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One thing that’s been bothering me a bit is that we don’t really know much about the morphological output we’re trying to predict. It would be a good addition to the data section as it would reinforce…
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I'm copying over a list of items from a recent email thread to be finalized before the run 1.1i run starts so we can checkoff on them. Please mark off the checks with the PRs are merged and comment f…
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I have finished a complete first draft of the code that rescales the stellar masses in protoDC2. I am raising this Issue so that people can understand the techniques I am using to solve the problem of…
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I wanted to ask for input on where to find the definition of position angle and whether external shear is used for Twinkles images. We produced images of lensed quasar hosts at the Fermilab hack week…
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Subtask of #56.
On a sprinkler-focused telecon Friday 12/15/17 I promised @rbiswas4, @jbkalmbach, and @linan7788626 small examples of glSN+host+lens catalogs that could be used for debugging purpo…
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@yymao @dkorytov For the ellipticity test, I need to recompute the ellipticity using the axis ratio for the galaxy. (because the data defintion differs from the schema definition). But I just checke…
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@adrianpope has access to some high level profiling codes at ANL that were already used to successfully profile and increase the throughput of PhoSim.
He can try to use these tools to identify hots…
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The current implementation of the reader does not define an `ellipticity` field for the galaxy, nor does it define fields like `disk_re_a_true` related to galaxy morphology. The information seems to b…
EiffL updated
6 years ago
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in one or any language
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Subtask of #56.
Given lensed image catalogs from @dannygoldstein, @rbiswas4 will generate time-evolving SEDs of lensed AGNs and supernovae (Type Ia + CCSNe) that can be called by PhoSim (and imSim?…