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How can we use exposure times and/or weight/depth maps to calibrate contamination modeling/extraction/redshift fitting magnitude depths?
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After collecting the first row of a mosaic:
```
2024-06-11T13:54:02.536265-07:00 Unexpected error:
RuntimeError: Task did not complete: Timed out waiting for
RuntimeError: Task did not compl…
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After I had installed paper-qa
```
mamba create -n paperqa2 python=3.11
mamba activate paperqa2
git clone https://github.com/Future-House/paper-qa.git
cd paper-qa
pip install -e .
```
...a…
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- **Etcher version: All recent 1.19.x releases
- **Operating system and architecture:All systems
- **Image flashed: .img.xz files
- **What do you think should have happened:Proper flash and verific…
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Currently if a user supplies an hdf5 file with object spectra for a WFSS simulation, `mirage` will use the source magnitudes from the catalog source file when making the seed image for the direct imag…
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Hi,
I know you support direct device, and or Kryoflux support.
I wonder if it would be possible to add support for greaseweazle boards to read floppy disks. I use one for imaging Amiga ADF disk…
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Hello,
I am using the Aharoni-Lab Miniscope-DAQ-QT-Software for live calcium imaging recordings and have a question regarding the timestamp mechanism used by the software. Specifically, I am trying…
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Hi all,
I realized that for the clang compiler for every major release only the first update version is available but not the latest one.
E.g. for 17.0.x only 17.0.1 is available but that does n…
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Several cockpit/control modifications are described on page 62 of the third printing of _Interstellar Operations: Alternate Eras_. These do not require slots or tonnage, but they do affect cost.
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As described in [1] and Chapter 7 of *Modern Digital Halftoning* by Lau & Are.
> [1] Analoui, M.; Allebach, J.P. (February 1992). "Model-based Halftoning by Direct Binary Search". Proceedings of th…