Table 5
Sample of the information in Lockman-SpReSO
| ID units (1) | RA (deg) (2) | Dec (deg) (3) | CAT (4) | mag (5) | mag err (6) | FIR (mJy) (7) | FIR err (mJy) (8) | zphot (9) | z (10) | z err (11) | z type (12) | line (13) | z line (14) | z line err (15) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 84957 | 163.07966 | 57.36440 | 4 | 19.085 | 0.002 | 260 | 30 | 0.082 | 0.07464 | 0.00006 | spec | [O III] λ4959 | 0.0746 | 0.0002 |
| [O III] λ5007 | 0.0747 | 0.0001 | ||||||||||||
| [S II] λ6716 | 0.0746 | 0.0002 | ||||||||||||
| [S II] λ6731 | 0.0746 | 0.0002 | ||||||||||||
| 128229 | 163.16754 | 57.61459 | 4 | 20.854 | 0.004 | 730 | 20 | 0.474 | 0.482938 | 0.000009 | spec | Ca II λ3934 | 0.48505 | - |
| Са II λ3968 | 0.48368 | - | ||||||||||||
| Hß | 0.48305 | 0.00002 | ||||||||||||
| Hα | 0.48291 | 0.00001 |
| ID units (1) | line obs. centre (Å) (16) | line obs. centre err (Å) (17) | line flu (erg s−1 cm2 × 10−7)(18) | line flux err (erg s−1 cm2 × 10−17) (19) | FWHM line (Å) (20) | line FWHM err (Å) (21) | line EW (Å) (22) | line S/N (Å) (23) | line quality (24) |
|---|---|---|---|---|---|---|---|---|---|
| 84957 | 5329 | 1 | 17 | 3 | 21 | 3 | −2.54 | 12 | 5 |
| 5381.5 | 0.5 | 29 | 2 | 19 | 1 | −7.03 | 19 | 5 | |
| 7217 | 1 | 15 | 2 | 17 | 2 | −5.21 | 13 | 5 | |
| 7234 | 1 | 16 | 2 | 17 | 2 | −5.75 | 14 | 5 | |
| 128229 | 5842 | - | 2 | - | 2 | - | 1.32 | 1 | 1 |
| 5887 | - | 2 | - | 3 | - | 1.85 | 1 | 1 | |
| 7209.5 | 0.1 | 38.2 | 0.9 | 10.0 | 0.2 | −55.67 | 19 | 5 | |
| 9732.36 | 0.07 | 91 | 1 | 16.4 | 0.2 | −241.34 | 35 | 5 |
Notes. Column 1 is the unique identification number for each object in the catalogue. Columns 2 and 3 give the optical coordinates (12000) of the object. Coordinates of counterparts in other bands, available in FT12, and FIR coordinates are also included. Column 4 is the flag to indicate to which catalogue the object belongs: (1) X-ray point sources or CV star candidates; (2) high-velocity halo stars; (3) poorly studied radio galaxies; (4) FIR-objects; (5) objects in both CAT = 1 and CAT = 4; (7) objects in both CAT = 3 and CAT = 4; (12) objects in both CAT = 1 and CAT = 2; 20) very red QSOs selected using the Glikman et al. (2013) method; (21) very red QSOs selected using the Ross et al. (2015) criteria; (23) objects in both CAT = 20 and CAT = 3; (24) objects in both CAT = 20 and CAT = 4; (25) objects in both CAT = 21 and CAT = 2; and (26) objects in both CAT = 21 and CAT = 3. Columns 5 and 6 are the AB magnitudes and errors for al the bands available in FT12 from FUV (GALEX) to 8 μm (Spitzer; see Sect. 3 in FT12 for more details). Columns 7 and 8 give the FIR fluxes and errors at 24, 100, and 160 μm from the PEP work expressed in mly (Lutz et al. 2011). Column 9 is the photometric redshift calculated in FT12. Columns 10 and 11 are the object redshift and the error measured in this work. Column 12 is the flag to mark how the redshift has been obtained. Two values are possible: ‘spec’ and ‘sup’. Columns 13–24 are the main parameters of the fitted line using the model explained in the text. Each parameter of the Gaussian and line model is included in the table, as well as the EW and S/N obtained in the fitting process, and the quality criterion assigned in the first visual inspection.
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