Last Update:  November 2013

The input files used for SNIa-lightcurve fits (SALT2 & mlcs2k2) 
in the DR paper are provided here as 
     SDSS_snfit*.nml   and   SDSS_SALT2mu_template.input. 
The '4par' fits refer to 4-parameter fits with an accurate spectaroscopic 
redshift, and the '5par' fits are photo-z fits with the redshift floated. 
The SDSS_snfit*.nml are input files to the snana script 'split_and_fit.pl, 
which calls the program 'snlc_fit.exe'. SALT2mu_template.input is an 
input to the snana script 'SALT2mu_fit.pl', which calls SALT2mu.exe. 
Note that these fits are intended for illustration and are not intended 
for any particular analysis.


SDSS_snfit4par_SALT2.nml (4-parameter SALT2 fits using spec redshift):
   Table 1, columns 16-28(SALT2 fit params)
   Table 12
   Figures 9, 10, 11, 12, 14, 15

SDSS_SALT2mu_template.input (translate SALT2 fits above into distances)
   Table 12 (mu and dmu columns)

SDSS_snfit5par_SALT2.nml (5-parameter photo-z fits, minimized)

SDSS_snfit5par_SALT2+marg.nml (5-parameter photo-z fits, marginalized)
   Table 1, columns 63-75

SDSS_snfit4par_mlcs2k2.nml (4-parameter mlcs2k2 fits using spec redshift)
   Table 1, columns 29-39 (mlcs fit params)

SDSS_snfit4par_repeatK09.nml (repeat K09 analysis)
   Fig 12


Each SDSS_snfit*.nml input file can be run interactively,
    snlc_fit.exe  <inputFile>
but the processing time will be quite long using a single core.
To distribute jobs using 'split_and_fit.pl' (manual section 12.4.1)
replace the following keys in each input file,
   [OUTDIR]  [BATCH_TEMPLATE]  [NCORE]
or replace the BATCH_INFO line with 
  NODELIST:  <node1> <node2> etc ...

The SALT2mu job is launched with
    SALT2mu_fit.pl  SDSS_SALT2mu_template.input