REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy
Mohammad Akhshik, Katherine E. Whitaker, Gabriel Brammer, Guillaume, Mahler, Keren Sharon, Joel Leja, Matthew B. Bayliss, Rachel Bezanson, Michael, D. Gladders, Allison Man, Erica J. Nelson, Jane R. Rigby, Francesca Rizzo,, Sune Toft, Sarah Wellons, Christina C. Williams

TL;DR
REQUIEM-2D introduces a Bayesian method combining photometry and HST grism spectroscopy to analyze spatially resolved stellar populations in high-redshift galaxies, enabling detailed age and star-formation history measurements.
Contribution
The paper presents a novel Bayesian approach and the requiem2d code for joint modeling of photometry and spectroscopy to resolve stellar populations in distant galaxies.
Findings
Successfully recovers star-formation histories from simulated data.
Provides spatially resolved age measurements of a high-redshift galaxy.
Finds a flat age gradient in the galaxy's core, supporting early formation.
Abstract
We present a novel Bayesian methodology to jointly model photometry and deep Hubble Space Telescope (HST) 2d grism spectroscopy of high-redshift galaxies. Our requiem2d code measures both unresolved and resolved stellar populations, ages, and star-formation histories (SFHs) for the ongoing REQIUEM (REsolving QUIEscent Magnified) Galaxies Survey, which targets strong gravitationally lensed quiescent galaxies at z~2. We test the accuracy of \texttt{requiem2d} using a simulated sample of massive galaxies at z~2 from the Illustris cosmological simulation and find we recover the general trends in SFH and median stellar ages. We further present a pilot study for the REQUIEM Galaxies Survey: MRG-S0851, a quintuply-imaged, massive () red galaxy at . With an estimated gravitational magnification of , we sample the…
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Code & Models
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Taxonomy
TopicsAstronomy and Astrophysical Research · Galaxies: Formation, Evolution, Phenomena · Gamma-ray bursts and supernovae
