Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/446/369 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-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/MNRAS/446/369 Colour and spectral index from the SLUGGS survey (Usher+, 2015)
*================================================================================
*The SLUGGS survey: globular cluster stellar population trends from weak
*absorption lines in stacked spectra.
* Usher C., Forbes D.A., Brodie J.P., Romanowsky A.J., Strader J., Conroy C.,
* Foster C., Pastorello N., Pota V., Arnold J.A.
* <Mon. Not. R. Astron. Soc., 446, 369-390 (2015)>
* =2015MNRAS.446..369U (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Galaxy properties
integer*4 nr__
parameter (nr__=10) ! Number of records
character*58 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 NGC (nr__) ! [1407/5846] Host galaxy name
character*1 n_NGC (nr__) ! [a] Note on NGC (1)
integer*4 RAh (nr__) ! (h) Simbad Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Simbad Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Simbad Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Simbad Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Simbad Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Simbad Arcminute of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Simbad Arcsecond of Declination (J2000)
integer*4 Vsys (nr__) ! (km/s) Systemic velocity from Cappellari et al.
* (2011, J/MNRAS/413/813)
real*4 Dist (nr__) ! (Mpc) Distance from Cappellari et al.
* (2011, J/MNRAS/413/813) (2)
real*4 KMag (nr__) ! (mag) K-band absolute magnitude from
* Cappellari et al. (2011, J/MNRAS/413/813) (3)
integer*4 Spectra (nr__) ! Total number of GC spectra
integer*4 GC (nr__) ! Number of unique GCs with spectra
*Note (1): NGC 1407 and NGC 3115 are not part of the Cappellari et al.
* (2011, J/MNRAS/413/813) sample so their radial velocities were taken
* from NED while their distances are from Tonry et al.
* (2001ApJ...546..681T) with the same -0.06 mag distance moduli offset
* as Cappellari et al. (2011, J/MNRAS/413/813).
* We assume that NGC 1400 and NGC 1407 are part of the same group and
* use the mean of their distance moduli for NGC 1407. Their K-band
* absolute magnitude is also calculated from the 2MASS total K apparent
* magnitude and the distance in the same manner as Cappellari et al.
* (2011, J/MNRAS/413/813).
*Note (2): Based on surface brightness fluctuations (SBF) of Tonry et al.
* (2001ApJ...546..681T). For NGC 4365, NGC 4473 and NGC 4649,
* Cappellari et al. (2011, J/MNRAS/413/813) used the SBF distance of
* Mei et al. (2007, J/ApJ/655/144).
*Note (3): Calculated from the 2MASS (Skrutskie et al. 2006, Cat. VII/233) total
* K-band apparent magnitude and the distance in the previous column,
* corrected for foreground extinction.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! Colour and spectral index measurements of
spectra stacked by colour for galaxies
