add refs

Author: zingale

paper/paper.bib

@@ -1,4 +1,4 @@
-@ARTICLE{pyro,
+@ARTICLE{pyroI,
    author = {{Zingale}, M.},
     title = "{pyro: A teaching code for computational astrophysical hydrodynamics}",
   journal = {Astronomy and Computing},
@@ -14,3 +14,40 @@ @ARTICLE{pyro
    adsurl = {http://adsabs.harvard.edu/abs/2014A%26C.....6...52Z},
   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
+
+@ARTICLE{castro,
+   author = {{Almgren}, A.~S. and {Beckner}, V.~E. and {Bell}, J.~B. and 
+	{Day}, M.~S. and {Howell}, L.~H. and {Joggerst}, C.~C. and {Lijewski}, M.~J. and 
+	{Nonaka}, A. and {Singer}, M. and {Zingale}, M.},
+    title = "{CASTRO: A New Compressible Astrophysical Solver. I. Hydrodynamics and Self-gravity}",
+  journal = {Astrophysical Journal},
+archivePrefix = "arXiv",
+   eprint = {1005.0114},
+ primaryClass = "astro-ph.IM",
+ keywords = {equation of state, gravitation, hydrodynamics, methods: numerical, nuclear reactions, nucleosynthesis, abundances},
+     year = 2010,
+    month = jun,
+   volume = 715,
+    pages = {1221-1238},
+      doi = {10.1088/0004-637X/715/2/1221},
+   adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...715.1221A},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{maestro,
+   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 = {Astrophysical Journal Supplement},
+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}
+}

paper/paper.md

@@ -59,13 +59,13 @@ algorithms before porting them to science codes.
 The current pyro solvers are:
 
   * linear advection (including a second-order unsplit CTU scheme, a
-    method-of-lines piecewise linear solver☆, a 4th-order
-    finite-volume scheme☆, and a WENO method☆)
+    method-of-lines piecewise linear solver$^\star$, a 4th-order
+    finite-volume scheme$^\star$, and a WENO method$^\star$)
 
   * compressible hydrodynamics (including a second-order unsplit CTU
-    scheme, a method-of-lines piecewise linear solver☆,
+    scheme, a method-of-lines piecewise linear solver$^\star$,
     and two 4th-order finite-volume schemes, one with Runge-Kutta
-    integration and the other using a spectral deferred corrections method☆)
+    integration and the other using a spectral deferred corrections method$^\star$)
 
   * diffusion using a second-order discretization
 
@@ -75,7 +75,7 @@ The current pyro solvers are:
 
   * shallow water equations solver
 
-(solvers since the first pyro paper are marked with a ☆).  Also
+(solvers since the first pyro paper are marked with a $^\star$).  Also
 new is support for Lagrangian tracer particles, which can be added to
 any solver that has a velocity field.