Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/610/A30 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-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/A+A/610/A30 B stars in 4 open clusters (Aidelman+, 2018)
*================================================================================
*Open clusters: III.
*Fundamental parameters of B stars in NGC 6087, NGC 6250, NGC 6383, and NGC 6530.
*B-type stars with circumstellar envelopes.
* Aidelman Y., Cidale L.S., Zorec J., Panei J.A.
* <Astron. Astrophys. 610, A30 (2018)>
* =2018A&A...610A..30A (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Log of observations of low-resolution spectra
integer*4 nr__
parameter (nr__=68) ! Number of records
character*110 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs (Epoch=2000)
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000, Epoch=2000
real*8 DEdeg (nr__) ! (deg) Declination J2000, Epoch=2000
C ---------------------------------- ! (position vector(s) in degrees)
character*13 Cl (nr__) ! Open cluster name
integer*4 Star (nr__) ! ?=0 Star number within the cluster (G1)
character*15 OName (nr__) ! Other designation
integer*4 RAh (nr__) ! (h) Right ascension (Eq=J2000 (Ep=2000)
integer*4 RAm (nr__) ! (min) Right ascension (Eq=J2000 (Ep=2000)
real*4 RAs (nr__) ! (s) Right ascension (Eq=J2000 (Ep=2000)
character*1 DE_ (nr__) ! Declination sign (Eq=J2000, Ep=2000)
integer*4 DEd (nr__) ! (deg) Declination (Eq=J2000, Ep=2000)
integer*4 DEm (nr__) ! (arcmin) Declination (Eq=J2000, Ep=2000)
real*4 DEs (nr__) ! (arcsec) Declination (Eq=J2000, Ep=2000)
real*4 AM1 (nr__) ! Air mass of first observation
real*4 AM2 (nr__) ! ?=99.99 Air mass of second observation
real*4 AM3 (nr__) ! ?=99.99 Air mass of third observation
character*10 Date1 (nr__) ! ("date") Date of first observation
character*10 Date2 (nr__) ! ("date") Date of second observation
character*10 Date3 (nr__) ! ("date") Date of third observation
integer*4 N (nr__) ! Number of observations
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Log of observations of high-resolution spectra
integer*4 nr__1
parameter (nr__1=63) ! Number of records
character*110 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs (Epoch=2000)
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000, Epoch=2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000, Epoch=2000
C ---------------------------------- ! (position vector(s) in degrees)
character*13 Cl_1 (nr__1) ! Open cluster name
integer*4 Star_1 (nr__1) ! ?=0 Star number within the cluster (G1)
character*15 OName_1 (nr__1) ! Other designation
integer*4 RAh_1 (nr__1) ! (h) Right ascension (Eq=J2000 (Ep=2000)
integer*4 RAm_1 (nr__1) ! (min) Right ascension (Eq=J2000 (Ep=2000)
real*4 RAs_1 (nr__1) ! (s) Right ascension (Eq=J2000 (Ep=2000)
character*1 DE__1 (nr__1) ! Declination sign (Eq=J2000, Ep=2000)
integer*4 DEd_1 (nr__1) ! (deg) Declination (Eq=J2000, Ep=2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (Eq=J2000, Ep=2000)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (Eq=J2000, Ep=2000)
real*4 AM1_1 (nr__1) ! Air mass of first observation
real*4 AM2_1 (nr__1) ! ?=99.99 Air mass of second observation
real*4 AM3_1 (nr__1) ! ?=99.99 Air mass of third observation
character*10 Date1_1 (nr__1) ! ("date") Date of first observation
character*10 Date2_1 (nr__1) ! ("date") Date of second observation
character*10 Date3_1 (nr__1) ! ("date") Date of third observation
integer*4 N_1 (nr__1) ! Number of observations
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table9.dat' ! Stellar fundamental parameters for NGC 6087
integer*4 nr__2
parameter (nr__2=18) ! Number of records
character*120 ar__2 ! Full-size record
integer*4 Star_2 (nr__2) ! ?=0 Star number within the cluster (G1)
character*15 OName_2 (nr__2) ! Other designation
character*2 n_OName (nr__2) ! [dd ] Second Balmer Discontinuity (2)
real*4 D (nr__2) ! Photospheric component of the Balmer
* discontinuity
integer*4 lambda1 (nr__2) ! (0.1nm) ? Mean spectral position of the Balmer
* discontinuity
real*4 Phib (nr__2) ! (um) Observed color gradient
character*8 SpType (nr__2) ! Spectral type
character*13 n_SpType (nr__2) ! Other object types (3)
integer*4 Teff (nr__2) ! (K) Effective Temperature
character*2 n_Teff (nr__2) ! [man: ] Extrapolated values flag for Teff (4)
