Table B.1
List of discovered grade-A strong-lens candidates.
Name | R.A. | Decl. | mi | ![]() |
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Classifier | Score | Reference |
---|---|---|---|---|---|---|---|---|---|
(1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
HSCJ000848+001550 | 2.20333 | 0.26412 | 18.46 | 0.35 ± 0.03 | 0.397 | — | 1 | 2.6 | SuGOHI-5 |
HSCJ012018+001125 | 20.07557 | 0.19048 | 20.14 | 0.63 ± 0.04 | 0.599 | — | 1,2 | 2.6 | C21 |
HSCJ012954+003801 | 22.47583 | 0.63363 | 20.27 | 0.67 ± 0.05 | — | — | 1 | 2.8 | C21 |
HSCJ015731−033057 | 29.38125 | −3.51603 | 20.02 | 0.68 ± 0.04 | 0.621 | — | 1,2 | 2.8 | SuGOHI-1 |
HSCJ015758−061426 | 29.49429 | −6.24057 | 18.96 | 0.35 ± 0.03 | — | — | 1,2 | 2.6 | C21 |
NOTE. — Column 1 is the system name. Columns 2 and 3 are right ascension and declination (J2000) of the lens galaxy. Columns 4 and 5 are the i–band CModel magnitude and photometric redshift of the lens galaxy provided by the HSC catalogue. Columns 6 and 7 give the spectroscopic redshifts of the lens and source inferred from auxiliary data. Column 8 indicates the classifier(s) that finds the lens system. Column 9 is the average visual-inspection score of the lens system. Column 10 provides the paper that first discovered the system. Shu22 indicates a completely new discovery. Other relevant references are: Brownstein12: Brownstein et al. (2012); C21: Cañameras et al. (2021); Diehl17: Diehl et al. (2017); Huang20: Huang et al. (2020); Huang21: Huang et al. (2021); Jacobs17: Jacobs et al. (2017); Jacobs19b: Jacobs et al. (2019a); Li20: Li et al. (2020); More12: More et al. (2012); More16: More et al. (2016); More17: More et al. (2017); Petrillo19: Petrillo et al. (2019); Ratnatunga95: Ratnatunga et al. (1995); Shu16: Shu et al. (2016a); Sonnenfeld13: Sonnenfeld et al. (2013); Stark13: Stark et al. (2013); Stein21: Stein et al. (2021); SuGOHI-1: Sonnenfeld et al. (2018); SuGOHI-2: Wong et al. (2018); SuGOHI-4: Chan et al. (2020); SuGOHI-5: Jaelani et al. (2020); SuGOHI-6: Sonnenfeld et al. (2020). ‘Guoyou Sun’ corresponds to candidates identified by an amateur astronomer, Guoyou Sun, through visual inspections of HSC cutouts6. Systems with† and/or‡ are independently discovered by Wong et al. (in prep.) and/or Jaelani et al. (in prep.). The full table is available at the CDS.
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