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Building on #4709, it would be useful to add a way to choose which photometry de-duplication strategy to use (e.g. a `deduplicate_strategy` argument). This could initially enable 3 different behavior…
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Currently the Examples and Tutorials section of the documentation re-creates the outline of the notebook tutorials, which are rendered on the same page as the documentation. Instead, this section shou…
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Some errors I encountered when I run it:
In **vizier_tools.py**, the print statement `print qs` should be converted to Python3 format.
Fixing that it fails on calibrate_photometry.py with the foll…
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filters like g', r', etc get ignored when fitting with mosfit
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Some suggested reads from Chris Miller:
DES: http://iopscience.iop.org/article/10.1086/684053/meta
https://arxiv.org/pdf/1504.02983.pdf
```
If you look at Table 1, Yuanyuan finds (weak) evid…
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### Contact Details
_No response_
### What is the process type?
None
### Measurand
Wavelength
Wavenumber
Color temperature, correlated
Absorbance, regular, spectral
Radiance factor,…
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Skeleton for script to do this.
Modified columns to track calibration changes.
Added in initial selection of data
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Related to #21, it was suggested by @paulmartini to include the rest-frame (absolute) photometry, as a tool for assessing the redshift (particularly for the QSOs).
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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
2 months ago
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BHTOM Harvesters:
- [ ] Gaia Alerts
- [ ] Antares
- [ ] OGLE EWS
BHTOM AliasBrokers:
- [ ] Antares
- [ ] Asassn
- [ ] Atlas
- [ ] Catalina
- [ ] Gaia
- [ ] gaia_dr3
- [ ] neowise
- [ …