Table A.2
COSMOS GALEX and Spitzer counterparts of the sample.
| ID | FUV | NUV | IRAC1 | IRAC2 | IRAC3 | IRAC4 | MIPS |
|
|
|||||||
| 1 | 25.17 ± 0.60∗ | 415.89 ± 0.46 | 835.39 ± 0.73 | 1431.50 ± 1.92 | 2070.05 ± 2.51 | 7.20 ± 0.06 | |
| 2 | 7.48 ± 0.15 | 9.79 ± 0.27 | 7.14 ± 0.98 | 10.32 ± 2.22 | <0.15 | ||
| 3 | 11.96 ± 0.15 | 14.94 ± 0.26 | 13.26 ± 0.91 | 9.02 ± 2.13∗ | 0.22 ± 0.02 | ||
| 4 | 11.37 ± 0.15 | 15.10 ± 0.26 | 24.18 ± 0.96 | 50.98 ± 2.09 | 0.89 ± 0.01 | ||
| 5 | 23.44 ± 0.40∗ | 179.79 ± 0.29 | 149.72 ± 0.35 | 121.56 ± 1.05 | 122.63 ± 2.12 | 0.48 ± 0.02 | |
| 6 | 25.97 ± 0.16 | 29.95 ± 0.25 | 29.85 ± 1.00 | 23.57 ± 1.93 | 0.16 ± 0.04∗ | ||
| 7 | 24.54 ± 0.16 | 28.28 ± 0.25 | 28.45 ± 1.00 | 13.74 ± 1.92 | <0.15 | ||
| 8 | 120.53 ± 1.25∗ | 90.79 ± 1.32∗ | 70.25 ± 1.94∗ | 49.12 ± 3.50∗ | <0.15 | ||
| 9 | 10.18 ± 0.15 | 12.21 ± 0.25 | 13.58 ± 0.91 | 16.94 ± 2.01 | <0.15 | ||
| 10 | 6.66 ± 0.14 | 10.09 ± 0.24 | 13.51 ± 0.89 | 33.11 ± 2.04 | 0.23 ± 0.02 | ||
| 11 | 55.75 ± 0.19 | 42.22 ± 0.28 | 24.53 ± 0.94 | 12.45 ± 2.06 | <0.15 | ||
| 12 | 9.46 ± 0.15 | 11.29 ± 0.24 | 10.95 ± 0.94 | 8.76 ± 1.98 | <0.08 | ||
| 13 | 17.10 ± 0.15 | 14.62 ± 0.27 | 7.18 ± 0.92 | 7.88 ± 2.22 | <0.08 | ||
| 14 | 31.60 ± 0.16 | 39.58 ± 0.26 | 27.60 ± 0.93 | 22.73 ± 1.97 | 0.19 ± 0.03∗ | ||
| 15 | 62.48 ± 0.18 | 46.91 ± 0.30 | 28.36 ± 0.89 | 22.13 ± 2.21 | <0.08 | ||
| 16 | 73.50 ± 0.40∗ | 50.67 ± 0.50∗ | 40.40 ± 1.60∗ | 25.54 ± 3.16∗ | 0.15 ± 0.02 | ||
| 17 | 30.72 ± 1.75∗ | 35.95 ± 1.50∗ | 28.05 ± 1.90∗ | 24.00 ± 2.20∗ | <0.15 | ||
| 18 | 93.82 ± 0.35∗ | 89.19 ± 0.43∗ | 83.76 ± 1.13 | 133.58 ± 2.46 | 1.43 ± 0.01 | ||
| 19 | 144.75 ± 0.26 | 115.41 ± 0.30 | 75.15 ± 1.04 | 48.2 ± 1.98 | 0.30 ± 0.02 | ||
| 20 | 22.54 ± 0.40∗ | 20.05 ± 0.50∗ | 16.15 ± 2.00∗ | 15.00 ± 2.50∗ | <0.15 | ||
| 21 | 44.56 ± 0.18 | 30.88 ± 0.25 | 17.57 ± 0.99 | 22.25 ± 2.06 | <0.15 | ||
| 22 | 7.28 ± 0.14 | 7.95 ± 0.26 | <9.81∗ | 14.23 ± 2.15 | 0.16 ± 0.03∗ | ||
| 23 | 41.87 ± 0.16 | 31.54 ± 0.27 | 26.96 ± 0.79 | 13.40 ± 2.05 | <0.15 | ||
| 24 | 22.21 ± 0.16 | 27.75 ± 0.29 | 37.36 ± 0.84 | 27.45 ± 2.40 | 0.67 ± 0.05∗ | ||
| 25 | 144.73 ± 0.26 | 96.56 ± 0.33 | 75.37 ± 1.03 | 34.72 ± 2.45 | 0.17 ± 0.05∗ | ||
