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Table A.3

PACS upper limits for previously known CepOB2 members with disks.

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

01-1152 M1.5 0.9 –5.5/– 21531982+6234004 <0.019 <0.021 TD/D U
DG-481 A7.0 1.5 21522113+6245034 <0.003 <0.010 TD/Db N
73-311 M1.5 1.1 –29/– 21352451+5733011 <0.003 <0.030 D Y n(160 μm)
73-71 K6.0 2.1 –12/–10 21353021+5731164 <0.003 <0.052 D Y c
213542993+573337049 M4.0 1.1 –16/– 21354299+5733370 <0.006 <0.124 D U n
72-875 M0.5 2.0 –21/– 21354975+5724041 <0.048±0.007: <0.09 TD: 0.11 n, extended
73-194 K6.5 1.5 –4/– 21355223+5732145 <0.006 <0.25 N N n
73-537 G1.5 3.3 –5/– 21360723+5734324 <0.014 <0.030 N N
21360745.5734296 1.7 21360745+5734296 <0.010 <0.4 F n
21362368+5732452 1.6 –/– 21362368+5732452 <0.12 <0.68 Unc. U/N n
21362507.5727502 M0.0 1.7 –86/–78 21362507+5727502 <0.007 <0.05 F 0.09 n, 160 μm extended
14-306 K6.5 1.850 –8/– 21362676+5732374 <0.12 <0.68 N N n
213626897+573304351 M0.0 3.6 –21/– 21362690+5733043 <0.12 <0.68 Y: n
213636909+573132683 K7.0 3.3 –20/– 21363691+5731326 <0.24 <4.6 F Y n, truncated disk?
21364596.5729339 1.6 –47/– 21364596+5729339 <3.7 <3.7 ClassI Y n
21364762.5729540 K6.0 1.6 –76/– 21364762+5729540 <3.7 <3.671 F Y n
11-1209 K6 0.6 –4/–6 21365850+5723257 <0.006 <0.012 D 0.56
21365947.5731349 M1/0.0 1.6/2.0 –109/–30 21365947+5731349 <1.3 F Y n1
11-1871 M2.0 0.8 –13/– 21370254+5726144 <0.003 <0.015 TD/D:/N N: 8 μm excess only
14-287 M0.0 2.2 –35/–18 21370649+5732316 <0.018 F 0.21 n
213708879+572107012 M2.0 1.4 –55/– 21370888+5721070 <0.021 <0.12 TD/D: Y e
14-197 K5.5 1.6 –2/– 21372368+5731538 0.006±0.0012 0.030±0.0082 N N
213726148+572330562 M4.5 1.3 –28/– 21372615+5723305 <0.018 <0.076 TD Y: e
21372643+5731386 K2.0 2.4 –2/– 21372643+5731386 <0.039 <0.077 TD:/N U 8 μm excess only, nearby object
213727418+573123620 M2.5 0.9 –11/– 21372742+5731236 <0.015 <0.080 F U
213733557+573550931 M1.5 1.7 –6/– 21373355+5735509 <0.003 <0.009 D N:
11-1864 G-K 1.6 –5/– 21373420+5726154 <0.003 <0.015 TD:/N N
14-2148 M1.5 1.5 –2/– 21374184+5740400 <0.006 <0.030 TD:/D:/N: N 8 μm excess only
213742167+573431486 M2.0 1.4 –60/– 21374216+5734314 <0.015 <0.017 TD n
213744131+573331130 K7.5/M1 2.7/1.9 –17/–19/– 21374412+5733311 <0.043 <0.016 F Y
213744543+572200213 M5.0 1.1 –51/– 21374453+5722002 <0.015 <0.13 U Y: n, Spitzer data contaminated
213746871+573156208 M1.5 2.9 –42/– 21374687+5731562 <0.006 <0.021 PTD Y m
213748237+572319411 M3.5 0.7 –8/–42 21374824+5723194 <0.006 <0.055 TD Y m
213748931+572320963 K5.0 2.7 –20/– 21374893+5723209 <0.010 <0.07 F Y
13-924 K5.0 1.6 –4/– 21375018+5733404 <0.003 <0.012 N N e
12-2519 K5.5 1.6 –8/– 21375107+5727502 <0.006 <0.14 D 0.07 160 μm extended
213751210+572436151 K7.5 3.3 –15/– 21375121+5724361 <0.003 <0.018 F/D Y:
12-1968 K6.0 1.2 –11/–8 21375487+5726424 <0.003 <0.008 F 0.34
213756779+573448171 M1.5 1.7 –9/– 21375677+5734481 <0.003 <0.012 TD U
13-669 K1 2.183 –22/–18 21380928+5733262 <0.003 <0.024 F 0.58 n, Herschel flux too low
21380979+5729428 1.6 –/– 21380979+5729428 <0.005 <0.009 TD/D N:
213809997+572352782 M2.0 2.2 –50/– 21381000+5723527 <0.005 <0.057 F Y
213810182+572708407 M1.5 1.5 –10/– 21381018+5727084 <0.003 <0.19 PTD U Herschel flux too low
213812023+572500774 M1.0 1.4 –3/– 21381202+5725007 <0.004 <0.012 F N:
