Title: Angular momentum distributions for observed and modeled exoplanetary systems
Corresponding

1. You can run "Angular_Momentum_Distribution.ipynb" to re-plot all figures in the paper.

2. The required data files are archived in the folder "data_Sep21":
	2.1. Observational data - "PS_2020.12.12_04.49.59.csv": 
		The data set was downloaded from the exoplanet archive (https://exoplanetarchive.ipac.caltech.edu/)
	2.2. Simulated data - : "_planets.csv" or "_stars.csv".
		The simulation is performed and the data products are generated by Remo Burn (co-author of this paper) 

		2.2.1 The columns of the "_planets.csv" files are (up to tdisk identical, new columns added at the end):

		the identifier
		t: time in years
		Mstar: Stellar mass in solar masses
		Rstar: Stellar radius in solar radii
		ain: inner edge of the disk in au
		Pstar: stellar rotation period in days
		Mplanet: planetary mass in earth masses
		Rplanet: planetary radius in earth radii
		aplanet: semi-major axis of the planet in au
		eccplanet: eccentricity of the planet (no units)
		incplanet: inclination of the planet in radian
		Pplanet: orbital period of the planet in days
		Lplanet: angular momentum of the planet in g cm^2/s
		systemnr: The system identifier
		tdisk: the disk lifetime in years
		dust_to_gas_ratio: the mass ratio of dust to gas in the disk. Is directly related to the metallicity
		Mdisk_ini: the initial gas disk mass in Solar Masses
		exponential_disk_cut_off: the exponential cut-off radius of the initial profile in au, roughly corresponds to disk size

		2.2.2 For the "_stars.csv" files, the same columns are also added at the end, so the columns are now:

		the system identifier
		t: time in years
		Mstar: Stellar mass in solar masses
		Rstar: Stellar radius in solar radii
		Pstar: stellar rotation period in days
		Lspin: stellar angular momentum in g cm^2/s
		Lorbit: sum of the angular momentum of all the planets in the system in g cm^2/s
		tdisk: the disk lifetime in years
		dust_to_gas_ratio: the mass ratio of dust to gas in the disk. Is directly related to the metallicity
		Mdisk_ini: the initial gas disk mass in Solar Masses
		exponential_disk_cut_off: the exponential cut-off radius of the initial profile in au, roughly corresponds to disk size
