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CCL will allow you to define a cosmology with a scale-dependent mu / Sigma parameterization, and ask for a 'boltzmann_camb' or 'boltzmann_class' transfer function (rather than an 'isitgr') transfer fu…
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- [ ] Explain basic KSB
- [ ] Add content from Viola et al. (2010)
- [ ] Add an appendix on Taylor expansions and its induced biases.
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Hi there!
I have an issue with classy (thus maybe with class?) and the computation of the shear power spectrum.
I noticed that the shear power spectrum (as obtained by cl['ll'][0], where cl = Class()…
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Includes a discussion of the dwarf luminosity function
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### Are you submitting a **bug report** or a **feature request**?
Bug report
### What is the current behavior?
Assuming
```typescript
type FormValue = {
user: {
name: string;
…
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AI: NR and GDA: have a final catalog with KiDS/450+GAMA (vel. disp.) samples
AI: NR and CR catalog with KiDS/450+BOSS (vel. disp.) samples
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Nivya and Angela check the way to use Galfit/GALAPAGOS on LSST images
NRN checks the documentation for the GalSim catalogs
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Let's discuss the metric we want to use to assess the quality of the deblending.
What I have in mind:
- Measure the flux of object in field without deblending
- Re-measure after deblending
We can …
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While working on Twinkles, discovered that all the values coming out of OM10 for 'REFF' are 0.0.
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@EiffL, @patricialarsen, and @jablazek have been working on getting 2pt correlation (e.g. ellipticity-direction) for IA model testing.
Can one of you list the items that we should test? And we can…
yymao updated
6 years ago