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Spliced Dataset UVSUM_1X_56644-56648



Dataset MODE−λcen Aper Range Texp MJD QF Vshft XC Fscl
E140H-1271_31x0.05NB_56644-56648 FITS
1160.0-1349.5 5140 56644.626 142 +0.18
1.462
E140M-1425_31x0.05NC_56644-56648 FITS
1163.7-1703.8 4923 56644.446 161 +0.01 1302.27 [0.12] 1.204
E230M-1978_31x0.05NC_56644-56648 FITS
1614.8-2334.5 5144 56644.493 210 +0.01
1.292
ocb6n2020 FITS E230H-2463 31×0.05NB 2329.1−2585.3 1913 56646.497 148 +0.01
1.098
ocb6n2030 FITS E230H-2513 31×0.05NB 2392.3−2639.6 2564 56646.554 169 +0.01
1.030
E230H-2713_31x0.05NB_56644-56648 FITS
2580.2-2807.0 3734 56644.560 178 −0.11 2600.33 [0.11] 1.555
ocb6n2040 FITS E230H-2912 31×0.05NB 2783.4−3046.8 2570 56646.620 158 −0.12 2796.53 [0.14] 1.000

Notes. Aper is abbreviated aperture code (31×0.05NB= 31″×0.05″NDB). Spectral Range is in Å. Texp is total exposure time (in s). MJD is first start time of a sequence. QF is quality factor (average S/N per resel). Vshft is wavelength correction (in km/s) derived from pair-wise cross-correlations. XC are cross-correlation template parameters (λ and [Δλ], in Å). Cross-correlation, if any, was applied between template spectrum and preceding one. If no template params are reported ("∼") beyond first spectrum, "blind" coaddition (no relative shifts) was performed. Fscl is flux scale factor bootstrapped from overlap zones with reliable flux ratios, relative to spectrum with best apparent throughput (Fscl= 1).

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