Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/139/1066 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 2026-Jun-08
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/139/1066 X-ray view of NGC 2403 central region (Yukita+, 2010)
*================================================================================
*An X-ray view of star formation in the central 3 kpc of NGC 2403.
* Yukita M., Swartz D.A., Tennant A.F., Soria R.
* <Astron. J., 139, 1066-1088 (2010)>
* =2010AJ....139.1066Y
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! X-ray point sources
integer*4 nr__
parameter (nr__=58) ! Number of records
character*56 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)
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*8 CRate (nr__) ! (10-4ct/s) Count rates for ASIC-S3, in 0.5-2.0keV band
real*4 e_CRate (nr__) ! (10-4ct/s) rms uncertainty on CRate
real*4 LX (nr__) ! (10+29W) X-ray luminosity in 0.5-2.0 keV band (1)
real*4 e_LX (nr__) ! (10+29W) rms uncertainty on LX
real*4 LHa (nr__) ! (10+30W) ? H{alpha} Luminosity (10^37^erg/s, table5)
character*2 Var (nr__) ! [L S] Short- and/or Long-term variability
* (table2 only)
*Note (1): LX in 10^36^erg/s.
* * For X-ray points source (table3), LX is computed using the
* bremsstrahlung model obtained from Table 3 (see the text).
* * For SNRs (table5), LX is computed using the one-temperature model with
* variable NH model as listed in Table 4 (see text).
* * For H II Regions (table7), LX is computed using the two-temperature
* model with the variable NH model listed in Table 6.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Supernova remnants (SNRs)
integer*4 nr__1
parameter (nr__1=24) ! Number of records
character*56 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)
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000)
character*1 DE__1 (nr__1) ! Declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000)
real*8 CRate_1 (nr__1) ! (10-4ct/s) Count rates for ASIC-S3, in 0.5-2.0keV band
real*4 e_CRate_1 (nr__1) ! (10-4ct/s) rms uncertainty on CRate
real*4 LX_1 (nr__1) ! (10+29W) X-ray luminosity in 0.5-2.0 keV band (1)
real*4 e_LX_1 (nr__1) ! (10+29W) rms uncertainty on LX
real*4 LHa_1 (nr__1) ! (10+30W) ? H{alpha} Luminosity (10^37^erg/s, table5)
character*2 Var_1 (nr__1) ! [L S] Short- and/or Long-term variability
* (table2 only)
*Note (1): LX in 10^36^erg/s.
* * For X-ray points source (table3), LX is computed using the
* bremsstrahlung model obtained from Table 3 (see the text).
* * For SNRs (table5), LX is computed using the one-temperature model with
* variable NH model as listed in Table 4 (see text).
* * For H II Regions (table7), LX is computed using the two-temperature
* model with the variable NH model listed in Table 6.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table7.dat' ! HII regions
integer*4 nr__2
parameter (nr__2=47) ! Number of records
character*56 ar__2 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_2 (nr__2) ! (deg) Right Ascension J2000
real*8 DEdeg_2 (nr__2) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 RAh_2 (nr__2) ! (h) Right ascension (J2000)
integer*4 RAm_2 (nr__2) ! (min) Right ascension (J2000)
real*4 RAs_2 (nr__2) ! (s) Right ascension (J2000)
character*1 DE__2 (nr__2) ! Declination sign (J2000)
integer*4 DEd_2 (nr__2) ! (deg) Declination (J2000)
integer*4 DEm_2 (nr__2) ! (arcmin) Declination (J2000)
real*4 DEs_2 (nr__2) ! (arcsec) Declination (J2000)
real*8 CRate_2 (nr__2) ! (10-4ct/s) Count rates for ASIC-S3, in 0.5-2.0keV band
real*4 e_CRate_2 (nr__2) ! (10-4ct/s) rms uncertainty on CRate
real*4 LX_2 (nr__2) ! (10+29W) X-ray luminosity in 0.5-2.0 keV band (1)
real*4 e_LX_2 (nr__2) ! (10+29W) rms uncertainty on LX
real*4 LHa_2 (nr__2) ! (10+30W) ? H{alpha} Luminosity (10^37^erg/s, table5)
character*2 Var_2 (nr__2) ! [L S] Short- and/or Long-term variability
* (table2 only)
*Note (1): LX in 10^36^erg/s.
* * For X-ray points source (table3), LX is computed using the
* bremsstrahlung model obtained from Table 3 (see the text).
* * For SNRs (table5), LX is computed using the one-temperature model with
* variable NH model as listed in Table 4 (see text).
