more refs and figures

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diff --git a/paper/average_models_nir_mir.png b/paper/average_models_nir_mir.png
diff --git a/paper/average_models_uv_nir.png b/paper/average_models_uv_nir.png
diff --git a/paper/grain_models.png b/paper/grain_models.png
diff --git a/paper/paper.bib b/paper/paper.bib
@@ -1,3 +1,195 @@
+@ARTICLE{Bastiaansen92,
+       author = {{Bastiaansen}, P.~A.},
+        title = "{Narrow band multicolor photometry of reddened and unreddened early-type stars.}",
+      journal = {\aaps},
+     keywords = {Early Stars, Interstellar Extinction, Stellar Spectrophotometry, Ubv Spectra, Narrowband, Polarization (Waves), Stellar Evolution, Astronomy},
+         year = 1992,
+        month = jun,
+       volume = {93},
+        pages = {449-462},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1992A&AS...93..449B},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Cardelli89,
+   author = {{Cardelli}, J.~A. and {Clayton}, G.~C. and {Mathis}, J.~S.},
+    title = "{The relationship between infrared, optical, and ultraviolet extinction}",
+  journal = {\apj},
+     year = 1989,
+    month = oct,
+   volume = 345,
+    pages = {245-256},
+      doi = {10.1086/167900},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1989ApJ...345..245C&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Compiegne11,
+   author = {{Compi{\`e}gne}, M. and {Verstraete}, L. and {Jones}, A. and 
+	{Bernard}, J.-P. and {Boulanger}, F. and {Flagey}, N. and {Le Bourlot}, J. and 
+	{Paradis}, D. and {Ysard}, N.},
+    title = "{The global dust SED: tracing the nature and evolution of dust with DustEM}",
+  journal = {\aap},
+archivePrefix = "arXiv",
+   eprint = {1010.2769},
+ primaryClass = "astro-ph.GA",
+ keywords = {radiation mechanisms: thermal, methods: numerical, dust, extinction, infrared: ISM},
+     year = 2011,
+    month = jan,
+   volume = 525,
+      eid = {A103},
+    pages = {A103},
+      doi = {10.1051/0004-6361/201015292},
+   adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...525A.103C},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Desert90,
+   author = {{Desert}, F.-X. and {Boulanger}, F. and {Puget}, J.~L.},
+    title = "{Interstellar dust models for extinction and emission}",
+  journal = {\aap},
+ keywords = {COSMIC DUST, EMISSION SPECTRA, INFRARED RADIATION, INTERSTELLAR MATTER, ASTRONOMICAL MODELS, CARBON, EXTINCTION, GRAIN SIZE, PARTICLE SIZE DISTRIBUTION, SILICATES},
+     year = 1990,
+    month = oct,
+   volume = 237,
+    pages = {215-236},
+   adsurl = {http://adsabs.harvard.edu/abs/1990A%26A...237..215D},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Draine03,
+   author = {{Draine}, B.~T.},
+    title = "{Interstellar Dust Grains}",
+  journal = {\araa},
+   eprint = {arXiv:astro-ph/0304489},
+     year = 2003,
+   volume = 41,
+    pages = {241-289},
+      doi = {10.1146/annurev.astro.41.011802.094840},
+   adsurl = {http://adsabs.harvard.edu/abs/2003ARA%26A..41..241D},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Fitzpatrick90,
+   author = {{Fitzpatrick}, E.~L. and {Massa}, D.},
+    title = "{An analysis of the shapes of ultraviolet extinction curves. III - an atlas of ultraviolet extinction curves}",
+  journal = {\apjs},
+     year = 1990,
+    month = jan,
+   volume = 72,
+    pages = {163-189},
+      doi = {10.1086/191413},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=1990ApJS...72..163F&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Fitzpatrick99,
+       author = {{Fitzpatrick}, Edward L.},
+        title = "{Correcting for the Effects of Interstellar Extinction}",
+      journal = {\pasp},
+     keywords = {ISM: DUST, EXTINCTION, Astrophysics},
+         year = 1999,
+        month = jan,
+       volume = {111},
+       number = {755},
+        pages = {63-75},
+          doi = {10.1086/316293},
+archivePrefix = {arXiv},
+       eprint = {astro-ph/9809387},