| 26 | 109.67 ± 0.22 | 66.80 ± 0.27 | 46.35 ± 0.93 | 23.93 ± 1.94 | <0.15 | ||
| 27 | 11.29 ± 0.13 | 13.09 ± 0.22 | 15.46 ± 0.77 | 5.99 ± 1.68 | <0.15 | ||
| 28 | 10.48 ± 0.14 | 13.85 ± 0.21 | 16.98 ± 0.88 | 22.97 ± 1.66 | 0.13 ± 0.03∗ | ||
| 29 | 24.07 ± 0.09 | 20.62 ± 0.02 | 140.90 ± 0.23 | 226.38 ± 0.37 | 316.10 ± 1.02 | 446.18 ± 2.18 | 1.49 ± 0.02 |
| 30 | 7.85 ± 0.16 | 9.91 ± 0.23 | 15.63 ± 1.08 | 14.24 ± 1.78 | <0.15 | ||
| 31 | 10.59 ± 0.16 | 15.30 ± 0.26 | 14.69 ± 0.97 | 24.92 ± 2.23 | <0.15 | ||
| 32 | 11.63 ± 0.14 | 9.35 ± 0.23 | 8.76 ± 0.84 | 13.57 ± 1.87 | <0.15 | ||
| 33 | 19.68 ± 0.19 | 17.11 ± 1.17 | <0.30 | ||||
| 34 | 62.26 ± 0.46 | 88.70 ± 0.58 | 96.12 ± 1.16 | 108.93 ± 2.14 | 0.27 ± 0.02 | ||
| 35 | 23.42 ± 0.06 | 52.47 ± 0.20 | 71.41 ± 0.30 | 81.98 ± 1.10 | 100.70 ± 2.17 | 0.40 ± 0.02 | |
| 36 | 14.83 ± 0.14 | 16.54 ± 0.26 | 19.27 ± 0.88 | 13.52 ± 2.05 | <0.15 | ||
| 37 | 21.15 ± 0.02 | 258.63 ± 0.39 | 405.22 ± 0.55 | 594.43 ± 1.54 | 794.89 ± 2.69 | 2.59 ± 0.02 | |
| 38 | 23.74 ± 0.18 | 27.74 ± 0.27 | 33.27 ± 1.04 | 22.81 ± 2.06 | 0.32 ± 0.02 | ||
| 39 | 16.22 ± 0.16 | 17.71 ± 0.27 | 17.13 ± 0.99 | 10.73 ± 2.15 | <0.15 | ||
| 40 | 53.68 ± 0.19 | 42.13 ± 0.29 | 22.46 ± 1.07 | 16.74 ± 2.31 | <0.15 | ||
| 41 | 24.05 ± 0.09 | 38.92 ± 0.17 | 38.52 ± 0.26 | 52.85 ± 0.93 | 167.18 ± 2.02 | 1.73 ± 0.14 | |
| 42 | 55.38 ± 4.00∗ | 49.06 ± 5.00∗ | 30.02 ± 4.00∗ | 27.03 ± 5.00∗ | <0.15 | ||
| 43 | 79.54 ± 2.00∗ | 69.96 ± 3.00∗ | 46.10 ± 3.00∗ | 36.23 ± 4.00∗ | <0.15 | ||
| 44 | 24.50 ± 0.25∗ | 49.14 ± 0.18 | 44.33 ± 0.28 | 36.46 ± 0.97 | 65.43 ± 2.26 | 0.84 ± 0.10 | |
| 45 | 66.08 ± 0.19 | 51.05 ± 0.25 | 34.95 ± 0.94 | 24.60 ± 1.78 | <0.15 | ||
| 46 | 36.56 ± 0.32∗ | 25.53 ± 0.48∗ | 17.10 ± 1.00∗ | 12.70 ± 2.00∗ | <0.15 | ||
Notes. Column description: (1) ID number of the object; (2), (3) GALEX FUV and NUV magnitudes with their errors; (4), (7) Spitzer/IRAC 4-channel (3.6, 4.5, 5.8, and 8.0 μm) fluxes with their errors; (8) Spitzer/MIPS flux at 24 μm with its error. The values marked by ∗ are measured by our 3′′-aperture photometry on the images.
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