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It is very exciting to see the new HOKI version which provides colour-magnitude diagrams, which are very useful for observational astronomers.
However, many people may depend on different filters t…
sunnc updated
4 years ago
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Hi, since you were so amazingly reactive with solutions last time, I'll give it a try:
Could you find a way to also export other types of data from the .raw? (UV, Light Scattering, CAD, ...)
For…
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Some PHA spectra have `RATE` column instead of `COUNTS`. This is allowed by the FITS OGIP standard. Sherpa reads the 'RATE column' and converts the rates per channel to counts per channel. However, by…
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Greetings,
It took me a while to figure out how to run OpenFAST (or FAST v7 and v8) and get it to process input files. Maybe it’s somewhere I could not find or I just missed, but anyway I hope to m…
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Hate to bother with more issues, but I'm only finding these because of how useful I've found ARAX/ARAX interface 😄
I tried running the following query for finding chemicals connected to SPMSY, which…
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The data loading class appears to be able to read both TTE and pre-binned counts data. However, I cannot find the functionality to handle the binning of the TTE data.
1. How would TTE data be handl…
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**Submitting author:** @grburgess (J. Michael Burgess)
**Repository:** https://github.com/grburgess/popsynth
**Version:** v1.0.3
**Editor:** @xuanxu
**Reviewer:** @HeloiseS, @warrickball
**Archive:** …
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Hi there,
Could you please help me with two errors (below) about Peptide Shaker? Thank you very much!
Lichun
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Comparing the values of the response spectrum of pseudo-accelerations (Sa) obtained from gmprocess and other independent code, I find important differences for the small periods. for example in gmpro…
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Hey!
I have a question about generating spectra (specially HI) in simulations that have radiative transfer (RT). Currently from what I understand, trident uses cloudy Ion balance tables to calcula…