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Table 1.

Measured He II line properties (rest frame) and derived physical properties of Bright sources in CDFS and UDS fields.

ID RA Dec Flux FWHM EW zsys log10(M) log10(SFR)
(×10−18 erg s−1 cm−2) (km s−1) (Å) (M) (M yr−1)
Narrow

CDFS009705 03:32:20.9 −27:49:16.1 2.2 ± 0.5 510 ± 130 1.3 ± 0.4 2.484 8.9 1.2
CDFS015347 03:32:13.2 −27:46:42.6 1.3 ± 0.7 240 ± 145 1.9 ± 1.3 3.514 9.4 1.1
CDFS019872 03:32:47.9 −27:44:29.4 1.1 ± 0.4 280 ± 110 1.8 ± 0.9 3.453 9.3 1.0
CDFS023170 03:32:37.8 −27:42:32.5 2.8 ± 1.5 455 ± 110 1.1 ± 0.6 2.977 9.7 2.0
CDFS023215 03:32:40.7 −27:42:34.7 4.3 ± 0.2 330 ± 110 4.1 ± 2.6 3.471 9.6 1.3
CDFS023527 03:32:18.8 −27:42:48.1 1.5 ± 0.9 260 ± 55 0.9 ± 0.4 3.108 9.4 1.7
CDFS113062 03:32:02.6 −27:52:23.7 4.0 ± 2.0 640 ± 275 1.4 ± 0.7 2.695 9.4 1.7
CDFS122687 03:33:00.1 −27:47:32.6 2.9 ± 0.8 495 ± 150 1.0 ± 0.4 2.643 9.7 2.0
CDFS126819 03:31:55.7 −27:45:33.1 9.5 ± 3.0 860 ± 110 8.0 ± 2.0 2.818 9.7 2.0
CDFS202040 03:32:02.5 −27:58:15.7 2.6 ± 0.7 620 ± 180 3.7 ± 1.9 3.474 9.1 1.1
CDFS229681 03:31:59.4 −27:45:46.5 1.2 ± 0.9 520 ± 280 1.9 ± 1.5 3.331 8.8 1.1
UDS004017 02:17:37.0 −05:15:15.4 1.7 ± 0.5 260 ± 75 1.4 ± 0.6 2.389 10.0 1.6
UDS013586 02:17:52.5 −05:12:04.8 3.1 ± 1.9 335 ± 100 0.6 ± 0.4 2.581 9.9 2.2
UDS019505 02:17:45.9 −05:10:09.1 2.1 ± 1.5 530 ± 275 0.7 ± 0.5 2.865 9.6 1.4
UDS020089 02:17:22.7 −05:09:54.1 2.1 ± 0.7 310 ± 110 2.6 ± 1.4 3.218 9.4 0.9
UDS021062 02:16:58.1 −05:09:35.4 1.2 ± 0.4 365 ± 145 1.1 ± 0.5 2.537 9.6 1.8
UDS196554 02:17:40.8 −05:05:56.3 3.5 ± 1.3 600 ± 255 2.4 ± 1.3 2.618 10.0 2.3
UDS200677 02:18:14.1 −05:04:49.2 4.7 ± 1.0 600 ± 130 2.4 ± 0.7 3.587 9.8 2.1
UDS281893 02:17:11.3 −05:22:17.6 2.9 ± 1.4 660 ± 220 1.1 ± 0.6 2.697 9.1 1.4
UDS292392 02:18:18.4 −05:20:41.4 3.6 ± 1.1 310 ± 110 5.5 ± 4.0 4.555 8.9 1.2

Broad

CDFS021470 03:32:21.9 −27:43:38.8 3.9 ± 0.9 1800 ± 500 2.6 ± 0.8 2.574 9.1 1.3
CDFS102149 03:31:59.7 −27:58:02.6 2.0 ± 0.7 1130 ± 480 2.0 ± 0.9 2.614 9.9 2.0
CDFS129134 03:31:59.0 −27:44:23.5 11.2 ± 1.6 2120 ± 970 3.8 ± 0.9 3.202 9.6 1.8
CDFS141081 03:33:10.1 −27:40:48.2 4.3 ± 0.9 1425 ± 385 3.5 ± 1.2 2.385 9.9 1.4
CDFS231194 03:33:02.6 −27:45:01.8 12.5 ± 2.0 1300 ± 530 2.2 ± 0.6 3.077 9.5 1.8
UDS137388 02:17:12.2 −05:22:31.5 23.1 ± 10.5 1420 ± 500 4.6 ± 3.5 2.598 9.6 1.9

AGN

CDFS006327* 03:32:42.8 −27:51:02.6 1.3 ± 0.3 440 ± 100 5.2 ± 2.8 3.493 8.8 1.1
CDFS028933* 03:32:07.1 −27:50:55.5 1.3 ± 0.3 440 ± 110 4.7 ± 2.1 3.787 8.8 1.0
CDFS208098* 03:32:52.3 −27:55:26.3 6.6 ± 1.6 1885 ± 530 3.5 ± 1.4 2.478 9.0 1.3
UDS020721x 02:17:38.1 −05:09:47.1 12.9 ± 2.1 840 ± 165 7.5 ± 2.8 2.520 10.7 2.1
UDS021234* 02:17:41.0 −05:09:31.3 1.8 ± 0.4 385 ± 145 3.7 ± 2.2 4.600 9.7 0.7
UDS025482*, x 02:17:03.4 −05:08:04.7 4.1 ± 0.7 710 ± 145 4.3 ± 1.8 3.523 10.3 0.9
UDS145830* 02:18:13.6 −05:20:11.4 8.6 ± 0.9 530 ± 75 21.4 ± 10.6 3.210 10.7 1.0

Notes. Based on the width of the He II line, the sources are grouped as Narrow and Broad, with the distinction at FWHM(He II) = 1000 km s−1.

Possible AGNs have been indicated using an asterisk for those sources with strong C IV emission in their spectra, and an “x” for sources with X-ray detections. Sources with ID > 100 000 have ground-based photometry only. The RA and Dec are in J2000 epoch.

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