Table 5.
Thirty-one sources clearly rejected as milli-lens systems so far.
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
---|---|---|---|---|---|---|---|---|---|
Source | z | S4.9 GHz | S22.2 GHz | Morphology | FR test | SBR test | Spectrum test | Separation test | Class |
[mJy] | [mJy] | ||||||||
J0010−0740 | 0.311, p | 29 | – | FAIL | PASS | FAIL | FAIL | PASS | CSO |
J0011+3443 | 0.892, s | 126 | – | PASS | PASS | FAIL | PASS | PASS | CSO |
J0024−4202 | 0.943, s | – | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO/Other |
J0044+2858 | 0.751, p | 51 | 13 | PASS | PASS | PASS | FAIL | PASS | CSO |
J0052+1633 | 0.431, p | 155 | 36 | FAIL | FAIL | FAIL | FAIL | PASS | CSO |
J0118+3810 | – | 124 | – | PASS | PASS | FAIL | PASS | PASS | CSO |
J0132+5211 | 0.984, p | 47 | – | PASS | PASS | FAIL | FAIL | FAIL | Core-jet |
J0139+0824 | 1.055, p | 91 | – | PASS | PASS | PASS | FAIL | PASS | CSO |
J0203+3041 | 0.966, s | 257 | 32 | PASS | PASS | FAIL | PASS | PASS | Core-jet/CSO |
J0210−2213 | 1.497, s | 282 | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO |
J0213+8717 | – | 141 | 57 | PASS | PASS | FAIL | FAIL | PASS | Core-jet/CSO |
J0222+0952 | – | 148 | – | FAIL | PASS | FAIL | FAIL | PASS | Core-jet/Other |
J0232−3422 | – | – | – | PASS | PASS | PASS | FAIL | PASS | Core-jet/CSO/Other |
J0237+1116 | 0.998, s | 67 | – | PASS | PASS | FAIL | PASS | PASS | Core-jet/CSO |
J0502+1626 | – | 37 | – | PASS | PASS | FAIL | FAIL | PASS | Core-jet/CSO |
J0527+1743 | 0.461, p | 49 | – | PASS | PASS | FAIL | PASS | PASS | CSO/SMBHB |
J0616−1957 | – | 135 | – | FAIL | PASS | FAIL | FAIL | PASS | CSO |
J0732+6023 | 1.065, p | 76 | – | PASS | PASS | FAIL | FAIL | PASS | CSO/Core-jet |
J0923−3435 | – | – | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO |
J1132+5100 | 1.155, p | 95 | – | FAIL | PASS | FAIL | FAIL | PASS | Core-jet/CSO/Other |
J1143+1834 | 1.109, p | 334 | 57 | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO/SMBHB |
J1218−2159 | – | 112 | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO |
J1306+0341 | – | 109 | – | PASS | PASS | FAIL | PASS | PASS | CSO |
J1340−0335 | 0.985, p | 238 | – | FAIL | PASS | FAIL | PASS | PASS | CSO/Other |
J1344−1739 | – | 77 | 11 | PASS | PASS | PASS | FAIL | PASS | CSO |
J1632+3547 | 1.085, p | – | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/SMBHB/Other |
J1653+3503 | 0.811, p | – | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/Other |
J1721+5207 | 1.305, p | 71 | – | PASS | PASS | FAIL | FAIL | PASS | CSO |
J1805−0438 | – | 103 | 21 | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO/Other |
J2010+1513 | – | 152 | 19 | FAIL | PASS | PASS | FAIL | PASS | CSO |
J2044+6649 | – | 107 | – | PASS | PASS | PASS | FAIL | PASS | CSO |
J2114+4036 | 0.1210, p | 101 | 21 | FAIL | PASS | PASS | FAIL | PASS | Core-jet/CSO |
J2209+6442 | – | 48 | 15 | PASS | PASS | FAIL | FAIL | PASS | Core-jet/CSO |
J2214−2521 | 0.0911, s | 166 | – | PASS | PASS | FAIL | FAIL | PASS | Core-jet/CSO |
J2225+0841 | 0.731, p | 104 | 21 | PASS | PASS | FAIL | FAIL | PASS | CSO |
J2259+4037 | – | 116 | 23 | FAIL | PASS | FAIL | FAIL | PASS | CSO |
J2312+0919 | 0.231, p | 19 | – | PASS | FAIL | PASS | PASS | PASS | CSO |
J2324−0058 | 0.371, p | 56 | 31 | PASS | FAIL | FAIL | FAIL | PASS | Core-jet |
J2337−0622 | 0.181, p | 45 | – | PASS | PASS | FAIL | FAIL | PASS | Core-jet |
J2347−1856 | 0.221, p | 408 | – | PASS | PASS | PASS | PASS | PASS | Milli-lens/CSO |
Notes. Column (1) denotes the source J2000 identifier; (2) the source redshift; (3) the total clean map flux density from our new EVN data at 4.9 GHz; (4) the total clean map flux density from our new EVN data at 22.2 GHz; we denote in column (5)-(9) if a source has passed or failed one of the five criteria outlined in Section 4.2; column (11) denotes our source class designation, following our discussion of the results in Section 6. References for redshifts: 1 SDSS (DR17, Abdurro’uf et al. 2022); 2 Vardoulaki et al. (2010); 3 Labiano et al. (2007); 4 Richards et al. (2015); 5 DES DR8; 6 Shaw et al. (2012); 7 de Vries et al. (2007); 8 Storey-Fisher et al. (2024); 9 DES DR10; 10 Bilicki et al. (2014); 11 Colless et al. (2003). The superscript p denotes photometric and s spectroscopic redshift.
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