[PIPE2D-331] Create line-list model of sky Created: 04/Feb/19 Updated: 18/Mar/21 Resolved: 18/Mar/21 |
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| Status: | Won't Fix |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | 5.0 |
| Fix Version/s: | 7.0 |
| Type: | Task | Priority: | Normal |
| Reporter: | hassan | Assignee: | Unassigned |
| Resolution: | Won't Fix | Votes: | 0 |
| Labels: | None | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Attachments: |
sky_schematic.png
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| Issue Links: |
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| Description |
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Create a line list model of the sky, split by v and with spatial structure. This code will be used for the 2D simulator to simulate sky lines, in addition to modeling those sky lines in the DRP pipeline. |
| Comments |
| Comment by murdock [ 07/Feb/19 ] |
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Hasan these papers by Osterbrock et al. have night sky spectra at shorter wavelengths than Rousselout. Osterbrock, Donald E., et al. "Night-sky high-resolution spectral atlas of OH and O2 emission lines for Echelle spectrograph wavelength calibration." Publications of the Astronomical Society of the Pacific 108.721 (1996): 277. Osterbrock, Donald E., Jon P. Fulbright, and Thomas A. Bida. "Night-Sky High-Resolution Spectral Atlas of OH Emission Lines for Echelle Spectrograph Wavelength Calibration. II." Publications of the Astronomical Society of the Pacific 109.735 (1997): 614. I have a list of OH lines, but these include faint high rotational states that may be below the detection limits of PFS. |
| Comment by rhl [ 07/Feb/19 ] |
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We need intensities as well as line lists. Do you (murdock) have them? I think they may be in the Rousselout paper, but they're not in the machine-readable version I have. |