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BHTOM Harvesters:
- [ ] Gaia Alerts
- [ ] Antares
- [ ] OGLE EWS
BHTOM AliasBrokers:
- [ ] Antares
- [ ] Asassn
- [ ] Atlas
- [ ] Catalina
- [ ] Gaia
- [ ] gaia_dr3
- [ ] neowise
- [ …
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### Instrument
MIRI (Stages 1-3)
### What is your suggestion?
For MIRI imaging (especially with long wavelength filters), the observations are quite background noise limited. Rather than just…
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This is a project to create a notebook to explore how aperture photometry works in the data processing stack. Suggested to me by @bechtol , some questions to be explored are:
* how are the apertur…
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There should be an option to reshape the photometry table so that the bands are columns.
For example:
txt = 'SELECT \* FROM photometry WHERE source_id=700'
t = db.query(txt, fmt='table')
df = t.to_pan…
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From FY24 Q2 QU
> We will also use the new HSC+VIDEO images and catalogues produced from the above pipeline run, to search for dwarf galaxies and test whether the addition of the near infrared photom…
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Search radius is currently hardcoded and noted for PanSTARRS forced photometry query.
Having a form option with limits would be ideal.
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Table output available [here](https://github.com/aleksds/bates_galaxies_lab/blob/master/hst/sg_fluxtable_nm.txt)
Code to make table available [here](https://github.com/aleksds/bates_galaxies_lab/bl…
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Use Andrea's source list to populate the SOURCES and PHOTOMETRY tables.
Make sure the photometry bands are renamed to match `svo_filters`.
Add `ra` and `dec` columns to the PHOTOMETRY table.
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The current library often uses "spectra", replace to "spectrum" where appropriate.
Also, the use of "filter_spectra" makes no sense. Change to the more normal "filter_profile", they are still Lezar…
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Hi Sean,
Thanks for creating this, it's incredibly helpful!
I just ran into a KeyError on ['nyquist_limit'] and checked main.py. You call this:
if image_fwhm < autophot_input['p…