CITATION

The latest, complete description of Maestro is found in the following
paper -- we appreciate citing this paper for all works that use
Maestro:

    @ARTICLE{2010ApJS..188..358N,
       author = {{Nonaka}, A. and {Almgren}, A.~S. and {Bell},
                  J.~B. and {Lijewski}, M.~J. and {Malone}, C.~M. and
                  {Zingale}, M.},
	title = "{MAESTRO: An Adaptive Low Mach Number Hydrodynamics
                  Algorithm for Stellar Flows}",
      journal = {\apjs},
    archivePrefix = "arXiv",
       eprint = {1005.0112},
     primaryClass = "astro-ph.IM",
     keywords = {convection, hydrodynamics, methods: numerical,
                  nuclear reactions, nucleosynthesis, abundances,
                  supernovae: general, white dwarfs},
	 year = 2010,
	month = jun,
       volume = 188,
	pages = {358-383},
	  doi = {10.1088/0067-0049/188/2/358},
       adsurl = {http://adsabs.harvard.edu/abs/2010ApJS..188..358N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

There are several other papers that may be appropriate to cite,
depending on which capabilities you are using.  These are discussed
below.

The development of the low Mach number formulation is described in the
following papers -- we ask that they be cited if you are discussing
the low Mach asymptotics or expansion of the background state (paper
II in particular):

    @ARTICLE{2006ApJ...637..922A,
       author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Rendleman},
                  C.~A. and {Zingale}, M.},
	title = "{Low Mach Number Modeling of Type Ia
                  Supernovae. I. Hydrodynamics}",
      journal = {\apj},
       eprint = {astro-ph/0509892},
     keywords = {Convection, Hydrodynamics, Methods: Numerical,
                  Nuclear Reactions, Nucleosynthesis, Abundances,
                  Stars: Supernovae: General, Stars: White Dwarfs},
	 year = 2006,
	month = feb,
       volume = 637,
	pages = {922-936},
	  doi = {10.1086/498426},
       adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...637..922A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    @ARTICLE{2006ApJ...649..927A,
       author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Rendleman},
		      C.~A. and {Zingale}, M.},
	title = "{Low Mach Number Modeling of Type Ia
		      Supernovae. II. Energy Evolution}",
      journal = {\apj},
       eprint = {astro-ph/0606496},
     keywords = {Convection, Hydrodynamics, Methods: Numerical, Nuclear
		      Reactions, Nucleosynthesis, Abundances, Stars:
		      Supernovae: General, Stars: White Dwarfs},
	 year = 2006,
	month = oct,
       volume = 649,
	pages = {927-938},
	  doi = {10.1086/507089},
       adsurl = {http://adsabs.harvard.edu/abs/2006ApJ...649..927A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }

    @ARTICLE{2008ApJ...684..449A,
       author = {{Almgren}, A.~S. and {Bell}, J.~B. and {Nonaka},
                  A. and {Zingale}, M.  },
	title = "{Low Mach Number Modeling of Type Ia
                  Supernovae. III. Reactions}",
      journal = {\apj},
     keywords = {convection, hydrodynamics, methods: numerical,
                  nuclear reactions, nucleosynthesis, abundances,
                  supernovae: general, white dwarfs },
	 year = 2008,
	month = sep,
       volume = 684,
	  eid = {449-470},
	pages = {449-470},
	  doi = {10.1086/590321},
       adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...684..449A},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }


If you use diffusion, we appreciate citing the following paper which
introduced the diffusion algorithm:

    @ARTICLE{2011ApJ...728..118M,
       author = {{Malone}, C.~M. and {Nonaka}, A. and {Almgren},
                  A.~S. and {Bell}, J.~B. and {Zingale}, M.},
	title = "{Multidimensional Modeling of Type I X-ray
                  Bursts. I. Two-dimensional Convection Prior to the
                  Outburst of a Pure $^{4}$He Accretor}",
      journal = {\apj},
    archivePrefix = "arXiv",
       eprint = {1012.0609},
     primaryClass = "astro-ph.HE",
     keywords = {convection, hydrodynamics, methods: numerical, stars:
                  neutron, X-rays: bursts},
	 year = 2011,
	month = feb,
       volume = 728,
	  eid = {118},
	pages = {118},
	  doi = {10.1088/0004-637X/728/2/118},
       adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...728..118M},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }


If you are dealing with a spherical geometry, we appreciate citing
this paper, which describes the spherical geometry:

    @ARTICLE{2009ApJ...704..196Z,
       author = {{Zingale}, M. and {Almgren}, A.~S. and {Bell},
                  J.~B. and {Nonaka}, A. and {Woosley}, S.~E.},
	title = "{Low Mach Number Modeling of Type IA
                  Supernovae. IV. White Dwarf Convection}",
      journal = {\apj},
    archivePrefix = "arXiv",
       eprint = {0908.2668},
     primaryClass = "astro-ph.HE",
     keywords = {convection, hydrodynamics, methods: numerical,
                  nuclear reactions, nucleosynthesis, abundances,
                  supernovae: general, white dwarfs},
	 year = 2009,
	month = oct,
       volume = 704,
	pages = {196-210},
	  doi = {10.1088/0004-637X/704/1/196},
       adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...704..196Z},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
    }