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Exploring the chemical content of Galaxies using the SAMI Zoom Survey: a data release of 92 spatially resolved H ii regions in nearby galaxies

Myszka, Aaron; Sweet, Sarah M; Nanayakkara, Themiya; Glazebrook, Karl; Groves, Brent; Cameron, Alex J; Grasha, Kathryn; Krumholz, Mark R; Li, Zefeng; López-Sánchez, Ángel R; Nicholls, David C; Rowlands, Stephanie; Ryan-Weber, Emma; Ting, Yuan-Sen

Exploring the chemical content of Galaxies using the SAMI Zoom Survey: a data release of 92 spatially resolved H ii regions in nearby galaxies Thumbnail


Authors

Aaron Myszka

Sarah M Sweet

Themiya Nanayakkara

Karl Glazebrook

Brent Groves

Alex J Cameron

Kathryn Grasha

Mark R Krumholz

Zefeng Li zefeng.li@durham.ac.uk
Postdoctoral Research Associate

Ángel R López-Sánchez

David C Nicholls

Stephanie Rowlands

Emma Ryan-Weber

Yuan-Sen Ting



Abstract

We present the SAMI Zoom Survey, spatially resolved IFU spectroscopy of 92 H ii regions from 7 nearby galaxies (distances 2–14 Mpc) utilizing the Sydney-AAO Multi-object IFS (SAMI) instrument. Each H ii region has two spectral data cubes (blue-arm sampling 1.05 Å pixel−1 between 3700–5746 Å, and red-arm sampling 0.57 Å pixel−1 between 6300–7399 Å) as well as two-dimensional emission line flux maps. The spatial sampling is 0.5 arcsec across 15 arcsec fields of view, with a mean angular resolution of 2.0 arcsec (18–150 pc). We investigate seven forms of common gas–phase metallicity determinations, contrasting metallicity calibrations including the direct electron temperature method and six strong-line methods. We determine these metallicities, temperatures, densities, and ionization parameters where possible, in spatially resolved form as well as an integrated-region data set where we focus our analysis. We find varying degrees of disparity between metallicity values using different methods, and likewise between derived abundance gradients of the host galaxies. In comparisons using metallicity as a baseline, mean disparities span 0.12–0.49 dex in oxygen abundance depending on the chosen alternative method, with a maximum of 0.65 dex when comparing against the direct electron temperature method. Host-galaxy abundance gradients deviate up to 0.66 dex in central oxygen abundance while slopes vary by up to 0.51 dex R−1. The SAMI Zoom Survey provides a data set with spatial resolution, spectral coverage, and radial extent to support the study of such astrophysical processes in nearby galaxies.

Citation

Myszka, A., Sweet, S. M., Nanayakkara, T., Glazebrook, K., Groves, B., Cameron, A. J., Grasha, K., Krumholz, M. R., Li, Z., López-Sánchez, Á. R., Nicholls, D. C., Rowlands, S., Ryan-Weber, E., & Ting, Y.-S. (2025). Exploring the chemical content of Galaxies using the SAMI Zoom Survey: a data release of 92 spatially resolved H ii regions in nearby galaxies. Monthly Notices of the Royal Astronomical Society, 540(1), 919-960. https://doi.org/10.1093/mnras/staf742

Journal Article Type Article
Acceptance Date Apr 29, 2025
Online Publication Date May 7, 2025
Publication Date 2025-06
Deposit Date Jul 8, 2025
Publicly Available Date Jul 8, 2025
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 540
Issue 1
Pages 919-960
DOI https://doi.org/10.1093/mnras/staf742
Public URL https://durham-repository.worktribe.com/output/3968188

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