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       \title{       
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       Neutron reaction on XXX under the CIELO Collaboration
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%       Neutron Reactions on 
%       $^{1}$H, $^{16}$O, $^{56}$Fe, $^{235,238}$U, and $^{239}$Pu
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       \author{author}
       \email[Corresponding author: ]{email@}
       \affiliation{Lab address}
       
       
       
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       %\received{8 March 2013; revised received XX June 2013; accepted XX September 2013}
       
       
       
       
       \begin{abstract}
Abstract.
   
{\bf Note we do not yet know page restrictions for these individual CIELO papers, but plan for somewhere between 4-10 pages each. (The same ND2018 issue will have a large 100+ paper on ENDF/B-VIII, and a large 30+ page paper on new standards). Thus we expect perhaps 150 pages reserved for separate CIELO papers.}


       \end{abstract}
       
       
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       \lhead{The CIELO Collaboration $\dots$}
       \chead{NUCLEAR DATA SHEETS}
       \rhead{M.B. Chadwick}
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       \section{INTRODUCTION}
       \label{sec:introduction}

{\bf The paper should be journal quality; it will be peer reviewed}.

{\bf Give background, e.g.} - The CIELO pilot project was commissioned
by the OECD's Nuclear Energy Agency WPEC (Working Party on
International Nuclear Data Evaluation Co-operation) during a meeting
held in May 2012. The goal has been to identify deficiencies and
discrepancies in our current understanding of neutron reactions on
high priority nuclides ${^1}$H, $^{16}$O, $^{56}$Fe, $^{235}$U,
$^{238}$U and $^{239}$Pu, and to develop proposed solutions and
improvements in our understanding. The goals of CIELO are documented
in Ref.~\cite{Chadwick2014}. This reference, together with other
papers such as Refs.~\cite{IAEA2012,Bauge2012,Salvatores2014} document
some of the questions being addressed.

{\bf Explain clearly which isotope and cross sections or energy/angle distributions will be addressed.}

{\bf Explain the background as to why our previous understanding was inadequate. Why - a lack of accurate experimental data? Insufficiently reliable model predictions? What were the assessed uncertainties prior to the present work?}

{\bf Possibly summarize the applications that have motivated the work}.

       \section{RESULTS}
       \label{sec:results}

{\bf Explain the basis for your new conclusions - new experiments made, theory, new analyses?}

{\bf What are your new proposed uncertainties?}

{\bf Proposed or recommended evalations should} 
(a) provide a ENDF-formatted file that can be archived on the NEA CIELO web site; and (b) be documented in this paper, with illustrative figures that compare the recommendation against  
the main evaluated
       data libraries, such a
 ENDF/B-VII.1 \cite{Chadwick2011,Kahler2011},
       JEFF-3.1 \cite{Koning2006,Koning2013}, JENDL-4.0 \cite{Shibata2011},
       BROND/ROSFOND \cite{Zabrodskaya2007}, and CENDL-3.1 \cite{Ge2011}.
       
%       \begin{figure}
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%        \caption{Calculated/measured root mean square deviation (in \%) from unity for 
%       nuclear criticality, $k_{\mathrm{eff}}$, for a suite of 119 critical assemblies, 
%       as a function of ENDF library version number.}
%        \label{fig:rmskeff}
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{\bf What are remaining open questions that remain unsolved?.}
  

       \begin{thebibliography}{999}
       
       \bibitem{Chadwick2014}
         M. B. Chadwick {\it et al.}, 
         {\sc Nucl. Data Sheets}  {\bf 118}, 1 (2014).

       \bibitem{IAEA2012}
         A. Plompen {\it et al.},
         IAEA report INDC(NDS)-0597 (2012).
       
       \bibitem{Bauge2012}
         E. Bauge {\it et al.},
         {\sc Eur. Phys. J. } A {\bf 48}, 113 (2012).
       
       \bibitem{Salvatores2014} M. Salvatores,    {\it et al.},
       %NUCL. DATA SHEETS (2013, submitted).
        {\sc Nucl. Data Sheets} {\bf 115},  xxx (2014).      
       
