Table 2
Line parameters of new aCWDBs in the eFEDS area.
ID | Hα | Hβ | HeI4471 | HeII4686 | |||||
---|---|---|---|---|---|---|---|---|---|
FW | F | EW | F | EW | F | EW | F | EW | |
J0840+0005 | 18.0 | 260 | 197 | 204 | 110.7 | 36 | 15.8 | − | − |
J0843–0148 | 22.6 | 635 | 28 | 391 | 19.7 | 69 | 4.2 | − | − |
J0844+0239 | 12.5 | 948 | 68 | 746 | 68.4 | 145 | 14.1 | − | − |
J0845+0339 | 32.5 | +82 | 105 | 70 | 61.0 | 9 | 3.6 | − | − |
J0846+0218 | 12.8 | 230 | 14 | 90 | 6.0 | 64 | 5.6 | 42 | 3.2 |
J0847+0145 | 40.4 | 129 | 151 | 118 | 110.8 | 14 | 10.8 | − | − |
J0851+0308 | 34.5 | 953 | 100 | 953 | 65.8 | 164 | 9.3 | − | − |
J0853+0204 | 47.2 | 91 | 142 | 65 | 82.4 | − | − | − | − |
J0855–0154 | 43.2 | 78 | 80 | 133 | 100.6 | − | − | − | − |
J0902–0142 | 46.1 | 102 | 52 | 82 | 36.2 | − | − | − | − |
J0904+0355 | 44.6 | 176 | 48 | 109 | 22.0 | − | − | − | − |
J0912–0007 | 13.3 | 133 | 67 | 99 | 72.1 | 50 | 38.9 | − | − |
J0914+0137 | 19.4 | 567 | 25 | 446 | 20.0 | 161 | 8.0 | 55 | 2.6 |
J0914+0137(S) | 15.7 | 620 | 26 | 460 | 19.0 | 115 | 5.1 | − | − |
J0918+0436 | 37.8 | 85 | 196 | 43 | 108.6 | − | − | − | − |
J0920+0042 | 26.0 | 2100 | 105 | 1328 | 51.8 | 312 | 13.8 | 226 | 8.6 |
J0926+0105 | 17.5 | 206 | 51 | 195 | 32.0 | 46 | 5.6 | 41 | 5.4 |
J0926+0345 | 37.1 | 189 | 59 | 198 | 46.0 | 26 | 4.8 | − | − |
J0926+0345(S) | 36.3 | 184 | 63 | 182 | 47.6 | − | − | − | − |
J0929+0053 | 17.5 | 45 | 69 | 32 | 50.2 | − | − | − | − |
J0929+0401 | 4.4 | 23 | 2 | 9 | 1.8 | − | − | − | − |
J0932+0343 | 28.6 | 662 | 42 | 195 | 9.0 | − | − | − | − |
J0932+0109 | 15.5 | 230 | 45 | 266 | 44.2 | 72 | 11.9 | 46 | 7.5 |
J0935+0429 | 11.6 | 195 | 33 | 82 | 25.7 | 9 | 2.7 | − | − |
J0844–0128 | − | − | − | − | − | 28 | 8.9 | 3.4 | 1.1 |
J0847+0119 | − | − | − | − | − | 34 | 27.1 | 3.7 | 3.3 |
J0903–0133 | − | − | − | − | − | 97 | 12.9 | 16.7 | 2.5 |
Notes. For Hα the FWHM of a single Gaussian fit to the line profile, the Flux F and the equivalent width EW are given, for the other lines (Hβ, HeI4471, HeII4686) only F and EW are given. Fluxes are given in units of 10−17 erg cm−2 s−1, the FWHM and EW in Å. Some objects were observed more than once in the SDSS project, older spectra (before the eFEDs survey) are labeled (S) in the first column. The three objects at the bottom of the table are the AM CVn objects that do not show Balmer emission lines. The typical uncertainties of the derived quantities are 5–10% statistically but might be larger for non-Gaussian line shapes and more complex continuum shapes than straight lines as assumed here.
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