+ primaryClass = {astro-ph},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1999PASP..111...63F},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@INPROCEEDINGS{Fitzpatrick04,
+       author = {{Fitzpatrick}, E.~L.},
+        title = "{Interstellar Extinction in the Milky Way Galaxy}",
+     keywords = {Astrophysics},
+    booktitle = {Astrophysics of Dust},
+         year = 2004,
+       editor = {{Witt}, Adolf N. and {Clayton}, Geoffrey C. and {Draine}, Bruce T.},
+       series = {Astronomical Society of the Pacific Conference Series},
+       volume = {309},
+        month = may,
+        pages = {33},
+          doi = {10.48550/arXiv.astro-ph/0401344},
+archivePrefix = {arXiv},
+       eprint = {astro-ph/0401344},
+ primaryClass = {astro-ph},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2004ASPC..309...33F},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Fitzpatrick19,
+       author = {{Fitzpatrick}, E.~L. and {Massa}, Derck and {Gordon}, Karl D. and
+         {Bohlin}, Ralph and {Clayton}, Geoffrey C.},
+        title = "{An Analysis of the Shapes of Interstellar Extinction Curves. VII. Milky Way Spectrophotometric Optical-through-ultraviolet Extinction and Its R-dependence}",
+      journal = {\apj},
+     keywords = {Interstellar dust, Interstellar dust extinction, Interstellar dust processes, Interstellar absorption, Interstellar reddening, Interstellar scattering, Astrophysics - Astrophysics of Galaxies, Astrophysics - Solar and Stellar Astrophysics},
+         year = 2019,
+        month = dec,
+       volume = {886},
+       number = {2},
+          eid = {108},
+        pages = {108},
+          doi = {10.3847/1538-4357/ab4c3a},
+archivePrefix = {arXiv},
+       eprint = {1910.08852},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2019ApJ...886..108F},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Gordon03,
+   author = {{Gordon}, K.~D. and {Clayton}, G.~C. and {Misselt}, K.~A. and 
+	{Landolt}, A.~U. and {Wolff}, M.~J.},
+    title = "{A Quantitative Comparison of the Small Magellanic Cloud, Large Magellanic Cloud, and Milky Way Ultraviolet to Near-Infrared Extinction Curves}",
+  journal = {\apj},
+   eprint = {astro-ph/0305257},
+     year = 2003,
+    month = sep,
+   volume = 594,
+    pages = {279-293},
+      doi = {10.1086/376774},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2003ApJ...594..279G&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Gordon09,
+   author = {{Gordon}, K.~D. and {Cartledge}, S. and {Clayton}, G.~C.},
+    title = "{FUSE Measurements of Far-Ultraviolet Extinction. III. The Dependence on R(V) and Discrete Feature Limits from 75 Galactic Sightlines}",
+  journal = {\apj},
+archivePrefix = "arXiv",
+   eprint = {0909.3087},
+ keywords = {dust, extinction},
+     year = 2009,
+    month = nov,
+   volume = 705,
+    pages = {1320-1335},
+      doi = {10.1088/0004-637X/705/2/1320},
+   adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...705.1320G},
+  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Gordon21,
+       author = {{Gordon}, Karl D. and {Misselt}, Karl A. and {Bouwman}, Jeroen and {Clayton}, Geoffrey C. and {Decleir}, Marjorie and {Hines}, Dean C. and {Pendleton}, Yvonne and {Rieke}, George and {Smith}, J.~D.~T. and {Whittet}, D.~C.~B.},
+        title = "{Milky Way Mid-Infrared Spitzer Spectroscopic Extinction Curves: Continuum and Silicate Features}",
+      journal = {\apj},
+     keywords = {Interstellar dust, Interstellar dust extinction, Silicate grains, Ultraviolet extinction, 836, 837, 1456, 1738, Astrophysics - Astrophysics of Galaxies},
+         year = 2021,
+        month = jul,
+       volume = {916},
+       number = {1},
+          eid = {33},
+        pages = {33},
+          doi = {10.3847/1538-4357/ac00b7},
+archivePrefix = {arXiv},
+       eprint = {2105.05087},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2021ApJ...916...33G},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
