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CSiBORG analysis tools.
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README.md | ||
setup.py |
CSiBORG Tools
Tools for analysing the suite of Constrained Simulations in BORG (CSiBORG) simulations. The interface is designed to work with the following suites of simulations: CSiBORG1 (dark matter-only RAMSES), CSiBORG2 (dark matter-only Gadget4), Quijote (dark-matter only Gadget2), however with little effort it can support other simulations as well.
Ongoing projects
Consistent halo reconstruction
- Make a sketch of the overlap definition and add it to the paper.
- Improve the storage system for overlaps and calculate it for all simulations.
Enviromental dependence of galaxy properties
- Calculate the SPH density field for CSiBORG1.
- Check that the velocity-field flipping of x and z coordinates is correct.
- Evaluate and share the density field for SDSS & SDSSxALFALFA for both CSiBORG2 and random fields.
- Check and verify the density field of galaxy colours (cannot do this now! Glamdring is super slow.)
Calculated data
SPH-density & velocity field
- CSiBORG2_main, CSiBORG2_random, CSiBORG2_varysmall
- Evaluated for SDSS and SDSSxALFALFA in: CSiBORG2_main, CSiBORG2_random
Radial velocity field
Mass-assembly of massive clusters
- Make a list of nearby most-massive clusters.
- Write code to identify a counterpart of such clusters.
- Write code to make a plot of mass-assembly of all clusters within a certain mass range from the random simulations.
- Write code to compare mass-assembly of a specific cluster with respect to random ones.
Effect of small-scale noise
- Study how the small-scale noise variation affects the overlap measure, halo concentration and spin.
Gravitational-wave and large-scale structure
- Make the velocity field data available.
CSiBORG meets X-ray
- Make available one example snapshot from the simulation. Mention the issue with x- and z-coordinates.
CSiBORG advertising
- Decide on the webpage design and what to store there.
- Write a short letter describing the simulations.