integer*4 e_Teff (nr__2) ! (K) Error in Effective Temperature
real*4 logg (nr__2) ! ([cm/s2]) Stellar surface gravity
character*2 n_logg (nr__2) ! [man: ] Extrapolated values flag for logg (4)
real*4 e_logg (nr__2) ! ([cm/s2]) Error in logg
real*4 VMAG (nr__2) ! (mag) Absolute Magnitude in V filter
character*2 n_VMAG (nr__2) ! [man: ] Extrapolated values flag for VMAG (4)
real*4 e_VMAG (nr__2) ! (mag) Error in Absolute Magnitude
real*4 Mbol (nr__2) ! (mag) Bolometric Magnitude
character*2 n_Mbol (nr__2) ! [man: ] Extrapolated values flag for Mbol (4)
real*4 e_Mbol (nr__2) ! (mag) Error in Bolometric Magnitude
real*4 Phi0 (nr__2) ! (um) Intrinsic color gradient
character*1 n_Phi0 (nr__2) ! [man: ] Extrapolated values flag fro Phi0 (4)
real*4 e_Phi0 (nr__2) ! (um) Error in Intrinsic color gradient
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Object types as follows:
* mk = Spectral types derived using the MK-system
* so = Spectral types derived using The Galactic O-Star Spectroscopic
* Survey Sota et al. (2011ApJS..193...24S, Cat. III/274)
* BE = Spectroscopic binary
* BE2 = Double line spectroscopic binary
* BEc = Eclipsing binary
* Be = Known Be star
* BS = Blue straggler star
* CP2 = Chemically peculiar star
* Em = Emission-line star
* Halpha = Star with emission in H{alpha}
* He = Helium star
* IR = Star with infrared excess
* MA = Magnetic Ap star
* p = Chemically peculiar star
* ST = Triple system
* V = Variable star
* VB = Reported as visual binary star
* Vr = Radial velocity variable
* Vv = Probable variable like Vega star
*Note (4): Extrapolated values flags as follows:
* a = Values interpolated from Cox & Pilachowski (2000PhT....53j..77C)
* m = Value calculated in this work, using a relation between Phi^0^_b_
* and (B-V)_0_ given by Moujtahid et al. (1998, Cat. J/A+AS/129/289)
* n = Stellar parameter given by Martins et al. (2005A&A...436.1049M)
*
* The symbol : is used to indicate extrapolated values.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table10.dat' ! Physical parameters and distance for NGC 6087
integer*4 nr__3
parameter (nr__3=18) ! Number of records
character*95 ar__3 ! Full-size record
integer*4 Star_3 (nr__3) ! ?=0 Star number within the cluster (G1)
character*15 OName_3 (nr__3) ! Other designation
character*2 n_OName_1 (nr__3) ! [dd ] Second Balmer Discontinuity (2)
real*4 Vmag_1 (nr__3) ! (mag) Visual magnitude in V filter (3)
real*4 E_B_V (nr__3) ! (mag) ?=99.99 Color excess (4)
real*4 e_E_B_V (nr__3) ! (mag) ?=99.99 Error in color excess
real*4 MOD (nr__3) ! (mag) True distance modulus
real*4 e_MOD (nr__3) ! (mag) Error in true distance modulus
character*3 Member (nr__3) ! Membership to the cluster (5)
real*4 AD (nr__3) ! (arcmin) Angular distance to the cluster center
real*4 Pmemb (nr__3) ! (%) Membership probability
real*4 logL (nr__3) ! ([Lsun]) ? Luminosity
real*4 e_logL (nr__3) ! ([Lsun]) ? Error in luminosity
real*4 Mass (nr__3) ! (Msun) ? Stellar mass
real*4 e_Mass (nr__3) ! (Msun) ? Error in stellar mass
integer*4 Age (nr__3) ! (Ma) ? Age of the star
real*4 e_Age (nr__3) ! (Ma) ? Error in age of the star
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Vmag values obtained from SIMBAD database
*Note (4): The distances of the stars with negative color gradients were
* determined using the distance modulus assigned to the cluster
*Note (5): Membership to the cluster codes as follows:
* m = Member stars
* pm = Probable member stars
* pnm = Probable non-member stars
* nm = Non-member stars
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table11.dat' ! Stellar fundamental parameters for NGC 6250
integer*4 nr__4
parameter (nr__4=15) ! Number of records
character*120 ar__4 ! Full-size record
integer*4 Star_4 (nr__4) ! ?=0 Star number within the cluster (G1)
character*15 OName_4 (nr__4) ! Other designation
character*2 n_OName_2 (nr__4) ! [dd ] Second Balmer Discontinuity (2)
real*4 D_1 (nr__4) ! Photospheric component of the Balmer
* discontinuity
integer*4 lambda1_1 (nr__4) ! (0.1nm) ? Mean spectral position of the Balmer
* discontinuity
real*4 Phib_1 (nr__4) ! (um) Observed color gradient
character*8 SpType_1 (nr__4) ! Spectral type
character*13 n_SpType_1 (nr__4) ! Other object types (3)
integer*4 Teff_1 (nr__4) ! (K) Effective Temperature
