Star Formation at the Epoch of Reionization with CANUCS: The ages of stellar populations in MACS1149-JD1

Grism Gravitational microlensing Balmer series Stellar mass
DOI: 10.48550/arxiv.2308.13288 Publication Date: 2023-01-01
ABSTRACT
We present measurements of stellar populations properties a z = 9.1 gravitationally lensed galaxy MACS1149-JD1 using deep JWST NIRISS slitless spectroscopy as well and NIRCam imaging from the CAnadian Unbiased Cluster Survey (CANUCS). The is split into four components. Three magnified (${\mu}$ ~ 17) star-forming components are unresolved, giving intrinsic sizes < 50pc. In addition, underlying extended component contains bulk mass, formed majority its stars 50Myr earlier than other three not site most active star formation currently. resolved photometry does confirm strong Balmer break previously seen in Spitzer. grism spectrum has been extracted for entire shows clear continuum Lyman-break, with no Lyman-${\alpha}$ detected.
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