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Table 2.

High-confidence lens candidates with ResNet scores p ≥ 0.1, and average grades G ≥ 1.5 from visual inspection.

Name RA [deg] Dec [deg] 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)
HSCJ2331+0037 352.87702 0.62594 0.91 3.00 0.00 0.56 Y N N 18 0.56 724 W18 C21
HSCJ2305−0002 346.34029 −0.03658 1.00 3.00 0.00 0.49 N N Y 22 0.62 609 W18 C21
HSCJ0128+0038 22.47583 0.63363 0.14 2.88 0.33 0.61 Y N Y 25 0.78 546 C21 S22
HSCJ0925+0017 141.43748 0.28450 0.20 2.88 0.33 1.36 Y N Y 24 0.76 833 J20 C21
HSCJ2332+0038 353.12887 0.63939 0.98 2.75 0.43 0.61 N N N 20 0.80 779 W18 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 of the recentered lens galaxy candidate 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) Literature (Oguri 2014; Oguri et al. 2018; Wen & Han 2018, 2021), (9) visual inspection, and (10) the photometric redshift analysis, (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 with 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), Ca20 for Cao et al. (2020) H20 for Huang et al. (2020) J20 for Jaelani et al. (2020b), S20 for Sonnenfeld et al. (2020), C21 for Cañameras 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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