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                    *      BESANCON MODEL OF STELLAR POPULATION SYNTHESIS 2003-12
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  (l =    30.0; b =    0.0)  Distance  0.0 a  50.0 kpc;  Solid angle      0.020  square degree
  Adaptive step in distance  (20,30,50)
  SELECTIONS :
      Absolute magnitude:    -7.00 - 20.00
      Apparent magnitudes Band   V  :-99.00- 99.00
                          Band   B  :-99.00- 99.00
                          Band   U  :-99.00- 99.00
                          Band   R  :-99.00- 99.00
                          Band   I  :-99.00- 99.00
                          Band   J  :-99.00- 99.00
                          Band   H  :-99.00- 99.00
                          Band   K  :-10.00- 19.00
                          Band   L  :-99.00- 99.00
                          Band   12 :-99.00- 99.00
                          Band   15 :-99.00- 99.00

      Selection in age: from .00E9Gyr to Bulge
      Spectral types: O0.0 - D5.0  Luminosity class    : 1 - 7  logTeff: 3.00 -  6.00  Log g:        -3.00-        8.00
      Colour :  B-V      -99.00 -  99.00 Step    10.00
                U-B      -99.00 -  99.00 Step    10.00
                V-I      -99.00 -  99.00 Step    10.00
                V-K      -99.00 -  99.00 Step    10.00

      Proper motions mu(a)*cos(d), mu(d) ICRS  in "/cen, range [    0.0000- 1000.0000[. Errors as a fct of magnitude:  0.0000+  0.0000*mag +  0.0000*mag^2)
      Heliocentric Radial velocities: range [-500.0- 500.0[  Errors as a fct of magnitude    0.0000+  0.0000*mag +  0.0000*mag^2)
   Computation mode :
      Poisson drawings (ran1) for N <=  6
      Photometric error laws:   K : 0.000000E+00+mag*0.000000E+00+mag^2*0.000000E+00
                                B : 0.000000E+00+mag*0.000000E+00+mag^2*0.000000E+00
                                U : 0.000000E+00+mag*0.000000E+00+mag^2*0.000000E+00
                                V : 0.000000E+00+mag*0.000000E+00+mag^2*0.000000E+00
                                I : 0.000000E+00+mag*0.000000E+00+mag^2*0.000000E+00
      System:  Johnson-Cousins-IRAS VBURIJHKL+12+25  0.323  0.257  0.300  0.412  0.718  0.824  0.892  0.949  0.972  0.986
      Creation of a catalogue of simulated stars
  
   Evolution model parameters 
     Nb of tracks : 881 (with masses)                                               
     Low masses from Vandenberg                                                     
     Masses >1Msun Schaller et al.                                                  
     Type of disc luminosity function: Hipparcos                                    
     Integration time (Gyr):  10.000                                                
          SFR : SFR consta    , nu : 0.400                                          
     June08     IMF : slope x  0.6 (<0.20Msun) 0.6(<0.60Msun) 0.6 (<1Msun), 2 (>1Msu
     Bolometric corrections : Flower                                                
     Grid :   mag(sup, inf)=(-11.000 , 17.00 ) 10.000                               
          LogTeff(sup, inf)=(  3.400 ,  5.50 )100.000                               
       WD disc Wood 10Gyr Bergeron colors                                           
     Pop   2  bv923m3.lf   hb3m3.lf     Age= 11.0Gyr  x=-0.5  WD IMF Salpeter 12Gyr 
     Pop   3  bv923m4.lf   hb3m4.lf     Age= 14.0Gyr  x=-0.5  WD IMF2 14Gyr halo DA 
     #  Bulbe : BC95, IMF x= 1.35 Y=0.28 Z=0.02 Age 10.0 Gyr                        
  
