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@murphyk
Their experiments seem like a great application (and are open-source).
M. Walmsley et al., “Galaxy Zoo: Probabilistic Morphology through Bayesian CNNs and Active Learning,” Mon. Not. R.…
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Tests on galsim simulations revealed ring-shaped artefacts in the residuals for bright sources.
The rings are not caused by monotonicity or any of the constraints, neither are they remnants from ini…
herjy updated
4 years ago
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**Problem description**
Hello,
this is a fresh install of termux on a Pixel 4 with the current Android 11 beta 3 / release candidate.
After installing texlive-full I tried running pdflate…
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\[Sorry if this isn't the right place or time for this issue.\]
In preparing the PZ DC1 paper, we [identified](https://github.com/LSSTDESC/PZDC1paper/issues/15) a need for "true" redshift PDFs, whi…
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Suggest tweaks to:
"The use of a small sample of synthetic images to calibrate and test our model clustering and fitting code has demonstrated our ability to recover galaxy morphology, despite a sys…
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Needs a bit of reorganizing and more of a lead in. I would suggest.
The calibration subset was a set of nine synthetic galaxy images created from Galaxy Builder models, which were then re-run thro…
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I don't understand this: "Disk classifications were doubled in effective radius to account for an observed tendency of volunteers to draw a smaller disk than needed." - why does that matter for cluste…
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See this ATLAS source:
https://star.pst.qub.ac.uk/sne/atlas4/candidate/1145713851494028200/
flagged as orphan but there is a bright nearby galaxy
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Before we even get to the upgrade to Gaia+PS1
I think we need to consider just replacing GSC with PPMXL
"PPMXL is a combination of the data from the USNO-B1.0 and the infrared 2MASS catalog. It …
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Sources are initialised by building coadds weighted by a pre-computed sed and applying a set of morphological constraints on the coadds to get a morphology. This means that the coad has to be computed…
herjy updated
4 years ago