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Table 2.
Spectroscopic observations of nine CMASS lens candidates from the SuGOHI sample.
| Lens name | Obs. date | PA | zs | Em. lines |
|---|---|---|---|---|
| HSC J023817−054555 | 2017-11-18 | −30 | 1.763 | Hα, Hβ, [OII]λ3727 |
| 2017-11-16 | −30 | |||
| HSC J121052−011905 | 2017-04-05 | 90 | 2.295 | Hα, [OIII]λ5007, [OII]λ3727 |
| HSC J140705−011256 | 2017-07-27 | 125 | … | None |
| HSC J140929−011410 | 2018-03-01 | 30 | 2.302 | Hα, [OIII]λ5007, [OIII]λ4959, Hβ, [OII]λ3727 |
| HSC J141300−012608 | 2017-04-17 | 5 | 2.666 | Hβ, [OIII]λ4959 |
| HSC J142053+005620 | 2017-04-07 | 150 | … | None |
| HSC J142720+001916 | 2017-04-08 | 55 | 1.266 | Hα, [OII]λ3727 |
| HSC J222801+012805 | 2017-07-25 | 25 | 2.462 | [OIII]λ5007, [OIII]λ4959, Hβ, Lyα |
| 2017-08-05 | 25 | |||
| HSC J223733+005015 | 2017-07-08 | −50 | 2.143 | Hα, [OIII]λ5007, [OIII]λ4959, [OII]λ3727 |
| 2017-07-08 | −50 |
Notes. Each row corresponds to one observation block. The third column indicates the position angle of the slit, in degrees east of north. The fourth and fifth columns list the source redshift and the emission lines detected in the spectrum.
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