SuGOHI . | Data release . | Area (deg|$^2$|) . | Inspected objects . | Grades (A, B, C) . | Description . |
---|---|---|---|---|---|
I | Up to S16A | 442 | |$\sim$| 43 000 (LRG) | (15, 36, 282) | YattaLensa, Chitahb, Spectroscopic |
II | Up to S17A | 776 | 31 286 (LRG) | (7, 34,...) | YattaLensa |
IV | Up to S16A | 456 | |$\sim$| 45 000 (LRG); |$\sim$| 110 000 (QSO) | (17, 26,...) | Chitahb |
V | Up to S18A | 1114 | |$\sim$| 39 500 (Galaxy clusters) | (47, 181, 413) | Cluster catalogues, Human-inspection |
VI | Up to S16A | 442 | |$\sim$| 300 000 | (14, 129, 581) | Citizen-Scientist |
VII | – | – | SQLS; Chandra catalogue | (3,...,...) | reinspection previous catalogues |
VIII | Up to S21A | 1310 | 103 191 (LRG) | (8, 28, 138) | YattaLensa |
IX | Pp to S21A | 1310 | 1652 329 (Quasar) | (73, 17, 53) | Colour similarity, YattaLensa |
SuGOHI . | Data release . | Area (deg|$^2$|) . | Inspected objects . | Grades (A, B, C) . | Description . |
---|---|---|---|---|---|
I | Up to S16A | 442 | |$\sim$| 43 000 (LRG) | (15, 36, 282) | YattaLensa, Chitahb, Spectroscopic |
II | Up to S17A | 776 | 31 286 (LRG) | (7, 34,...) | YattaLensa |
IV | Up to S16A | 456 | |$\sim$| 45 000 (LRG); |$\sim$| 110 000 (QSO) | (17, 26,...) | Chitahb |
V | Up to S18A | 1114 | |$\sim$| 39 500 (Galaxy clusters) | (47, 181, 413) | Cluster catalogues, Human-inspection |
VI | Up to S16A | 442 | |$\sim$| 300 000 | (14, 129, 581) | Citizen-Scientist |
VII | – | – | SQLS; Chandra catalogue | (3,...,...) | reinspection previous catalogues |
VIII | Up to S21A | 1310 | 103 191 (LRG) | (8, 28, 138) | YattaLensa |
IX | Pp to S21A | 1310 | 1652 329 (Quasar) | (73, 17, 53) | Colour similarity, YattaLensa |
Notes. aI (Sonnenfeld et al. 2018); II (Wong et al. 2018); IV (Chan et al. 2020); V (Jaelani et al. 2020b); VI (Sonnenfeld et al. 2020); VII (Jaelani et al. 2021); VIII (Wong et al. 2022); IX (Chan et al. 2023); b(Chan et al. 2015). LRG is luminous red galaxies, QSO is quasi-stellar objects, and SQLS is Sloan Digital Sky Survey Quasar Lens Search. The SuGOHI database has around 2000 lens candidates (|$\sim$| 800 are grades A and B) from previous searches.
SuGOHI . | Data release . | Area (deg|$^2$|) . | Inspected objects . | Grades (A, B, C) . | Description . |
---|---|---|---|---|---|
I | Up to S16A | 442 | |$\sim$| 43 000 (LRG) | (15, 36, 282) | YattaLensa, Chitahb, Spectroscopic |
II | Up to S17A | 776 | 31 286 (LRG) | (7, 34,...) | YattaLensa |
IV | Up to S16A | 456 | |$\sim$| 45 000 (LRG); |$\sim$| 110 000 (QSO) | (17, 26,...) | Chitahb |
V | Up to S18A | 1114 | |$\sim$| 39 500 (Galaxy clusters) | (47, 181, 413) | Cluster catalogues, Human-inspection |
VI | Up to S16A | 442 | |$\sim$| 300 000 | (14, 129, 581) | Citizen-Scientist |
VII | – | – | SQLS; Chandra catalogue | (3,...,...) | reinspection previous catalogues |
VIII | Up to S21A | 1310 | 103 191 (LRG) | (8, 28, 138) | YattaLensa |
IX | Pp to S21A | 1310 | 1652 329 (Quasar) | (73, 17, 53) | Colour similarity, YattaLensa |
SuGOHI . | Data release . | Area (deg|$^2$|) . | Inspected objects . | Grades (A, B, C) . | Description . |
---|---|---|---|---|---|
I | Up to S16A | 442 | |$\sim$| 43 000 (LRG) | (15, 36, 282) | YattaLensa, Chitahb, Spectroscopic |
II | Up to S17A | 776 | 31 286 (LRG) | (7, 34,...) | YattaLensa |
IV | Up to S16A | 456 | |$\sim$| 45 000 (LRG); |$\sim$| 110 000 (QSO) | (17, 26,...) | Chitahb |
V | Up to S18A | 1114 | |$\sim$| 39 500 (Galaxy clusters) | (47, 181, 413) | Cluster catalogues, Human-inspection |
VI | Up to S16A | 442 | |$\sim$| 300 000 | (14, 129, 581) | Citizen-Scientist |
VII | – | – | SQLS; Chandra catalogue | (3,...,...) | reinspection previous catalogues |
VIII | Up to S21A | 1310 | 103 191 (LRG) | (8, 28, 138) | YattaLensa |
IX | Pp to S21A | 1310 | 1652 329 (Quasar) | (73, 17, 53) | Colour similarity, YattaLensa |
Notes. aI (Sonnenfeld et al. 2018); II (Wong et al. 2018); IV (Chan et al. 2020); V (Jaelani et al. 2020b); VI (Sonnenfeld et al. 2020); VII (Jaelani et al. 2021); VIII (Wong et al. 2022); IX (Chan et al. 2023); b(Chan et al. 2015). LRG is luminous red galaxies, QSO is quasi-stellar objects, and SQLS is Sloan Digital Sky Survey Quasar Lens Search. The SuGOHI database has around 2000 lens candidates (|$\sim$| 800 are grades A and B) from previous searches.
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