CODE	NUCLIDE	ORIGINAL DATA TAKEN FROM	MODIFICATION	ADDITIONAL FILE MODIFICATIONS	ORIGINAL DATA TAKEN FROM	MODIFICATION	ADDITIONAL FILE MODIFICATIONS	COMMENTS
1042094	042_Mo_094	JENDL-3.3	(1,451) Updated. (3.1) Revised. (3,2) Re-calculated. (3,203-207) Added. (3,251) Deleted. (4,2) Transformation matrix deleted. (4,16-91) Deleted. (5,16-91) Deleted. (6,16-91) Taken from JENDL fusion file. (12,102) Added. (13,3) Added. (14,3),(14,102) Added. (15,3),(15,102) Added.	File obtained by merging: - Resolved Resonances (MLBW) <20 keV : Ref.1 - Unresolved Resonances 20 keV - 100 keV : JENDL-3.3 - Fast neutron region >100 keV : JENDL-3.3 Reference: 1) S.F.Mughabghab: Atlas of Neutron Resonances, to be published by Elsevier, 2006 (5-th edition of BNL-325) Covariances, BNL, July 2011	JENDL-3.2	(3,2), (3,4), (3,51-91), (3,16), (3,17), (3,22), (3,28) (4,16-91) (5,16-91) These data were adopted from JENDL fusion file (3,32) deleted		"File produced by WPEC Subgroup 23 in 2004-2005 Covariances from COMMARA-2.0 were adopted for the Mo isotopes. Here, new sets of covariances were obtained at BNL in 2010 using the kernel approach in the resonance region and EMPIRE/KALMAN analysis of experimental data in the fast neutron region. Dispersion analysis provided expected uncertainties of the order of 10% for total, elastic and capture with tendency to increase above 10 MeV. Some isotopic data are available for all channels but the results still depend heavily on elemental data. The EMPIRE/KALMAN analysis was performed using ""nuisance"" parameters scaling total and reaction cross sections to account for systematic uncertainties."