update README.md

README.md

@@ -1,8 +1,8 @@
 # chemcomp
+
 Modeling the chemical composition of gas giants by accretion of pebbles, planetesimals and gas.
 
-## Usage:
-If you use this code in your work and found it useful, please cite [Schneider & Bitsch (2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S)
+**docs: [WIKI](https://chemcomp.readthedocs.io/en/latest/ "wiki")**
 
 ## install:
 clone project:
@@ -17,16 +17,95 @@ Install conda environment:
 
 `conda create -n chemcomp numpy "astropy>=4.0" scipy matplotlib pyyaml jupyter parse h5py pip pytables`
 
-Install `chemcomp`:
+Install a development version `chemcomp`:
 
 `pip install -e .`
 
+or install from pypi
+
+``pip install chemcomp``
+
 Adjust paths in `chemcomp/helper/main_helper` if you need different directories for output and config.
 
+## Publications
+### Original Publications
+
+-   
+
+    [Schneider & Bitsch (2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S)
+
+    :   How drifting and evaporating pebbles shape giant planets. I.
+        Heavy element content and atmospheric C/O
+
+-   
+
+    [Schneider & Bitsch (2021b)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..72SS)
+
+    :   How drifting and evaporating pebbles shape giant planets. II.
+        Volatiles and refractories in atmospheres
+
+-   
+
+    [Bitsch, Schneider & Kreidberg (2022)](https://ui.adsabs.harvard.edu/abs/2022A&A...665A.138B)
+
+    :   How drifting and evaporating pebbles shape giant planets. III.
+        The formation of WASP-77A b and $\tau$ Boötis b
+
+Please cite [Schneider & Bitsch(2021a)](https://ui.adsabs.harvard.edu/abs/2021A&A...654A..71S), if you use `chemcomp` in your work.
+
+### Publications using `chemcomp`
+
+-   
+
+    [Bitsch et al. (2021)](https://ui.adsabs.harvard.edu/abs/2021A&A...649L...5B)
+
+    :   Dry or water world? How the water contents of inner sub-Neptunes
+        constrain giant planet formation and the location of the water
+        ice line
+
+-   
+
+    [Hühn & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023A&A...676A..87H)
+
+    :   How accretion of planet-forming disks influences stellar
+        abundances
+
+-   
+
+    [Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230900509B)
+
+    :   Enriching inner discs and giant planets with heavy elements
+
+-   
+
+    [Mah & Bitsch (2023a)](https://ui.adsabs.harvard.edu/abs/2023A&A...673A..17M)
+
+    :   Forming super-Mercuries: Role of stellar abundances
+
+-   
+
+    [Mah & Bitsch (2023b)](https://ui.adsabs.harvard.edu/abs/2023A&A...677L...7M)
+
+    :   Close-in ice lines and the super-stellar C/O ratio in discs
+        around very low-mass stars
+
+-   
+
+    [Savvidou & Bitsch (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv230903807S)
+
+    :   How to make giant planets via pebble accretion
+
+-   
+
+    [Danti, Bitsch & Mah (2023)](https://ui.adsabs.harvard.edu/abs/2023arXiv231002886D)
+
+    :   Composition of giant planets: the roles of pebbles and
+        planetesimals
+
+And several more in preperation (last updated: 22.11.2023)
+
+
 ## Thanks:
 - I would like to thank Bertram Bitsch for his enormous support during the development of this code and for continuing to use the code together with his students.
 - I would like to thank Cornelis Dullemond for providing the solver which (in adapted version) is used to solve the gas viscous disk equation and dust transport equation.
-- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.
-
-## Help:
-Check the [WIKI](https://chemcomp.readthedocs.io/en/latest/ "wiki")
+- I would like to thank everyone, who has already used chemcomp in their work and has contributed in fixing small bugs.