Conversion of standardized ReadMe file for
file /./home/cats/J/ApJ/788/55 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 2026-May-18
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/788/55 HST/WFC3 SNR discoveries in M83 (NGC5236) (Blair+, 2014)
*================================================================================
*An expanded HST/WFC3 survey of M83:
*project overview and targeted supernova remnant search.
* Blair W.P., Chandar R., Dopita M.A., Ghavamian P., Hammer D., Kuntz K.D.,
* Long K.S., Soria R., Whitmore B.C., Frank Winkler P.
* <Astrophys. J., 788, 55 (2014)>
* =2014ApJ...788...55B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Small diameter and new supernova remnants in M83
revealed by HST/WFC3
integer*4 nr__
parameter (nr__=63) ! Number of records
character*123 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 ! [1/63] Running sequence number
* (<[BCD2014] NN> in Simbad)
character*7 AName ! Previous name (G1)
integer*4 RAh ! (h) Hour of right ascension (J2000)
integer*4 RAm ! (min) Minute of right ascension (J2000)
real*4 RAs ! (s) Second of right ascension (J2000)
character*1 DE_ ! Sign of declination (J2000)
integer*4 DEd ! (deg) Degree of declination (J2000)
integer*4 DEm ! (arcmin) Arcminute of declination (J2000)
real*4 DEs ! (arcsec) Arcsecond of declination (J2000)
real*4 Rad ! (arcsec) [0.07/0.8] Source radius
real*4 Diam ! (pc) [3.1/34.3] Source diameter (1)
real*4 GCD ! (kpc) [0.1/5.3] Galactocentric distance (1)
integer*4 Field ! [1/7] WFC3 field number
character*1 l_F657N ! Limit flag on F657N
real*4 F657N ! (mW/m2) The F657N flux in erg/cm^2^/s (G2)
character*1 l_F673_657 ! Limit flag on F673/657
real*4 F673_657 ! [0.06/6.6]? Lower limit to the observed
* F673N/F657N (F([SII])/F(H{alpha})) ratio (G3)
character*52 Comm ! Comments
*Note (1): The galactocentric distances (GCDs) of each object are based on the
* same assumptions for galactic inclination and major axis angle as
* used in Blair et al. (2012, Cat. J/ApJS/203/8) and the assumed
* distance of 4.61Mpc.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! M83 supernova remnant WFC3 image ratios and
supporting information
integer*4 nr__1
parameter (nr__1=63) ! Number of records
character*171 ar__1 ! Full-size record
integer*4 Seq_1 ! [1/63] Running sequence number
* (<[BCD2014] NN> in Simbad)
character*7 AName_1 ! Previous name (G1)
character*1 l_F657N_1 ! Limit flag on F657N
real*4 F657N_1 ! (mW/m2) The F657N flux in erg/cm^2^/s (G2)
real*4 F164N ! (mW/m2) ? The F164N flux (objects showing only [FeII]
* emission) (G2)
character*1 l_F673_657_1 ! Limit flag on F673/657
real*4 F673_657_1 ! [0.06/6.6]? Lower limit to the observed
* F673N/F657N (F([SII])/F(H{alpha})) ratio (G3)
character*1 l_F164_657 ! Limit flag on F164/657
real*4 F164_657 ! [0.01/10]? Lower limit to the observed
* F([FeII])/F(H{alpha}) ratio (G3)
character*1 l_F164_673 ! Limit flag on F614/673
real*4 F164_673 ! [0.01/4.86]? Lower limit to the observed
* F([FeII]])/F([SII]) ratio
character*1 l_F502_657 ! Limit flag on F502/657
real*4 F502_657 ! ? Lower limit to the observed
* F([OIII])/F(H{alpha}) ratio (G3)
character*1 u_F502_657 ! Uncertainty flag on F502/657
character*4 XID ! X-Ray ID in Chandra (2)
character*1 u_XID ! Uncertainty flag on XID
* (less reliable alignments)
character*104 Comm_1 ! Comments
*Note (2): X-ray ID from Chandra catalog of Long et al. 2014 (J/ApJS/212/21);
* <[LKB2014] XNNN> in Simbad.
C=============================================================================
C Loading file 'table3.dat' ! Small diameter and new supernova remnants in M83
* revealed by HST/WFC3
C Format for file interpretation
1 format(
+ I2,1X,A7,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.2,
+ 1X,F4.1,1X,F4.2,1X,I1,1X,A1,1X,E8.3,1X,A1,1X,F4.2,1X,A52)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,63
read(1,'(A123)')ar__
read(ar__,1)
+ Seq,AName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Rad,Diam,GCD,Field,
+ l_F657N,F657N,l_F673_657,F673_657,Comm
if(ar__(67:70) .EQ. '') F673_657 = rNULL__
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,AName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Rad,Diam,GCD,Field,
+ l_F657N,F657N,l_F673_657,F673_657,Comm
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! M83 supernova remnant WFC3 image ratios and
* supporting information
C Format for file interpretation
2 format(
+ I2,1X,A7,1X,A1,1X,E8.3,1X,E7.2,1X,A1,1X,F4.2,1X,A1,1X,F5.2,1X,
+ A1,1X,F4.2,1X,A1,1X,F5.2,A1,1X,A4,A1,1X,A104)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,63
read(1,'(A171)')ar__1
read(ar__1,2)
+ Seq_1,AName_1,l_F657N_1,F657N_1,F164N,l_F673_657_1,F673_657_1,
+ l_F164_657,F164_657,l_F164_673,F164_673,l_F502_657,F502_657,
+ u_F502_657,XID,u_XID,Comm_1
if(ar__1(23:29) .EQ. '') F164N = rNULL__
if(ar__1(33:36) .EQ. '') F673_657_1 = rNULL__
if(ar__1(40:44) .EQ. '') F164_657 = rNULL__
if(ar__1(48:51) .EQ. '') F164_673 = rNULL__
if(ar__1(55:59) .EQ. '') F502_657 = rNULL__
c ..............Just test output...........
write(6,2)
+ Seq_1,AName_1,l_F657N_1,F657N_1,F164N,l_F673_657_1,F673_657_1,
+ l_F164_657,F164_657,l_F164_673,F164_673,l_F502_657,F502_657,
+ u_F502_657,XID,u_XID,Comm_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end