The following plots show the ratio of the
measured F2 to theory (calculated with CTEQ5D PDFs) for 96/97
data (red dots), 99/00 data (black dots) and the combined data set (blue
dots):

(from
Matthias' page)
The consistency of the two measurements
can be verified from the pull distribution defined as (F296/97-F299/00)/d,
where the d is the combined error calculated assuming uncorrelated errors
from the two measurements, d=sqrt(d296/97+d299/00).
The pull distribution width is close to 1 as expected, but there is a small
relative normalisation difference between the measurements.
The relative normalisation of the two
data sets was studied by multiplying the 99/00 F2 measurement
by a normalisation factor and calculating the mean of the pull distribution
as this factor was varied.

A normalisation shift of 2.35% was found
to produce the best agreement between the measurements. This is consistent
with luminosity uncertainties of 2% in 96/97 and 2.25% in 99/00. The luminosity
uncertainties should not be considered as totally correlated due changes
in the luminosity monitor filters and acceptance and to varying beam conditions.