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Looking at the Cross correlations in the QLP, the red and green CCDs a small offset on the plots, about 4 km/s. I cannot tell if this is a plotting issue , has to do with the new WLS in the post-serv…
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The RV uncertainties in the L2 files appear to be too large. The is apparent in multiple RM observation sequences, one of which is shown below. Note in that plot that the post-egress RVs vary by sig…
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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…
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See attached Quicklook images of spectra taken when the tip-tilt stage had a problem and a normal exposure.
The test could be to identify massive outlier in the time series of guiding corrections i…
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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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## Ray Trace Files
- [x] #5 Keck 2 Observatory (M1-M3)
- [x] Scott Lilly?
- [x] #6
- [x] Scott Lilly?
- [x] #7
- [ ] Max has this
## Coating Data
- [x] #8
- [x] #9
- [ ] #10
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As discussed in the DRP meeting, @aaronhouseholder should make one or more Quality Control (QC) and Diagnostics tests for the LFC 2D files. The idea is to identify LFC spectra that have enough flux t…
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For example, if 'Keck' is selected, then 'Mauna Kea Observatories' should also be selected. And the dependents should come after.
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This issue is to gauge interest in an Australian-led 8m-class discovery optical imager with fast spectroscopic follow up for the transient community to be operational near the start of this Decadal Pl…
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PypeIt v1.16 has changed the output directories and file names slightly. Some new files exist, too.
pypeit_files/keck_deimos_A/keck_deimos_A/Masters --> Calibrations
- MasterArc_A_1_MSC02.fits --> A…