png preview

Spliced Dataset UVSUM_1X_57034-57037



Dataset MODE−λcen Aper Range Texp MJD QF Vshft XC Fscl
E140H-1271_0.2x.05N2_57034-57035 FITS
1160.2-1350.6 5208 57034.347 67 +2.89
1.102
E140M-1425_0.2x.05N2_57034-57037 FITS
1168.0-1639.2 4698 57034.296 95 +0.95 1303.20 [0.25] 1.137
E230M-1978_0.2x.05N2_57034-57035 FITS
1612.6-2345.3 5204 57034.413 118 +1.09 1630.97 [0.14] 1.129
ocb6k2020 FITS E230H-2463 31×0.05NC 2330.7−2590.9 1861 57037.207 111 −0.56 2344.06 [0.20] 1.677
ocb6k2030 FITS E230H-2513 31×0.05NC 2392.2−2603.8 2574 57037.264 127 −0.92 2586.50 [0.28] 1.691
E230H-2713_31x0.05NC_57034-57035 FITS
2580.3-2809.5 3750 57034.489 190 −2.39 2600.01 [0.26] 1.000
ocb6k2040 FITS E230H-2912 31×0.05NC 2783.7−3047.0 2580 57037.330 107 −1.07 2798.56 [0.25] 1.808

Notes. Aper is abbreviated aperture code (31×0.05NC= 31″×0.05″NDC). 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).

Home