Eureka
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Eureka! is a data reduction and analysis pipeline intended for time-series observations with JWST.
Holding off on merging this until I can test more thoroughly, but this should allow for WFC3 exposures of inconsistent read lengths to be properly handled.
### Instrument NIRSpec (Stages 1-3) ### What happened? I am currently Running Stage 3 of Eureka! Pipeline, specifically in generating 2-D spectrum plot with linear wavelength x-axis. It seems that...
### What is your suggestion? It would be really helpful if Eureka! could provide a demo on how to reduce and fit data from HST STIS G430L and G750L observations....
This PR reformats the fitted variable names in Stage 5 to use _ch# for different channels and _pl# for different planets. This will make the code far more robust since...
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Other (any stage) ### What happened? Some WFC3 datasets don't have...
Addressed #638 and also enables users to supply a wavelength file in S4 for pre-computed bins. Also adds joint white light curve fitting to docs and demo ecf to address...
### Instrument Light curve fitting (Stages 4-6) ### What is your suggestion? The current settings (e.g., `pc_offset` and `pc_amp`) calculate the phase curve offset and amplitude of the individual orders,...
This PR resolves #519 by changing the convention to mask=0 for bad data to mask=True for bad data. I've run all the tests locally and don't get any crashes, but...
### Instrument Light curve fitting (Stages 4-6) ### What is your suggestion? The docs didn't get fully updated after PR #659. The docs still say `When fitting for multiple planets,...
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Light curve fitting (Stages 4-6) ### What happened? For my stage...