Using JADES NIRCam photometry to investigate the dependence of stellar mass inferences on the IMF in the early universe

The detection of numerous and relatively bright galaxies at redshifts <i>z</i> > 9 has prompted new investigations into the star-forming properties of high-redshift galaxies. Using local forms of the initial mass function (IMF) to estimate stellar masses of these galaxies from their light output leads to galaxy masses that are at the limit allowed for the state of the Lambda Cold Dark Matter (ΛCDM) Universe at their redshift. We explore how varying the IMF assumed in studies of galaxies in the early universe changes the inferred values for the stellar masses of these galaxies. We infer galaxy properties with the spectral energy distribution (SED) fitting code Prospector using varying IMF parameterizations for a sample of 102 galaxies with photometry from the James Webb Space Telescope, JWST Advanced Deep Extragalactic Survey that are spectroscopically confirmed to be at [Formula: see text], with additional photometry from the JWST Extragalactic Medium Band Survey for twenty-one of the galaxies. We demonstrate that models with stellar masses reduced by a factor of three or more do not affect the modeled SED.

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Publication Details

Journal
Proceedings of the National Academy of Sciences
Published
2024-10-08
DOI
https://doi.org/10.1073/pnas.2317375121
Citations
9
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
2.98

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article

Using JADES NIRCam photometry to investigate the dependence of stellar mass inferences on the IMF in the early universe

Zhiyuan Ji, Jakob M. Helton, Fengwu Sun, Benjamin D. Johnson et al.
9 citations
Proceedings of the National Academy of Sciences
Galaxies: Formation, Evolution, Phenomena
2.98
article

Using JADES NIRCam photometry to investigate the dependence of stellar mass inferences on the IMF in the early universe

Zhiyuan Ji, Jakob M. Helton, Fengwu Sun, Benjamin D. Johnson, Lily Whitler, Kevin Hainline, Sandro Tacchella, Rachana Bhatawdekar, S. Charlot, Christina C. Williams, Daniel J. Eisenstein, Emma Curtis-Lake, Christopher N. A. Willmer, William Baker, Andrew J. Bunker, Brant E. Robertson, Marcia Rieke, Raphael E. Hviding, Charity Woodrum, Ryan Hausen
article en
9 citations

Abstract

The detection of numerous and relatively bright galaxies at redshifts <i>z</i> > 9 has prompted new investigations into the star-forming properties of high-redshift galaxies. Using local forms of the initial mass function (IMF) to estimate stellar masses of these galaxies from their light output leads to galaxy masses that are at the limit allowed for the state of the Lambda Cold Dark Matter (ΛCDM) Universe at their redshift. We explore how varying the IMF assumed in studies of galaxies in the early universe changes the inferred values for the stellar masses of these galaxies. We infer galaxy properties with the spectral energy distribution (SED) fitting code Prospector using varying IMF parameterizations for a sample of 102 galaxies with photometry from the James Webb Space Telescope, JWST Advanced Deep Extragalactic Survey that are spectroscopically confirmed to be at [Formula: see text], with additional photometry from the JWST Extragalactic Medium Band Survey for twenty-one of the galaxies. We demonstrate that models with stellar masses reduced by a factor of three or more do not affect the modeled SED.

Proceedings of the National Academy of SciencesVol. 121(42)
Centre National de la Recherche Scientifique (FR), University of Arizona (US), University of Hertfordshire (GB), Johns Hopkins University (US), University of California, Santa Cruz (US), University of Cambridge (GB), Institut d'Astrophysique de Paris (FR), Sorbonne Université (FR), University of Oxford (GB), European Space Astronomy Centre (ES), Max Planck Institute for Astronomy (DE), Center for Astrophysics Harvard & Smithsonian (US), NSF NOIRLab (US)
National Science Foundation, National Aeronautics and Space Administration, Johns Hopkins University, University of Arizona, UK Research and Innovation, European Commission, Goddard Space Flight Center, Science and Technology Facilities Council
Affordable and clean energy
Openalex Percentile: Top 9%
Galaxies: Formation, Evolution, Phenomena
2.98
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