Scan data collected on 2014-04-27.
|Type||Time [UT]||CW [nm]||θ z|
Notes. The central wavelengths (CWs) of the CRISP prefilters are nominally one or a few tenths of a nm to the red of the wavelengths listed here, but tilted by small angles to center the passbands on the core wavelengths of the spectral lines for which they are usually used. θz denotes the zenith angle of the telescope pointing. The 11:49 scans are referred to below as the “extra” DA scans.
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