论文标题
SDSS J1226+2152的基于HST的镜头模型，为JWST-ERS模板做准备
HST-Based Lens Model of SDSS J1226+2152, in Preparation for JWST-ERS TEMPLATES
论文作者
论文摘要
强烈的镜头Z = 2.9233 Lyman Break Galaxy，SGAS J122651.3+215220，由Z = 0.4358的集群镜头，JWST作为JWST-ERS程序模板的一部分，是JWST的一部分：针对极其放大的Panchrasomic Panchromanic Panchromanic Panchromanic镜头镜头和其扩展的零星形成。为了将JWST的精致功能与强烈的镜头相结合，这些观察结果将在宇宙中午凝视到星系中，并探测恒星形成的基础。在这里，我们提出了一个哈勃太空望远镜强透镜分析，镜头模型，源平面解释以及在源固有属性中分析JWST观察所需的镜头输出。镜头模型输出通过Mikulski Space望远镜（MAST）门户网站公开向社区公开使用。
The strongly lensed z=2.9233 Lyman break galaxy, SGAS J122651.3+215220, lensed by a cluster at z=0.4358, was first targeted by JWST as part of the JWST-ERS program TEMPLATES: Targeting Extremely Magnified Panchromatic Lensed Arcs and their Extended Star formation. Aiming to combine the exquisite capabilities of JWST with the extreme magnification provided by strong gravitational lensing, these observations will peer into galaxies at cosmic noon and probe the building blocks of star formation. Here, we present an Hubble Space Telescope strong lensing analysis, lens model, source-plane interpretation, and the lensing outputs needed to analyze the JWST observations in the context of the source's intrinsic properties. The lens model outputs are made publicly available to the community through the Mikulski Archive for Space Telescopes (MAST) Portal.
