Dennis Zaritsky
LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies
Zaritsky, Dennis; Golini, Giulia; Donnerstein, Richard; Trujillo, Ignacio; Akhlaghi, Mohammad; Chamba, Nushkia; D’Onofrio, Mauro; Eskandarlou, Sepideh; Hosseini-ShahiSavandi, S. Zahra; Infante-Sainz, Raúl; Martin, Garreth; Montes, Mireia; Román, Javier; Sedighi, Nafise; Sharbaf, Zahra
Authors
Giulia Golini
Richard Donnerstein
Ignacio Trujillo
Mohammad Akhlaghi
Nushkia Chamba
Mauro D’Onofrio
Sepideh Eskandarlou
S. Zahra Hosseini-ShahiSavandi
Raúl Infante-Sainz
Dr GARRETH MARTIN Garreth.Martin@nottingham.ac.uk
RESEARCH FELLOW
Mireia Montes
Javier Román
Nafise Sedighi
Zahra Sharbaf
Abstract
We present an overview of the LBT Imaging of Galactic Halos and Tidal Structures survey, which currently includes 25 nearby galaxies that are on average ∼1 mag fainter than the Milky Way, and a catalog of 54 low central surface brightness (24 < μ 0,g /mag arcsec−2 < 28) satellite galaxy candidates, most of which were previously uncatalogued. The depth of the imaging exceeds the full 10 yr depth of the Rubin Observatory’s Legacy Survey of Space and Time. We find, after applying completeness corrections, rising numbers of candidate satellites as we approach the limiting luminosity (M r ∼ −8 mag) and central surface brightness (μ 0,g ∼ 28 mag arcsec−2). Over the parameter range we explore, each host galaxy (excluding those that are in overdense regions, apparently groups) has nearly four such candidate satellites to a projected radius of ∼100 kpc. These objects are mostly just at or beyond the reach of spectroscopy unless they are H i rich or have ongoing star formation. We identify three, possibly four, ultra-diffuse satellite galaxies (effective radius >1.5 kpc). This incidence rate falls within expectations of the extrapolation of the published relationship between the number of ultra-diffuse satellite galaxies and host halo mass. Last, we visually identify 12 candidate satellites that host a nuclear star cluster (NSC). The NSC occupation fraction for the sample (12/54) matches that published for satellites of early-type galaxies, suggesting that the parent’s morphological type plays at most a limited role in determining the NSC occupation fraction.
Citation
Zaritsky, D., Golini, G., Donnerstein, R., Trujillo, I., Akhlaghi, M., Chamba, N., D’Onofrio, M., Eskandarlou, S., Hosseini-ShahiSavandi, S. Z., Infante-Sainz, R., Martin, G., Montes, M., Román, J., Sedighi, N., & Sharbaf, Z. (2024). LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies. Astronomical Journal, 168(2), Article 69. https://doi.org/10.3847/1538-3881/ad543f
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 3, 2024 |
Online Publication Date | Jul 11, 2024 |
Publication Date | Aug 1, 2024 |
Deposit Date | Jul 22, 2024 |
Publicly Available Date | Jul 23, 2024 |
Journal | The Astronomical Journal |
Print ISSN | 0004-6256 |
Electronic ISSN | 1538-3881 |
Publisher | IOP Publishing |
Peer Reviewed | Peer Reviewed |
Volume | 168 |
Issue | 2 |
Article Number | 69 |
DOI | https://doi.org/10.3847/1538-3881/ad543f |
Keywords | Companion galaxies, Low surface brightness galaxies, Dwarf galaxies, Galaxy stellar halos |
Public URL | https://nottingham-repository.worktribe.com/output/37301479 |
Publisher URL | https://iopscience.iop.org/article/10.3847/1538-3881/ad543f |
Additional Information | Article Title: LIGHTS. Survey Overview and a Search for Low Surface Brightness Satellite Galaxies; Journal Title: The Astronomical Journal; Article Type: paper; Copyright Information: © 2024. The Author(s). Published by the American Astronomical Society.; Date Received: 2024-02-29; Date Accepted: 2024-06-03; Online publication date: 2024-07-11 |
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Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
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