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Detections with Celeste #46

@andrevitorelli

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@andrevitorelli

Shear Reading 2021-04-08 10:00

Bastien: Celeste

  • Not detection, but a full generative model.
  • Completely different from sextractor & tractor
  • build a model from the parameter disribution space
  • more like a model fitting than a detection procedure
  • choose 1 reference band and colors to find other filters
  • testing on SDSS-like generated images
  • some parameters are fixed in advance
  • each pixel may have contributions from several objects
  • brightness: gamma function distributed
  • color distribution: multivariate gaussian
  • mixture component is a categorical distribution
  • galaxy models: bulge + disk
  • mu_s position/detection
  • priors from the position, from other surveys
  • proceed with fitting
  • when no positions available: convolve wihth matched filters to increase snr. find pixels value exceeds local + upper bound of noise.
  • Test: Stripe82 using Photo (Lupton) as prior.
  • positions are better by ~1-% (N=654)

Axel:

  • are they detecting galaxies? (Table 2 of celeste paper)
  • why are they detecting more galaxies? Blends?

Andre:

  • The input catalogue is just a prior.

Bastien:

  • Then the fit is optimized.

Andre:

  • Starnet partitions images to control positions/parameter space

Bastien:

  • part of LSST DESC, same people
  • generative models in starnet represent objects better.

Andre:

  • do they quote size/storage demands?

Bastien:

  • celeste takes 5 min in a 4 megapixel image with hundreds of obj.
  • in starnet tiling, in celeste, are there limits of objects contributing to a pixel?

Axel:

  • at least one problem: fit the number of obj at some point: you have to fix the # of obj at some point.
  • not see the point, you'll have to fix # at some point.

Andre:

  • you can integrate on all distributions (but it ridiculous).
  • could this give us a mitigation for the starlink problem?

Bastien:

  • Celeste was kind of a first step, starnet came after.

Axel:

  • do they assume models for galaxies:

Bastien:

  • yes, bulge plus disk

Axel:

  • is this used for the detection

Bastien:

  • as you fit everything at once, yes, you can't separate it

Axel:

  • if you have too much variables, things explode, its computationally difficult, and gains of it are low.

Bastien:

  • in the end they do fix a lot of things.

Axel:

  • interesting for metadetection. there are artifacts on images that are difficult to treat.
  • for blends is a really good way

Bastien:

  • in non-blends maybe this wont get better positions, but in blends, maybe yes.
  • starnet uses the same tests on coadds

Andre:

  • first & second pass

Axel:

  • do they need a prior on the psf?

Bastien:

  • they use a mix of Gaussian fitted to known stars.

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