Table A.5.
Pair candidates without ALLWISE photometry.
| Prime QSO | RA/Decl. (2000.0) | g′ | r′ | i′ | z′ | J | H | K | ID |
|---|---|---|---|---|---|---|---|---|---|
| CFHQSJ1509-1749 | 227.4413 −17.8303 | >23.47 | >23.94 | >23.32 | 22.31±0.16 | 21.28±0.27 | >21.01 | >20.32 | QSO/M8 |
| DESJ0454-4448 | 73.5198 −44.8196 | >23.65 | >24.21 | 23.49±0.26 | 21.60±0.08 | 20.05±0.10 | 20.41±0.20 | 19.70±0.29 | L1 |
| IMSJ2204+0012 | 331.0878 +01.2344 | >23.79 | >24.20 | >23.66 | 22.09±0.11 | 20.95±0.21 | 20.37±0.21 | >19.71 | QSO/M8 |
| PSOJ009.7355-10.4316 | 9.7185−10.4161 | >24.52 | >24.36 | >23.17 | 21.79±0.12 | 20.85±0.28 | 20.54±0.30 | >19.99 | QSO/M9 |
| PSOJ011.3899+09.0325 | 11.3462 +09.0813 | >23.84 | >23.84 | >23.51 | 21.54±0.09 | >21.67 | 20.96±0.33 | >20.13 | QSO/M6 |
| PSOJ036.5078+03.0498 | 36.5245 +03.0958 | >24.79 | >24.69 | 23.30±0.28 | 21.60±0.09 | 20.06±0.10 | 20.02±0.14 | >20.08 | |
| PSOJ045.1840-22.5408 | 45.1936 −22.5280 | >25.37 | >24.59 | >23.60 | 21.97±0.12 | 20.66±0.19 | 20.16±0.20 | >19.33 | QSO/M9 |
| PSOJ071.0322-04.5591 | 71.0745 −04.5348 | >24.87 | >24.38 | >24.08 | 22.29±0.13 | 21.22±0.20 | >20.94 | 19.74±0.18 | |
| PSOJ071.4507-02.3332 | 71.4815 −02.3637 | >25.08 | >24.75 | 23.25±0.18 | 21.65±0.07 | 20.45±0.11 | 20.52±0.18 | >20.11 | |
| PSOJ261.0364+19.0286 | 261.0269 +19.0228 | >25.23 | >24.85 | 23.90±0.23 | 22.23±0.09 | >21.48 | >20.84 | >19.89 | QSO/? |
| PSOJ267.0021+22.7812 | 266.9979 +22.7922 | >23.07 | >23.51 | >23.14 | 21.35±0.09 | 20.85±0.23 | 20.28±0.25 | >19.86 | QSO/T6 |
| PSOJ328.7339-09.5076 | 328.7633 −09.4779 | >23.80 | >24.10 | 23.25±0.32 | 21.63±0.09 | 20.44±0.14 | 20.03±0.13 | >19.38 | |
| SDSSJ0303-0019 | 45.8859 −00.3281 | >25.72 | >25.16 | >24.49 | 22.89±0.14 | >22.02 | >21.53 | >20.06 | T8 |
| SDSSJ2053+0047_1 | 313.3294 +00.7677 | >23.53 | >23.91 | >23.41 | 22.20±0.14 | 21.01±0.25 | 21.04±0.33 | >19.99 | M9 |
| SDSSJ2053+0047_3 | 313.3766 +00.7606 | >23.78 | >23.70 | >23.49 | 22.06±0.15 | 21.34±0.30 | >20.91 | >20.34 | M5 |
| SDSSJ2054-0005_3 | 313.5334 −00.0914 | >24.00 | >24.25 | >23.71 | 21.81±0.10 | 20.82±0.18 | 20.44±0.25 | >19.73 | |
| SDSSJ2054-0005_4 | 313.5450 −00.0525 | >24.00 | >24.25 | >23.71 | 22.16±0.12 | 20.98±0.20 | 20.79±0.28 | >19.98 |
Notes. Magnitudes are not corrected for foreground AV, all in the AB system. The ID column gives the best-fitting Le PHARE spectral template. The objects marked in boldface are those where the Le PHARE fit preferred a QSO high-z template, and we obtained optical spectroscopy. Except for PSOJ071.0322-04.5591, our spectra argue against a QSO nature, and we therefore provide the next best-fitting templates, mostly dwarf stars (see text). For objects with an asterisk () in the last column, see Table A.6.
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