Table 1.
High-confidence galaxy-scale lens candidates with ResNet scores > 0.1, and average grades ≥1.5 from visual inspection.
| Name | RA | Dec | p | G | σG | #G = 3 | gKron | rKron | iKron | z | Notes |
|---|---|---|---|---|---|---|---|---|---|---|---|
| HSCJ0102+0158 | 15.6597 | 1.98247 | 0.12 | 3.0 | 0.0 | 5 | 27.61 | 21.62 | 20.58 | 0.8669(*) | (i) |
| HSCJ0157−0330 | 29.3812 | −3.51603 | 0.16 | 3.0 | 0.0 | 5 | 21.9 | 21.02 | 20.14 | 0.6212(*) | (a) |
| HSCJ0200−0344 | 30.1981 | −3.73763 | 0.6 | 3.0 | 0.0 | 5 | 22.23 | 21.17 | 20.04 | 0.72 | |
| HSCJ0232−0323 | 38.2078 | −3.39058 | 0.19 | 3.0 | 0.0 | 5 | 20.89 | 19.37 | 18.62 | 0.42 | (h) (e) (i) |
| HSCJ0236−0332 | 39.1554 | −3.53893 | 1.0 | 3.0 | 0.0 | 5 | 20.48 | 19.09 | 18.54 | 0.2695(*) | (a) (e) |
| HSCJ0238−0545 | 39.5741 | −5.76545 | 0.72 | 3.0 | 0.0 | 5 | 20.75 | 19.96 | 19.18 | 0.5993(*) | (a) (c) |
| HSCJ0850+0039 | 132.6942 | 0.65146 | 0.61 | 3.0 | 0.0 | 5 | 24.66 | 22.08 | 21.25 | 1.00 | (d) |
| HSCJ0904−0059 | 136.0331 | −0.99807 | 0.69 | 3.0 | 0.0 | 5 | 22.42 | 21.23 | 20.26 | 0.56 | (k) |
Notes. The full table is available at the CDS. Some systems in this table are also found in separate lens searches and cross-references will be added to the corresponding publications (Shu et al., in prep.; Jaelani et al., in prep.). Columns are: source name; right ascension; declination; output score from the ResNet; average visual grades from five authors; dispersion in the grades; number of classifiers assigning the highest grade of 3; g-, r-, and i-band Kron magnitudes from PDR2; CNN photometric redshift estimates from Schuldt et al. (2021b) or spectroscopic redshifts marked as (*) where available; references for systems previously published, either as spectroscopically-confirmed lenses or as grade A or B candidates.
References. (a) Sonnenfeld et al. (2018), (b) Wong et al. (2018), (c) Chan et al. (2020), (d) Sonnenfeld et al. (2020), (e) Jaelani et al. (2020), (f) Cañameras et al. (2020), (g) Huang et al. (2020), (h) Stark et al. (2013), (i) Jacobs et al. (2019), (j) Li et al. (2020), (k) More et al. (2012), (l) Petrillo et al. (2019), (m) Brownstein et al. (2012), (n) Gavazzi et al. (2014), (o) Diehl et al. (2017), (p) More et al. (2016), (q) Shu et al. (2016), (r) Jacobs et al. (2017), (s) Ratnatunga et al. (1995), (t) Tanaka et al. (2016), and (u) More et al. (2017). Candidates marked with a † have a lower grade C in SuGOHI.
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