csiborgtools/README.md

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# CSiBORGTools
Within halo work and NFW fit (#4) * add listing of snapshots * change distance to comoving * ignore cp files * rename nb * add str to list * add NFW profile shapes * add fits imports * Rename to Nsnap * in clumps_read only select props * make clumpid int * expand doc * add import * edit readme * distribute halos * add profile & posterior * add import * add import * add documentation * add rvs and init guess * update todo * update nb * add file * return end index too * change clump_ids format to int32 * skeleton of dump particle * update nb * add func to drop 0 clump indxs parts * add import * add halo dump * switch to float32 * Update TODO * update TODO * add func that loads a split * add halo object * Rename to clump * make post work with a clump * add optimiser * add Nsplits * ignore submission scripts * ignore .out * add dumppath * add job splitting * add split halos script * rename file * renaem files * rm file * rename imports * edit desc * add pick clump * add number of particles * update TODO * update todo * add script * add dumping * change dumpdir structure * change dumpdir * add import * Remove tqdm * Increase the number of splits * rm shuffle option * Change to remove split * add emojis * fix part counts in splits * change num of splits * rm with particle cut * keep splits * fit only if 10 part and more * add min distance * rm warning about not set vels * update TODO * calculate rho0 too * add results collection * add import * add func to combine splits * update TODO * add extract cols * update nb * update TODO
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### Questions
- How well can observed clusters be matched to CSiBORG? Do their masses agree?
- Is the number of clusters in CSiBORG consistent?
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## CSiBORG Galaxy Environmental Dependence
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### TODO
- [ ] Add gradient and Hessian of the overdensity field.
Within halo work and NFW fit (#4) * add listing of snapshots * change distance to comoving * ignore cp files * rename nb * add str to list * add NFW profile shapes * add fits imports * Rename to Nsnap * in clumps_read only select props * make clumpid int * expand doc * add import * edit readme * distribute halos * add profile & posterior * add import * add import * add documentation * add rvs and init guess * update todo * update nb * add file * return end index too * change clump_ids format to int32 * skeleton of dump particle * update nb * add func to drop 0 clump indxs parts * add import * add halo dump * switch to float32 * Update TODO * update TODO * add func that loads a split * add halo object * Rename to clump * make post work with a clump * add optimiser * add Nsplits * ignore submission scripts * ignore .out * add dumppath * add job splitting * add split halos script * rename file * renaem files * rm file * rename imports * edit desc * add pick clump * add number of particles * update TODO * update todo * add script * add dumping * change dumpdir structure * change dumpdir * add import * Remove tqdm * Increase the number of splits * rm shuffle option * Change to remove split * add emojis * fix part counts in splits * change num of splits * rm with particle cut * keep splits * fit only if 10 part and more * add min distance * rm warning about not set vels * update TODO * calculate rho0 too * add results collection * add import * add func to combine splits * update TODO * add extract cols * update nb * update TODO
2022-10-30 20:16:56 +00:00
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### Questions
- Environmental dependence of:
- $M_*$, colour and SFR.
- Galaxy alignment.
- HI content.
Within halo work and NFW fit (#4) * add listing of snapshots * change distance to comoving * ignore cp files * rename nb * add str to list * add NFW profile shapes * add fits imports * Rename to Nsnap * in clumps_read only select props * make clumpid int * expand doc * add import * edit readme * distribute halos * add profile & posterior * add import * add import * add documentation * add rvs and init guess * update todo * update nb * add file * return end index too * change clump_ids format to int32 * skeleton of dump particle * update nb * add func to drop 0 clump indxs parts * add import * add halo dump * switch to float32 * Update TODO * update TODO * add func that loads a split * add halo object * Rename to clump * make post work with a clump * add optimiser * add Nsplits * ignore submission scripts * ignore .out * add dumppath * add job splitting * add split halos script * rename file * renaem files * rm file * rename imports * edit desc * add pick clump * add number of particles * update TODO * update todo * add script * add dumping * change dumpdir structure * change dumpdir * add import * Remove tqdm * Increase the number of splits * rm shuffle option * Change to remove split * add emojis * fix part counts in splits * change num of splits * rm with particle cut * keep splits * fit only if 10 part and more * add min distance * rm warning about not set vels * update TODO * calculate rho0 too * add results collection * add import * add func to combine splits * update TODO * add extract cols * update nb * update TODO
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- Fields to calculate:
1. Overdensity field $\delta$
2. Gradient and Hessian of $\delta$
3. Gravitational field $\Phi$
4. Gradient and Hessian of $\Phi$