Table 2.
Photometry of COSMOS-FRI 16, 31, and 70.
| Telescope/survey | Band | COSMOS-FRI 16 | COSMOS-FRI 31 | COSMOS-FRI 70 |
|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) |
| CFHT | u* | 26.07 ± 0.12 | 24.75 ± 0.08 | 26.16 ± 0.14 |
| i* | 23.10 ± 0.14 | 22.33 ± 0.08 | 24.34 ± 0.58 | |
| K | 20.50 ± 0.11 | 20.32 ± 0.09 | 21.40 ± 0.27 | |
| Subaru | BJ | 25.71 ± 0.12 | 24.50 ± 0.06 | 25.14 ± 0.09 |
| g+ | 25.32 ± 0.11 | 24.51 ± 0.05 | 25.27 ± 0.14 | |
| VJ | 24.84 ± 0.08 | 23.94 ± 0.04 | 24.79 ± 0.08 | |
| r+ | 24.23 ± 0.05 | 23.42 ± 0.03 | 24.51 ± 0.06 | |
| i+ | 23.15 ± 0.03 | 22.33 ± 0.02 | 24.35 ± 0.06 | |
| z+ | 22.16 ± 0.02 | 21.61 ± 0.02 | 24.01 ± 0.09 | |
| HST/ACS | F814W | 22.85 ± 0.10 | 22.07 ± 0.07 | 24.13 ± 0.43 |
| UKIRT | J | 21.47 ± 0.08 | 20.97 ± 0.08 | 23.42 ± 0.50 |
| NOAO | Ks | 20.40 ± 0.08 | 20.12 ± 0.05 | 21.76 ± 0.09 |
| GALEX | FUV | – | – | – |
| NUV | – | 25.15 ± 0.24 | – | |
| Spitzer | IRAC1 | (44.29 ± 0.18) μJy | (47.86 ± 0.16) μJy | (17.58 ± 0.16) μJy |
| IRAC2 | (32.54 ± 0.28) μJy | (34.60 ± 0.25) μJy | (20.57 ± 0.26) μJy | |
| IRAC3 | (26.19 ± 0.94) μJy | (24.98 ± 0.81) μJy | (29.83 ± 1.04) μJy | |
| IRAC4 | (18.39 ± 2.26) μJy | (19.36 ± 1.78) μJy | (21.32 ± 2.17) μJy | |
| MIPS (24 μm) | (0.22 ± 0.02) mJy | <0.15 mJy | (0.13 ± 0.03) mJy | |
| MIPS (70 μm) | <5.1 mJy | <5.1 mJy | <5.1 mJy | |
| MIPS (160 μm) | <39 mJy | <39 mJy | <39 mJy | |
| WISE | W1 | 16.923 ± 0.114 | 17.360 ± 0.162 | > 17.672 |
| W2 | 16.711 ± 0.388 | 16.924 ± 0.418 | > 18.324 | |
| W3 | > 10.680 | > 16.955 | > 16.955 | |
| W4 | >7.712 | >7.283 | >15.009 | |
Notes. (1) Survey/telescope; (2) reference band; (3–5) photometric data associated with the sources, along with their uncertainties. Magnitudes from CFHT, Subaru, HST/ACS, UKIRT, NOAO, and GALEX are in AB system and from B13. Spitzer IRAC and MIPS (24 μm) fluxes are also from B13. We report the symbol “–” when the GALEX magnitudes are absent. WISE W1, W2, W3, and W4 magnitudes and magnitude lower limits are in the Vega system.
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