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Table 2.

Counts per squared degree for objects detected in at least four bands.

z Total Spiral SB SF-AGN SB-AGN AGN1 AGN2 Elliptical Irregular HIEROs
2 ≤ z < 3 73 906 508 4612 784 3498 1267 480 598 62 159 152
(17.08%) (9.47%) (18.32%) (6.08%) (20.19%) (5.22%) (18.22%) (22.92%) (17.13%) (27.17%)
3 ≤ z < 4 30 205 111 2447 205 2195 568 165 10 24 504 1107
(17.38%) (11.1%) (14.97%) (7.05%) (18.11%) (6.0%) (10.94%) (67.0%) (17.87%) (7.81%)
4 ≤ z < 5 14 027 62 1179 125 1092 258 57 0 11 253 1979
(19.31%) (7.54%) (12.41%) (5.9%) (17.03%) (8.89%) (9.88%) (100%) (20.61%) (4.55%)
5 ≤ z < 6 6554 34 595 78 526 120 20 0 5182 1443
(22.45%) (6.36%) (12.66%) (6.66%) (16.26%) (10.72%) (9.46%) (0%) (24.54%) (3.57%)
6 ≤ z < 7 3144 18 311 49 255 60 7 0 2444 801
(21.49%) (7.55%) (13.79%) (5.92%) (10.58%) (10.7%) (10.48%) (0%) (23.91%) (3.94%)
7 ≤ z < 8 1540 11 175 31 125 30 3 0 1166 356
(25.85%) (10.13%) (16.18%) (8.7%) (19.66%) (9.79%) (16.67%) (0%) (28.5%) (17.88%)

Notes. Counts per squared degree for different redshift intervals and spectral types for objects detected at least in four bands. In parentheses we indicate the percentage of objects lost during data cleaning, which does not show a strong dependence on redshift. We lose 100% of elliptical galaxies at 4 ≤ z < 5, but the starting catalogue contained only eight of them in this redshift range. We also present the counts for HIEROs, which are also only marginally affected by our data cleaning process.

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