,F4.2,1X,F4.2,1X,A1,1X,A22)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,225
read(1,'(A90)')ar__
read(ar__,1)
+ Seq,f_Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Rad,Diam,F_Ha,F__SII_,
+ F__OIII_,v_SII__Ha,v_OIII__Ha,X,OName
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)
+ Seq,f_Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Rad,Diam,F_Ha,F__SII_,
+ F__OIII_,v_SII__Ha,v_OIII__Ha,X,OName
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! [OIII]-selected objects and supernova remnant
* candidates; updated version from the erratum
* (2017, ApJS, 229, 43)
C Format for file interpretation
2 format(
+ I3,1X,A1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F4.1,
+ 1X,F3.1,1X,F5.1,1X,F4.1,1X,F5.1,1X,F4.2,1X,F4.2,1X,A1,1X,A22)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,46
read(1,'(A90)')ar__1
read(ar__1,2)
+ Seq_1,f_Seq_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Rad_1,
+ Diam_1,F_Ha_1,F__SII__1,F__OIII__1,v_SII__Ha_1,v_OIII__Ha_1,
+ X_1,OName_1
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)
+ Seq_1,f_Seq_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,Rad_1,
+ Diam_1,F_Ha_1,F__SII__1,F__OIII__1,v_SII__Ha_1,v_OIII__Ha_1,
+ X_1,OName_1
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end