From 970d0c95423e8abe0eab7a8ef81934534e117725 Mon Sep 17 00:00:00 2001
From: "Carlos A. Arguelles" <carguelles@fas.harvard.edu>
Date: Mon, 27 Dec 2021 12:05:08 -0500
Subject: [PATCH] fixed bibliography

---
 resources/paper/nusquids.bib | 61 ++++++++++++++++++++++++++++++++++--
 resources/paper/nusquids.tex |  8 ++---
 2 files changed, 63 insertions(+), 6 deletions(-)

diff --git a/resources/paper/nusquids.bib b/resources/paper/nusquids.bib
index 11525ea6..e00b3707 100644
--- a/resources/paper/nusquids.bib
+++ b/resources/paper/nusquids.bib
@@ -1,12 +1,54 @@
 %% This BibTeX bibliography file was created using BibDesk.
 %% http://bibdesk.sourceforge.net/
-
-
 %% Created for Carlos Arguelles at 2014-09-29 16:26:30 -0500 
 
 
 %% Saved with string encoding Unicode (UTF-8) 
 
+@article{Super-Kamiokande:2010tar,
+    author = "Abe, K. and others",
+    collaboration = "Super-Kamiokande",
+    title = "{Solar neutrino results in Super-Kamiokande-III}",
+    eprint = "1010.0118",
+    archivePrefix = "arXiv",
+    primaryClass = "hep-ex",
+    doi = "10.1103/PhysRevD.83.052010",
+    journal = "Phys. Rev. D",
+    volume = "83",
+    pages = "052010",
+    year = "2011"
+}
+
+@article{Borexino:2013zhu,
+    author = "Bellini, G. and others",
+    collaboration = "Borexino",
+    title = "{Final results of Borexino Phase-I on low energy solar neutrino spectroscopy}",
+    eprint = "1308.0443",
+    archivePrefix = "arXiv",
+    primaryClass = "hep-ex",
+    doi = "10.1103/PhysRevD.89.112007",
+    journal = "Phys. Rev. D",
+    volume = "89",
+    number = "11",
+    pages = "112007",
+    year = "2014"
+}
+
+@article{Super-Kamiokande:2015qek,
+    author = "Richard, E. and others",
+    collaboration = "Super-Kamiokande",
+    title = "{Measurements of the atmospheric neutrino flux by Super-Kamiokande: energy spectra, geomagnetic effects, and solar modulation}",
+    eprint = "1510.08127",
+    archivePrefix = "arXiv",
+    primaryClass = "hep-ex",
+    doi = "10.1103/PhysRevD.94.052001",
+    journal = "Phys. Rev. D",
+    volume = "94",
+    number = "5",
+    pages = "052001",
+    year = "2016"
+}
+
 @article{Vincent:2017svp,
     author = {Vincent, Aaron C. and Arg\"uelles, Carlos A. and Kheirandish, Ali},
     title = "{High-energy neutrino attenuation in the Earth and its associated uncertainties}",
@@ -2046,6 +2088,21 @@ @article{Esteban:2020cvm
     year = "2020"
 }
 
+@article{Gonzalez-Garcia:2021dve,
+    author = "Gonzalez-Garcia, Maria Concepcion and Maltoni, Michele and Schwetz, Thomas",
+    title = "{NuFIT: Three-Flavour Global Analyses of Neutrino Oscillation Experiments}",
+    eprint = "2111.03086",
+    archivePrefix = "arXiv",
+    primaryClass = "hep-ph",
+    reportNumber = "IFT-UAM/CSIC-21-114",
+    doi = "10.3390/universe7120459",
+    journal = "Universe",
+    volume = "7",
+    number = "12",
+    pages = "459",
+    year = "2021"
+}
+
 @article{deSalas:2017kay,
       author         = "de Salas, P. F. and Forero, D. V. and Ternes, C. A. and
                         Tortola, M. and Valle, J. W. F.",
diff --git a/resources/paper/nusquids.tex b/resources/paper/nusquids.tex
index e8f6f5ad..d695899d 100644
--- a/resources/paper/nusquids.tex
+++ b/resources/paper/nusquids.tex
@@ -207,8 +207,8 @@ \section{Introduction}
 In recent decades a large body of evidence that neutrinos change
 flavor as they propagate macroscopic distances due to the
 non-alignment of their mass and flavor eigenstates has accumulated from
-solar~\citep{Abe:2010hy, Borexino2014},
-atmospheric~\citep{PhysRevD.91.072004,Richard:2015aua,IceCube:2019dqi,ANTARES:2018rtf},
+solar~\citep{Super-Kamiokande:2010tar, Borexino:2013zhu},
+atmospheric~\citep{PhysRevD.91.072004,Super-Kamiokande:2015qek,IceCube:2019dqi,ANTARES:2018rtf},
 accelerator~\citep{PhysRevLett.112.181801,
   PhysRevD.93.051104,PhysRevLett.116.151806, PhysRevLett.110.251801}, and
 reactor~\citep{An:2013zwz,Abe:2015rcp, Kim:2016yvm} experiments.
@@ -4174,7 +4174,7 @@ \subsubsection{Single-energy mode}
 \end{figure}
 
 nuSQuIDs has some predefined oscillation mixing angles ($\theta_{ij}$) and mass splittings ($\Delta m^2_{ij}$),
-which we have taken from~\cite{nufit}.
+which we have taken from~\cite{Esteban:2020cvm}.
 We can change the square mass differences by using the following function
 \begin{lstlisting}[language=Python, breaklines=true]
 nuSQ.Set_SquareMassDifference(1,2.0e-1) # sets dm^2_{21} in eV^2.
@@ -4384,7 +4384,7 @@ \subsubsection{Multiple-energy mode}
 \end{figure}
 
 nuSQuIDs has some predefined oscillation mixing angles ($\theta_{ij}$) and mass splittings ($\Delta m^2_{ij}$),
-which we have taken from~\cite{nufit}.
+which we have taken from~\cite{Esteban:2020cvm,Gonzalez-Garcia:2021dve}.
 We can change the square mass differences by using the following function
 \begin{lstlisting}[language=Python, breaklines=true]
 nuSQ.Set_SquareMassDifference(1,2.0e-1) # sets dm^2_{21} in eV^2.