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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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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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Roman Coronagraph will use images of Uranus/Neptune as astrophysical flat sources. The planet will be dithered and imaged across the relevant field on EXCAM and the average astrophysical signal will b…
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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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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
4 months 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 …