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Hey AstroImageJ team,
some of the newer CMOS cameras from ASI and QHY use the first N rows of an image to encode metadata about the image. When performing a plate solve these pixels are picked up a…
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Objective: simulate the science use case that we call “MICADO-SCAO-GaiaRef”. It assesses the achievable accuracy in absolute astrometry for science objects observed with MICADO at the ELT in SCAO mode…
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It would be great to have one page where we can easily see which twinkles datasets have been produced, how each one was produced, and how the data can be access.
For each data release we could inclu…
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Solving a FITS file with thousand of NaNs values, I get the next error:
fitstable.c:956:read_array_into: Failed to read column from FITS file
fitstable.c:956:read_array_into: Failed to read column fr…
ppmim updated
9 years ago
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digicampipe has a strict dependence on python=3.6 in environment.yml. However, on Mac with M1 processors (arm64 architecture ) Python 3.6 is not available and "There are no plans to backport support t…
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Ekta, as part of checking whether all SA quantities are ordered ugriz, can you plot g-r vs the g-r you would infer from the half-light sb quantities, ie
```
cg_sb50g - cg_sb50i
```
Also, can you tak…
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fix this already!
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The 'supergiant' region of the diagram comes from bad absmag values in the HGY catalog.
Stars with uncertain parallax are given a distance of 10 million parsecs (and for some reason that is used in t…
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The atrometric precision in some sub-images, which are at the corner of the full image, depends on the position in the sub-image. The plot below shows the astrometric precision within sub-sub-images o…