SDSS J2222 2745 - mbronikowski/cluster-models GitHub Wiki
| Quick Information | |
|---|---|
| Cluster Name | SDSS J2222+2745 |
| RA | 22:22:08.58 |
| DEC | +27:45:35.63 |
| Redshift | 0.489 |
| Alternate names | |
| Online database links | |
| Telescope images |
Publications and models
Napier et al. (2023)
The cluster was modeled by Napier et al. (2023), along with SDSS J1029+2623 and SDSS J1004+4112, to obtain a Hubble constant measurement from time delays.
Acebron et al. (2022)
The cluster was modeled gravitationally by Acebron et al. (2022). The paper also describes the gravitationally lensed background quasar behind this cluster.
Sharon et al. (2017)
Sharon et al. (2017) constructed a lens model of the cluster and time delay predictions for the multiply-imaged quasar.
Additional information
The cluster is one of the few currently known clusters with multiple images of a background quasar (see e.g. Acebron et al. 2022).