        Simulation of the stellar content of the Galaxy                       
  
  DENSITY LAWS (distances in pc, densities in M0/PC3)
      Disc density law: Einasto; bulge Dwek G2; with warp and flare 
      Distance Sun - Galactic Center : 8500.00  Disc outer truncation :14000.00
      Sun position z_0  :15.00 Warp: starting position   8400.00 pc, angle  1.57080 radians, slope  0.18000 Flare: slope    0.5450E-06 starting position   9500.00 pc
      Disc scale length: Young disc: 5000.0 3000.0; Old disc: 2530.0 1320.0
      Disc excentricities : 0.0140 0.0268 0.0375 0.0551 0.0696 0.0785 0.0791
      Thick disc: Modified exponential    800.00 2500.00  400.00 density correction   1.000 White dwarfs: 0.50609E-03/pc3
      Spheroid: excentricity: 0.7600 exponent:  2.440 density correction   1.000 Halo white dwarfs: 0.28286E-03/pc3
      Interstellar matter: Einasto law: excentricity and scale lengths in pc 0.0140  7222.0  5777.0
      Disc mass density as a fct of age in M/pc3 :.003999  .007902  .006224  .004020  .005814  .004928  .006590
      Stellar densities in */pc3 for Mv<8 (disc, Th.Disc, Spheroid) :.154E-01  .103E-02  .794E-05  . White dwarfs:.660E-02  .506E-03  .283E-03
      Interstellar matter ( M/pc3) :.0210
  KINEMATICS :
      Disc velocity dispersions:
                   U :     16.7    19.8    27.2    30.2    36.7    43.1    43.1
                   V :     10.8    12.8    17.6    19.5    23.7    27.8    27.8
                   W :      6.0     8.0    10.0    13.2    15.8    17.4    17.5
      Thick disc, spheroid and bulge
                   U :     67.0   131.0   113.0
                   V :     51.0   106.0   115.0
                   W :     42.0    85.0   100.0
      Solar velocities U,V,W :    10.3     6.3     5.9
      Rotation velocities: thick disc:   176.0 spheroid:      0.0  bulge:    150.0 LSR :   226.4
      Radial velocity gradients on U (disc), U (bulge) W (in km/s/pc): -0.20E-03  0.00E+00  0.00E+00
      Spheroid ellipsoid pointing towards z axis
  
      bulge Dwek G2;    1.590/ 0.424/ 0.42(kpc)  alpha (deg) 78.90 gamma  91.27 beta   3.50 Normalisation    0.2544E+11 x   1.0000 Cutoff   2.54kpc

  METALLICITIES     .15E9  1. E9  2. E9  3. E9  5. E9  7. E9  10.E9  Th.D.  Spher  Bulge
      [FE/H]         0.01   0.03   0.03   0.01  -0.07  -0.14  -0.37  -0.78  -1.78   0.00
      Dispersion     0.12   0.12   0.10   0.11   0.18   0.17   0.20   0.30   0.50   0.40
      Gradient -    -0.07  -0.07  -0.07  -0.07  -0.07  -0.07  -0.07   0.00   0.00   0.00
      Gradient |     0.00   0.00   0.00   0.00   0.00   0.00   0.00   0.00   0.00   0.00
  Absorption at s.n. : 0.70 mag./kpc   0 clouds
  Dist    Mv  CL Typ  LTef  logg Age Mass  B-V    U-B    V-I    V-K    K        mux     muy        Vr    UU      VV      WW   [Fe/H] l           b         Av   Mbol
  0.111  9.70  5 7.15 3.570  4.78  2 0.52  1.428  1.226  1.927  3.907 11.022    0.298   -4.765  -19.69   -6.27  -28.53  -12.83  0.16  30.00000   0.00000  0.070  8.203
  0.131 13.80  5 7.65 3.492  5.05  3 0.17  1.765  1.458  3.027  5.382 14.171   -0.522   -4.318    7.45   19.10  -18.18   -9.34 -0.20  30.00000   0.00000  0.084 12.048
  0.151 15.00  5 7.71 3.469  5.13  2 0.12  1.837  1.615  3.409  6.235 14.736    2.649    2.617  -31.71  -40.09    6.02   -8.30  0.08  30.00000   0.00000  0.098 13.185
  0.191  9.60  5 7.15 3.572  4.78  5 0.54  1.488  1.244  1.922  4.031 12.155    0.114    0.251   30.52   25.19   17.41    0.12 -0.09  30.00000   0.00000  0.126  8.103
  0.290 15.10  5 7.74 3.467  5.12  6 0.12  1.940  1.696  3.491  6.138 16.554    0.798   -0.841   -4.94   -1.64   -7.05  -15.06 -0.10  30.00000   0.00000  0.198 13.253
 27.850  1.20  3 5.79 3.679  2.53  8 0.93  5.411  4.149  6.571 14.498 17.579   -0.075   -0.077   51.53  112.61  -91.99   41.40 -0.64  30.00000   0.00000 13.651  0.862
  Dist    Mv  CL Typ  LTef  logg Age Mass  B-V    U-B    V-I    V-K    K        mux     muy        Vr    UU      VV      WW   [Fe/H] l           b         Av   Mbol
  Star density before selection     2481586.567 after  theorical selection    2481586.282 Nb of stars generated      2482508
  Stars ejected by selection in mag :    2360904.0 in color :          0.0 in mu :          0.0 in Vrad :          0.0 total :    2360904.0 released stars:       121604


  TOTAL NUMBER OF STARS :    6

