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Table B.1.

Radio quasars from the literature within the RACS+DES and RACS+Pan-STARRS area with magz < 21.3 and S888MHz > 1 mJy.

Name R.A. Dec. z S888MHz magz Comments Ref.
(deg) (deg) mJy beam−1 (mag AB)
RACS J0001−03 0.448498 −3.879857 5.27 1.2±0.4 20.80±0.04 not detected in RACS [1]
RACS J0131−03 22.863917 −3.350053 5.18 23.2±2.5 18.12±0.01 [2]
RACS J0141−54 25.385002 −54.463861 5.00 167.4±14.4 21.20±0.04 [3]
RACS J0309+27 47.447667 27.299333 6.10 32.5±3.3 21.18±0.30 [4]
RACS J0341−00 55.424417 −0.803539 5.68 3.0±0.2 20.35±0.05 not detected in RACS [5]
RACS J0741+25 115.477980 25.34156 5.19 2.1±1.4 18.39±0.01 Sint/Speak > 1.5 [6]
RACS J0836+00 129.182750 0.914790 5.82 2.6±1.2 18.82±0.02 Opt.–Radio distance > 3″ [7]
RACS J0901+16 135.386042 16.251897 5.63 5.6±1.3 20.60±0.04 [5]
RACS J1013+35 153.407793 35.3138347 5.03 1.2±0.2 20.30±0.03 Opt.-Radio distance > 3″ [8]
RACS J1026+25 156.598453 25.716513 5.25 290.4±24.3 19.97±0.05 [9]
RACS J1034+20 158.577705 20.550059 5.01 4.3±1.0 19.86±0.02 [6]
RACS J1111+05 167.798840 5.607160 5.24 7.10±1.3 20.70±0.04 mag_z_psf – mag_z_kron > 0.07 [1]
RACS J1146+40 176.740840 40.619110 5.01 10.0±1.4 19.41±0.03 [10]
RACS J1427+33 216.910792 33.211667 6.12 2.7±0.3 21.00±0.10* not detected in optical [11]
RACS J1621+11 245.369399 11.557065 5.05 1.6±0.5 20.90±0.16 not detected in RACS [1]
RACS J1629+10 247.488671 10.006531 5.00 67.3±6.1 20.47±0.05 [12]
RACS J1702+13 255.688789 13.017273 5.47 12.0±1.7 20.60±0.06 mag_i_psf – mag_i_kron > 0.1 [13]
RACS J2201+23 330.281708 23.643875 5.83 2.1±0.8 20.42±0.04 err_mag_Y > 0.4 [8]
RACS J2329−15 352.403400 −15.337300 5.84 23.9±2.8 21.08±0.01 [14]
RACS J2329+30 352.413750 30.064106 5.24 4.67±0.7 19.17±0.02 [2]
RACS J2329−20 352.469917 −20.010886 5.04 3.88±1.0 18.47±0.01 [15, 16]
RACS J2344+16 356.139583 16.887911 5.00 12.8±1.8 18.74±0.01 [2]

Notes. Col. (1, 2, 3): name and coordinates of the source; Col. (4): redshift; Col. (5): peak flux densities at 888 MHz from the RACS-low source lists; Col. (6):z-band magnitude from DES or Pan-STARRS. The * indicates sources for which the magnitude was computed from other filters available in the literature; Col. (7): reason why the specific quasar was not recovered in our selection; Col. (8): reference for the discovery of the source: [1] Yang et al. (2023), [2] Wang et al. (2016), [3] Belladitta et al. (2019), [4] Belladitta et al. (2020), [5] Bañados et al. (2015), [6] McGreer et al. (2009), [7] Fan et al. (2001), [8] Gloudemans et al. (2022), [9] Sbarrato et al. (2012), [10] Ghisellini et al. (2014), [11] McGreer et al. (2006), [12] Caccianiga et al. (2019), [13] Khorunzhev et al. (2021), [14] Bañados et al. (2018), [15] Wenzl et al. (2021), [16] Onken et al. (2022).

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