Group Class¶
- class group.Cloud(obj)[source]¶
Bases:
group.Group
Cloud class which has the central boolean.
- class group.Galaxy(obj)[source]¶
Bases:
group.Group
Galaxy class which has the central boolean.
- class group.Group(obj)[source]¶
Bases:
object
Parent class for halo and galaxy and halo objects.
- _assign_local_data()[source]¶
Assign glist/slist/dmlist/bhlist/dlist for this group. Also sets the ngas/nstar/ndm/nbh/ndust attributes.
- _calculate_center_of_mass_quantities()[source]¶
Calculate center-of-mass position and velocity. From caesar_mika
- _calculate_velocity_dispersions()[source]¶
Calculate velocity dispersions for the various components.
- _calculate_virial_quantities()[source]¶
Calculates virial quantities such as r200, circular velocity, and virial temperature.
- _process_group()[source]¶
Process each group after creation. This entails calculating the total mass, iteratively unbinding (if enabled), then calculating more masses, radial quants, virial quants, velocity dispersions, angular quants, and final gas quants.
- property _valid¶
Check against the minimum number of particles to see if this object is ‘valid’.
- contamination_check(lowres=[2, 3, 5], search_factor=1.0, printer=True)[source]¶
Check for low resolution particle contamination.
This method checks for low-resolution particles within
search_factor
of the maximum halo radius. When this method is called on a galaxy, it refers to the parent halo.- Parameters
lowres (list, optional) –
Particle types to be considered low-res. Defaults to [2,3,5]; if your simulation contains blackholes you will want to pass in [2,3]; if your simulation contains active
dust particles you will not include 3.
search_factor (float, optional) – Factor to expand the maximum halo radius search distance by. Default is 2.5
printer (boolean, optional) – Print results?
Notes
This method currently ONLY works on GADGET/GIZMO HDF5 files.
- vtk_vis(rotate=False)[source]¶
Method to render this group’s points via VTK.
- Parameters
rotate (boolean) – Align angular momentum vector with the z-axis before rendering?
Notes
Opens up a pyVTK window; you must have VTK installed to use this method. It is easiest to install via
conda install vtk
.
- write_IC_mask(ic_ds, filename, search_factor=2.5, radius_type='total')[source]¶
Write MUSIC initial condition mask to disk. If called on a galaxy it will look for the parent halo in the IC.
- Parameters
ic_ds (yt dataset) – The initial condition dataset via
yt.load()
.filename (str) – The filename of which to write the mask to. If a full path is not supplied then it will be written in the current directory.
search_factor (float, optional) – How far from the center to select DM particles. Default is 2.5
print_extents (bool, optional) – Print MUSIC extents for cuboid after mask creation
Examples
>>> import yt >>> import caesar >>> >>> snap = 'my_snapshot.hdf5' >>> ic = 'IC.dat' >>> >>> ds = yt.load(snap) >>> ic_ds = yt.load(ic) >>> >>> obj = caesar.load('caesar_my_snapshot.hdf5', ds) >>> obj.galaxies[0].write_IC_mask(ic_ds, 'mymask.txt')
- class group.GroupProperty(source_dict, name)[source]¶
Bases:
object
Class to return default values for the quantities held in the category_mapper dictionaries.
- class group.Halo(obj)[source]¶
Bases:
group.Group
Halo class which has the dmlist attribute, and child boolean.
- group.create_new_group(obj, group_type)[source]¶
Simple function to create a new instance of a specified
group.Group
.- Parameters
obj (
main.CAESAR
) – Main caesar object.group_type ({'halo', 'galaxy','cloud'}) – Which type of group? Options are: halo and galaxy.
- Returns
group – Subclass
group.Halo
orgroup.Galaxy
.- Return type