Table A.1.
Parameters derived from the fits of the lines of J0802+25.
| Line | FWHM | vs | Flux x10−15 | Flux fraction |
|---|---|---|---|---|
| [km s−1] | [km s−1] | [erg cm−2 s−1)] | [%] | |
| Paα (n) | 443±12 | 0±5 | 7.74±1.11 | 56 |
| Paα (i) | 719±48 | 580±32 | 2.41±0.39 | 17 |
| Paα (b) | 1183 | -325 | 3.52±0.58 | 25 |
| He II (n) | 443 | -165±19 | 1.18±0.18 | 100 |
| He I (n) | 443 | 42±30 | 0.95±0.16 | 100 |
| Brδ (n) | 445 | -84±81 | 0.3±0.07 | 100 |
| [Si VI] (n) | 593±106 | -47±41 | 1.83±0.45 | 59 |
| [Si VI] (i) | 753±186 | 775±151 | 0.97±0.3 | 31 |
| [Si VI] (b) | 1361 | -313 | 0.28±0.3 | 9 |
| H2 1-0S(1) (n) | 421±19 | 17±7 | 1.43±0.21 | 100 |
| H2 1-0S(2) (n) | 453±81 | -94±26 | 0.67±0.17 | 100 |
| H2 1-0S(3) (n) | 420±30 | -16±11 | 1.55±0.26 | 100 |
Notes. Emission line and component fit: narrow (n), intermediate (i), and broad (b). (2) FWHM corrected for instrumental broadening. (3) Velocity relative to the narrow component(s) of either Paα or Brγ. (4) Integrated line flux. Since the measurements were done in the rest-frame spectrum, the fluxes include a multiplicative factor of (1+z). Errors were computed as the quadratic sum of the errors from the fit and the flux calibration error estimated from the standard star spectrum. Parameters without errors have been fixed to their initial guess.
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