integer*4 nr__1
parameter (nr__1=45) ! Number of records
character*201 ar__1 ! Full-size record
character*6 Group (nr__1) ! [faint bright] Galaxy group (1)
integer*4 NGC_1 (nr__1) ! [1407/5846]? Host galaxy name
real*4 g_i (nr__1) ! (mag) Subaru/Suprime-Cam (g-i) colour index
real*4 E_g_i (nr__1) ! (mag) Upper limit uncertainty in g-i
real*4 e_g_i_1 (nr__1) ! (mag) Lower limit uncertainty in g-i
real*8 iMag (nr__1) ! (mag) Subaru/Suprime-Cam i-band absolute magnitude
real*4 E_iMag (nr__1) ! (mag) Upper limit uncertainty in iMag
real*4 e_iMag_1 (nr__1) ! (mag) Lower limit uncertainty in iMag
real*4 CaT (nr__1) ! (0.1nm) Ca II triplet spectral index strength ({AA})
real*4 E_CaT (nr__1) ! (0.1nm) Upper limit uncertainty in CaT
real*4 e_CaT_1 (nr__1) ! (0.1nm) Lower limit uncertainty in CaT
real*4 Fe86 (nr__1) ! (0.1nm) Fe86 spectral index strength ({AA})
real*4 E_Fe86 (nr__1) ! (0.1nm) Upper limit uncertainty in Fe86
real*4 e_Fe86_1 (nr__1) ! (0.1nm) Lower limit uncertainty in Fe86
real*4 Mg88 (nr__1) ! (0.1nm) Mg88 spectral index strength ({AA})
real*4 E_Mg88 (nr__1) ! (0.1nm) Upper limit uncertainty in Mg88
real*4 e_Mg88_1 (nr__1) ! (0.1nm) Lower limit uncertainty in Mg88
real*4 Na82 (nr__1) ! (0.1nm) Na82 spectral index strength ({AA})
real*4 E_Na82 (nr__1) ! (0.1nm) Upper limit uncertainty in Na82
real*4 e_Na82_1 (nr__1) ! (0.1nm) Lower limit uncertainty in Na82
real*4 TiO89 (nr__1) ! TiO89 spectral index strength
real*4 E_TiO89 (nr__1) ! Upper limit uncertainty in TiO89
real*4 e_TiO89_1 (nr__1) ! Lower limit uncertainty in TiO89
real*4 Halpha (nr__1) ! (0.1nm) H{alpha} spectral index strength ({AA})
real*4 E_Halpha (nr__1) ! (0.1nm) Upper limit uncertainty in Halpha
real*4 e_Halpha_1 (nr__1) ! (0.1nm) Lower limit uncertainty in Halpha
real*4 PaT (nr__1) ! (0.1nm) Paschen line spectral index strength ({AA})
real*4 E_PaT (nr__1) ! (0.1nm) Upper limit uncertainty in PaT
real*4 e_PaT_1 (nr__1) ! (0.1nm) Lower limit uncertainty in PaT
real*4 sigma (nr__1) ! (km/s) ? Velocity dispersion
real*4 E_sigma (nr__1) ! (km/s) ? Upper limit uncertainty in sigma
real*4 e_sigma_1 (nr__1) ! (km/s) ? Lower limit uncertainty in sigma
*Note (1): NGC 1407, NGC 4278, NGC 4365 and NGC 4649 are in the bright group;
* NGC 3115, NGC 3377, NGC 4473 and NGC 4494 are in the faint group.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! Colour and spectral index measurements of
spectra stacked by colour for groups
integer*4 nr__2
parameter (nr__2=20) ! Number of records
character*201 ar__2 ! Full-size record
character*6 Group_1 (nr__2) ! [faint bright] Galaxy group (1)
integer*4 NGC_2 (nr__2) ! [1407/5846]? Host galaxy name
real*4 g_i_1 (nr__2) ! (mag) Subaru/Suprime-Cam (g-i) colour index
real*4 E_g_i_2 (nr__2) ! (mag) Upper limit uncertainty in g-i
real*4 e_g_i_3 (nr__2) ! (mag) Lower limit uncertainty in g-i
real*8 iMag_1 (nr__2) ! (mag) Subaru/Suprime-Cam i-band absolute magnitude
real*4 E_iMag_2 (nr__2) ! (mag) Upper limit uncertainty in iMag
