Abell 2744 - mbronikowski/cluster-models GitHub Wiki
Image sourced from Wikimedia Commons.
Quick Information | |
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Cluster Name | Abell 2744 |
RA | 00:14:21.16 |
DEC | -30:23:52.4 |
Redshift | 0.306 |
Alternate names | AM 0011-303; MACS J0014.3-3022; AC 118; MCXC J0014.3-3023 |
Online database links | NED; SIMBAD; |
Telescope images |
Publications and models
- GLASS-JWST Program
- JWST UNCOVER Program
- Bergamini et al. (2023)
- Richard et al. (2021)
- Sebesta et al. (2019)
- Mahler et al. (2018)
- Hubble Frontier Fields
- Mistele & Durakovic (2024)
GLASS-JWST Program
The GLASS-JWST Program has yielded a publicly available model based on JWST observations. Program page on MAST. Model publication: Bergamini et al. (2023). Model download.
JWST UNCOVER Program
The JWST UNCOVER Program has yielded a publicly available model based on JWST observations. Program page: https://jwst-uncover.github.io/. Lens model download: v2.0; older models available here. Please cite Furtak et al. (2023) and Price et al. (2024) when using this model.
Bergamini et al. (2023)
This pre-JWST model is now considered obsolete (see P. Bergamini's page here). Publication: Bergamini et al. 2023; model download.
Richard et al. (2021)
This pre-JWST model by Richard et al. (2021) is based on MUSE observations of the cluster. Model available here; project page here.
Sebesta et al. (2019)
Sebesta et al. (2019) constructed a free-form lens model using GRALE.
Mahler et al. (2018)
Mahler et al. (2018) constructed a parametric lens model using MUSE and HFF observations.
Hubble Frontier Fields
The cluster was observed as part of the Hubble Frontier Fields program. Program data products available here; models available here; acknowledgement information here.
Mistele & Durakovic (2024)
Mistele & Durakovic (2024) created a model of Abell 1835 and Abell 2744 as part of their tests of their new non-parametric method to infer galaxy cluster masses from weak lensing, which is the main focus of the paper.