Open Access
Table A.1
Detailed description of the released catalog, as previewed with five lines in Table 2 for a selected subset of columns.
| Column | Header | Description |
|---|---|---|
| (1) | Name | name for grade A and B lens candidates |
| (2) | RA [deg] | Right Ascension of the inspected candidate |
| (3) | Dec [deg] | Declination of the inspected candidate |
| (4) | p | average score predicted by the network committee |
| (5) | G | average grade between 0 and 3 obtained through visual inspection (see Sect. 4) |
| (6) | sigma_G | standard deviation of obtained visual inspection grades |
| (7) | N_graders | number of visual inspectors (see Sect. 4) |
| (8) | i_kronflux_radius | Kron radius in the i band provided by HSC used for source selection (see Sect. 2) |
| (9) | Binary | Flag to indicate sources inspected only in the binary stage (two different graders) |
| (10) | Round1 | Flag to indicate systems inspected also in the first round (four different graders) |
| (11) | Round2 | Flag to indicate systems inspected also in the second round (eight different graders) |
| (12) | A24 | Flag to indicate if system jointly inspected with candidates discovered by Andika et al. (2025) |
| (13) | S25 | Flag to indicate systems discovered by this network committee but not re-inspected. Instead, we report the visual inspection grade from our earlier work S25 |
| (14) | S22 | Flag to indicate systems discovered by this network committee but not re-inspected. Instead, we report the visual inspection grade from our earlier work Shu et al. (2022) |
| (15) | C21 | Flag to indicate systems discovered by this network committee but not re-inspected. Instead, we report the visual inspection grade from our earlier work Cañameras et al. (2021) |
| (16) | x_med | x-center coordinate predicted by the modeling network from Schuldt et al. (2023a, hereafter S23a) |
| (17) | x_err | 1 σ value for the x-center coordinate predicted by the modeling network from S23a |
| (18) | y_med | y-center coordinate predicted by the modeling network from S23a |
| (19) | y_err | 1 σ value for the y-center coordinate predicted by the modeling network from S23a |
| (20) | ex_med | x-component of the complex ellipticity predicted by the modeling network from S23a |
| (21) | ex_err | 1 σ value for the x-component of the complex ellipticity predicted by the modeling network from S23a |
| (22) | ey_med | y-component of the complex ellipticity predicted by the modeling network from S23a |
| (23) | ey_err | 1 σ value for the y-component of the complex ellipticity predicted by the modeling network from S23a |
| (24) | rE_med [″] | Einstein radius value of the given candidate predicted by the modeling network from S23a |
| (25) | rE_err [″] | 1 σ value of the Einstein radius predicted by the modeling network from S23a |
| (26) | gam1_med | γ1-component of the external shear predicted by the modeling network from S23a |
| (27) | gma1_err | 1 σ value of the γ1-component predicted by the modeling network from S23a |
| (28) | gam2_med | γ2-component of the external shear predicted by the modeling network from S23a |
| (29) | gam2_err | 1 σ value of the γ2-component predicted by the modeling network from S23a |
| (30) | Model | Flag if the model predict is reliable, only for systems inspected in the second round |
| (31) | z | photometric redshift value from the catalog compiled by S25 based on DEmP (Hsieh & Yee 2014), Mizuki (Tanaka et al. 2018), and NetZ (Schuldt et al. 2021) |
| (32) | OD_vis | Flag if the system falls into a significant overdense region |
| (33) | OD_z | Flag if the system is in a significant overdense environment according to the criteria defined by S25 |
| (34) | N_max | Peak of the photo-z histogram following the procedure of S25 |
| (35) | zlow | Lower bound of N_max in the photo-z histogram indicating the redshift of the overdensity |
| (36) | Ntot | Sum of objects with photo-z within a box of 200″ on a side. |
| (37) | References | List of publications that report the inspected candidate (within 5″) as lens candidate according to the HOLISMOKES Suyu et al. (2020) lens compilation with status of the publication, using B04 for Bolton et al. (2004), C07 for Cabanac et al. (2007), B08 for Bolton et al. (2008), G14 for Gavazzi et al. (2014), H15 for Holwerda et al. (2015), M16 for More et al. (2016), P16 for Paraficz et al. (2016), S16 for Shu et al. (2016), D17 for Diehl et al. (2017), J17 for Jacobs et al. (2017), S18 for Sonnenfeld et al. (2018), W18 for Wong et al. (2018), J19 for Jacobs et al. (2019), L19 for Li et al. (2019), P19 for Petrillo et al. (2019), H20 for Huang et al. (2020), C20 for Chan et al. (2020), Ca20 for Cañameras et al. (2020), Cao20 for Cao et al. (2020), L20 for Li et al. (2020), J20 for Jaelani et al. (2020), S20 for Sonnenfeld et al. (2020), C21 for Cañameras et al. (2021), H21 for Huang et al. (2021), L21 for Li et al. (2021), T21 for Talbot et al. (2021), R22 for Rojas et al. (2022), S22 for Shu et al. (2022), Sa22 for Savary et al. (2022), St22 Stein et al. (2022), W22 for Wong et al. (2022), Z22 for Zhong et al. (2022), A23 for Andika et al. (2023), J24 for Jaelani et al. (2024), G24 for Grespan et al. (2024), St24 for Storfer et al. (2024), S25 for Schuldt et al. (2025), ML for the master lens catalog at http://admin.masterlens.org, and ‘Guoyou Sun’ corresponds to candidates identified by an amateur astronomer, Guoyou Sun, through visual inspections of HSC cutouts (see http://sunguoyou.lamost.org/glc.html.). |
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