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Table 5

Star formation or AGN?

Method Method
B2/3C Balmer Diagn. FIR/MIR P.L. Overall B2/3C Balmer Diagn. FIR/MIR P.L. Overall
1 2 3 4 5 6 7 8 9 10 11 12

0648+27d SF AGN SF 1621+38 AGN AGN
0755+37c SF SF 1626+39c No SF SF SF SF
0836+29 SF SF 1652+39d No AGN
0913+38 Mix Mix 1658+30Ac SF SF SF
1003+26 SF SF 192d ? AGN AGNa SF AGN
1005+28 SF SF 219d ? AGN AGN AGN AGN
1037+30d SF SF SF 223d No AGN SF Mix
1141+37 SF SF 234d No AGN AGN Mix AGN
1144+35d ? AGN AGN 264 ? SF Mix Mix
1204+34d ? AGN SF Mix 272.1 No SF Mix Mix
1217+29c No SF Mix SF Mix 274c ? SF SF SF
1254+27 ? ? 285d SFb AGN Mixa SF SF
1339+26 ? ? 296 No SF Mix Mix
1346+26c SF SF SF 303d No AGN Mix Mix
1350+31c SFb SF SFa SF 305d SFb AGN SF Mix
1430+25 SF SF SF SF 321c SFb Mixa Mix
1613+27 SF SF SF 326c ? Mix SF SF
1615+32d No AGN Mix AGN AGN 346d AGN AGN AGN

Notes. All other data refer to 24 and 70 μm.

(a)

Mid/far-IR data from Dicken et al. (2010), at 25 and 60 μm.

(b)

Tadhunter et al. (2011).

(c)

LEG.

(d)

HEG.

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