54-1781 M1.0 1.2 –13/– 21381612+5719357 <0.003 <0.018 TD 0.3
213819411+572203907 M2.0 2.7 –14/– 21381941+5722039 <0.012 <0.018 TD8 U 8 μm excess only
213823950+572736175 M1.0 1.4 –18/– 21382395+5727361 <0.004 <0.029 F Y:
213828028+574736432 M2.5 1.0 –4/– 21382803+5747364 out <0.042 D N: e
13-232 M0.0 1.1 –3/– 21382834+5731072 <0.003 <0.006 F: N
213829367+573726567 M2.0 2.0 –10/– 21382936+5737265 <0.003 <0.031 TD U lower than expected
213830349+572618227 K7.0 2.1 –13/– 21383035+5726182 <0.003 <0.006 F Y: m
21383216.5726359 M0.0 1.6 –129/–43 21383216+5726359 <0.003 <0.009 F Y m
13-52 K7.0 1.3 –1/– 21383255+5730161 <0.003 <0.009 TD N
13-566 K5.5 2.4 –5/– 21383481+5732500 <0.003 <0.038 TD8 N strong 8 μm excess only
213837298+573103776 K7.0 2.1 –4/– 21383730+5731037 <0.003 <0.009 TD N:
213839571+572916412 M1.5 4.7 –22/– 21383956+5729164 <0.003 <0.063 TD/D Y:
213839749+572753080 M2.5 1.6 –5/– 21383956+5729164 <0.003 <0.029 D N: n
13-1891 M0 1.0 –11/– 21384001+5739303 <0.003 <0.018 F Y:
213842249+573533902 M4.0 0.8 –1/– 21384224+5735339 <0.004 <0.021 F N: m
54-1613 K5.0 1.2 –1/– 21384332+5718359 <0.006 <0.064 TD N
213844343+573626211 M1.5 1.0 –34/– 21384434+5736262 <0.012 <0.061 D Y: anomalous SED
213847282+573114405 M1.0 1.6 –29/– 21384727+5731144 <0.003 <0.076 F Y
213854760+572450268 M1.0 1.1 –5/– 21385476+5724502 <0.006 <0.019 D U
21385669.5730484 K5.0 1.6 –4/– 21385669+5730484 <0.003 <0.04 F U
213859738+572216816 M2.5 2.2 –10/– 21385973+5722168 <0.012 <0.067 F U n
12-1027 M0 1.3 –11/– 21390319+5722318 <0.006 <0.014 N N:
213903212+571555316 M1.0 0.8 –6/– 21390320+5715553 <0.013 <0.032 TD U n
12-1617 M1.0 1.6 –30/–13 21390468+5725128 <0.006 <0.012 PTD 0.16 m
213905519+572349596 K7.0/6.0 1.2/1.521 –1/– 21390552+5723496 <0.053 <1.0 TD8 N: n, 8 μm excess only
21-840 M1.0 2.2 –14/– 21391012+5722323 <0.006 <0.038 F 0.06 m
213910429+572235727 M0.0 3.2 –103/– 21391042+5722357 <0.006 <0.044 F Y
213911452+572425205 M1.0 2.2 –26/– 21391145+5724252 <0.10 <1.0 F Y n
213914453+572304758 M3.5 1.4 –8/– 21391444+5723047 <0.013 <0.056 TD8 U 8 μm excess only
213914837+573756779 M0.0 3.3 –13/– 21391483+5737567 <0.003 <0.015 TD U
213914988+574050473 M4.0 3.1 –25/– 21391498+5740504 <0.012 <0.073 TD U
54-1488 K7.0/6.0 2.2 –13/–33/– 21391748+5717474 <0.021 <0.069 PTD Y: e
21392059+5726269 - 1.6 –34/– 21392059+5726269 <0.004 <0.052 TD Y: n
213924711+571912672 M2.5 2.8 –37/– 21392471+5719126 <0.006 <0.050 F Y:
21392570+5729455 1.670 –/– 21392570+5729455 <0.009 <0.050 TD N m,n
213926421+572538470 M1.0 3.2 –164/– 21392641+5725384 <0.004 <0.017 F Y
213929250+572530299 M1.0 3.7 –14/– 21392925+5725303 <0.006 <0.056 PTD U
213930129+572651433 M0.5 2.0 –4/– 21393012+5726514 <0.004 <0.028 D N:/U
213930870+572227446 K7.0 2.3 –108/– 21393086+5722274 <0.009 <0.015 F Y
21393301+5728175 M1.5 2.31 3/– 21393301+5728175 <0.003 <0.020 F/TD U lower than expected
21-33 M0 1.7 –107/–51 21393561+5718220 <0.005 <0.016 D 0.07 n(160 μm)
213937132+572459030 M3.0 1.0 –49/– 21393713+5724590 <0.005 <0.030 F Y m
21394010+5730113 M2.0 1.6 –24/– 21394010+5730113 <0.003 <0.012 TD/D Y:
213942289+572902679 M2.5 2.1 –12/– 21394229+5729026 <0.003 <0.018 D U
213942399+573431184 M3.5 2.0 –51/– 21394240+5734311 <0.003 <0.024 D Y:
213943237+574139252 M5.0 1.8 –2/– 21394324+5741392 <0.004 <0.009 F N:
