Table A.2
PACS photometry of CepOB2 members identified by Spitzer/X-ray/Hα photometry.
| 2MASS ID | Sp.T. | F70 μm (Jy) | F160 μm (Jy) | Ref. | Disk | Comments |
|
|
||||||
| 21351021+5731475 | – | ≤0.010±0.002 | <0.027 | B11 | – | No IRAC data |
| 21351687+5732422 | late K/M | 0.009±0.002 | <0.045 | B11 | – | |
| 21352723+5731301 | K/M | 0.016±0.003 | <0.036 | B11 | – | |
| 21353135+5731279 | early M | ≤0.010±0.002 | <0.015 | B11 | TD | |
| 21354586+5736401 | late K/M | ≤0.009±0.002 | <0.015 | B11 | F | |
| 21363802+5726579 | late M | ≤0.011±0.003 | <0.052 | MC09 | F | High extinction |
| 21364964+5722270 | F/G | 0.033±0.007 | 0.039±0.010 | G12 | TD | |
| 21370909+5725485 | late K/M | 0.023±0.004 | 0.054±0.012 | B11 | TD | n |
| 21371389+5727270 | late K | 0.040±0.006 | 0.037±0.009: | B11 | F | |
| 21371420+5736177 | K/M | 0.013±0.002 | <0.048 | G12 | F | |
| 21371545+5727170 | K/M | 0.025±0.004 | 0.049±0.012 | G12 | F/PTD | n |
| 21372152+5726123 | late K/M | 0.015±0.003 | <0.047 | G12 | F | |
| 21372475+5729089 | early M | ≤0.007±0.002 | <0.022 | B11 | F | n |
| 21373786+5728467 | mid K | 0.009±0.001:1 | <0.019 | G12 | N:1 | n |
| 21373885+5732494 | late K | 0.008±0.002:1 | <0.021 | G21 | N:1 | n |
| 21374292+5736314 | G/F | 0.405±0.059 | 0.338±0.067 | G12 | TD | |
| 21374612+5734280 | early/mid M | ≤0.005±0.001 | <0.012 | B11 | F | |
| 21385760+5729205 | O6.5 | 0.013±0.002 | <0.09 | M09 | N | HD 206267 |
| 21385963+5730080 | late K | 0.006±0.001: | <0.018 | M09 | F | |
| 21390321+5730420 | late K/M | 0.004±0.001: | <0.12 | B11 | F | No optical counterpart |
Notes. All spectral types (except the one from HD 206267) are derived from SED fitting and thus subject to large uncertainties, assuming the extinction will be within the usual cluster values AV = 1−3 mag. References: M09 (Mercer et al. 2009); MC09 (Morales-Calderón et al. 2009); B11 (Barentsen et al. 2011); G12 (Getman et al. 2012). The disk type is labelled as N (no disk), F (full disk), TD (transition disk), PTD (pre-transitional disk), D (depleted disk), – (not enough information). The comments include “m” (marginal detection, marked as ≤to distinguish from non-detection), “n” (nebular contamination in the region resulting in very high upper limits), “e” (near edge, the data are fine but the S/N is poorer than at the map centre).
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