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- Run the pipeline with required parameters
- ensure nothing breaks
- make sure resulting deep coadd looks ok
- this will iterate since almost certainly items will break.
- a few iterations will there…
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During the Sprint Week, @DouglasLeeTucker and @saharallam have made progress on creating color magnitude diagrams for GCR Catalogs (protoDC2 and Buzzard).
@DouglasLeeTucker and @saharallam, can you…
yymao updated
6 years ago
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I tried to obtain the star PSF for a very large image of HST. The original image was huge, I tried to obtain the stars first and put them into individual fits. After subtracted the background and mas…
oxno2 updated
1 month ago
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Currently the zoom speed for the companion module goes from 0 - 15. It seems in the new update there are options much higher than 15. I have presets for Speed of 0 and Speed of 8 and those seem to b…
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### FAQ check
- [X] Yes, I checked the FAQ and my question has not been addressed.
### Instrument
NIRSpec (Stages 1-3)
### What happened?
I was running Eureka! with 6 MAST files of WASP…
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_Issue [HLA-1112](https://jira.stsci.edu/browse/HLA-1112) was created on JIRA by [Jennifer Mack](https://jira.stsci.edu/secure/ViewProfile.jspa?name=mack):_
Comment from Rick White in team_burgundy…
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_Issue [JP-3547](https://jira.stsci.edu/browse/JP-3547) was created on JIRA by [Melanie Clarke](https://jira.stsci.edu/secure/ViewProfile.jspa?name=mclarke):_
I am looking into a couple of potentia…
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_Issue [JP-3238](https://jira.stsci.edu/browse/JP-3238) was created on JIRA by [Alicia Canipe](https://jira.stsci.edu/secure/ViewProfile.jspa?name=acanipe):_
NIRCam is working on addressing an issu…
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Assess feasibility of using existing HSC pipeline to do photometry of sources on deepCoadd images, to enable automated tracking of surface brightness metrics as part of FARO.
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At present, the position of the spacecraft for WISE, SOHO, Gaia, etc.-based observations can be provided in ADES, via `pos1`, `pos2`, and `pos3`. You can even specify the upper triangular part …