The inner halo of M 87: a first direct view of the red-giant population
A&A, 524 (2010) A71
Published online: 2010-11-24
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The limb-brightened jet of M87 down to the 7 Schwarzschild radii scale
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The Carnegie–Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch∗
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Resolving the Discrepancy of Distance to M60, a Giant Elliptical Galaxy in Virgo
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Resolving the Base of the Relativistic Jet in M87 at 6Rsch Resolution with Global mm-VLBI
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The Planetary Nebulae Luminosity Function (PNLF): current perspectives
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Ubiquitous time variability of integrated stellar populations
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Probing the spacetime around supermassive black holes with ejected plasma blobs
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Tracing the stellar halo of an early type galaxy out to 25 effective radii
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Resolved Stellar Halos of M87 and NGC 5128: Metallicities from the Red-Giant Branch
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MUSE tells the story of NGC 4371: The dawning of secular evolution
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