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To let the user know beforehand the units of the spectrum.
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Dear Adam, thank you for making this code available!
I am currently in a situation where I want to plot some things like posterior photometry and spectroscopy samples, photometry and spectroscopy …
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##### Description
The Kepler Point Spread Function (PSF), like any real-world optical instrument, depends on its location in the focal plane, both *x, y*, and radial distance *z*. The conspicuous …
gully updated
6 years ago
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Error is:
"""
Traceback (most recent call last):
File "/usr/lib64/python3.7/multiprocessing/pool.py", line 121, in worker
result = (True, func(*args, **kwds))
File "/home/rowe/Documents…
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DR1 did not include any new measurements made on the SDSS images. In the future, we should include this as forced photometry on the individual images.
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Apologies if there is some obvious way to do this, I couldn't find anything in the documentation.
I'm wanting to fit a 'realistic' SN with host and mw dust. When simulating photometry using realiz…
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In the process of making the SED for the object 2MASS 0415, I have acquired more publicly available data that needs to be ingested.
- [x] AKARI Spectrum
- [ ] LRIS Spectrum
- [ ] MKO. M' band …
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Hello,
I have an issue with the flatpak Siril 1.0RC2. This problem is absent from the Siril AppImage 1.0 RC2 which works fine.
In the "image processing" menu, when I want use the "color calibrat…
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Hi Ken, seems as though the forced photometry in the eyeball list often doesn't show up, or shows up for just a few objects. Could you take a look when you get a chance?
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The Y band photometry for [WISE J111838.70+312537.9](https://simple-bd-archive.org/load_solo/WISE%20J111838.70+312537.9) uses the instrument FanCam which is mounted on a telescope in Fan Mountain Obse…