The LOFAR Two-metre Sky Survey Deep Fields - The star-formation rate–radio luminosity relation at low frequencies

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Table 2

Percentage of sources in our parent sample with measured photometry (middle column) and a ≥ 3σ detection in at least N bands.

Number of bands	% with photometry	% ≥ 3σ
7	100	100
8	100	99
9	100	98
10	100	96
11	100	94
12	99	92
13	98	89
14	98	86
15	98	77
16	98	62
17	98	44
18	84	28
19	72	16
20	67	8
21	61	4
22	61	2
23	61	1
24	25	0
25	21	0

Notes. For example, 98% of our sample has measured photometry in 17 or more bands, and more than half have ≥ 3σ detections in at least 16 bands.

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Number of bands	% with photometry	% ≥ 3σ
7	100	100
8	100	99
9	100	98
10	100	96
11	100	94
12	99	92
13	98	89
14	98	86
15	98	77
16	98	62
17	98	44
18	84	28
19	72	16
20	67	8
21	61	4
22	61	2
23	61	1
24	25	0
25	21	0

Number of bands	% with photometry	% ≥ 3σ
7	100	100
8	100	99
9	100	98
10	100	96
11	100	94
12	99	92
13	98	89
14	98	86
15	98	77
16	98	62
17	98	44
18	84	28
19	72	16
20	67	8
21	61	4
22	61	2
23	61	1
24	25	0
25	21	0

Number of bands	% with photometry	% ≥ 3σ
7	100	100
8	100	99
9	100	98
10	100	96
11	100	94
12	99	92
13	98	89
14	98	86
15	98	77
16	98	62
17	98	44
18	84	28
19	72	16
20	67	8
21	61	4
22	61	2
23	61	1
24	25	0
25	21	0