Requires the grid files
    DNS1LO.GRID
    DNS1NLO.GRID
    DNS2LO.GRID
    DNS2NLO.GRID
dns2005.uu
is a tarred, gzipped and uuencoded version of the complete
package (973 KB).
CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC C C C POLARIZED PARTON DISTRIBUTIONS (NLO) C C FROM PRD71, 094018 (2005) C C hep-ph/0504155 C C D. de Florian G.A. Navarro and R. Sassot. C C C C MODE: 1 SET 1 NLO (MSbar) (based on KRETZER ffs) C C 2 SET 2 NLO (MSbar) (based on KKP ffs) C C 3 SET 1 LO (based on KRETZER ffs) C C 4 SET 2 LO (based on KKP ffs) C C C C Q2=Q^2 C C DUV : X * U VALENCE DISTRIBUTION C C DDV : X * D VALENCE DISTRIBUTION C C DUBAR : X * UBAR DISTRIBUTION C C DDBAR : X * DBAR DISTRIBUTION C C DSTR : X * STRANGE DISTRIBUTION C C DGLU : X * GLUON DISTRIBUTION C C G1P : X * POLARIZED STRUCTURE FUNCTION (PROTON) C C G1N : X * POLARIZED STRUCTURE FUNCTION(NEUTRON) C C C C REMEMBER: ALWAYS X*DISTRIBUTION !!! C C C C BEFORE CALLING THE SUBRUTINE `POLFIT` FOR THE FIRST TIME, THE C C SUBROUTINE `INI` MUST BE CALLED (ONLY ONCE) TO READ THE GRIDS. C C (CALL INI) C RANGE OF VALIDITY OF THE INTERPOLATION: C C 10**(-4)< X < 0.9 C C 1 < Q**2 < 5*10**4 C C C C IN CASE OF PROBLEMS, DOUBTS, ETC, PLEASE REPORT TO C C dflorian@df.uba.ar C C sassot@df.uba.ar C C C CCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCCC