RELICS: Strong Lens Model of SMACSJ0723.3-7327
arXiv:2208.08483 · doi:10.3847/1538-4365/aca7c3
Abstract
We present the details of a strong lens model of SMACS J0723.3-7327, which was made public as part of the data and high level science products (HLSP) release of the RELICS HST treasury program (Reionization Lensing Cluster Survey; GO-14096, PI: Coe). The model products were made available on the Mikulski Archive for Space Telescopes (MAST) via 10.17909/T9SP45 in 2017. Here, we provide the list of constraints that were used in the HST-based RELICS lens model, as well as other information related to our modeling choices, which were not published with the data and HLSP release. This model was computed with Lenstool, used multiple images of 8 sources, with no spectroscopic redshifts. The image plane RMS was 0".58.
4 pages, 1 figure, 1 table. Submitted to ApJS
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Cited by in corpus (4)
- On the correlation between dark matter, intracluster light and globular cluster distribution in SMACS0723
- X-ray analysis of JWST's first galaxy cluster lens SMACS J0723.3-7327
- The First Weak-lensing Analysis with the James Webb Space Telescope: SMACS J0723.3-7327
- Discovery of a Low-mass Strong-lens System in SMACS J0723.3-7327