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Table 2.

Crossmatch results of HQ UDG candidates with nearby clusters/groups.

Cluster/Group RA Dec Redshift Dist (Mpc) N UDG ( tot ) Mathematical equation: $ N_\mathrm{{UDG}}(\rm{tot}) $ NUDG (new) NUDG matched/total (reference)
With previous literature

Fornax 54.621 −35.450 0.0048 20.8 5 3 1+1/12+1 (Venhola et al. 2017)
NGC 5846 226.622 1.605 0.0062 26.8 5 2 3/7 (Marleau et al. 2021)*
NGC 5576 215.265 3.271 0.0051 22.5 4 2 2/2 (Marleau et al. 2021)
NGC 4690 191.981 −1.656 0.0092 40.1 5 3 2/3 (this work vs. Zaritsky et al. 2023)**
NGC 4073 181.112 1.895 0.020 87.5 15 10 5/12 (this work vs. Zaritsky et al. 2023)
IC 1860 42.391 −31.189 0.022 96.5 2 0 2/8 (this work vs. Zaritsky et al. 2023 )
NGC 0439 18.447 −31.747 0.019 83.1 5 4 1/9 (this work vs. Zaritsky et al. 2023)
NGC 4636 190.707 2.687 0.004 17.5 4 3 1/3 (this work vs. Zaritsky et al. 2023)
UGC 07813 189.755 0.366 0.023 100.8 4 1 3/7 (this work vs. Zaritsky et al. 2023)

Without previous literature

IC 5157 330.862 −34.941 0.0147 64.1 4 4
IC 5358 356.938 −28.141 0.028 123.0 2 2
NGC 7176 330.535 −31.990 0.0084 36.4 6 6
NGC 7507 348.031 −28.539 0.0053 22.9 2 2
ESO466-021 329.479 −28.805 0.023 100.8 1 1
2MASS J2259-3334 344.755 −33.572 0.028 123.0 3 3

Notes. *One of the MATLAS UDGs was earlier discovered by Forbes et al. (2019). **Associations are produced in this work based on the catalog of Zaritsky et al. (2023).

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