Co-Added Dataset o47k020p0
| Dataset | MODE−λcen | Aper | Range | Texp | MJD | QF | Vshft | XC / Fscl |
|---|---|---|---|---|---|---|---|---|
| o47k020p0_1 | E230M-2707 | 0.2×0.2C | 2280−3118 | 360 | 50712.793 | 56 | +0.00 | 2600.08 [0.21] |
| o47k020p0_2 | E230M-2707 | 0.2×0.2C | 2280−3118 | 360 | 50712.799 | 56 | −0.34 | 0.992 |
| o47k020p0_3 | E230M-2707 | 0.2×0.2C | 2280−3118 | 360 | 50712.805 | 56 | −1.31 | 0.992 |
| o47k020p0_4 | E230M-2707 | 0.2×0.2C | 2280−3118 | 360 | 50712.810 | 56 | −1.90 | 0.996 |
Notes. Aper is abbreviated aperture code (0.2×0.2C= 0.2″×0.2″FPC). Spectral Range is in Å. Texp is integration time (in s). MJD is U.T. start time of each sub-exposure. QF is quality factor (average S/N per resel) . Vshft is wavelength correction (in km/s) derived by cross-correlation relative to first spectrum listed. Datasets normally are time-ordered, unless later sub-exposure of the sequence had significantly higher throughput, in which case it would be in first position. Cross-correlation template parameters (XC: λ and [Δλ], in Å), if any, are provided for first spectrum, but refer to entire group. Null template ("∼") indicates simple co-addition (no shifts). Values in that column for subsequent datasets are flux scale factors (Fscl) relative to leading spectrum (for which Fscl= 1). Wavelengths and fluxes for sub-exposure "_n" can be found in FITS extension n+1 of co-added dataset o47k020p0.