 @ARTICLE{Gordon23,
        author = {{Gordon}, Karl D. and {Clayton}, Geoffrey C. and {Decleir}, Marjorie and {Fitzpatrick}, E.~L. and {Massa}, Derck and {Misselt}, Karl A. and {Tollerud}, Erik J.},
         title = "{One Relation for All Wavelengths: The Far-ultraviolet to Mid-infrared Milky Way Spectroscopic R(V)-dependent Dust Extinction Relationship}",
@@ -15,4 +207,112 @@ @ARTICLE{Gordon23
  primaryClass = {astro-ph.GA},
        adsurl = {https://ui.adsabs.harvard.edu/abs/2023ApJ...950...86G},
       adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Hensley23,
+       author = {{Hensley}, Brandon S. and {Draine}, B.~T.},
+        title = "{The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium}",
+      journal = {\apj},
+     keywords = {Dust composition, Dust continuum emission, Dust formation, Dust physics, Astrophysical dust processes, Interstellar dust extinction, Interstellar dust processes, Optical constants (Dust), Starlight polarization, 2271, 412, 2269, 2229, 99, 837, 838, 2270, 1571, Astrophysics - Astrophysics of Galaxies},
+         year = 2023,
+        month = may,
+       volume = {948},
+       number = {1},
+          eid = {55},
+        pages = {55},
+          doi = {10.3847/1538-4357/acc4c2},
+archivePrefix = {arXiv},
+       eprint = {2208.12365},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2023ApJ...948...55H},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Jones13,
+       author = {{Jones}, A.~P. and {Fanciullo}, L. and {K{\"o}hler}, M. and {Verstraete}, L. and {Guillet}, V. and {Bocchio}, M. and {Ysard}, N.},
+        title = "{The evolution of amorphous hydrocarbons in the ISM: dust modelling from a new vantage point}",
+      journal = {\aap},
+     keywords = {dust, extinction, photon-dominated region, ISM: molecules, Astrophysics - Astrophysics of Galaxies},
+         year = 2013,
+        month = oct,
+       volume = {558},
+          eid = {A62},
+        pages = {A62},
+          doi = {10.1051/0004-6361/201321686},
+archivePrefix = {arXiv},
+       eprint = {1411.6293},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2013A&A...558A..62J},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{ODonnell94,
+       author = {{O'Donnell}, James E.},
+        title = "{R v-dependent Optical and Near-Ultraviolet Extinction}",
+      journal = {\apj},
+     keywords = {Interstellar Extinction, Light (Visible Radiation), Near Infrared Radiation, Ultraviolet Radiation, Astronomical Photometry, Iue, Astrophysics, ISM: DUST, EXTINCTION},
+         year = 1994,
+        month = feb,
+       volume = {422},
+        pages = {158},
+          doi = {10.1086/173713},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/1994ApJ...422..158O},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{MaizApellaniz14,
+       author = {{Ma{\'\i}z Apell{\'a}niz}, J. and {Evans}, C.~J. and {Barb{\'a}}, R.~H. and {Gr{\"a}fener}, G. and {Bestenlehner}, J.~M. and {Crowther}, P.~A. and {Garc{\'\i}a}, M. and {Herrero}, A. and {Sana}, H. and {Sim{\'o}n-D{\'\i}az}, S. and {Taylor}, W.~D. and {van Loon}, J. Th. and {Vink}, J.~S. and {Walborn}, N.~R.},
+        title = "{The VLT-FLAMES Tarantula Survey. XVI. The optical and NIR extinction laws in 30 Doradus and the photometric determination of the effective temperatures of OB stars}",
+      journal = {\aap},
+     keywords = {open clusters and associations: individual: 30 Doradus, dust, extinction, Magellanic Clouds, stars: early-type, stars: fundamental parameters, Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - Solar and Stellar Astrophysics},
+         year = 2014,
+        month = apr,
+       volume = {564},
+          eid = {A63},
+        pages = {A63},
+          doi = {10.1051/0004-6361/201423439},
+archivePrefix = {arXiv},
+       eprint = {1402.3062},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2014A&A...564A..63M},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Valencic04,
