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Table 3.

High-confidence lens candidates reported by C21 but not listed in Table 2; an analysis of their environment is now included.

Name RA Dec p G σG z ODlit ODvis ODz Nmax zlow Ntot References
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)
HSCJ1004−0031 151.21577 −0.52915 0.17 3.00 0.00 1.05 Y Y N 17 0.50 513 C21 A23
HSCJ1224−0042 186.20954 0.704233 0.28 3.00 0.00 0.38 Y Y Y 23 0.50 791 J20 P19 C21
HSCJ1434−0056 218.72664 −0.94963 0.94 3.00 0.00 0.76 Y Y Y 27 0.72 820 S18 J20 C21 J23
HSCJ0102+0158 15.65975 1.98276 0.12 3.00 0.00 N N N 10 0.74 259 C21 A23
HSCJ0238−0545 39.57340 −5.76603 0.72 3.00 0.00 1.77 N N N 8 0.86 357 S18 C21

Notes. Column description: (1) Source name, (2) right ascension (J2000), (3) declination (J2000), (4) network score, (5) average grade from our visual inspection, (6) dispersion among the eight graders, (7) photometric redshift from our combined catalog based on DEmP (Hsieh & Yee 2014), Mizuki (Tanaka et al. 2018), and NetZ (Schuldt et al. 2021b), flag on the overdensity (OD) based on (8) galaxy cluster catalogs (Oguri 2014; Oguri et al. 2018; Wen & Han 2018, 2021), (9) visual inspection, and (10) photometric redshift, (11) absolute height of photo-z distribution, (12) photo-z lower bound, (13) total number of photo-z in considered area, and (14) references of their previous discovery, apart from C21, with S13 for Sonnenfeld et al. (2013), G14 for Gavazzi et al. (2014), M16 for More et al. (2016), D17 for Diehl et al. (2017), S18 for Sonnenfeld et al. (2018), W18 for Wong et al. (2018), H19 for Huang et al. (2019), P19 for Petrillo et al. (2019), Ch20 for Chan et al. (2020), Ca20 for Cao et al. (2020) L20 for Li et al. (2020), J20 for Jaelani et al. (2020b), S20 for Sonnenfeld et al. (2020), C21 for Cañameras et al. (2021), T21 for Talbot et al. (2021), R22 for Rojas et al. (2022), S22 for Shu et al. (2022), A23 for Andika et al. (2023), J23 for Jaelani et al. (2023), and ML for the master lens catalog http://admin.masterlens.org. Full table is available at the CDS.

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