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Goal: constraints on the DM sub halo mass function in the Galactic halo using photometric microlensing. DM subhalos are diffuse, and the microlensing signal depends on the slope of the DM density dis…
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Noticed that Galsim throws an error when trying to draw a convolution between a chromatic PSF and the pixel response function. Here is a code snippet showing the issue:
```
import galsim
import …
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Hello,
In running the script `luvoir_demo.py` demo, the dark current appears to precipitously drop off around 1 micron.
![Figure_1](https://user-images.githubusercontent.com/1314227/73049168-c1…
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The catalog bulge/disk/AGN normalizations are specified at a one wavelength but multiply different SEDs, so this issue is to combine the normalization parameters (`fluxnorm_bulge/disk/agn`) with the a…
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At this point, neither webbpsf nor pandeia have changed their use of WFIRST to Roman. This is a tracking issue set up to remind us to make the necessary changes to how we call webbpsf and pandeia when…
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The `optics` module allows specification of an aberrated optics PSF by means of Zernike coefficients of the wavefront. But, the `wavefront` method is specific to a single field location. To model mult…
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In both `$PIPPIN_OUTPUT/PIPPIN_ROMAN_TRANS/1_SIM/SUPERNOVA/LOGS` and `$PIPPIN_OUTPUT/PIPPIN_ROMAN_TRANS/1_SIM/ROMAN_PLAsTiCC/LOGS` simulation jobs are failing with the inability to get use the spectro…
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Hello!
When running `jdi.run_pandexo()` with all instruments, or specifically with WFC3 G141, a KeyError returns.
Appears that in line 652 of `hst.py`, `calRamp = pandeia_input['strategy']['calc…
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I thought I opened an issue about it but I cannot find it.
I need the data models to read `jwst` ASDF files but I don't want to ever run `jwst` pipeline. When I install `jwst` to just get to the da…
pllim updated
1 month ago
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Hey all,
Would it be possible to include the JWST filters by any chance?
Cheers!
Miles
By the way, what is the proper way to specify a custom set of filters? (e.g., if I simply have a numpy …