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FuseTS should support using ccdc for change detection, this is a potential library to use:
https://code.usgs.gov/lcmap/pyccd
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Processing of iTelescope images from T32 and T09, in particular, fails in `ap_find_stars.py`:
```
2021-01-16 19:41:12,069 | __main__ | DEBUG | FITS keywords found in image: {'IMG_FILE': ('calibrated…
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I've just committed a new version of the INDIClient module with many of the features we were discussing in other posts (apparent positions, better management of image properties/keywords, etc).
Lots …
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We currently have
- _pdbx_diffrn_merge_stat.number_all (`The total number of reflections contributing to this data set.`)
- _pdbx_diffrn_merge_stat.number_obs (`The number of reflections satisfying …
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I'm trying to walk through the instruction in the README.md file to create a custom environment.
Summarizing, the steps I took were to copy avalon/datagen/godot to another location, per instructions
…
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# Validation of test runs of DESC/Roman sims
There is a plan to carry out test runs for the DESC/Roman simulations (see #roman-desc-sims on Slack) before sprint week. During sprint week, we hope t…
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### User Story
- **As a** satellite observer
- **I want** to graphically enter observations
- **So that** I can estimate a satellite's orbit
### Acceptance Criteria
- **Given** a configured ob…
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I've run into a rare case that throws a
`numpy.linalg.linalg.LinAlgError: Singular matrix` error.
To my understanding:
- The fit function uses a closed form regression technique to calcula…
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Hello sir,
I am chornelis, I hope you are in a good condition. I want to finish my thesis about analysis data photometry using your code with my data. But, when i try the tutorial 3, "img=si.SingleI…
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This code would measure background in inter-order regions of the 2D image and fit a 2D polynomial to it.
Background light is currently visible in the continuum of L1 ThAr spectra.