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How will the source based data be named? Possible sources:
- MultiSlitModel.slit.name
- MultiSlitModel.slit.slitlet_id
- MultiSlitModel.slit.source_id
- Same combination involving filenames.
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In TSO mode, the data arrays are 3D, where each plane of the cube corresponds to the countrate image for a given integration within the exposure. I think we've already enabled the various calwebb_spec…
sosey updated
6 years ago
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When opening 1D spectra from 2D view, two tabs are opened instead of one, see screenshot.
![screen shot 2018-04-04 at 13 07 46](https://user-images.githubusercontent.com/6149805/38306844-bad12fe6-380…
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* Rebinning according to an input bin edges vector
* `rebin_like(spec)` to use the binning from another spectrum
Please expand on this, I'm not very familiar with rebinning methods or needs.
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(This is based in part on the discussion in #700)
We should add a function/class that retrieves the Schlegel, Finkbeiner, and Davis 1998 dustmaps, caches them, and uses that to get E(B-V) at arbitra…
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Now that a .setup file has become integral to the data reduction,
I propose a refactor where ARMLSD loops on setup and then
science exposure as opposed to looping on science exposure alone.
This…
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SDP is adding a new table extension to all level-1b products that will contain time stamps for each integration within an exposure (see https://jira.stsci.edu/browse/JSDP-387). While primarily intende…
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`PSpec` is a new container object for power spectrum data. It will contain certain methods to ensure consistency of the data (e.g. keeping track of units), and support for basic operations like conver…
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Hi,
When submitting a parallel job I get the following error. I suspect that this issue has something to do with my OpenMPI installation, since it does not occur when I use the same protocol with M…
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How do people normally interpolate the magnitudes/spectra on the age–metallicity grid? 2D linear? Something more intelligent?