character*2 n_Teff_1 (nr__4) ! [man: ] Extrapolated values flag for Teff (4)
integer*4 e_Teff_1 (nr__4) ! (K) Error in Effective Temperature
real*4 logg_1 (nr__4) ! ([cm/s2]) Stellar surface gravity
character*2 n_logg_1 (nr__4) ! [man: ] Extrapolated values flag for logg (4)
real*4 e_logg_1 (nr__4) ! ([cm/s2]) Error in logg
real*4 VMAG_2 (nr__4) ! (mag) Absolute Magnitude in V filter
character*2 n_VMAG_1 (nr__4) ! [man: ] Extrapolated values flag for VMAG (4)
real*4 e_VMAG_1 (nr__4) ! (mag) Error in Absolute Magnitude
real*4 Mbol_1 (nr__4) ! (mag) Bolometric Magnitude
character*2 n_Mbol_1 (nr__4) ! [man: ] Extrapolated values flag for Mbol (4)
real*4 e_Mbol_1 (nr__4) ! (mag) Error in Bolometric Magnitude
real*4 Phi0_1 (nr__4) ! (um) Intrinsic color gradient
character*1 n_Phi0_1 (nr__4) ! [man: ] Extrapolated values flag fro Phi0 (4)
real*4 e_Phi0_1 (nr__4) ! (um) Error in Intrinsic color gradient
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Object types as follows:
* mk = Spectral types derived using the MK-system
* so = Spectral types derived using The Galactic O-Star Spectroscopic
* Survey Sota et al. (2011ApJS..193...24S, Cat. III/274)
* BE = Spectroscopic binary
* BE2 = Double line spectroscopic binary
* BEc = Eclipsing binary
* Be = Known Be star
* BS = Blue straggler star
* CP2 = Chemically peculiar star
* Em = Emission-line star
* Halpha = Star with emission in H{alpha}
* He = Helium star
* IR = Star with infrared excess
* MA = Magnetic Ap star
* p = Chemically peculiar star
* ST = Triple system
* V = Variable star
* VB = Reported as visual binary star
* Vr = Radial velocity variable
* Vv = Probable variable like Vega star
*Note (4): Extrapolated values flags as follows:
* a = Values interpolated from Cox & Pilachowski (2000PhT....53j..77C)
* m = Value calculated in this work, using a relation between Phi^0^_b_
* and (B-V)_0_ given by Moujtahid et al. (1998, Cat. J/A+AS/129/289)
* n = Stellar parameter given by Martins et al. (2005A&A...436.1049M)
*
* The symbol : is used to indicate extrapolated values.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table12.dat' ! Physical parameters and distance for NGC 6250
integer*4 nr__5
parameter (nr__5=15) ! Number of records
character*95 ar__5 ! Full-size record
integer*4 Star_5 (nr__5) ! ?=0 Star number within the cluster (G1)
character*15 OName_5 (nr__5) ! Other designation
character*2 n_OName_3 (nr__5) ! [dd ] Second Balmer Discontinuity (2)
real*4 Vmag_3 (nr__5) ! (mag) Visual magnitude in V filter (3)
real*4 E_B_V_1 (nr__5) ! (mag) ?=99.99 Color excess (4)
real*4 e_E_B_V_1 (nr__5) ! (mag) ?=99.99 Error in color excess
real*4 MOD_1 (nr__5) ! (mag) True distance modulus
real*4 e_MOD_1 (nr__5) ! (mag) Error in true distance modulus
character*3 Member_1 (nr__5) ! Membership to the cluster (5)
real*4 AD_1 (nr__5) ! (arcmin) Angular distance to the cluster center
real*4 Pmemb_1 (nr__5) ! (%) Membership probability
real*4 logL_1 (nr__5) ! ([Lsun]) ? Luminosity
real*4 e_logL_1 (nr__5) ! ([Lsun]) ? Error in luminosity
real*4 Mass_1 (nr__5) ! (Msun) ? Stellar mass
real*4 e_Mass_1 (nr__5) ! (Msun) ? Error in stellar mass
integer*4 Age_1 (nr__5) ! (Ma) ? Age of the star
real*4 e_Age_1 (nr__5) ! (Ma) ? Error in age of the star
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Vmag values obtained from SIMBAD database
*Note (4): The distances of the stars with negative color gradients were
* determined using the distance modulus assigned to the cluster
*Note (5): Membership to the cluster codes as follows:
* m = Member stars
* pm = Probable member stars
* pnm = Probable non-member stars
* nm = Non-member stars
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table13.dat' ! Stellar fundamental parameters for NGC 6383
integer*4 nr__6
parameter (nr__6=12) ! Number of records
character*120 ar__6 ! Full-size record
integer*4 Star_6 (nr__6) ! ?=0 Star number within the cluster (G1)
character*15 OName_6 (nr__6) ! Other designation
character*2 n_OName_4 (nr__6) ! [dd ] Second Balmer Discontinuity (2)
real*4 D_2 (nr__6) ! Photospheric component of the Balmer
* discontinuity
integer*4 lambda1_2 (nr__6) ! (0.1nm) ? Mean spectral position of the Balmer
* discontinuity
real*4 Phib_2 (nr__6) ! (um) Observed color gradient
character*8 SpType_2 (nr__6) ! Spectral type
