Millimeter imaging of submillimeter galaxies in the COSMOS field: redshift distribution

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Table 8

Summary of P-statistic results compared to intermediate resolution mm-mapping.

Sample	Radio fraction		24 μm		m_{3.6 μm} − m_{4.5 μm} ≥ 0		Combined
	P-statistic^*	correct ID	P-statistic^*	correct ID	P-statistic^*	correct ID	P-statistic^*	correct ID


1.1 mm-selected^a	8/15 (53.3%)	7/10 (70%)	5/15 (33.3%)	5/6 (83.3%)	5/15 (33.3%)	5/6 (83.3%)	8/15 (53.3%)	7/10 (70%)
870 μm-selected^b	11/26 (42.3%)	7/12 (58.3%)	6/26 (23.1%)	4/6 (66.7%)	10/26 (38.5%)	7/11 (63.6%)	17/26 (65.4%)	12/18 (66.7%)

Notes.

^(*)

Only robust (P_c ≤ 0.05) counterparts are considered here.

^(a)

Out of 15 bolometer SMGs, 2 robust statistical counterparts are found for each of sources AzTEC-5 and AzTEC-8 (see Table 7).

^(b)

Out of 26 bolometer SMGs, 2 robust statistical counterparts are found for each of sources COSLA-73 and COSLA-161 (see Table 6).

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