a bit of text

bibliographie.bib

@@ -18,28 +18,26 @@
 }
 
 @Article{dvorakMoon,
-  author        = {{Dvorak}, Rudolf and {Loibnegger}, Birgit and {Maindl}, Thomas I.},
-  title         = {{On the probability of the collision of a Mars-sized planet with the Earth to form the Moon}},
-  journal       = {arXiv e-prints},
-  year          = {2015},
-  eid           = {arXiv:1506.09043},
-  month         = {Jun},
-  pages         = {arXiv:1506.09043},
-  eprint        = {1506.09043},
-  adsnote       = {Provided by the SAO/NASA Astrophysics Data System},
-  adsurl        = {https://ui.adsabs.harvard.edu/abs/2015arXiv150609043D},
-  archiveprefix = {arXiv},
-  file          = {:2015arXiv150609043D - On the probability of the collision of a Mars-sized planet with the Earth to form the Moon.pdf:PDF},
-  keywords      = {Astrophysics - Earth and Planetary Astrophysics},
-  primaryclass  = {astro-ph.EP},
+  author       = {{Dvorak}, Rudolf and {Loibnegger}, Birgit and {Maindl}, Thomas I.},
+  title        = {{On the probability of the collision of a Mars-sized planet with the Earth to form the Moon}},
+  journaltitle = {arXiv e-prints},
+  date         = {2015-06},
+  eid          = {arXiv:1506.09043},
+  pages        = {arXiv:1506.09043},
+  eprint       = {1506.09043},
+  eprintclass  = {astro-ph.EP},
+  eprinttype   = {arXiv},
+  adsnote      = {Provided by the SAO/NASA Astrophysics Data System},
+  adsurl       = {https://ui.adsabs.harvard.edu/abs/2015arXiv150609043D},
+  file         = {:2015arXiv150609043D - On the probability of the collision of a Mars-sized planet with the Earth to form the Moon.pdf:PDF},
+  keywords     = {Astrophysics - Earth and Planetary Astrophysics},
 }
 
 @InProceedings{MaindlSummary,
   author    = {{Maindl}, T.~I. and {Sch{\"a}fer}, C.~M. and {Haghighipour}, N. and {Burger}, C. and {Dvorak}, R.},
   title     = {{Collisional water transport and water-loss relevant to formation of habitable planets}},
   booktitle = {Proceedings of the First Greek-Austrian Workshop on Extrasolar Planetary Systems},
-  year      = {2017},
-  month     = {Mar},
+  date      = {2017-03},
   pages     = {137-153},
   adsnote   = {Provided by the SAO/NASA Astrophysics Data System},
   adsurl    = {https://ui.adsabs.harvard.edu/abs/2017pfga.proc..137M},
@@ -48,23 +46,22 @@
 }
 
 @Article{Burger2018,
-  author        = {{Burger}, C. and {Maindl}, T.~I. and {Sch{\"a}fer}, C.~M.},
-  title         = {{Transfer, loss and physical processing of water in hit-and-run collisions of planetary embryos}},
-  journal       = {Celestial Mechanics and Dynamical Astronomy},
-  year          = {2018},
-  volume        = {130},
-  number        = {1},
-  eid           = {2},
-  month         = {Jan},
-  pages         = {2},
-  doi           = {10.1007/s10569-017-9795-3},
-  eprint        = {1710.03669},
-  adsnote       = {Provided by the SAO/NASA Astrophysics Data System},
-  adsurl        = {https://ui.adsabs.harvard.edu/abs/2018CeMDA.130....2B},
-  archiveprefix = {arXiv},
-  file          = {:/home/lukas/Bachelorarbeit/papers/2018CeMDA.130....2B - Transfer, loss and physical processing of water in hit-and-run collisions of planetary embryos.pdf:PDF},
-  keywords      = {Hydrodynamics, Methods: numerical, Planets and satellites: formation, Astrophysics - Earth and Planetary Astrophysics},
-  primaryclass  = {astro-ph.EP},
+  author       = {{Burger}, C. and {Maindl}, T.~I. and {Sch{\"a}fer}, C.~M.},
+  title        = {{Transfer, loss and physical processing of water in hit-and-run collisions of planetary embryos}},
+  journaltitle = {Celestial Mechanics and Dynamical Astronomy},
+  date         = {2018-01},
+  volume       = {130},
+  number       = {1},
+  eid          = {2},
+  pages        = {2},
+  doi          = {10.1007/s10569-017-9795-3},
+  eprint       = {1710.03669},
+  eprintclass  = {astro-ph.EP},
+  eprinttype   = {arXiv},
+  adsnote      = {Provided by the SAO/NASA Astrophysics Data System},
+  adsurl       = {https://ui.adsabs.harvard.edu/abs/2018CeMDA.130....2B},
+  file         = {:/home/lukas/Bachelorarbeit/papers/2018CeMDA.130....2B - Transfer, loss and physical processing of water in hit-and-run collisions of planetary embryos.pdf:PDF},
+  keywords     = {Hydrodynamics, Methods: numerical, Planets and satellites: formation, Astrophysics - Earth and Planetary Astrophysics},
 }
 
