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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

Dennis Zaritsky

Giulia Golini

Richard Donnerstein

Ignacio Trujillo

Mohammad Akhlaghi

Nushkia Chamba

Mauro D’Onofrio

Sepideh Eskandarlou

S. Zahra Hosseini-ShahiSavandi

Raúl Infante-Sainz

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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Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/

Copyright Statement
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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