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Table A.1

PACS photometry of previously known CepOB2 members identified by optical spectroscopy.

ID Sp.T. A V HαEW 2MASS ID F 70 μm F 160 μm Disk Accretion Comments
(mag) (Å) (Jy) (Jy) (10-8M/yr)

01-580 K4.5 1.6 –96/– 21533707+6228469 0.010±0.002 <0.005 F 4
73-758 K6.5 1.9 –9/– 21350835+5736028 0.008±0.002 <0.012 TD N:/U
72-1427 M1.0 1.4 –77/–16 21351627+5728222 0.027±0.004 0.067±0.017 TD 0.15 n
73-472 K5.0 1.7 –10/–23 21351861+5734092 0.084±0.012 0.078±0.016 TD Y
MVA-1312 B4 1.5 21355654+5720529 0.044±0.008 <0.4 TD/Db N n(160 μm)
213639147+572953326 G9.0 5.3 –3/– 21363915+5729533 0.362±0.056 <0.6 F Y: near IC 1396A
213642470+572523186 M3.5 1.4 –27/– 21364247+5725231 0.037±0.007 <0.03 F Y: n
213655201+573030103 1.6 –45/– 21365520+5730301 0.178±0.036 <8 Class I Y
213655283+572551668 K2.5 2.6 1/– 21365527+5725516 0.028±0.004 0.031±0.009: TD N:/U
11-2146 K6.0 2.6 –33/–28 21365767+5727331 0.064±0.010 0.075±0.019 F 0.99
213701319+573418289 M1/M3 1.4 –2/–22/– 21365947+5731349 0.007±0.002 TD U n
11-2322 M1.0 0.9 –23/–18 21370191+5728222 0.010±0.002 F 1.6
11-2037 K4.5 1.6 –50/–43 21370703+5727007 0.019±0.003 0.031±0.009 F <9
213708137+573616213 M4.0 1.7 –45/– 21370814+5736162 0.020±0.004 <0.025 F Y e
21370936.5729483 M0.5 1.7 –21/– 21370936+5729483 0.036±0.006 F Y
14-125 K5.0 1.7 –13/–14 21371054+5731124 0.023±0.004 F 0.34 near IC 1396A
11-2131 K6.5 2.3 –10/– 21371215+5727262 0.019±0.003 0.044±0.010 F 0.25
11-2397 K7.0 1.2 –81/– 21371450+5728409 0.026±0.004 0.030±0.009 F Y
11-2031 K2 1.7 –5/–5 21371591+5726591 0.017±0.003 0.027±0.011 F <1
213716349+572640200 K7.0 6.0 –17/– 21371635+5726402 0.075±0.011 0.065±0.014 F Y
213724102+572411541 K5.5 2.4 –107/– 21372410+5724115 0.015±0.003 <0.023 F/PTD Y
21372447+5731359 M1.0 3.1 –62/– 21372447+5731359 0.009±0.002 <0.08 F Y
14-160 K5.0 1.8 –22/– 21372732+5731295 0.039±0.006 0.080±0.017 F Y n(160 μm)
14-1017 M0 2.1 –55/– 21372894+5736042 0.015±0.002 0.052±0.013 F <1.5 n(160 μm)
14-335 K6.5 1.5 –20/– 21372915+5732534 0.020±0.003 <0.012 F <0.14
213732341+572503204 G9.0 1.8 –47/– 21373234+5725032 0.015±0.003 <0.009 F Y
213734113+573431198 M0.0 2.1 –56/– 21373411+5734311 0.011±0.002 <0.016 F Y
213735713+573258349 M2.0 1.5 –62/– 21373571+5732583 0.008±0.001 <0.015±0.004 TD Y
14-183 K7/K5 2.0 –65/–14 21373849+5731408 0.064±0.009 0.052±0.012 PTD 0.16
213738830+572936901 K3.5 5.1 –7/– 21373883+5729369 0.050±0.007 0.035±0.007 F Y:
213740471+573433203 M2.5 2.0 –7/– 21374047+5734332 0.022±0.003 <0.015 TD U n
CCDM J2137+5734w/e B3/B5 1.6 21374093+5733372 0.012±0.002 <0.018 TD/Db N
21374275.5733250 F9.0 1.7 –54/–32 21374275+5733250 0.042±0.006 <0.017 F Y
213747963+573242323 M1.0 1.4 –61/– 21374795+5732423 0.026±0.004 0.036±0.008 PTD Y n(160 μm)
12-1091 G2.5 2.8 –17/–2 21375762+5722476 0.017±0.004 0.058±0.009 F <0.4 n(160 μm)
13-1238 M1.0 2.6 –64/–31 21375926+5736162 0.024±0.004 <0.018 F 0.6
82-272 G9.0 3.6 –13/–15 21380350+5741349 0.044±0.007 0.058±0.013 F <0.9
13-1426 M0 3.2 –109/–40 21380856+5737076 0.008±0.001 <0.0012 F 0.6
21380924+5720198 1.7 –/–17 21380924+5720198 0.013±0.003 0.022±0.005 F/D Y
13-350 M1 0.7 –9/– 21381384+5731414 0.004±0.001 <0.012 TD N
MVA-426 B7 1.4 21380845+5726476 0.480±0.070 0.194±0.039 F Y
213812641+572033696 K7.0 2.3 –159/– 21381264+5720336 0.010±0.003 <0.009 PTD Y
13-1877 K7.0 1.9 –68/–33 21381703+5739265 0.027±0.004 0.023±0.006 F 1.6
13-277 G8 2.0 –10/–14 21381731+5731220 1.187±0.172 0.983±0.194 F 14
213822810+574017294 M0.0 2.5 –18/– 21382281+5740172 0.012±0.002 0.023±0.008: F Y: n(160 μm)
213825831+574207487 K2.0 4.6 –2/– 21382583+5742074 0.021±0.003 0.014±0.005: TD U