* * For H II Regions (table7), LX is computed using the two-temperature
* model with the variable NH model listed in Table 6.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Luminosities and sizes of 19 star-forming regions
integer*4 nr__3
parameter (nr__3=19) ! Number of records
character*96 ar__3 ! Full-size record
character*16 SF (nr__3) ! Source name (JHHMMSS.s+DDMMSS),
* <[YST2010] SF JHHMMSS.s+DDMMSS> in Simbad
real*4 LFUV (nr__3) ! (10+32W) FUV luminosity in 10^39^erg/s (1)
real*4 e_LFUV (nr__3) ! (10+32W) rms uncertainty on LFUV
real*4 RFUV (nr__3) ! (arcsec) FUV radius
real*4 LNUV (nr__3) ! (10+32W) NUV luminosity in 10^39^erg/s (1)
real*4 e_LNUV (nr__3) ! (10+32W) rms uncertainty on LNUV
real*4 L3_6 (nr__3) ! (10+31W) 3.6um luminosity in 10^38^erg/s
real*4 e_L3_6 (nr__3) ! (10+31W) rms uncertainty on L3.6
real*4 L4_5 (nr__3) ! (10+31W) 4.5um luminosity in 10^38^erg/s
real*4 e_L4_5 (nr__3) ! (10+31W) rms uncertainty on L4.5
real*4 L24 (nr__3) ! (10+32W) 24um luminosity in 10^39^erg/s
real*4 e_L24 (nr__3) ! (10+32W) rms uncertainty on L24
real*4 R24 (nr__3) ! (arcsec) 24um radius
real*4 LHa_3 (nr__3) ! (10+31W) H{alpha} luminosity in 10^38^erg/s (1)
real*4 RHa (nr__3) ! (arcsec) H{alpha} radius
real*4 LX_3 (nr__3) ! (10+28W) X-ray luminosity in 10^35^erg/s
real*4 e_LX_3 (nr__3) ! (10+28W) rms uncertainty on LX
*Note (1): FUV, NUV, and H{alpha} luminosities are Galactic extinction corrected.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table10.dat' ! Derived values of 19 star-forming regions
integer*4 nr__4
parameter (nr__4=19) ! Number of records
character*67 ar__4 ! Full-size record
character*16 SF_1 (nr__4) ! Source name (JHHMMSS.s+DDMMSS),
real*4 Mass (nr__4) ! (10+5Msun) Mass of region
integer*4 Age (nr__4) ! (Myr) Age
real*4 AV (nr__4) ! (mag) Absorption in V band
real*4 NH (nr__4) ! (10+21cm-2) H column density (1)
real*4 LW (nr__4) ! (10+31W) Mechanical luminosity in 10^38^erg/s (2)
real*4 LFUVi (nr__4) ! (10+32W) Integrated FUV luminosity in 10^39^erg/s
real*4 e_LFUVi (nr__4) ! (10+32W) rms uncertainty on LFUVi
real*4 LHai (nr__4) ! (10+32W) Integrated H{alpha} luminosity in 10^39^erg/s
real*4 LXi (nr__4) ! (10+28W) Integrated X -ray luminosity in 10^35^erg/s
real*4 e_LXi (nr__4) ! (10+28W) rms uncertainty on LXi
*Note (1): Listed NH values include a Galactic component of NH=0.4x10^21^cm^-2^.
*Note (2): under assumption of a constant energy injection rate.