+   author = {{Valencic}, L.~A. and {Clayton}, G.~C. and {Gordon}, K.~D.},
+    title = "{Ultraviolet Extinction Properties in the Milky Way}",
+  journal = {\apj},
+     year = 2004,
+    month = dec,
+   volume = 616,
+    pages = {912-924},
+      doi = {10.1086/424922},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJ...616..912V&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Weingartner01,
+   author = {{Weingartner}, J.~C. and {Draine}, B.~T.},
+    title = "{Dust Grain-Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud}",
+  journal = {\apj},
+     year = 2001,
+    month = feb,
+   volume = 548,
+    pages = {296-309},
+      doi = {10.1086/318651},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2001ApJ...548..296W&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
+}
+
+@ARTICLE{Zubko04,
+   author = {{Zubko}, V. and {Dwek}, E. and {Arendt}, R.~G.},
+    title = "{Interstellar Dust Models Consistent with Extinction, Emission, and Abundance Constraints}",
+  journal = {\apjs},
+     year = 2004,
+    month = jun,
+   volume = 152,
+    pages = {211-249},
+      doi = {10.1086/382351},
+   adsurl = {http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2004ApJS..152..211Z&db_key=AST},
+  adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System}
 }
diff --git a/paper/paper.md b/paper/paper.md
@@ -41,16 +41,23 @@ ranges.
 
 The types of extinction models supported are Averages, Parameter Averages, Grain Models, and Shape.  [explain each kind]  [provide plots]
 
-![Parameter Average models [@Gordon23].\label{fig:parameter_averages}](parameter_average_models.png)
+![Examples of Average models [@Bastiaansen92; @Gordon03; @Gordon09; @Gordon21; @Gordon24].\label{fig:averages}](average_models_uv_nir.png)
+
+![Examples of Parameter Average models [@Cardelli89; @ODonnell94; @Fitzpatrick99; @Fitzpatrick04; @Valencic04; @Gordon09; @MaizApellaniz14; @Fitzpatrick19; @Decleir22; @Gordon23].\label{fig:parameter_averages}](parameter_average_models.png)
+
+![Examples of Grain models [@Desert90; @Weingartner01; @Draine03; @Zubko04; @Compiegne11; @Jones13; @Hensley23].\label{fig:grain}](parameter_average_models.png)
+
+![Examples of a Shape models [@Fitzpatrick90].\label{fig:shapes}](shape_models.png)
 
 The wavelength dependence of extinction for a model is computing by passing a
 wavelength or frequency vector with astropy units. Each model has a valid
-wavelength range this is enforced to ensure as extrapolation is not supported.
-The model output is in the standard $A(\lambda)/A(V)$ units where $A(\lambda)
-is the extinction at wavelength $\lambda$ and $A(V)$ is the extinction in the 
-Johnson V band.  Every model has a helper `extinguish` function that alternatively
-provides the fractional effects of extinction for a specific dust column $A(V)$.
-This allows for the effects of dust to be modeled for or removed from an observation.
+wavelength range this is enforced as extrapolation is not supported. The model
+output is in the standard $A(\lambda)/A(V)$ units where $A(\lambda) is the
+extinction at wavelength $\lambda$ and $A(V)$ is the extinction in the Johnson
+V band. Every model has a helper `extinguish` function that alternatively
+provides the fractional effects of extinction for a specific dust column
+$A(V)$. This allows for the effects of dust to be modeled for or removed from
+an observation.
 
 This package does not implement dust attenuation models. Dust attenuation
 results in observations of more complex systems like a star with nearby,
@@ -60,4 +67,6 @@ come from scattering into the observer beam. Thus, the wavelength dependence of
 dust attenuation is dependent on the dust grain properties and dust radiative
 transfer.
 
+Any published dust extinction model is welcome for inclusion in this package.
+
 # References
diff --git a/paper/shape_models.png b/paper/shape_models.png