real*4 e_iMag_3 (nr__2) ! (mag) Lower limit uncertainty in iMag
real*4 CaT_1 (nr__2) ! (0.1nm) Ca II triplet spectral index strength ({AA})
real*4 E_CaT_2 (nr__2) ! (0.1nm) Upper limit uncertainty in CaT
real*4 e_CaT_3 (nr__2) ! (0.1nm) Lower limit uncertainty in CaT
real*4 Fe86_1 (nr__2) ! (0.1nm) Fe86 spectral index strength ({AA})
real*4 E_Fe86_2 (nr__2) ! (0.1nm) Upper limit uncertainty in Fe86
real*4 e_Fe86_3 (nr__2) ! (0.1nm) Lower limit uncertainty in Fe86
real*4 Mg88_1 (nr__2) ! (0.1nm) Mg88 spectral index strength ({AA})
real*4 E_Mg88_2 (nr__2) ! (0.1nm) Upper limit uncertainty in Mg88
real*4 e_Mg88_3 (nr__2) ! (0.1nm) Lower limit uncertainty in Mg88
real*4 Na82_1 (nr__2) ! (0.1nm) Na82 spectral index strength ({AA})
real*4 E_Na82_2 (nr__2) ! (0.1nm) Upper limit uncertainty in Na82
real*4 e_Na82_3 (nr__2) ! (0.1nm) Lower limit uncertainty in Na82
real*4 TiO89_1 (nr__2) ! TiO89 spectral index strength
real*4 E_TiO89_2 (nr__2) ! Upper limit uncertainty in TiO89
real*4 e_TiO89_3 (nr__2) ! Lower limit uncertainty in TiO89
real*4 Halpha_1 (nr__2) ! (0.1nm) H{alpha} spectral index strength ({AA})
real*4 E_Halpha_2 (nr__2) ! (0.1nm) Upper limit uncertainty in Halpha
real*4 e_Halpha_3 (nr__2) ! (0.1nm) Lower limit uncertainty in Halpha
real*4 PaT_1 (nr__2) ! (0.1nm) Paschen line spectral index strength ({AA})
real*4 E_PaT_2 (nr__2) ! (0.1nm) Upper limit uncertainty in PaT
real*4 e_PaT_3 (nr__2) ! (0.1nm) Lower limit uncertainty in PaT
real*4 sigma_1 (nr__2) ! (km/s) ? Velocity dispersion
real*4 E_sigma_2 (nr__2) ! (km/s) ? Upper limit uncertainty in sigma
real*4 e_sigma_3 (nr__2) ! (km/s) ? Lower limit uncertainty in sigma
*Note (1): NGC 1407, NGC 4278, NGC 4365 and NGC 4649 are in the bright group;
* NGC 3115, NGC 3377, NGC 4473 and NGC 4494 are in the faint group.
C=============================================================================
C Loading file 'table1.dat' ! Galaxy properties
C Format for file interpretation
1 format(
+ 3X,I4,A1,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,I4,1X,
+ F4.1,1X,F5.1,1X,I3,1X,I3)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,10
read(1,'(A58)')ar__
read(ar__,1)
+ NGC(i__),n_NGC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),Vsys(i__),Dist(i__),KMag(i__),
+ Spectra(i__),GC(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)
+ NGC(i__),n_NGC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
+ DEd(i__),DEm(i__),DEs(i__),Vsys(i__),Dist(i__),KMag(i__),
+ Spectra(i__),GC(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 'tablea1.dat' ! Colour and spectral index measurements of
* spectra stacked by colour for galaxies
C Format for file interpretation
2 format(
+ A6,4X,I4,1X,F6.4,1X,F6.4,1X,F6.4,1X,F7.3,1X,F5.3,1X,F5.3,1X,
+ F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,
+ 1X,F5.3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F6.4,1X,F6.4,1X,F6.4,1X,
+ F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.2,1X,F4.2,
