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Table A.3

Spitzer IRAC and MIPS data for confirmed members and probable members.

Spect. ID IRAC-1 (μJy) IRAC-2 (μJy) IRAC-3 (μJy) IRAC-4 (μJy) MIPS-1 (μJy) SED Comments

213542993+573337049 2683 ± 72 1982 ± 57 1808 ± 222 1211 ± 86 881 ± 157 Dep.
213607980+572637096 19 571 ± 94 39 189 ± 78 103 489 ± 512 1 159 200 ± 6406 ClassI
213618699+573626870 1251 ± 53 835 ± 53 708 ± 197 146 ± 43 ND
213619969+573527805 522 ± 3 343 ± 3 257 ± 15 163 ± 48 ND
213622159+572327898 2220 ± 53 1434 ± 58 1244 ± 273 Neb. contamination
213622379+573141225 1669 ± 43 1066 ± 55 1305 ± 196 1984 ± 230 ND
213625078+572750265 3060 ± 58 3013 ± 61 3021 ± 224 4872 ± 26 9196 ± 103 Full
213626897+573304351 1392 ± 54 750 ± 54 ND Neb.
213633647+573517477 10 624 ± 79 6568 ± 51 4339 ± 221 2982 ± 72 1800 ± 310 TD/Dep. Var.?
213636909+573132683 10 712 ± 33 10 062 ± 77 10 814 ± 257 15 797 ± 95 13 900 ± 3802 Full
213639147+572953326 156 347 ± 511 155 812 ± 641 150 577 ± 2912 Full
213641152+573702713 1045 ± 50 717 ± 54 488 ± 220 235 ± 36 ND
213641358+572204113 876 ± 41 589 ± 53 272 ± 178 ND
213642470+572523186 1513 ± 56 1220 ± 55 1093 ± 201 1046 ± 86 1525 ± 100 Full
213648190+573402084 1203 ± 32 686 ± 42 314 ± 155 1809 ± 67 ND
213653210+572052112 732 ± 50 395 ± 52 673 ± 208 ND: 24 μm marginal
213655201+573030103 38 820 ± 158 41 537 ± 165 41 378 ± 345 43 405 ± 11034 ClassI
213655283+572551668 3304 ± 56 1803 ± 43 1195 ± 252 1045 ± 53 2166 ± 101 TD
213658737+573848181 2764 ± 60 2294 ± 54 2463 ± 205 1866 ± 86 16 507 ± 456 PTD
213659108+573905636 6278 ± 62 6339 ± 53 7337 ± 209 10 397 ± 91 47 929 ± 108 Full
213659472+573134908 5918 ± 18 5496 ± 50 5118 ± 213 8387 ± 48 Full
213701319+573418289 1616 ± 53 1282 ± 54 1091 ± 210 887 ± 79 6561 ± 106 TD
213701401+572445873 5219 ± 61 3358 ± 61 3050 ± 272 1278 ± 73 ND: 24 μm marginal

Notes. The full table is available at the CDS. Under “SED” we specify the SED type (ND = no disk; ClassI= Class I object; Full= typical full disk; TD = transition disk; PTD = pre-transition disk; Dep. = dust-depleted disk; Unc. = Uncertain SED type). Objects listed as “marginal detection” at 24 μm have probably excesses but their photometry is compromised by low S/N or different sources of contamination.

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