213943450+573634560 M0.0 1.6 –5/– 21394345+5736345 <0.008 <0.018 F N: m
213944898+573537212 M4.0 0.8 –4/– 21394489+5735372 <0.003 <0.012 D N:
24-820 K6.5 1.2 –2/– 21394746+5735059 <0.003 <0.012 N N
213948050+572049544 K7.0 1.7 –1/– 21394805+5720495 <0.036 <0.054 F U nearby object
24-78 M2.0 1.3 –6/– 21394936+5730546 <0.003 <0.020 N N
213949540+574330324 M3.5 0.7 –18/– 21394954+5743303 <0.012 <0.088 F Y: e
92-1162 M2.0 1.4 –7/– 21394974+5746468 <0.009 <0.015 D:/N N weak IRAC excess only
213949767+574733740 M2.0 1.9 –10/– 21394977+5747337 <0.021 <0.036 TD U
213951092+574119848 M3.0 1.1 1/– 21395109+5741198 <0.003 <0.012 D N:
213952060+572506212 M2.5 2.3 –10/– 21395205+5725062 <0.003 <0.015 D U
213954003+573519730 M3.5 0.8 –2/– 21395400+5735197 <0.003 <0.015 TD N: n
21-1974 G7.5 2.5 –8/– 21395861+5728404 <0.004 <0.026 D Y:
213959078+572643784 M3.5 0.5 –10/– 21395908+5726437 <0.003 <0.009 F U
21-895 K5.0 1.4 –1/– 21400321+5722505 <0.015 <0.024 TD 0.21
24-1736 M1 1.0 –61/–33 21401134+5739518 <0.006 <0.018 F 0.3
KUN-196 B9 2.2 21401508+5740513 <0.008 <0.046 TD/Db N n
214019073+572509288 M2.5 2.0 –12/– 21401907+5725092 <0.006 <0.027 F U
214019849+573922857 M3.5 1.3 –47/– 21401984+5739228 <0.003 <0.015 F Y
22-2651 M1.5 0.9 –34/–48 21402130+5726579 <0.004 <0.015 F 0.05 lower than expected
22-1418 M1.5 0.7 –2/– 21402287+5727329 <0.003 <0.012 D <0.3
214026262+573402317 M4.5 1.1 –4/– 21402625+5734023 <0.005 <0.05 D N:
214029551+572453893 M4.0 1.0 –18/– 21402955+5724538 <0.009 <0.021 TD U
214033472+573605378 M1.0 2.2 –16/– 21403347+5736053 <0.005 <0.031 F Y: n
23-570 K6.0 1.3 –47/–18 21403574+5734550 <0.006 <0.053 D 0.7
93-540 M0.0 2.2 –18/–5 21403586+5758130 <0.021 <0.077 - Y m
21403721.5729127 K7.5/M2 1.7/1.3 –41/–42/–21 21403721+5729127 <0.003 <0.012 F Y
214042281+573513316 M4.0 1.4 –20/– 21404228+5735133 <0.006 <0.018 F U
214048489+573202607 M4.5 1.0 –4/– 21404848+5732026 <0.004 <0.012 TD: N: 8 μm excess only
23-798 K6 2.2 –150/–70 21412864+5736432 <0.005 <0.025 PTD Y n, lower than expected

Notes. The comments include “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). Spectral types, extinction and Hα EW from Sicilia-Aguilar et al. (2005, 2013a,b). Many of the objects in the IC 1396A globule appear without photometric data in the red since the upper limits that can be constrained are of a few Jy and thus not informative. The disk type is labelled as N (no disk), F (full disk), TD (transition disk), TD8 (transition disk with an excess at 8 μm only, usually too faint to be detected at 24 μm), PTD (pre-transitional disk), D (depleted disk), U (uncertain, usually due to photometric errors/contamination), – (not enough information). 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 [-], added [:] indicates a border-line case) 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. 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).

(1)

The object is clearly seen in the blue although due to the surrounding nebular emission, the photometry is very uncertain.

(2)

There is a clear point-source detection, but given the small offset with respect to the optical counterparts and the lack of Spitzer excess, it may correspond to a background source.

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