Galaxy And Mass Assembly (GAMA): extended intragroup light in a group at z = 0.2 from deep Hyper Suprime-Cam images
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We present a pilot study to assess the potential of Hyper Suprime-Cam Public Data Release 2 (HSC-PDR2) images for the analysis of extended faint structures within groups of galaxies. We examine the intragroup light (IGL) of the group 400138 (Mdyn = 1.3 ± 0.5 × 1013 M⊙, z ∼ 0.2) from the Galaxy And Mass Assembly (GAMA) survey using Hyper Suprime-Cam Subaru Strategic Program Public Data Release 2 (HSC-SSP PDR2) images in g, r, and i bands. We present the most extended IGL measurement to date, reaching down to $\mu _{g}^{\rm {lim}}=30.76$ mag arcsec−2 (3σ; 10 × 10 arcsec2) at a semimajor axis of 275 kpc. The IGL shows mean colour values of g − i = 0.92, g − r = 0.60, and r − i = 0.32 (±0.01). The IGL stellar populations are younger (2–2.5 Gyr) and less metal rich ([Fe/H] ∼ −0.4) than those of the host group galaxies. We find a range of IGL fractions as a function of total group luminosity of ${\sim} 2\!-\!36 {{\ \rm per\ cent}}$ depending on the definition of IGL, with larger fractions the bluer the observation wavelength. The early-type to late-type galaxy ratio suggests that 400138 is a more evolved group, dominated by early-type galaxies, and the IGL fraction agrees with that of other similarly evolved groups. These results are consistent with tidal stripping of the outer parts of Milky Way-like galaxies as the main driver of the IGL build-up. This is supported by the detection of substructure in the IGL towards the galaxy member 1660615 suggesting a recent interaction (<1 Gyr ago) of that galaxy with the core of the group.
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The HSC-SSP Ultradeep field spans an area of 3.5 deg^2 and reaches μ_r ∼ 29.82 mag arcsec^-2, a surface brightness depth faint enough to detect tidal features.
“We use the Ultradeep field, which spans an area of 3 . 5 deg 2 and reaches 𝜇 𝑟 ∼ 29.82 mag arcsec -2 (Martínez-Lombilla et al. 2023), a surface brightness depth faint enough to detect tidal features.”
From Detecting galaxy tidal features using self-supervised representation learning (2024) · cites this paper as Martínez-Lombilla et al. 2023
Section 3.5 reports an r-band surface-brightness limit of 29.82 mag arcsec⁻² for the authors’ HSC ultradeep data, measured at 3σ in 10 × 10 arcsec² boxes. Section 4.1 describes detection of a faint diffuse-light tail, but our copy does not establish that the Ultradeep field spans 3.5 deg²; Section 2.2 gives 1.77 deg² as the camera’s imaging area, not the field’s area. (LLM, conf=0.86)
Experimental — accuracy not yet measuredHSC-PDR2 has been widely tested for low surface brightness studies and fulfils the requirements for this study.
“HSC-PDR2 has been widely tested for low surface brightness studies (e.g. Huang et al. 2018, 2020; Li et al. 2022; Martínez-Lombilla et al. 2023) and fulfils the requirements for our study.”
From Detecting galaxy tidal features using self-supervised representation learning (2024) · cites this paper as Martínez-Lombilla et al. 2023
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Self-citationDeep Imaging of Diffuse Light Around Galaxies and Clusters: Progress and ChallengesPreprint
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Analysing the prevalence of tidal features in HSC-SSP using self-supervised representation learning
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Self-citationOn the Origin of Intracluster Light Based on the High-resolution Simulation, NewCluster
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Galaxy And Mass Assembly: the xSAGA galaxy complement in nearby galaxy groups
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Self-citation
- Authors
- Martínez-Lombilla, C., Brough, S., Montes, M., Baena-Gallé, R., Akhlaghi, M., Infante-Sainz, R., Driver, S. P., Holwerda, B. W., Pimbblet, K. A., & Robotham, A. S. G.
- Affiliations
- Australian Research Council (AU)
- UNSW Sydney (AU)
- Space Telescope Science Institute (US)
- Universidad Internacional de La Rioja (ES)
- Centro de Estudios de Física del Cosmos de Aragón (ES)
- Centro de Estudios de Física del Cosmos de Aragón (CEFCA) , Plaza San Juan 1, E-44001 Teruel, Spain
- The University of Western Australia (AU)
- University of Louisville (US)
- University of Hull (GB)
- Corresponding author
- Martínez-Lombilla, Cristina
- ORCID
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2022-11-24
- Volume
- 518
- Issue
- 1
- Pages
- 1195-1213
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W4309818276
- Cited by
- 27
- References
- 146
- Citations by year
- 2026: 4 · 2025: 10 · 2024: 4 · 2023: 9
- FWCI
- 2.27
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Licence
- academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model (vor)
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- UWA Profiles and Research Repository (UWA) (submittedVersion, other-oa)
- Repository@Hull (Worktribe) (University of Hull) (submittedVersion, cc-by)
- Re-Unir (International University of La Rioja) (submittedVersion, other-oa)
- ThinkIR: The University of Louisville's Institutional Repository (University of Louisville) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Australian Research Council (DP190101943, CE170100013)
- Spanish State Research Agency
- AEI
- Spanish Ministry of Science and Innovation (PID2019-105602GB-I00)
- European Union (ICTS-MRR-2021-03-CEFCA)
- Ministerio de Ciencia, Innovación y Universidades
- FEDER (PGC2018-097585-B-C21)
- STFC
- ARC
- UNSW
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysical Phenomena and Observations
- Keywords
- galaxy groups, tidal stripping, Hyper Suprime-Cam, GAMA survey, stellar populations, galaxy interactions, early-type galaxies, Milky Way-like galaxies
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