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This email from Joel from August 13th provides details:
Hi Ani and Jordan,
This appears to be a typo in skyserver. The correct link is https://www.sdss.org/dr15/algorithms/, not https://www.sdss.or…
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**ppxf_kinematics_example_sdss.py**: ran ok
**ppxf_population_example_sdss.py**: gave me a best fit but matplotlib warned: warnings.warn("tight_layout : falling back to Agg renderer")
**ppxf_kinematic…
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Mansi suggested that instead of throwing out u-band data that is not in SDSS fields, we use the zeropoint from a SDSS field that was observed on the same night. We need to think about how to quantify …
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Hello.
I want to use BADASS to fit non-SDSS spectrum, so I run non-SDSS code to fit SDSS spectrum as a test. I find the profile of spectrum is changed when resampling spectrum to log scale (blue l…
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dobos updated
6 years ago
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One of our super-users cannot get to the SDSS/NVSS links. Has posted in bug reports, but here's the summary. We're definitely missing out from this person running blind, thanks.
@WizardHowl
http:…
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I'm routinely looking up paths for SDSS-5 data and SDSS-4 data.
I use a dictionary to lookup instances of `SDSSPath(...)` so that I don't have to create a `SDSSPath` object every time I evaluate a …
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legacyhalos-upenn-parent.fits is a MEF with three sets of photometry of interest --
* SDSSPHOT - (shallow) SDSS ugriz + forced unWISE photometry
* LSPHOT - (deeper) LegacySurvey grz + forced unWISE …
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The header currently contains keywords 'HIERARCH GEOCORONAL SKYE SHADOW_HEIGHT' (also for SKYW and SCI), however these do not agree with what I calculate myself from the shadow_calc python code that i…
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For a final catalogs we're going to want consistent magnitudes across all the SLUGGs galaxies. Right now, our method of computing zero point relies on querying SDSS and getting the difference between …