The bernardi.tab*.dat tables list the following quantities:

I) bernardi.tab1.dat

1) the spectrum ID 
2) the ID of the redshift bin used to define which galaxies contribute to 
   the co-added spectrum (z_ID = 1 for 0.05 < z_gal < 0.07; 2 for  
   0.07 < z_gal < 0.09; 3 for 0.09 < z_gal < 0.12; 4 for 0.12 < z_gal < 0.14);
3) the mean redshift of the galaxies which made that composite;
4) the ID of the magnitude (r-band) bin used to define which galaxies 
   contribute to the co-added spectrum (mag_ID = 1 for -19.5 < absmag_r < -20;
   2 for -20 < absmag_r < -20.5, .... 9 for -23.5 < absmag_r < -24);
5) the mean absolute magnitude in the r-band of the galaxies which made that 
   composite (corrected for evolution following the results of 
   Bernardi et al. 2003b: absmag_corr=absmag_nocorr+0.85*z);
6) the mean absolute magnitude in the i-band of the galaxies which made that 
   composite (corrected for evolution: absmag_corr=absmag_nocorr+0.75*z);
7) the ID of the velocity dispersion bin used to define which galaxies 
   contribute to the co-added spectrum (sigma_ID = 1 for 2.00 < logsig < 2.05;
   2 for 2.05 < logsig < 2.10;  ..... 11 for 2.50 < logsig < 2.55, where 
   logsig is Log_{10} sigma [km/s]);
8) the mean velocity dispersion of the galaxies which made that composite;
9) the ID of the effective radius (r-band) bin used to define which galaxies 
   contribute to the co-added spectrum (Re_ID = 0.00 < logre < 0.10; 
   2 for 0.10 < logre < 0.20; ..... 11 for 1.00 < logre < 1.10, where logre 
   is Log_{10} Re [Kpc h^{-1}])
10) the mean effective radius (r-band) of the galaxies which made that 
    composite;
11) the mean color g-r of the galaxies which made that composite;
12) the mean fracPSF (r-band) (see text for the definition of fracPSF)
    of the galaxies which made that composite;
13) The ID for the environment (1 for high density and 0 for low density)
14) the number of galaxies used to make that composite;
15) the signal-to-noise of the composite spectrum. 


II) bernardi.tab2.dat

1) the spectrum ID 
2) OII [A]
3) error OII [A]
4) H{\delta}_A [A]
5) error H{\delta}_A [A]
6) H{\delta}_F [A]
7) error H{\delta}_F [A]
8) H{\gamma}_A [A]
9) error H{\gamma}_A [A]
10) H{\gamma}_F [A]
11) error H{\gamma}_F [A]
12) D4000
13) error D4000

III) bernardi.tab3.dat

1) the spectrum ID 
2) CN_1 [mag]       
3) error
4) CN_2 [mag]       
5) error
6) Ca4227 [\AA]   
7) error
8) G4300 [\AA]    
9) error
10) Fe4383 [\AA]   
11) error
12) Ca4455 [\AA]   
13) error
14) Fe4531 [\AA]   
15) error
16) C_24668 [\AA]
17) error
18) H\beta [\AA]
19) error
20) Fe5015 [\AA]   
21) error

IV) bernardi.tab4.dat

1) the spectrum ID 
2) Mg_1 [mag]       
3) error
4) Mg_2 [mag]       
5) error
6) Mgb [\AA]   
7) error
8) Fe5270 [\AA]   
9) error
10) Fe5335 [\AA]   
11) error
12) Fe5406 [\AA]   
13) error
14) Fe5709 [\AA]   
15) error
16) Fe5782 [\AA]   
17) error
18) NaD [\AA]      
19) error
20) TiO_1 [mag]      
21) error
22) TiO_2 [mag]      
23) error

V) bernardi.tab7.dat (Index-strengths from composite spectra convolved to 
                      Lick resolution)

1) the spectrum ID 
2) H{\gamma}_F [A]
3) error 
4) H\beta [\AA]
5) error
6) Mgb [\AA]   
7) error
8) Fe5270 [\AA]   
9) error
10) Fe5335 [\AA]   
11) error

IV) bernardi.tab8.dat

1) the spectrum ID 
2) Age [Gyrs]  (obtained using H\beta, Mgb, and <Fe>)
3) error
4) [Z/H]
5) error
6) [\alpha/Fe]
7) error
8) Age [Gyrs]  (obtained using H{\gamma}_F, Mgb, and <Fe>)
9) error
10) [Z/H]
11) error
12) [\alpha/Fe]
13) error