updated citation info and fixed codecov badge

Author: mirochaj

CITATION

@@ -1,10 +1,7 @@
-If you use any of the global 21-cm signal or UV/X-ray radiation background stuff, you should cite 
-citing: 
+If you use any of the global 21-cm signal or UV/X-ray radiation background stuff, you should cite:
 
     Mirocha, J., 2014, MNRAS, 443, 1211
 
-For BibTex users:
-
 @ARTICLE{2014MNRAS.443.1211M,
    author = {{Mirocha}, J.},
     title = "{Decoding the X-ray properties of pre-reionization era sources}",
@@ -21,12 +18,10 @@ archivePrefix = "arXiv",
   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
 
-For the 1-D radiative transfer or SED optimization, please cite:
+For the 1-D radiative transfer please cite:
 
     Mirocha, J., Skory, S., Burns, J.O., Wise, J.W., 2012, ApJ, 756, 94
 
-For BibTex users:
-
 @ARTICLE{2012ApJ...756...94M,
    author = {{Mirocha}, J. and {Skory}, S. and {Burns}, J.~O. and {Wise}, J.~H.
 	},
@@ -46,7 +41,7 @@ archivePrefix = "arXiv",
   adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
 
-For global 21-cm calculations using new UVLF-based model, please cite
+For global 21-cm calculations using the UVLF-based model, please cite
 
 @ARTICLE{2017MNRAS.464.1365M,
        author = {{Mirocha}, Jordan and {Furlanetto}, Steven R. and {Sun}, Guochao},
@@ -87,4 +82,22 @@ archivePrefix = {arXiv},
       adsnote = {Provided by the SAO/NASA Astrophysics Data System}
 }
 
+If you use any of the more sophisticated galaxy modeling stuff, e.g., dust reddening, spectral synthesis, please consider citing
 
+@ARTICLE{2020MNRAS.498.2645M,
+       author = {{Mirocha}, Jordan and {Mason}, Charlotte and {Stark}, Daniel P.},
+        title = "{Effects of self-consistent rest-ultraviolet colours in semi-empirical galaxy formation models}",
+      journal = {\mnras},
+     keywords = {dust, extinction, galaxies: evolution, galaxies: high-redshift, galaxies: ISM, Astrophysics - Astrophysics of Galaxies},
+         year = 2020,
+        month = oct,
+       volume = {498},
+       number = {2},
+        pages = {2645-2661},
+          doi = {10.1093/mnras/staa2586},
+archivePrefix = {arXiv},
+       eprint = {2005.07208},
+ primaryClass = {astro-ph.GA},
+       adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.498.2645M},
+      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
+}

README.md

@@ -1,5 +1,5 @@
 # **ARES**
-[![Documentation Status](https://readthedocs.org/projects/ares/badge/?version=latest)](http://ares.readthedocs.io/en/latest/?badge=latest) ![Tests](https://github.com/mirochaj/ares/actions/workflows/test_suite.yaml/badge.svg) [![codecov](https://codecov.io/gh/mirochaj/ares/branch/master/graph/badge.svg?token=Q3CCKIMQJF)](https://codecov.io/gh/mirochaj/ares) [![Last Commit](https://img.shields.io/github/last-commit/mirochaj/ares)](https://img.shields.io/github/last-commit/mirochaj/ares)
+[![Documentation Status](https://readthedocs.org/projects/ares/badge/?version=latest)](http://ares.readthedocs.io/en/latest/?badge=latest) ![Tests](https://github.com/mirochaj/ares/actions/workflows/test_suite.yaml/badge.svg) [![codecov](https://codecov.io/gh/mirochaj/ares/branch/main/graph/badge.svg?token=Q3CCKIMQJF)](https://codecov.io/gh/mirochaj/ares) [![Last Commit](https://img.shields.io/github/last-commit/mirochaj/ares)](https://img.shields.io/github/last-commit/mirochaj/ares)
 
 The Accelerated Reionization Era Simulations (ARES) code was designed to
 rapidly generate models for the global 21-cm signal. It can also be used as a
@@ -26,12 +26,12 @@ risk! Correctness of results is not guaranteed.
 
 ## Citation
 
-If you use ARES in paper please reference [Mirocha (2014)](http://adsabs.harvard.edu/abs/2014MNRAS.443.1211M) if it's an application of the global 21-cm modeling machinery and [Mirocha et al. (2012)](http://adsabs.harvard.edu/abs/2012ApJ...756...94M) if you use the 1-D radiative transfer and/or SED optimization. Note that for some applications, ARES relies heavily on lookup tables and publicly-available software packages that should be referenced as well. These include:
+If you use ARES in paper please reference [Mirocha (2014)](http://adsabs.harvard.edu/abs/2014MNRAS.443.1211M) if it's an application of the global 21-cm modeling machinery and [Mirocha et al. (2012)](http://adsabs.harvard.edu/abs/2012ApJ...756...94M) if you use the 1-D radiative transfer. Note that for some applications, ARES relies heavily on lookup tables and publicly-available software packages that should be referenced as well. These include:
 
 - [CAMB](https://camb.readthedocs.io/en/latest/)
 - [hmf](https://hmf.readthedocs.io/en/latest/)
 - Collisional coupling coefficients from [Zygelman (2005)](https://ui.adsabs.harvard.edu/abs/2005ApJ...622.1356Z/abstract).
-- Lyman:math:`\alpha` transition probabilities from [Pritchard \& Furlanetto](https://ui.adsabs.harvard.edu/abs/2006MNRAS.367.1057P/abstract).
+- Lyman-alpha transition probabilities from [Pritchard \& Furlanetto](https://ui.adsabs.harvard.edu/abs/2006MNRAS.367.1057P/abstract).
 
 Please also provide a link to [this page](https://github.com/mirochaj/ares) as a footnote.