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Table 1
Source sample and photometry in the MIR (Spitzer), UV (GALEX), and Hα.
| ID | RA | Dec | r | 3.6 μm | 4.5 μm | 5.8 μm | 8.0 μm | 24 μm | 70 μm | Hα × 1014 | FUV | NUV |
| deg | deg | arcmin | mJy | mJy | mJy | mJy | mJy | mJy | erg s-1 cm-2 | magAB | magAB | |
|
|
||||||||||||
| s1 | 23.34048 | +30.60659 | 9.20 | 0.85 | 0.99 | 1.52 | 2.85 | 3.99 | (8.2) | 0.23 | 30.4 ± 3.9 | 29.8 ± 1.6 |
| s2 | 23.35623 | +30.59784 | 8.11 | 0.77 | 1.28 | 1.54 | 1.84 | 1.35 | ... | 0.01 | ..... ... | ..... ... |
| s3 | 23.55369 | +30.49387 | 15.17 | 1.26 | 2.40 | 3.11 | 3.56 | 3.07 | ... | 0.16 | 30.6 ± 4.2 | 30.7 ± 2.5 |
| s4 | 23.68463 | +30.28031 | 35.46 | 0.62 | 1.12 | 2.84 | 7.14 | 8.70 | 115 | .... | 32.4 ± 9.6 | 31.8 ± 4.2 |
| s5 | 23.18128 | +30.80183 | 27.06 | 0.14 | 0.06 | 0.16 | 0.57 | 3.93 | 15.5 | 0.73 | 27.8 ± 1.1 | 28.2 ± 0.8 |
| s6 | 23.39795 | +30.43258 | 14.29 | 0.54 | 0.35 | 1.81 | 5.65 | 7.55 | 30.7 | 7.27 | 27.6 ± 1.1 | 27.8 ± 0.6 |
| s7 | 23.43383 | +30.80995 | 10.92 | 0.42 | 0.22 | 1.81 | 4.59 | 4.91 | 21.6 | 3.16 | 27.9 ± 1.2 | 28.1 ± 0.8 |
| s8 | 23.44272 | +30.87069 | 14.59 | 0.23 | 0.18 | 0.95 | 3.18 | 6.94 | 25.5 | 5.24 | 28.7 ± 1.7 | 28.8 ± 1.0 |
| s9 | 23.44566 | +30.45644 | 13.18 | 0.62 | 0.29 | 0.99 | 2.75 | 6.19 | 29.8 | 21.65 | 26.3 ± 0.6 | 26.4 ± 0.3 |
| s10 | 23.49555 | +30.92542 | 16.95 | 0.19 | 0.14 | 0.71 | 2.32 | 12.55 | 18.3 | 5.44 | 28.2 ± 1.4 | 28.4 ± 0.9 |
| s11 | 23.51050 | +30.96968 | 19.65 | 0.21 | 0.19 | 1.16 | 2.85 | 5.45 | 32.5 | 2.36 | 28.6 ± 1.7 | 28.8 ± 1.0 |
| s12 | 23.66479 | +30.52090 | 21.20 | 0.35 | 0.16 | 2.59 | 9.37 | 21.35 | 47.7 | 1.09 | 29.0 ± 2.0 | 29.5 ± 1.4 |
| s13 | 23.70374 | +30.62468 | 20.33 | 0.14 | 0.08 | 0.18 | 0.86 | 3.19 | 10.9 | 0.43 | 31.9 ± 7.7 | ..... ... |
| s14 | 23.24606 | +30.69297 | 18.12 | 3.99 | 2.46 | 4.21 | 19.5 | 12.61 | 44.6 | 1.56 | 31.4 ± 6.2 | 30.0 ± 1.8 |
| s15 | 23.55395 | +30.45810 | 17.34 | 0.26 | 0.19 | 0.38 | 4.85 | 14.30 | 21.1 | 0.82 | 30.6 ± 4.3 | 30.4 ± 2.2 |
| s16 | 23.56527 | +30.46270 | 17.69 | 1.66 | 1.23 | 1.30 | 4.11 | 11.23 | 20.9 | 0.45 | 29.7 ± 2.7 | 29.5 ± 1.4 |
| s17 | 23.61698 | +30.93344 | 18.30 | 0.20 | 0.25 | 0.52 | 1.85 | 7.33 | 12.5 | 0.28 | 30.6 ± 4.3 | 31.5 ± 3.5 |
| s18 | 23.69661 | +30.63216 | 19.49 | 0.30 | 0.17 | 1.23 | 5.31 | 5.09 | 31.7 | 4.57 | 27.9 ± 1.2 | 28.1 ± 0.8 |
| s19 | 23.67558 | +30.40020 | 28.08 | 0.08 | 0.06 | 0.30 | 0.95 | 0.9 | (8.1) | 1.8 | 29.6 ± 2.6 | 29.4 ± 1.4 |
| s20 | 23.74792 | +30.61717 | 23.99 | 0.54 | 0.71 | 0.64 | 0.95 | ... | ... | 4.0 | 27.8 ± 1.2 | 27.7 ± 0.6 |
Notes. In Cols. 2–4 we also give the source right ascension, declination, and the galactocentric distance r.
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