13-236 K2 1.8 –47/–56 21382742+5731081 0.010±0.002 <0.008 F 0.51
12-2113 K6.0 2.5 –28/–15 21382743+5727207 0.044±0.006 0.057±0.012 F 1.4±0.2
13-157 K5.5 1.2 –14/–20 21382804+5730464 0.007±0.001 <0.007 F 4.2
213830308+573255218 M1.0 1.7 –31/– 21383031+5732552 0.013±0.002 <0.013 TD Y
91-155 M2.5 1.2 –8/– 21383470+5741274 0.024±0.004 0.016±0.006 F U nearby star
21384350.5727270 M2.0 1.7 –23/– 21384350+5727270 0.004±0.001 <0.012 TD N:/U n
54-1547 K5.5 1.1 –34/–33 21384446+5718091 0.031±0.006 0.068±0.011 PTD 0.18
91-506 K6.5 1.4 –47/–31 21385807+5743343 0.055±0.008 0.080±0.016 PTD 0.09
13-1048 M0.0 1.7 –7/–8 21391088+5735181 0.015±0.002 <0.016 F <0.3
13-1250 K4.5 1.4 –2/–4 21391213+5736164 0.016±0.002 <0.019 PTD 0.33
21392541+5733202 1.7 21392541+5733202 0.011±0.002 <0.06 PTD Y
21393104+5747140 1.7 –/–16 21393104+5747140 0.053±0.011 0.034±0.006 F Y
213933219+573300533 M3.5 2.0 –35/– 21393321+5733005 0.009±0.002 <0.017 TD Y n
24-515 M0.5 1.1 –11/– 21393407+5733316 0.009±0.002 <0.03 TD 0.10
21-998 K5.5 1.9 –16/– 21393480+5723277 0.024±0.005 0.017±0.004 F 0.33
92-393 M2.0 1.9 –34/–21 21394408+5742159 0.023±0.005 <0.008 TD Y
21-1536 M0.0 1.8 –26/– 21394570+5726242 0.016±0.003 0.023±0.007 PTD 0.18 n(160 μm)
213945860+573051704 K6.0 2.0 –227/– 21394586+5730517 0.013±0.002 0.016±0.005 F Y n(160 μm)
213954058+572933454 K7.5 2.0 –30/– 21395406+5729334 0.016±0.002 <0.012 PTD Y
213955699+571638273 M0.5 1.4 –31/– 21395569+5716382 0.023±0.006 0.031±0.008 TD Y
21395813+5728335 1.7 –/–15 21395813+5728335 0.017±0.003 0.026±0.006:1 F Y
21400451.5728363 K5.0 1.7 –32/– 21400451+5728363 0.026±0.004 0.026±0.006 F 0.71
93-720 1.7 –/–16 21400999+5800036 0.027±0.006 <0.033/0.048±0.008 F Y
24-1796 K7.0 1.2 –124/–73 21401182+5740121 0.027±0.005 0.029±0.006 TD 0.6 n(160 μm)
21-2006 K5.0 1.5 –2/– 21401390+5728481 0.005±0.001 <0.009 F 0.12
21401438+5740507 1.7 –/–46 21401438+5740507 0.012±0.002 <0.05 F Y n
214025369+573416284 M2.0 1.4 –72/– 21402536+5734162 0.007±0.002 <0.05 PTD Y n
23-405 K5.0 1.1 –14/–9 21403134+5733417 0.026±0.004 0.033±0.008 F 0.22
214035490+572831395 K3.0 1.7 –2/– 21403549+5728314 0.016±0.003 <0.012 TD U/Y:
23-162 K7.0 1.7 –6/– 21404450+5731314 0.009±0.002 <0.009 F Y
23-969 K5.5 1.1 –36/–26 21411497+5738149 0.021±0.005 0.021±0.006 F Y

Notes. The disk type is labelled as N (no disk), F (full disk), TD (transition disk), PTD (pre-transitional disk), D (depleted disk), Db (debris disk), – (not enough information). Spectral types, extinction and Hα EW from Sicilia-Aguilar et al. (2005, 2013a,b). Information on massive stars from Contreras et al.(2002). Marginal detections (detected objects for which visual inspection suggests there could be some problems) are marked as to distinguish from non-detections. The comments include “n” (nebular contamination in the region, although unless stated, the object is detected), “e” (near edge, the data are fine but the S/N is poorer than at the map centre). The “Accretion” column lists either the value of the accretion derived from U band photometry (Sicilia-Aguilar et al. 2005, 2010), or the presence (yes [Y], no [N], uncertain [U], not measured [–]) of accretion as revealed by optical spectroscopy (Sicilia-Aguilar et al. 2005, 2006b). Only high-resolution spectroscopy produces conclusive values in case of border-line objects with weak Hα EW, which are otherwise labelled as “uncertain”. The detectability limit for objects considered as non-accreting is 10-11M/yr. Note that all objects with accretion upper limits are confirmed to be accreting (via Hα spectroscopy).

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The 160 μm point may be a background object.

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