Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
J. Bhattacharyya,A. H. G. Peter,P. Martini,B. Mutlu-Pakdil,A. Drlica-Wagner,A. B. Pace,L. E. Strigari,T. -y. Cheng, D. Roberts,D. Tanoglidis,M. Aguena,O. Alves,F. Andrade-Oliveira,D. Bacon,D. Brooks,A. Carnero Rosell,J. Carretero,L. N. da Costa,M. E. S. Pereira,T. M. Davis,S. Desai,P. Doel,I. Ferrero,J. Frieman,J. Garcia-Bellido,G. Giannini,D. Gruen,R. A. Gruendl,S. R. Hinton,D. L. Hollowood,K. Honscheid,D. J. James,K. Kuehn,J. L. Marshall,J. Mena-Fernandez,R. Miquel,A. Palmese,A. Pieres,A. A. Plazas Malagon, E. Sanchez,B. Santiago,M. Schubnell,I. Sevilla-Noarbe,M. Smith,E. Suchyta,M. E. C. Swanson,G. Tarle,M. Vincenzi,A. R. Walker,N. Weaverdyck,P. Wiseman ASTROPHYSICAL JOURNAL（2024）
Key words
Galaxy colors,Low surface brightness galaxies,Galaxy quenching,Galaxy evolution
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