character*13 n_SpType_2 (nr__6) ! Other object types (3)
integer*4 Teff_2 (nr__6) ! (K) Effective Temperature
character*2 n_Teff_2 (nr__6) ! [man: ] Extrapolated values flag for Teff (4)
integer*4 e_Teff_2 (nr__6) ! (K) Error in Effective Temperature
real*4 logg_2 (nr__6) ! ([cm/s2]) Stellar surface gravity
character*2 n_logg_2 (nr__6) ! [man: ] Extrapolated values flag for logg (4)
real*4 e_logg_2 (nr__6) ! ([cm/s2]) Error in logg
real*4 VMAG_4 (nr__6) ! (mag) Absolute Magnitude in V filter
character*2 n_VMAG_2 (nr__6) ! [man: ] Extrapolated values flag for VMAG (4)
real*4 e_VMAG_2 (nr__6) ! (mag) Error in Absolute Magnitude
real*4 Mbol_2 (nr__6) ! (mag) Bolometric Magnitude
character*2 n_Mbol_2 (nr__6) ! [man: ] Extrapolated values flag for Mbol (4)
real*4 e_Mbol_2 (nr__6) ! (mag) Error in Bolometric Magnitude
real*4 Phi0_2 (nr__6) ! (um) Intrinsic color gradient
character*1 n_Phi0_2 (nr__6) ! [man: ] Extrapolated values flag fro Phi0 (4)
real*4 e_Phi0_2 (nr__6) ! (um) Error in Intrinsic color gradient
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Object types as follows:
* mk = Spectral types derived using the MK-system
* so = Spectral types derived using The Galactic O-Star Spectroscopic
* Survey Sota et al. (2011ApJS..193...24S, Cat. III/274)
* BE = Spectroscopic binary
* BE2 = Double line spectroscopic binary
* BEc = Eclipsing binary
* Be = Known Be star
* BS = Blue straggler star
* CP2 = Chemically peculiar star
* Em = Emission-line star
* Halpha = Star with emission in H{alpha}
* He = Helium star
* IR = Star with infrared excess
* MA = Magnetic Ap star
* p = Chemically peculiar star
* ST = Triple system
* V = Variable star
* VB = Reported as visual binary star
* Vr = Radial velocity variable
* Vv = Probable variable like Vega star
*Note (4): Extrapolated values flags as follows:
* a = Values interpolated from Cox & Pilachowski (2000PhT....53j..77C)
* m = Value calculated in this work, using a relation between Phi^0^_b_
* and (B-V)_0_ given by Moujtahid et al. (1998, Cat. J/A+AS/129/289)
* n = Stellar parameter given by Martins et al. (2005A&A...436.1049M)
*
* The symbol : is used to indicate extrapolated values.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table14.dat' ! Physical parameters and distance for NGC 6383
integer*4 nr__7
parameter (nr__7=12) ! Number of records
character*95 ar__7 ! Full-size record
integer*4 Star_7 (nr__7) ! ?=0 Star number within the cluster (G1)
character*15 OName_7 (nr__7) ! Other designation
character*2 n_OName_5 (nr__7) ! [dd ] Second Balmer Discontinuity (2)
real*4 Vmag_5 (nr__7) ! (mag) Visual magnitude in V filter (3)
real*4 E_B_V_1 (nr__7) ! (mag) ?=99.99 Color excess (4)
real*4 e_E_B_V_1 (nr__7) ! (mag) ?=99.99 Error in color excess
real*4 MOD_2 (nr__7) ! (mag) True distance modulus
real*4 e_MOD_2 (nr__7) ! (mag) Error in true distance modulus
character*3 Member_2 (nr__7) ! Membership to the cluster (5)
real*4 AD_2 (nr__7) ! (arcmin) Angular distance to the cluster center
real*4 Pmemb_2 (nr__7) ! (%) Membership probability
real*4 logL_2 (nr__7) ! ([Lsun]) ? Luminosity
real*4 e_logL_2 (nr__7) ! ([Lsun]) ? Error in luminosity
real*4 Mass_2 (nr__7) ! (Msun) ? Stellar mass
real*4 e_Mass_2 (nr__7) ! (Msun) ? Error in stellar mass
integer*4 Age_2 (nr__7) ! (Ma) ? Age of the star
real*4 e_Age_2 (nr__7) ! (Ma) ? Error in age of the star
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Vmag values obtained from SIMBAD database
*Note (4): The distances of the stars with negative color gradients were
* determined using the distance modulus assigned to the cluster
*Note (5): Membership to the cluster codes as follows:
* m = Member stars
* pm = Probable member stars
* pnm = Probable non-member stars
* nm = Non-member stars
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table15.dat' ! Stellar fundamental parameters for NGC 6530
integer*4 nr__8
parameter (nr__8=23) ! Number of records
character*120 ar__8 ! Full-size record
integer*4 Star_8 (nr__8) ! ?=0 Star number within the cluster (G1)
character*15 OName_8 (nr__8) ! Other designation
character*2 n_OName_6 (nr__8) ! [dd ] Second Balmer Discontinuity (2)
real*4 D_3 (nr__8) ! Photospheric component of the Balmer
* discontinuity
integer*4 lambda1_3 (nr__8) ! (0.1nm) ? Mean spectral position of the Balmer
* discontinuity
