The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to similar to 10(6)L(circle dot) and Comparisons with Galaxy Formation Models

We use deep optical photometry from the Next Generation Virgo Cluster Survey (NGVS) to investigate the colormagnitude diagram for the galaxies inhabiting the core of this cluster. The sensitivity of the NGVS imaging allows us to continuously probe galaxy colors over a factor of similar to 2 x 105 in luminosity, from brightest cluster galaxies to scales overlapping classical satellites of the Milky Way (M-g' similar to -9; M-*. similar to 10(6)M(circle dot)), within a single environment. Remarkably, we find the first evidence that the red sequence (RS) flattens in all colors at the faint-magnitude end (starting between -14 <= M-g' <= -13, around M-* similar to 4 x 10(7)M(circle dot)), with the slope decreasing to similar to 60% or less of its value at brighter magnitudes. This could indicate that the stellar populations of faint dwarfs in Virgo's core share similar characteristics (e.g., constant mean age) over similar to 3 mag in luminosity, suggesting that these galaxies were quenched coevally, likely via pre-processing in smaller hosts. We also compare our results to galaxy formation models, finding that the RS in model clusters have slopes at intermediate magnitudes that are too shallow, and in the case of semianalytic models, do not reproduce the flattening seen at both extremes (bright/faint) of the Virgo RS. Deficiencies in the chemical evolution of model galaxies likely contribute to the model-data discrepancies at all masses, while overly efficient quenching may also be a factor at dwarf scales. Deep UV and near-IR photometry are required to unambiguously diagnose the cause of the faint-end flattening.National Natural Science Foundation of China [11173003]; National Key Basic Research Program of China [2015CB857002]; NSFC [11673017, 11203017, 11433002]; CORFO project [15COTE-46317]; French Agence Nationale de la Recherche (ANR) [ANR10-BLANC-0506-01]; Institut Universitaire de France (IUF); PRIN INAF "EXCALIBURS: EXtragalactic distance scale CALIBration Using first-Rank Standard candles"; Natural Science and Engineering Research Council of Canada; FONDECYT [1161817]; BASAL Center for Astrophysics and Associated Technologies [PFB-06]; NSF [AST-1010039, AST-1412504]; Canadian Advanced Network for Astronomical Research (CANFAR); CANARIE under the Network-Enabled Platforms programSCI(E)ARTICLE183