Table A.1.
Example entries of the spectroscopic table for the two sources presented in Fig. 6.
| ID | IDFROM | RA | Dec | z | zconf | mF606W | […] | zforbid | zforbiderr | zbalmer | zbalmererr | zLyα | zLyαerr | μ | μerr | MUL |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| [deg] | [deg] | [mag] | ||||||||||||||
| 183 | PRIOR | 145.22577 | 7.73872 | 4.03679 | 3 | 22.62 | […] | 4.03354 | 0.00029 | – | – | 4.03658 | 0.00002 | 12.8 | 2.6 | 1.2 |
| 364 | MUSELET | 145.22850 | 7.73786 | 0.33751 | 2 | – | […] | 0.33769 | 0.00002 | 0.33774 | 0.00007 | – | – | 1.0 | 0.0 | – |
| … | … | … | … | … | … | … | […] | … | … | … | … | … | … | … | … | … |
Notes. From left to right: source identification and origin of catalog (PRIOR, MUSELET or EXTERN), sky coordinates, redshift and confidence level, HST photometry in all bands, redshift measurements and errors from pyplatefit for each family of spectral lines, magnification and error estimate, and multiple image identification.
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