real*4 Phib_3 (nr__8) ! (um) Observed color gradient
character*8 SpType_3 (nr__8) ! Spectral type
character*13 n_SpType_3 (nr__8) ! Other object types (3)
integer*4 Teff_3 (nr__8) ! (K) Effective Temperature
character*2 n_Teff_3 (nr__8) ! [man: ] Extrapolated values flag for Teff (4)
integer*4 e_Teff_3 (nr__8) ! (K) Error in Effective Temperature
real*4 logg_3 (nr__8) ! ([cm/s2]) Stellar surface gravity
character*2 n_logg_3 (nr__8) ! [man: ] Extrapolated values flag for logg (4)
real*4 e_logg_3 (nr__8) ! ([cm/s2]) Error in logg
real*4 VMAG_6 (nr__8) ! (mag) Absolute Magnitude in V filter
character*2 n_VMAG_3 (nr__8) ! [man: ] Extrapolated values flag for VMAG (4)
real*4 e_VMAG_3 (nr__8) ! (mag) Error in Absolute Magnitude
real*4 Mbol_3 (nr__8) ! (mag) Bolometric Magnitude
character*2 n_Mbol_3 (nr__8) ! [man: ] Extrapolated values flag for Mbol (4)
real*4 e_Mbol_3 (nr__8) ! (mag) Error in Bolometric Magnitude
real*4 Phi0_3 (nr__8) ! (um) Intrinsic color gradient
character*1 n_Phi0_3 (nr__8) ! [man: ] Extrapolated values flag fro Phi0 (4)
real*4 e_Phi0_3 (nr__8) ! (um) Error in Intrinsic color gradient
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Object types as follows:
* mk = Spectral types derived using the MK-system
* so = Spectral types derived using The Galactic O-Star Spectroscopic
* Survey Sota et al. (2011ApJS..193...24S, Cat. III/274)
* BE = Spectroscopic binary
* BE2 = Double line spectroscopic binary
* BEc = Eclipsing binary
* Be = Known Be star
* BS = Blue straggler star
* CP2 = Chemically peculiar star
* Em = Emission-line star
* Halpha = Star with emission in H{alpha}
* He = Helium star
* IR = Star with infrared excess
* MA = Magnetic Ap star
* p = Chemically peculiar star
* ST = Triple system
* V = Variable star
* VB = Reported as visual binary star
* Vr = Radial velocity variable
* Vv = Probable variable like Vega star
*Note (4): Extrapolated values flags as follows:
* a = Values interpolated from Cox & Pilachowski (2000PhT....53j..77C)
* m = Value calculated in this work, using a relation between Phi^0^_b_
* and (B-V)_0_ given by Moujtahid et al. (1998, Cat. J/A+AS/129/289)
* n = Stellar parameter given by Martins et al. (2005A&A...436.1049M)
*
* The symbol : is used to indicate extrapolated values.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table16.dat' ! Physical parameters and distance for NGC 6530
integer*4 nr__9
parameter (nr__9=23) ! Number of records
character*95 ar__9 ! Full-size record
integer*4 Star_9 (nr__9) ! ?=0 Star number within the cluster (G1)
character*15 OName_9 (nr__9) ! Other designation
character*2 n_OName_7 (nr__9) ! [dd ] Second Balmer Discontinuity (2)
real*4 Vmag_7 (nr__9) ! (mag) Visual magnitude in V filter (3)
real*4 E_B_V_1 (nr__9) ! (mag) ?=99.99 Color excess (4)
real*4 e_E_B_V_1 (nr__9) ! (mag) ?=99.99 Error in color excess
real*4 MOD_3 (nr__9) ! (mag) True distance modulus
real*4 e_MOD_3 (nr__9) ! (mag) Error in true distance modulus
character*3 Member_3 (nr__9) ! Membership to the cluster (5)
real*4 AD_3 (nr__9) ! (arcmin) Angular distance to the cluster center
real*4 Pmemb_3 (nr__9) ! (%) Membership probability
real*4 logL_3 (nr__9) ! ([Lsun]) ? Luminosity
real*4 e_logL_3 (nr__9) ! ([Lsun]) ? Error in luminosity
real*4 Mass_3 (nr__9) ! (Msun) ? Stellar mass
real*4 e_Mass_3 (nr__9) ! (Msun) ? Error in stellar mass
integer*4 Age_3 (nr__9) ! (Ma) ? Age of the star
real*4 e_Age_3 (nr__9) ! (Ma) ? Error in age of the star
*Note (2): Flag as follows:
* dd = Star with a Second Balmer Discontinuity
*Note (3): Vmag values obtained from SIMBAD database
*Note (4): The distances of the stars with negative color gradients were
* determined using the distance modulus assigned to the cluster
*Note (5): Membership to the cluster codes as follows:
* m = Member stars
* pm = Probable member stars
* pnm = Probable non-member stars
* nm = Non-member stars
C=============================================================================
C Loading file 'table1.dat' ! Log of observations of low-resolution spectra
C Format for file interpretation
1 format(
+ A13,1X,I3,1X,A15,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,
+ 1X,F4.2,1X,F5.2,1X,F5.2,1X,A10,1X,A10,1X,A10,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,68
read(1,'(A110)')ar__
read(ar__,1)
