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Type:
Task
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Status: Done (View Workflow)
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Priority:
Normal
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Resolution: Done
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Affects Version/s: None
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Fix Version/s: None
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Component/s: None
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Labels:
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Epic Link:
This is a ticket continued from PIPE2D-1582 and addresses the wavelength windows to inter/extrapolate PFS spectra to measure the HSC and Gaia broad-band fluxes for the focal plane fitting. The assumption here is that we first apply the 'master' flux calibration vector to pfsMerged so that we can ignore the discontinuities between the dichroics and telluric absorption lines.
case 6: n is missing. Interpolate between b and m, and extrapolate m to n. Use G and Bp. The extrapolation to n is a bit scary, but G should be fine as the extrapolation covers a limited part of the G-band. It covers a significant fraction of Rp, and let' not use Rp.