GS
Giulia A. D. Savorgnan
astro-ph.GAastro-ph.CO
On Valency
published · living versionsW_sf7n2jaa·v1 · currentpublished
A normal supermassive black hole in NGC 1277
with Alister W. Graham, Mark Durré, Anne M. Medling, D. Batcheldor +3
1 version
Preprints & journals
18 papers in the corpus · 2011–2019Angular momentum of galaxies and their local analogues with adaptive optics1903.04746v1 · Sarah M. Sweet, Deanne B. Fisher, Giulia Savorgnan et al.2019 · 18 citationsarXiv
The UVES Spectral Quasar Absorption Database (SQUAD) Data Release 1: The first 10 million seconds1810.06136v1 · Michael T. Murphy, Glenn G. Kacprzak, Giulia A. D. Savorgnan et al.2018 · 100 citationsarXiv
The SLUGGS Survey: stellar masses and effective radii of early-type galaxies from Spitzer Space Telescope 3.6m imaging1610.02037v1 · Duncan A. Forbes, Luciana Sinpetru, Giulia Savorgnan et al.2016 · 56 citationsarXiv
Disky elliptical galaxies and the allegedly over-massive black hole in the compact massive `ES' galaxy NGC 12711608.00711v2 · Alister W. Graham, Bogdan C. Ciambur, Giulia A. D. Savorgnan2016 · 30 citationsarXiv
Supermassive black holes and their host spheroids III. The correlation1603.01910v1 · Giulia A. D. Savorgnan2016 · 20 citationsarXiv
Selection bias in dynamically-measured super-massive black hole samples: its consequences and the quest for the most fundamental relation1603.01276v2 · Francesco Shankar, Mariangela Bernardi, Ravi K. Sheth et al.2016 · 263 citationsMNRAS 460, 3119, 2016
A normal supermassive black hole in NGC 12771601.05151v2 · Alister W. Graham, Mark Durr'e, Giulia A. D. Savorgnan et al.2016 · 39 citationsarXivon Valency
Supermassive black holes and their host spheroids I. Disassembling galaxies1511.07446v2 · Giulia A. D. Savorgnan, Alister W. Graham2015 · 69 citations2016, ApJS, 222, 10
Explaining the reportedly over-massive black holes in early-type galaxies with intermediate-scale discs1511.05654v2 · Giulia A. D. Savorgnan, Alister W. Graham2015 · 46 citationsarXiv
The role of bars in quenching star formation from z = 3 to the present epoch. Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA, VI1505.07836v2 · G. Gavazzi, G. Consolandi, M. Dotti et al.2015 · 153 citationsarXiv
Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. V: The Coma Supercluster survey completion1505.07423v1 · Giuseppe Gavazzi, Guido Consolandi, Elisa Viscardi et al.2015 · 20 citations2015 Astronomy & Astrophysics, Volume 576, id.A16, 41 pp
Hiding in plain sight: An abundance of compact massive spheroids in the local Universe1502.07024v2 · Alister W. Graham, Bililign T. Dullo, Giulia A. D. Savorgnan2015 · 84 citationsarXiv
Overmassive black holes in the diagram do not belong to over (dry) merged galaxies1410.7405v1 · Giulia A. D. Savorgnan, Alister W. Graham2014 · 53 citationsarXiv
Red-channel (6000-8000 Å) nuclear spectra of 376 local galaxies1308.1400v2 · Giuseppe Gavazzi, Guido Consolandi, Massimo Dotti et al.2013 · 21 citationsarXiv
The supermassive black hole mass - Sérsic index relations for bulges and elliptical galaxies1306.2679v1 · Giulia Savorgnan, Alister W. Graham, Alessandro Marconi et al.2013 · 49 citationsarXiv
Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. III. Nurture shapes up the Hubble sequence in the Great Wall1303.2374v2 · Giuseppe Gavazzi, Giulia Savorgnan, Matteo Fossati et al.2013 · 31 citationsarXiv
Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. IV. Structure of galaxies in the Local and Coma Superclusters1303.0840v2 · Matteo Fossati, Giuseppe Gavazzi, Giulia Savorgnan et al.2013 · 62 citationsarXiv
The complete census of optically selected AGNs in the Coma Supercluster: the dependence of AGN activity on the local environment1107.3702v3 · Giuseppe Gavazzi, Giulia Savorgnan, Mattia Fumagalli2011 · 47 citationsarXiv
Career total: 48 works. 18 are in this corpus.
Profile built from the corpus for this byline.
Author records are still filling in while the Hub is in alpha. If this is your page, you'll be able to claim it soon. Spot a mistake? Tell us.