+ Cl(i__),Star(i__),OName(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),AM1(i__),AM2(i__),
+ AM3(i__),Date1(i__),Date2(i__),Date3(i__),N(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)
+ Cl(i__),Star(i__),OName(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),AM1(i__),AM2(i__),
+ AM3(i__),Date1(i__),Date2(i__),Date3(i__),N(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 'table2.dat' ! Log of observations of high-resolution spectra
C Format for file interpretation
2 format(
+ A13,1X,I3,1X,A15,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,
+ 1X,F4.2,1X,F5.2,1X,F5.2,1X,A10,1X,A10,1X,A10,1X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,63
read(1,'(A110)')ar__1
read(ar__1,2)
+ Cl_1(i__),Star_1(i__),OName_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ AM1_1(i__),AM2_1(i__),AM3_1(i__),Date1_1(i__),Date2_1(i__),
+ Date3_1(i__),N_1(i__)
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)
+ Cl_1(i__),Star_1(i__),OName_1(i__),RAh_1(i__),RAm_1(i__),
+ RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
+ AM1_1(i__),AM2_1(i__),AM3_1(i__),Date1_1(i__),Date2_1(i__),
+ Date3_1(i__),N_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 'table9.dat' ! Stellar fundamental parameters for NGC 6087
C Format for file interpretation
3 format(
+ I3,1X,A15,1X,A2,1X,F4.2,1X,I2,1X,F4.2,1X,A8,1X,A13,1X,I5,A2,
+ 1X,I4,1X,F4.2,A2,1X,F4.2,1X,F5.2,A2,1X,F4.2,1X,F5.2,A2,1X,
+ F4.2,1X,F4.2,A1,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table9.dat')
write(6,*) '....Loading file: table9.dat'
do i__=1,18
read(1,'(A120)')ar__2
read(ar__2,3)
+ Star_2(i__),OName_2(i__),n_OName(i__),D(i__),lambda1(i__),
+ Phib(i__),SpType(i__),n_SpType(i__),Teff(i__),n_Teff(i__),
+ e_Teff(i__),logg(i__),n_logg(i__),e_logg(i__),VMAG(i__),
+ n_VMAG(i__),e_VMAG(i__),Mbol(i__),n_Mbol(i__),e_Mbol(i__),
+ Phi0(i__),n_Phi0(i__),e_Phi0(i__)
if(ar__2(29:30) .EQ. '') lambda1(i__) = iNULL__
c ..............Just test output...........
write(6,3)
+ Star_2(i__),OName_2(i__),n_OName(i__),D(i__),lambda1(i__),
+ Phib(i__),SpType(i__),n_SpType(i__),Teff(i__),n_Teff(i__),
+ e_Teff(i__),logg(i__),n_logg(i__),e_logg(i__),VMAG(i__),
+ n_VMAG(i__),e_VMAG(i__),Mbol(i__),n_Mbol(i__),e_Mbol(i__),
+ Phi0(i__),n_Phi0(i__),e_Phi0(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table10.dat' ! Physical parameters and distance for NGC 6087
C Format for file interpretation
4 format(
+ I3,1X,A15,1X,A2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F3.1,1X,A3,
+ 1X,F6.2,1X,F5.1,1X,F3.1,1X,F3.1,1X,F5.1,1X,F4.1,1X,I3,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table10.dat')
write(6,*) '....Loading file: table10.dat'
do i__=1,18
read(1,'(A95)')ar__3
read(ar__3,4)
+ Star_3(i__),OName_3(i__),n_OName_1(i__),Vmag_1(i__),
+ E_B_V(i__),e_E_B_V(i__),MOD(i__),e_MOD(i__),Member(i__),
+ AD(i__),Pmemb(i__),logL(i__),e_logL(i__),Mass(i__),
+ e_Mass(i__),Age(i__),e_Age(i__)
if(ar__3(68:70) .EQ. '') logL(i__) = rNULL__
if(ar__3(72:74) .EQ. '') e_logL(i__) = rNULL__
if(ar__3(76:80) .EQ. '') Mass(i__) = rNULL__
if(ar__3(82:85) .EQ. '') e_Mass(i__) = rNULL__
if(ar__3(87:89) .EQ. '') Age(i__) = iNULL__
if(ar__3(91:95) .EQ. '') e_Age(i__) = rNULL__
c ..............Just test output...........
write(6,4)
+ Star_3(i__),OName_3(i__),n_OName_1(i__),Vmag_1(i__),
+ E_B_V(i__),e_E_B_V(i__),MOD(i__),e_MOD(i__),Member(i__),
+ AD(i__),Pmemb(i__),logL(i__),e_logL(i__),Mass(i__),
+ e_Mass(i__),Age(i__),e_Age(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table11.dat' ! Stellar fundamental parameters for NGC 6250
C Format for file interpretation
5 format(
+ I3,1X,A15,1X,A2,1X,F4.2,1X,I2,1X,F4.2,1X,A8,1X,A13,1X,I5,A2,
+ 1X,I4,1X,F4.2,A2,1X,F4.2,1X,F5.2,A2,1X,F4.2,1X,F5.2,A2,1X,
+ F4.2,1X,F4.2,A1,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table11.dat')
write(6,*) '....Loading file: table11.dat'
do i__=1,15
read(1,'(A120)')ar__4
read(ar__4,5)
+ Star_4(i__),OName_4(i__),n_OName_2(i__),D_1(i__),
+ lambda1_1(i__),Phib_1(i__),SpType_1(i__),n_SpType_1(i__),
+ Teff_1(i__),n_Teff_1(i__),e_Teff_1(i__),logg_1(i__),
+ n_logg_1(i__),e_logg_1(i__),VMAG_2(i__),n_VMAG_1(i__),
+ e_VMAG_1(i__),Mbol_1(i__),n_Mbol_1(i__),e_Mbol_1(i__),
+ Phi0_1(i__),n_Phi0_1(i__),e_Phi0_1(i__)
if(ar__4(29:30) .EQ. '') lambda1_1(i__) = iNULL__
c ..............Just test output...........
