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As a database generator, I want to validate the accuracy of the synthetic database by comparing the summary statistics of a database of patients that would go to Keck Hospital to the actual summary st…
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@jspineda
Keck LRIS and DEIMOS spectra of L and T dwarfs. Will probably need to be converted.
kelle updated
5 months ago
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These three observations are of HD 10700, but have incorrect targname values.
Update header with correct starname where appropriate.
DCS name keyword in the header confirms the star is HD 10700.
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Summary of request: Add a new organization to ROR
Add record:
Name of organization: W.M. Keck Center for Nanoscale Optofluidics*en
Website: https://cfno.soe.ucsc.edu
Domains:
Link to publications: …
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We got the files, let's start with a dummy coating to generate the first jones pupil
![image](https://github.com/Jashcraf/keck-polarization/assets/25557892/25f9e691-41fa-44c7-bf4e-3e9e180c2c3e)
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The LFC master stacks are using etalon spectra to derive the WLS. This has been diagnosed a few ways, 1) by the SCI-OBJ keywords in the header of the LFC WLS master 2) by looking at the etalon spectru…
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The Keck OSIRIS development branch has already worked out how to connect pytest and IDL. Since the OSIRIS pipeline is one of the parents of the GPI data pipeline, it ought to be reasonably straightfor…
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In Henney & O'Dell (1999) we published only 4959, 6568, 6563, 6300, 6312, 5875. But there are many other lines in there too.
First step would be to get the spectra from Bob.
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Add a custom Finder Chart to the Source page that queries a public database not currently listed. [The Keck AO Guide Star Tool](https://www2.keck.hawaii.edu/software/findChartGW/acqTool.php) can creat…