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Dijet NLO theory at $\sqrt{s}=200$ GeV

Updated on Sat, 2018-08-04 20:48. Originally created by veprbl on 2016-01-12 14:51.

See also:

Presentation on January 2016 Collaboration Meeting


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CT10, Scale uncertainty (yoda, root)
CT10, PDF 90% C.L. (or ~1.65-sigma) uncertainty (yoda, root)


d01-x02-y01	d01-x02-y02	d01-x02-y03

Scale uncertainties (yoda, root)


d01-x02-y01	d01-x02-y02	d01-x02-y03

DSSV2008 / MRST2002 (yoda, root)
DSSV2014 / MRST2008 (yoda, root)
NNPDFpol10 / NNPDF23 (yoda, root)
NNPDFpol11 / NNPDF23 (yoda, root)

d01-x02-y01

CTEQ6M (yoda, root)


d01-x02-y01	d01-x02-y02	d01-x02-y03

NNPDFpol11 / NNPDF23 1-sigma uncertainty (yoda, root, replicas)

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