write(6,5)
+ Star_4(i__),OName_4(i__),n_OName_2(i__),D_1(i__),
+ lambda1_1(i__),Phib_1(i__),SpType_1(i__),n_SpType_1(i__),
+ Teff_1(i__),n_Teff_1(i__),e_Teff_1(i__),logg_1(i__),
+ n_logg_1(i__),e_logg_1(i__),VMAG_2(i__),n_VMAG_1(i__),
+ e_VMAG_1(i__),Mbol_1(i__),n_Mbol_1(i__),e_Mbol_1(i__),
+ Phi0_1(i__),n_Phi0_1(i__),e_Phi0_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table12.dat' ! Physical parameters and distance for NGC 6250
C Format for file interpretation
6 format(
+ I3,1X,A15,1X,A2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F3.1,1X,A3,
+ 1X,F6.2,1X,F5.1,1X,F3.1,1X,F3.1,1X,F5.1,1X,F4.1,1X,I3,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table12.dat')
write(6,*) '....Loading file: table12.dat'
do i__=1,15
read(1,'(A95)')ar__5
read(ar__5,6)
+ Star_5(i__),OName_5(i__),n_OName_3(i__),Vmag_3(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_1(i__),e_MOD_1(i__),
+ Member_1(i__),AD_1(i__),Pmemb_1(i__),logL_1(i__),
+ e_logL_1(i__),Mass_1(i__),e_Mass_1(i__),Age_1(i__),
+ e_Age_1(i__)
if(ar__5(68:70) .EQ. '') logL_1(i__) = rNULL__
if(ar__5(72:74) .EQ. '') e_logL_1(i__) = rNULL__
if(ar__5(76:80) .EQ. '') Mass_1(i__) = rNULL__
if(ar__5(82:85) .EQ. '') e_Mass_1(i__) = rNULL__
if(ar__5(87:89) .EQ. '') Age_1(i__) = iNULL__
if(ar__5(91:95) .EQ. '') e_Age_1(i__) = rNULL__
c ..............Just test output...........
write(6,6)
+ Star_5(i__),OName_5(i__),n_OName_3(i__),Vmag_3(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_1(i__),e_MOD_1(i__),
+ Member_1(i__),AD_1(i__),Pmemb_1(i__),logL_1(i__),
+ e_logL_1(i__),Mass_1(i__),e_Mass_1(i__),Age_1(i__),
+ e_Age_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table13.dat' ! Stellar fundamental parameters for NGC 6383
C Format for file interpretation
7 format(
+ I3,1X,A15,1X,A2,1X,F4.2,1X,I2,1X,F4.2,1X,A8,1X,A13,1X,I5,A2,
+ 1X,I4,1X,F4.2,A2,1X,F4.2,1X,F5.2,A2,1X,F4.2,1X,F5.2,A2,1X,
+ F4.2,1X,F4.2,A1,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table13.dat')
write(6,*) '....Loading file: table13.dat'
do i__=1,12
read(1,'(A120)')ar__6
read(ar__6,7)
+ Star_6(i__),OName_6(i__),n_OName_4(i__),D_2(i__),
+ lambda1_2(i__),Phib_2(i__),SpType_2(i__),n_SpType_2(i__),
+ Teff_2(i__),n_Teff_2(i__),e_Teff_2(i__),logg_2(i__),
+ n_logg_2(i__),e_logg_2(i__),VMAG_4(i__),n_VMAG_2(i__),
+ e_VMAG_2(i__),Mbol_2(i__),n_Mbol_2(i__),e_Mbol_2(i__),
+ Phi0_2(i__),n_Phi0_2(i__),e_Phi0_2(i__)
if(ar__6(29:30) .EQ. '') lambda1_2(i__) = iNULL__
c ..............Just test output...........
write(6,7)
+ Star_6(i__),OName_6(i__),n_OName_4(i__),D_2(i__),
+ lambda1_2(i__),Phib_2(i__),SpType_2(i__),n_SpType_2(i__),
+ Teff_2(i__),n_Teff_2(i__),e_Teff_2(i__),logg_2(i__),
+ n_logg_2(i__),e_logg_2(i__),VMAG_4(i__),n_VMAG_2(i__),
+ e_VMAG_2(i__),Mbol_2(i__),n_Mbol_2(i__),e_Mbol_2(i__),
+ Phi0_2(i__),n_Phi0_2(i__),e_Phi0_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table14.dat' ! Physical parameters and distance for NGC 6383
C Format for file interpretation
8 format(
+ I3,1X,A15,1X,A2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F3.1,1X,A3,
+ 1X,F6.2,1X,F5.1,1X,F3.1,1X,F3.1,1X,F5.1,1X,F4.1,1X,I3,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table14.dat')
write(6,*) '....Loading file: table14.dat'
do i__=1,12
read(1,'(A95)')ar__7
read(ar__7,8)
+ Star_7(i__),OName_7(i__),n_OName_5(i__),Vmag_5(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_2(i__),e_MOD_2(i__),
+ Member_2(i__),AD_2(i__),Pmemb_2(i__),logL_2(i__),
+ e_logL_2(i__),Mass_2(i__),e_Mass_2(i__),Age_2(i__),
+ e_Age_2(i__)
if(ar__7(68:70) .EQ. '') logL_2(i__) = rNULL__
if(ar__7(72:74) .EQ. '') e_logL_2(i__) = rNULL__
if(ar__7(76:80) .EQ. '') Mass_2(i__) = rNULL__
if(ar__7(82:85) .EQ. '') e_Mass_2(i__) = rNULL__
if(ar__7(87:89) .EQ. '') Age_2(i__) = iNULL__
if(ar__7(91:95) .EQ. '') e_Age_2(i__) = rNULL__
c ..............Just test output...........
