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@drphilmarshall and I were talking about the paper today and identified a potential problem with Eq. 2. An integral over d_i makes this an integral over one galaxy's photometry. The sum of Eq. 3 wou…
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When attempting to run a standard DE fitting process, e.g.:
> fit_1 = DE_fit.DEfit(pspl)
Python raises RunTimeErrors stemming from the multiprocessing library, which complains that the code is usi…
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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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ADES 2022a (and previous versions) allow reporting photometric information within the 'photometry group'. When the group is present, the keys 'mag' and 'band' are required. 'mag' is defined as the app…
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At least one source (Hya04) has a Gaia parallax from the Ultracool sheet, but we haven't ingested its Gaia proper motion, photometry, etc. This makes me think it's time to do another big Gaia ingest. …
kelle updated
4 months ago
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Core-collapse "templates" in SNANA are created from photometric light curves of individual SNe: An existing spectral time series (e.g., Nugent tempate) is warped to match the observed photometry of th…
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Hi, thank you for developpoing this tools.
I'm a beginner in coding and using fiber photometry. I would like to use your tool to analyse my data but I encounter an error in the installation process …
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Accessing SDSS Legacy Survey photometry and single fiber spectroscopy will be a common task. Can we make this doable in Marvin?
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Hello,
Thank you very much for this great code! I am an undergraduate student and right now I am using BASE-9 for my research project about determining the age of open cluster NGC 2509 with Gaia ED…
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Attempting forced photometry of sources not in an image throws an exception. Thus we should only attempt photometry of sources that fall in iamge.
1. [ ] Check to see which sources are in an image…