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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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README.md
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README.md
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# CSiBORG analysis tools
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# CSiBORG analysis tools :dart:
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## TODO :scroll:
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- [ ] Calculate $\left\{M_{\rm vir}, R_{\rm vir}, c\right\}$ from $\left\{R_s, \rho_0, \ldots \right\}$
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- [ ] Calculate $M_{\rm 500c}$ by sphere shrinking
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- [ ] Calculate the cross-correlation in CSiBORG. Should see the scale of the constraints?
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## Open questions :bulb:
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- Get uncertainty on the fitted $R_{\rm s}$? If so get this directly from JAX.
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