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This article has an erratum: [https://doi.org/10.1051/0004-6361/202346801e]


Table A.4.

Northern galactic plane and equatorial sources, without spectroscopic redshift measurements, not selected in (or dropped from) z-GAL from the HerBS, HeLMS, and HerS catalogues.

Source name Herschel Coordinates Flux density
(J2000.0) Herschel SCUBA-2
Herschel Name Other S250 μm S350 μm S500 μm S850 μm
(mJy)
HerBS sources

H-ATLAS 141004.7+020306 HerBS-16 14:10:04.7 +02:03:06 119.4±7.3 151.0±8.4 176.0±8.7 86.0±4.7 Blazar
H-ATLAS 091809.5+001929 HerBS-99 09:18:09.5 +00:19:29 93.2±7.4 116.6±8.2 94.3±8.7 23.9±5.0
H-ATLAS 133108.4+303034 HerBS-112 13:31:08.4 +30:30:34 71.8±5.8 87.0±5.8 92.2±7.0 220.3±6.2 Blazar
H-ATLAS 113833.8−014655 HerBS-119 11:38:33.8 −01:46:55 68.5±7.2 85.6±8.1 91.2±8.6 12.5±5.5
H-ATLAS 142706.4+002258 HerBS-130 14.27:06.4 +00:22:58 119.4±7.3 118.7±8.1 88.8±8.6 15.5±5.1
H-ATLAS 134441.5+240345 HerBS-133 13:44:41.5 +24:03:45 85.4±5.5 98.5±6.1 88.1±7.3 17.4±5.9
H-ATLAS 134855.6+240745 HerBS-139 13:48:55.6 +24:07:45 76.9±5.9 82.9±5.9 87.4±6.8 15.2±6.0
H-ATLAS 091454.0−010358 HerBS-142 09:14:54.0 −01:03:58 69.0±7.3 72.2±8.1 87.2±8.5 22.4±5.7
H-ATLAS 133057.5+311734 HerBS-152 13:30:57.5 +31:17:34 47.7±5.6 53.4±6.0 85.8±6.9 14.1±5.0
H-ATLAS 132329.9+311528 HerBS-158 13:23:29.9 +31:15:28 64.7±5.4 75.7±6.2 85.1±7.2 24.4±4.1
H-ATLAS 122407.4−003247 HerBS-161 12:24:40.7 −00:32:47 56.5±7.3 75.7±8.1 82.4±8.8 9.8± 4.3
H-ATLAS 145754.2+000018 HerBS-195 14:57:54.2 +00:00:18 70.3±7.3 92.7±8.1 81.0±8.8 17.3±5.3
H-ATLAS 134403.1+242628 HerBS-196 13:44:03.1 +24:26:28 86.9±5.7 92.3±6.3 81.0±7.1 13.9±6.3
H-ATLAS 141827.4−001703 HerBS-203 14:18:27.4 −00:17:03 117.2±6.5 116.4±7.4 80.2±7.6 15.0±4.8

HeLMS and HerS sources

HERMES 003032.1−021153 HeLMS-33 00:30:32.1 −02:11:53 81±7 98±6 118±8 Blazar
HERMES 004532.6−000123 HeLMS-53 00:45:32.6 −00:01:23 48±7 85±6 103±8

Notes. The source names and Herschel flux densities are from Bakx et al. (2018) and Nayyeri et al. (2016). The SCUBA-2 flux densities of the HerBS sources are the revised values from Bakx et al. (2020c). The SCUBA-2 flux densities indicated in italics are classified as non-detections, as discussed in Sect. 3 of Bakx et al. (2018). The sources are listed in order of decreasing S500μ flux density. For the sources that are identified as blazars the reader is referred to Sect. 2.

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