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As a long term goal and as we move into data taking, we would like to make produced images after ISR look as realistic as we can. We should work with experts in camera and survey data to identify imp…
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Today I heard a talk by Gregory Snyder ( @gsnyder206 ) in which he showed something super cool:
He's been making synthetic galaxy images from the Illustris simulation to simulate data in various passb…
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**Submitting author:** @wmarg (Margret Westerkamp)
**Repository:** https://github.com/NIFTy-PPL/J-UBIK
**Branch with paper.md** (empty if default branch): main
**Version:** 0.2
**Editor:** Pending
**R…
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z>2 Lyman-break galaxies are likely to be QSO contaminants so we should develop and include appropriate templates for this class of objects. My instinct is that the ELG templates may be sufficient bu…
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Hi Kyle (& Avery),
Thanks again for your help.
All the work you see here is based on the catalogue (rgz_75 which has about 33,000 lines) used for the WISE color-color map in Paper 1. Using the sam…
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Last week I got told off by Peter Draper for overloading the meta-data server of the cosma7 file system. The reason: I was running 192 parallel instances of a script that uses swiftsimio to extract ga…
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GM 17/12/2018
AI @MariaAngelaRaj write a brief description of the issue and the steps we need to undertake.
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We are still in the process of planning the Simulation inputs for SN in TWINKLES 3. We are interested in keeping things somewhat realistic, but this is to be able to evaluate questions we want to in s…
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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 …