Eureka
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kevin218
Eureka! is a data reduction and analysis pipeline intended for time-series observations with JWST.
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Light curve fitting (Stages 4-6) ### What happened? When using GPs...
This pull request adds in hexagonal apertures to the NIRCam photometry modes, since the defocused image is hexagonal (like the observatory main mirror), and not circular. Thanks to Ian for...
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Light curve fitting (Stages 4-6) ### What happened? I get a...
This draft PR introduces the `S1MetaClass` which is a child of the original `readECF.MetaClass` object. This new class holds Stage 1 specific defaults for different instruments. This will allow for...
### Instrument Light curve fitting (Stages 4-6) ### What happened? The current naming scheme is confusing when fitting multiple planets over multiple channels. While we're at it, we should either:...
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Other (any stage) ### What happened? Because lc.driftmask isn't created when...
### Instrument NIRSpec (Stages 1-3) ### What is your suggestion? Just like the title: allow users to supply custom bad pixel mask in Stage 1. ### Error traceback output _No...
### Instrument Light curve fitting (Stages 4-6) ### What happened? The ECFs are missing important parameters for joint white LC fitting, as is the documentation. ### Error traceback output _No...
My former intern Isaac Edelman who contributed significant changes/improvements to the Stage 3 photometry code was wondering if he could be added to the Copyright page at https://eurekadocs.readthedocs.io/en/latest/copyright.html which made...
### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument Other (any stage) ### What happened? When performing a joint fit...