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Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
by
Cheng, T.-Y
, Hinton, S. R
, Wiseman, P
, Frieman, J
, Palmese, A
, García-Bellido, J
, Miquel, R
, Pace, A. B
, Vincenzi, M
, Schubnell, M
, Andrade-Oliveira, F
, Tarle, G
, Strigari, L. E
, Weaverdyck, N
, Gruen, D
, Kuehn, K
, Bacon, D
, Santiago, B
, Plazas Malagón, A. A
, Mena-Fernández, J
, Suchyta, E
, Alves, O
, Honscheid, K
, Sanchez, E
, Carretero, J
, Bhattacharyya, J
, Swanson, M. E. C
, Walker, A. R
, Gruendl, R. A
, Hollowood, D. L
, Roberts, D
, Peter, A. H. G
, Brooks, D
, da Costa, L. N
, Doel, P
, Tanoglidis, D
, Pereira, M. E. S
, Giannini, G
, Carnero Rosell, A
, Smith, M
, Mutlu-Pakdil, B
, James, D. J
, Marshall, J. L
, Ferrero, I
, Martini, P
, Desai, S
, Aguena, M
, Sevilla-Noarbe, I
, Pieres, A
, Davis, T. M
, Drlica-Wagner, A
in
Astronomy
/ Astrophysics
/ Clusters
/ Collaboration
/ Color
/ Cosmology
/ Dark energy
/ Density
/ Galaxies
/ Magellanic clouds
/ Milky Way
/ Observatories
/ Particle physics
/ Preprocessing
/ Quenching
/ Satellites
/ Sky surveys (astronomy)
/ Star & galaxy formation
/ Stars & galaxies
/ Surface brightness
2024
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Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
by
Cheng, T.-Y
, Hinton, S. R
, Wiseman, P
, Frieman, J
, Palmese, A
, García-Bellido, J
, Miquel, R
, Pace, A. B
, Vincenzi, M
, Schubnell, M
, Andrade-Oliveira, F
, Tarle, G
, Strigari, L. E
, Weaverdyck, N
, Gruen, D
, Kuehn, K
, Bacon, D
, Santiago, B
, Plazas Malagón, A. A
, Mena-Fernández, J
, Suchyta, E
, Alves, O
, Honscheid, K
, Sanchez, E
, Carretero, J
, Bhattacharyya, J
, Swanson, M. E. C
, Walker, A. R
, Gruendl, R. A
, Hollowood, D. L
, Roberts, D
, Peter, A. H. G
, Brooks, D
, da Costa, L. N
, Doel, P
, Tanoglidis, D
, Pereira, M. E. S
, Giannini, G
, Carnero Rosell, A
, Smith, M
, Mutlu-Pakdil, B
, James, D. J
, Marshall, J. L
, Ferrero, I
, Martini, P
, Desai, S
, Aguena, M
, Sevilla-Noarbe, I
, Pieres, A
, Davis, T. M
, Drlica-Wagner, A
in
Astronomy
/ Astrophysics
/ Clusters
/ Collaboration
/ Color
/ Cosmology
/ Dark energy
/ Density
/ Galaxies
/ Magellanic clouds
/ Milky Way
/ Observatories
/ Particle physics
/ Preprocessing
/ Quenching
/ Satellites
/ Sky surveys (astronomy)
/ Star & galaxy formation
/ Stars & galaxies
/ Surface brightness
2024
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Do you wish to request the book?
Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
by
Cheng, T.-Y
, Hinton, S. R
, Wiseman, P
, Frieman, J
, Palmese, A
, García-Bellido, J
, Miquel, R
, Pace, A. B
, Vincenzi, M
, Schubnell, M
, Andrade-Oliveira, F
, Tarle, G
, Strigari, L. E
, Weaverdyck, N
, Gruen, D
, Kuehn, K
, Bacon, D
, Santiago, B
, Plazas Malagón, A. A
, Mena-Fernández, J
, Suchyta, E
, Alves, O
, Honscheid, K
, Sanchez, E
, Carretero, J
, Bhattacharyya, J
, Swanson, M. E. C
, Walker, A. R
, Gruendl, R. A
, Hollowood, D. L
, Roberts, D
, Peter, A. H. G
, Brooks, D
, da Costa, L. N
, Doel, P
, Tanoglidis, D
, Pereira, M. E. S
, Giannini, G
, Carnero Rosell, A
, Smith, M
, Mutlu-Pakdil, B
, James, D. J
, Marshall, J. L
, Ferrero, I
, Martini, P
, Desai, S
, Aguena, M
, Sevilla-Noarbe, I
, Pieres, A
, Davis, T. M
, Drlica-Wagner, A
in
Astronomy
/ Astrophysics
/ Clusters
/ Collaboration
/ Color
/ Cosmology
/ Dark energy
/ Density
/ Galaxies
/ Magellanic clouds
/ Milky Way
/ Observatories
/ Particle physics
/ Preprocessing
/ Quenching
/ Satellites
/ Sky surveys (astronomy)
/ Star & galaxy formation
/ Stars & galaxies
/ Surface brightness
2024
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Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
Journal Article
Environmental Quenching of Low-surface-brightness Galaxies Near Hosts from Large Magellanic Cloud to Milky Way Mass Scales
2024
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Overview
Low-surface-brightness galaxies (LSBGs) are excellent probes of quenching and other environmental processes near massive galaxies. We study an extensive sample of LSBGs near massive hosts in the local universe that are distributed across a diverse range of environments. The LSBGs with surface-brightness μeff,g>24.2magarcsec−2 are drawn from the Dark Energy Survey Year 3 catalog while the hosts with masses 9.0
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