 @Thesis{Dorninger,
@@ -72,7 +69,7 @@
   title       = {Realistic physical collision model in planet formation},
   type        = {Bachelor's Thesis},
   institution = {Department of Astrophysics, University of Vienna},
-  year        = {2019},
+  date        = {2019},
   subtitle    = {Benchmark of GPU-environments},
 }
 
@@ -86,7 +83,7 @@
   series        = {IAU Symposium},
   month         = {Jan},
   pages         = {370-373},
-  doi           = {10.1017/S1743921313008971},
+  doi           = {10.1017/s1743921313008971},
   eprint        = {1307.1643},
   adsnote       = {Provided by the SAO/NASA Astrophysics Data System},
   adsurl        = {https://ui.adsabs.harvard.edu/abs/2014IAUS..299..370M},
@@ -96,4 +93,23 @@
   primaryclass  = {astro-ph.EP},
 }
 
+@Article{CollisionTypes,
+  author       = {{Stewart}, Sarah T. and {Leinhardt}, Zo{\"e} M.},
+  title        = {{Collisions between Gravity-dominated Bodies. II. The Diversity of Impact Outcomes during the End Stage of Planet Formation}},
+  journaltitle = {\apj},
+  date         = {2012-05},
+  volume       = {751},
+  number       = {1},
+  eid          = {32},
+  pages        = {32},
+  doi          = {10.1088/0004-637X/751/1/32},
+  eprint       = {1109.4588},
+  eprintclass  = {astro-ph.EP},
+  eprinttype   = {arXiv},
+  adsnote      = {Provided by the SAO/NASA Astrophysics Data System},
+  adsurl       = {https://ui.adsabs.harvard.edu/abs/2012ApJ...751...32S},
+  file         = {:file\:/home/lukas/Bachelorarbeit/papers/CollisionTypes.pdf:PDF},
+  keywords     = {Earth, planets and satellites: composition, planets and satellites: formation, Astrophysics - Earth and Planetary Astrophysics},
+}
+
 @Comment{jabref-meta: databaseType:biblatex;}

main.tex

@@ -20,11 +20,14 @@
 
 \chapter{Introduction}\label{introduction}
 
+
+Here comes some short science explanation about how planets form and water is transported.
 \lipsum[1]
 
-\section{\blabla}
+\section{The perfect merging assumption}
+
+To better understand how this process works, large n-body simulations over the lifetime of the solar systems have been conducted.\todo{give an example} Most of these neglect the physical details of collisions when two bodies collide for simplicity and instead assume that a perfect merging occurs. So all of the mass of the two progenitor bodies and especially all of their water is retained in the newly created body. Obviously this is a simplification as in real collisions perfect merging is very rare and most of the time either partial accretion or a hit-and-run encounter occurs. (\cite{CollisionTypes}) Therefore the amount of water retained after collisions is consistently overestimated in these simulations.
 
-\lipsum[1-2]
 
 
 \begin{figure}
@@ -71,7 +74,7 @@ See Chapter  \ref{introduction}.
 \appendix
 \chapter{Some data}
 
-\lipsum[1]\footcite{Schaefer2016}\footcite{dvorakMoon}\footcite{MaindlSummary}\footcite{Burger2018}\footcite{Dorninger}\footcite{CollisionParameters}
+\lipsum[1]\footcite{Schaefer2016}\footcite{dvorakMoon}\footcite{MaindlSummary}\footcite{Burger2018}\footcite{Dorninger}\footcite{CollisionParameters}\footcite{CollisionTypes}
 
 \printbibliography
 

template.tex

@@ -56,7 +56,7 @@ british, % language of the document
 \usepackage{subcaption} % allows to nicely put two images next to each other
 \usepackage{tabularx}
 \usepackage{booktabs} % nicer table seperations
-
+\usepackage{todonotes}
 %----------------------------------- Style decisions -----------------------------------
 
 \hyphenpenalty=750 % break less words than default - try different values for success