Improved constraint on the MINERvA medium energy neutrino flux using
$\bar{\nu}e^{-} \!\rightarrow \bar{\nu}e^{-}$ data
L. Zazueta,S. Akhter,Z. Ahmad Dar,F. Akbar,V. Ansari,M. V. Ascencio,M. Sajjad Athar,A. Bashyal,A. Bercellie,M. Betancourt,A. Bodek,J. L. Bonilla,A. Bravar,H. Budd,T. Cai,G. A. Díaz,H. da Motta,J. Felix,L. Fields,A. Filkins,R. Fine,A. M. Gago,H. Gallagher,A. Ghosh,S. M. Gilligan,R. Gran,E. Granados,D. A. Harris,S. Henry,D. Jena,S. Jena,J. Kleykamp,A. Klustová,M. Kordosky,D. Last,A. Lozano,X. -G. Lu,E. Maher,S. Manly,W. A. Mann,K. S. McFarland,B. Messerly,J. Miller,O. Moreno,J. G. Morfín,J. K. Nelson,C. Nguyen,A. Olivier,V. Paolone,G. N. Perdue,K. -J. Plows,M. A. Ramírez,D. Ruterbories,H. Schellman,C. J. Solano Salinas,H. Su,M. Sultana,E. Valencia,N. H. Vaughan,A. V. Waldron,B. Yaeggy OSTI OAI (US Department of Energy Office of Scientific and Technical Information)（2022）
Key words
flux,improved constraint
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