       \bibitem{Chadwick2011}
         M. B. Chadwick {\it et al.}, 
         {\sc Nucl. Data Sheets}  {\bf 112}, 2887 (2011).
       
       \bibitem{Kahler2011} 
         A. Kahler {\it et al.},
         {\sc Nucl. Data Sheets}  {\bf 112}, 2997 (2011).
       
       \bibitem{Koning2006}
         A.J. Koning {\it et al.},
         JEFF Report {\bf 21}, NEA (2006).
       
       \bibitem{Koning2013}
         A.J. Koning {\it et al.},
         JEFF Report {\bf 23}, NEA (2013).
       
       \bibitem{Shibata2011}
         K. Shibata {\it et al.},
        {\sc  J. Nucl. Sci. Technol. } {\bf 48}, 1 (2011).
       
       \bibitem{Zabrodskaya2007}
         S.V. Zabrodskaya, {\it et al.},
        {\sc Nucl. Const.} {\bf 1-2}, 3 (2007).
       
       \bibitem{Ge2011}
         Z.G. Ge  {\it et al.},
         {\sc J. Korean Phys. Soc.}  {\bf 59}, No. 2, 1052 (2011).
       

       
       \end{thebibliography}
       

\newpage
\section{Appendix - Possible CIELO NDS papers?}
       
First, the big ENDF/B-VIII paper will include many co-authors who
contributed CIELO work that was adopted for ENDF/B-VIII. The big
ENDF/B-VIII paper will fully document the new evaluation, reasons for
evaluation choices, and how B-VIII compares to B-VII.1 and other
evaluations. Many co-authors of this paper will not want to write
separate CIELO papers - {\bf we certaintly do not want to be
duplicative.} But some co-authors will reasonably want to have
additional CIELO papers, because (a) they may want to go into more
detail there; (b) there may be work they have done that was not
adopted in VIII, and it should be documented still for CIELO; and (c)
they may want first-author credit for what they have done.

I am aware of the following possible separate CIELO papers for NDS
January 2018, and I will refine this list over the coming months, with
CIELO collaborators and with the NDS editor, Pavel Oblozinsky (many
people listed below have not yet affirmed their interest/willingness; and
there will be additions to this list).

\begin{itemize}

\item{Chadwick - short overview of CIELO SG40 objectives and accomplishments}

\item{Hale et al - 16O evaluation ?}

\item{Hale, Kunieda, Livermore collaborators, ... 
Broader O16 collaboration conclusions on magitude of n,a based on unitarity}

\item{Georginis, Plompen et al - conclusions on 16O (n,a) corrections on 
historic data}

\item{Plompen et al, the low energy 16O total elastic cross section}

\item{Leal? - his R-matrix 16O evaluation (not in B-VIII)}

\item{Herman et al - BNL staff - more details on 56Fe in fast region?}

\item{Trkov et al - resonance region of 56Fe}

\item{Leal et al - new resonance analysis of 56Fe}

\item{Chinese work on 56Fe - eg inelastic scattering evaluation}

\item{Romain, Morillon, Bauge et al - CEA fast actinide evaluations}

\item{Chinese work on 235U}

\item{M.Pigni et al (Trkov) resonance analysis of 235U}

\item{R. Capote et al, fast 235U and 238U analysis}

\item{L. Leal resonance analysis of 235U}

\item{Schillebeeckx et al., new Geel 238U resonance analysis - MBC notes not yet in B-VIII-beta1}

\item{Kawano - 238U and LANSCE capture theory and moel calculations}

\item{Neudecker - PFNS evaluations of actinides - incl those that did not make it into B-VIII, eg thermal 239Pu}

\item{Talou - multiplicity dependent fission neutrons and gamma-rays}

\item{Kawano, Capote, Romain, et al, latest conclusions on actinide inelastic cross sections}

\end{itemize}

       \end{document}
       
       
       