C=============================================================================
C Loading file 'table2.dat' ! X-ray point sources
C Format for file interpretation
1 format(
+ I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F7.2,1X,F5.2,1X,
+ F6.2,1X,F4.2,1X,F5.1,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,58
read(1,'(A56)')ar__
read(ar__,1)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),CRate(i__),e_CRate(i__),LX(i__),e_LX(i__),LHa(i__),
+ Var(i__)
if(ar__(50:54) .EQ. '') LHa(i__) = rNULL__
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)
+ RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
+ DEs(i__),CRate(i__),e_CRate(i__),LX(i__),e_LX(i__),LHa(i__),
+ Var(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 'table5.dat' ! Supernova remnants (SNRs)
C Format for file interpretation
2 format(
+ I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F7.2,1X,F5.2,1X,
+ F6.2,1X,F4.2,1X,F5.1,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,24
read(1,'(A56)')ar__1
read(ar__1,2)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),CRate_1(i__),e_CRate_1(i__),LX_1(i__),
+ e_LX_1(i__),LHa_1(i__),Var_1(i__)
if(ar__1(50:54) .EQ. '') LHa_1(i__) = rNULL__
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)
+ RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),DEd_1(i__),
+ DEm_1(i__),DEs_1(i__),CRate_1(i__),e_CRate_1(i__),LX_1(i__),
+ e_LX_1(i__),LHa_1(i__),Var_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=============================================================================
C Loading file 'table7.dat' ! HII regions
C Format for file interpretation
3 format(
+ I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,F7.2,1X,F5.2,1X,
+ F6.2,1X,F4.2,1X,F5.1,A2)
C Effective file loading
open(unit=1,status='old',file=
+'table7.dat')
write(6,*) '....Loading file: table7.dat'
do i__=1,47
read(1,'(A56)')ar__2
read(ar__2,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),CRate_2(i__),e_CRate_2(i__),LX_2(i__),
+ e_LX_2(i__),LHa_2(i__),Var_2(i__)
if(ar__2(50:54) .EQ. '') LHa_2(i__) = rNULL__
RAdeg_2(i__) = rNULL__
DEdeg_2(i__) = rNULL__
c Derive coordinates RAdeg_2 and DEdeg_2 from input data
c (RAdeg_2 and DEdeg_2 are set to rNULL__ when unknown)
if(RAh_2(i__) .GT. -180) RAdeg_2(i__)=RAh_2(i__)*15.
if(RAm_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAm_2(i__)/4.
if(RAs_2(i__) .GT. -180) RAdeg_2(i__)=RAdeg_2(i__)+RAs_2(i__)/240.
if(DEd_2(i__) .GE. 0) DEdeg_2(i__)=DEd_2(i__)
if(DEm_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEm_2(i__)/60.
if(DEs_2(i__) .GE. 0) DEdeg_2(i__)=DEdeg_2(i__)+DEs_2(i__)/3600.
if(DE__2(i__).EQ.'-'.AND.DEdeg_2(i__).GE.0) DEdeg_2(i__)=-DEdeg_2(i__)
c ..............Just test output...........
write(6,3)
+ RAh_2(i__),RAm_2(i__),RAs_2(i__),DE__2(i__),DEd_2(i__),
+ DEm_2(i__),DEs_2(i__),CRate_2(i__),e_CRate_2(i__),LX_2(i__),
+ e_LX_2(i__),LHa_2(i__),Var_2(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_2(i__),DEdeg_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table9.dat' ! Luminosities and sizes of 19 star-forming regions
C Format for file interpretation
4 format(
+ 3X,A16,1X,F5.1,1X,F3.1,1X,F3.1,1X,F5.1,1X,F3.1,1X,F4.1,1X,
+ F3.1,1X,F4.1,1X,F3.1,1X,F5.1,1X,F3.1,1X,F4.1,1X,F4.1,1X,F4.1,
+ 1X,F4.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,19
read(1,'(A96)')ar__3
read(ar__3,4)
+ SF(i__),LFUV(i__),e_LFUV(i__),RFUV(i__),LNUV(i__),e_LNUV(i__),
+ L3_6(i__),e_L3_6(i__),L4_5(i__),e_L4_5(i__),L24(i__),
+ e_L24(i__),R24(i__),LHa_3(i__),RHa(i__),LX_3(i__),e_LX_3(i__)
c ..............Just test output...........
write(6,4)
+ SF(i__),LFUV(i__),e_LFUV(i__),RFUV(i__),LNUV(i__),e_LNUV(i__),
+ L3_6(i__),e_L3_6(i__),L4_5(i__),e_L4_5(i__),L24(i__),
+ e_L24(i__),R24(i__),LHa_3(i__),RHa(i__),LX_3(i__),e_LX_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table10.dat' ! Derived values of 19 star-forming regions
C Format for file interpretation
5 format(
+ 3X,A16,1X,F4.1,1X,I2,1X,F4.2,1X,F3.1,1X,F4.1,1X,F5.1,1X,F3.1,
+ 1X,F4.1,1X,F5.1,1X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table10.dat')
write(6,*) '....Loading file: table10.dat'
do i__=1,19
read(1,'(A67)')ar__4
read(ar__4,5)
+ SF_1(i__),Mass(i__),Age(i__),AV(i__),NH(i__),LW(i__),
+ LFUVi(i__),e_LFUVi(i__),LHai(i__),LXi(i__),e_LXi(i__)
c ..............Just test output...........
write(6,5)
+ SF_1(i__),Mass(i__),Age(i__),AV(i__),NH(i__),LW(i__),
+ LFUVi(i__),e_LFUVi(i__),LHai(i__),LXi(i__),e_LXi(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end