Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions

Brough, S.; Ahad, S.L.; Bahé, Y.M.; Ellien, A.; Gonzalez, A.H.; Jiménez-Teja, Y.; Kimmig, L.C.; Martin, G.; Martínez-Lombilla, C.; Montes, M.; Pillepich, A.; Ragusa, R.; Remus, R.-S.; Collins, C.A.; Knapen, J.H.; Mihos, J.C.

doi:10.1093/mnras/stad3810

Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions

Author(s):: Brough, S.; Ahad, S.L.; Bahé, Y.M.; Ellien, A.; Gonzalez, A.H.; Jiménez-Teja, Y.; Kimmig, L.C.; Martin, G.; Martínez-Lombilla, C.; Montes, M.; Pillepich, A.; Ragusa, R.; Remus, R.-S.; Collins, C.A.; Knapen, J.H.; Mihos, J.C.

Published: 2023
Publication type: Article / Letter to editor

Galaxies: clusters: generalGalaxies: haloesGalaxies: evolutionGalaxies: photometryAstrophysics - Cosmology and nongalactic astrophysicsAstrophysics - Astrophysics of galaxies

Date issued: 2023
Language: English
Is part of: Monthly Notices of the Royal Astronomical Society (2023), Vol. 528, no. 1, p. 771–795
hdl: 1887/3718812
doi: 10.1093/mnras/stad3810
URL: https://ui.adsabs.harvard.edu/abs/2023MNRAS.tmp.3670B

Preparing for low surface brightness science with the Vera C. Rubin Observatory: a comparison of observable and simulated intracluster light fractions

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