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20112019
most citedSelection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation

263 citations · 1.2k across the 19 of their papers we have counts for

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Showing 2016Show all

5 papers · 1 filter

astro-ph.GA2016★ 57 cited

The SLUGGS Survey: stellar masses and effective radii of early-type galaxies from Spitzer Space Telescope 3.6m imaging

Duncan A. Forbes, Luciana Sinpetru, Giulia Savorgnan +3

Galaxy starlight at 3.6m is an excellent tracer of stellar mass. Here we use the latest 3.6m imaging from the Spitzer Space Telescope to measure the total stellar mass and ef…

astro-ph.GA2016★ 29 cited

Disky elliptical galaxies and the allegedly over-massive black hole in the compact massive `ES' galaxy NGC 1271

Alister W. Graham, Bogdan C. Ciambur, Giulia A. D. Savorgnan

While spiral and lenticular galaxies have large-scale disks extending beyond their bulges, and most local early-type galaxies with 10^{10} < M_*/M_Sun < 2x10^{11} contain a disk (e…

astro-ph.GA2016★ 19 cited

Supermassive black holes and their host spheroids III. The correlation

Giulia A. D. Savorgnan

The Sérsic model is the best approximation known to date for describing the light distribution of stellar spheroidal and disk components, with the Sérsic index provid…

astro-ph.GA2016★ 263 cited

Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation

Francesco Shankar, Mariangela Bernardi, Ravi K. Sheth +7

We compare the set of local galaxies having dynamically measured black holes with a large, unbiased sample of galaxies extracted from the Sloan Digital Sky Survey. We confirm earli…

astro-ph.GA2016★ 40 cited

A normal supermassive black hole in NGC 1277

Alister W. Graham, Mark Durré, Giulia A. D. Savorgnan +5

The identification of galaxies with `overly massive' black holes requires two measurements: a black hole mass (M_bh) and a host spheroid mass (M_sph,*). Here we provide our measure…