write(6,8)
+ Star_7(i__),OName_7(i__),n_OName_5(i__),Vmag_5(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_2(i__),e_MOD_2(i__),
+ Member_2(i__),AD_2(i__),Pmemb_2(i__),logL_2(i__),
+ e_logL_2(i__),Mass_2(i__),e_Mass_2(i__),Age_2(i__),
+ e_Age_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table15.dat' ! Stellar fundamental parameters for NGC 6530
C Format for file interpretation
9 format(
+ I3,1X,A15,1X,A2,1X,F4.2,1X,I2,1X,F4.2,1X,A8,1X,A13,1X,I5,A2,
+ 1X,I4,1X,F4.2,A2,1X,F4.2,1X,F5.2,A2,1X,F4.2,1X,F5.2,A2,1X,
+ F4.2,1X,F4.2,A1,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table15.dat')
write(6,*) '....Loading file: table15.dat'
do i__=1,23
read(1,'(A120)')ar__8
read(ar__8,9)
+ Star_8(i__),OName_8(i__),n_OName_6(i__),D_3(i__),
+ lambda1_3(i__),Phib_3(i__),SpType_3(i__),n_SpType_3(i__),
+ Teff_3(i__),n_Teff_3(i__),e_Teff_3(i__),logg_3(i__),
+ n_logg_3(i__),e_logg_3(i__),VMAG_6(i__),n_VMAG_3(i__),
+ e_VMAG_3(i__),Mbol_3(i__),n_Mbol_3(i__),e_Mbol_3(i__),
+ Phi0_3(i__),n_Phi0_3(i__),e_Phi0_3(i__)
if(ar__8(29:30) .EQ. '') lambda1_3(i__) = iNULL__
c ..............Just test output...........
write(6,9)
+ Star_8(i__),OName_8(i__),n_OName_6(i__),D_3(i__),
+ lambda1_3(i__),Phib_3(i__),SpType_3(i__),n_SpType_3(i__),
+ Teff_3(i__),n_Teff_3(i__),e_Teff_3(i__),logg_3(i__),
+ n_logg_3(i__),e_logg_3(i__),VMAG_6(i__),n_VMAG_3(i__),
+ e_VMAG_3(i__),Mbol_3(i__),n_Mbol_3(i__),e_Mbol_3(i__),
+ Phi0_3(i__),n_Phi0_3(i__),e_Phi0_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table16.dat' ! Physical parameters and distance for NGC 6530
C Format for file interpretation
10 format(
+ I3,1X,A15,1X,A2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,1X,F3.1,1X,A3,
+ 1X,F6.2,1X,F5.1,1X,F3.1,1X,F3.1,1X,F5.1,1X,F4.1,1X,I3,1X,F5.1)
C Effective file loading
open(unit=1,status='old',file=
+'table16.dat')
write(6,*) '....Loading file: table16.dat'
do i__=1,23
read(1,'(A95)')ar__9
read(ar__9,10)
+ Star_9(i__),OName_9(i__),n_OName_7(i__),Vmag_7(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_3(i__),e_MOD_3(i__),
+ Member_3(i__),AD_3(i__),Pmemb_3(i__),logL_3(i__),
+ e_logL_3(i__),Mass_3(i__),e_Mass_3(i__),Age_3(i__),
+ e_Age_3(i__)
if(ar__9(68:70) .EQ. '') logL_3(i__) = rNULL__
if(ar__9(72:74) .EQ. '') e_logL_3(i__) = rNULL__
if(ar__9(76:80) .EQ. '') Mass_3(i__) = rNULL__
if(ar__9(82:85) .EQ. '') e_Mass_3(i__) = rNULL__
if(ar__9(87:89) .EQ. '') Age_3(i__) = iNULL__
if(ar__9(91:95) .EQ. '') e_Age_3(i__) = rNULL__
c ..............Just test output...........
write(6,10)
+ Star_9(i__),OName_9(i__),n_OName_7(i__),Vmag_7(i__),
+ E_B_V_1(i__),e_E_B_V_1(i__),MOD_3(i__),e_MOD_3(i__),
+ Member_3(i__),AD_3(i__),Pmemb_3(i__),logL_3(i__),
+ e_logL_3(i__),Mass_3(i__),e_Mass_3(i__),Age_3(i__),
+ e_Age_3(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end