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Spliced Dataset UVSUM_1X_56936-56939



Dataset MODE−λcen Aper Range Texp MJD QF Vshft XC Fscl
E140H-1271_0.2x0.09_56936-56938 FITS
1160.0-1349.5 5228 56936.300 98 +0.89
1.090
E140M-1425_0.2x0.09_56936-56939 FITS
1170.0-1705.3 5067 56936.249 165 −0.40 1249.79 [0.23] 1.027
E230M-1978_31x0.05NA_56936-56938 FITS
1614.1-2337.2 3726 56936.443 113 −0.03 1632.65 [0.14] 1.000
ocb6u2020 FITS E230H-2463 0.2×0.09 2329.5−2590.1 2614 56939.418 103 +0.10 2333.45 [0.34] 1.353
ocb6u2030 FITS E230H-2513 0.2×0.09 2391.0−2616.4 2614 56939.484 107 +0.20 2494.03 [0.29] 1.333
E230H-2713_0.2x0.09_56936-56938 FITS
2580.7-2830.4 5228 56936.366 165 −0.37 2612.65 [0.38] 1.247
ocb6u2040 FITS E230H-2912 0.2×0.09 2783.5−3046.7 2614 56939.551 108 −0.39 2815.85 [0.14] 1.260

Notes. Aper is abbreviated aperture code (0.2×0.09= 0.2″×0.09″). 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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