Co-Added Dataset E230H-2013_0.2x0.09_51680-51690
| Dataset | MODE−λcen | Aper | Range | Texp | MJD | QF | Vshft | XC / Fscl | |
|---|---|---|---|---|---|---|---|---|---|
| o5cn01010 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 1884 | 51685.635 | 9 | +0.00 | 2142.89 [0.08] |
| o5cn01020 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51685.690 | 11 | +0.25 | 1.039 |
| o5cn01030 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51685.757 | 11 | +0.06 | 1.039 |
| o5cn01040 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2074 | 51685.832 | 9 | −0.21 | 1.034 |
| o5cn01050 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51685.891 | 11 | −0.24 | 1.043 |
| o5cn02010 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 1884 | 51680.742 | 9 | +0.68 | 1.014 |
| o5cn02020 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51680.797 | 11 | +0.44 | 1.023 |
| o5cn02030 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51680.864 | 11 | +0.34 | 1.018 |
| o5cn02040 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2074 | 51680.939 | 9 | +0.48 | 1.021 |
| o5cn03010 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 1884 | 51690.662 | 9 | +0.86 | 1.033 |
| o5cn03020 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51690.717 | 11 | +0.61 | 1.076 |
| o5cn03030 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51690.784 | 11 | +0.42 | 1.074 |
| o5cn03040 | FITS | E230H-2013 | 0.2×0.09 | 1879−2149 | 2906 | 51690.851 | 11 | +0.49 | 1.070 |
Notes. Aper is abbreviated aperture code (0.2×0.09= 0.2″×0.09″). Spectral Range is in Å. Texp is total integration time of dataset (in s). MJD is U.T. start time of observation. 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. Dataset with highest throughput normally is 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).