+ 1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,45
read(1,'(A201)')ar__1
read(ar__1,2)
+ Group(i__),NGC_1(i__),g_i(i__),E_g_i(i__),e_g_i_1(i__),
+ iMag(i__),E_iMag(i__),e_iMag_1(i__),CaT(i__),E_CaT(i__),
+ e_CaT_1(i__),Fe86(i__),E_Fe86(i__),e_Fe86_1(i__),Mg88(i__),
+ E_Mg88(i__),e_Mg88_1(i__),Na82(i__),E_Na82(i__),e_Na82_1(i__),
+ TiO89(i__),E_TiO89(i__),e_TiO89_1(i__),Halpha(i__),
+ E_Halpha(i__),e_Halpha_1(i__),PaT(i__),E_PaT(i__),
+ e_PaT_1(i__),sigma(i__),E_sigma(i__),e_sigma_1(i__)
if(ar__1(11:14) .EQ. '') NGC_1(i__) = iNULL__
if(ar__1(187:191) .EQ. '') sigma(i__) = rNULL__
if(ar__1(193:196) .EQ. '') E_sigma(i__) = rNULL__
if(ar__1(198:201) .EQ. '') e_sigma_1(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ Group(i__),NGC_1(i__),g_i(i__),E_g_i(i__),e_g_i_1(i__),
+ iMag(i__),E_iMag(i__),e_iMag_1(i__),CaT(i__),E_CaT(i__),
+ e_CaT_1(i__),Fe86(i__),E_Fe86(i__),e_Fe86_1(i__),Mg88(i__),
+ E_Mg88(i__),e_Mg88_1(i__),Na82(i__),E_Na82(i__),e_Na82_1(i__),
+ TiO89(i__),E_TiO89(i__),e_TiO89_1(i__),Halpha(i__),
+ E_Halpha(i__),e_Halpha_1(i__),PaT(i__),E_PaT(i__),
+ e_PaT_1(i__),sigma(i__),E_sigma(i__),e_sigma_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea2.dat' ! Colour and spectral index measurements of
* spectra stacked by colour for groups
C Format for file interpretation
3 format(
+ A6,4X,I4,1X,F6.4,1X,F6.4,1X,F6.4,1X,F7.3,1X,F5.3,1X,F5.3,1X,
+ F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,
+ 1X,F5.3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F6.4,1X,F6.4,1X,F6.4,1X,
+ F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.2,1X,F4.2,
+ 1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea2.dat')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,20
read(1,'(A201)')ar__2
read(ar__2,3)
+ Group_1(i__),NGC_2(i__),g_i_1(i__),E_g_i_2(i__),e_g_i_3(i__),
+ iMag_1(i__),E_iMag_2(i__),e_iMag_3(i__),CaT_1(i__),
+ E_CaT_2(i__),e_CaT_3(i__),Fe86_1(i__),E_Fe86_2(i__),
+ e_Fe86_3(i__),Mg88_1(i__),E_Mg88_2(i__),e_Mg88_3(i__),
+ Na82_1(i__),E_Na82_2(i__),e_Na82_3(i__),TiO89_1(i__),
+ E_TiO89_2(i__),e_TiO89_3(i__),Halpha_1(i__),E_Halpha_2(i__),
+ e_Halpha_3(i__),PaT_1(i__),E_PaT_2(i__),e_PaT_3(i__),
+ sigma_1(i__),E_sigma_2(i__),e_sigma_3(i__)
if(ar__2(11:14) .EQ. '') NGC_2(i__) = iNULL__
if(ar__2(187:191) .EQ. '') sigma_1(i__) = rNULL__
if(ar__2(193:196) .EQ. '') E_sigma_2(i__) = rNULL__
if(ar__2(198:201) .EQ. '') e_sigma_3(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ Group_1(i__),NGC_2(i__),g_i_1(i__),E_g_i_2(i__),e_g_i_3(i__),
+ iMag_1(i__),E_iMag_2(i__),e_iMag_3(i__),CaT_1(i__),
+ E_CaT_2(i__),e_CaT_3(i__),Fe86_1(i__),E_Fe86_2(i__),
+ e_Fe86_3(i__),Mg88_1(i__),E_Mg88_2(i__),e_Mg88_3(i__),
+ Na82_1(i__),E_Na82_2(i__),e_Na82_3(i__),TiO89_1(i__),
+ E_TiO89_2(i__),e_TiO89_3(i__),Halpha_1(i__),E_Halpha_2(i__),
+ e_Halpha_3(i__),PaT_1(i__),E_PaT_2(i__),e_PaT_3(i__),
+ sigma_1(i__),E_sigma_2(i__),e_sigma_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end