Abell 2744
Pandora's Cluster
- Right ascension
- 00:14:21.16 (3.58817°)
- Declination
- -30:23:52.4 (-30.39789°)
- Redshift
- 0.306
- Position
- Lensed transients
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- SN HFF14Tom supernova, single image
Designations
- SZ surveys
- ACT-CL J0014.3-3022, SPT-CL J0014-3022, PLCKESZ G008.93-81.23, PSZ1 G009.02-81.22, PSZ2 G008.94-81.22
- X-ray surveys
- MACS J0014.3-3022, MCXC J0014.3-3023, RXC J0014.3-3023, RXC J0014.3-3022
- Optical/IR surveys
- Abell 2744, AM 0011-303, AC 118
Nearby clusters in this catalogue
None within 2°. The nearest is Abell 2667, 6.6° away.
Lens models 8
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Paper: Bergamini et al. (2023c)Program: GLASS-JWST
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Papers: Furtak et al. (2023b), Price et al. (2025)Program: UNCOVER
Lens model v2.0 (UNCOVER DR4)Older model versions
Please cite Furtak et al. (2023b) and Price et al. (2025) when using this model.
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Paper: Bergamini et al. (2023a)
Model downloadSee also: Ferrara lens-model page
Pre-JWST model, now considered obsolete.
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Paper: Richard et al. (2021)Program: MUSE DR
Pre-JWST model.
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Paper: Sebesta et al. (2019)Software: GRALETags: free form
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Paper: Mahler et al. (2018)Tags: parametric
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Program: HFF
Lens models from all HFF teams (MAST)
Models from several independent teams; see the HFF program page for credits and acknowledgement requirements.
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Paper: Mistele & Durakovic (2024)Tags: weak lensing, method test
Test case for a new non-parametric method of measuring cluster masses from weak lensing, the main focus of the paper; Abell 1835 is the other test case.