Massimo Dotti
Identifiers
- name variant Massimo Dotti 0.60 · backfill
Papers (99)
- Searching for unresolved massive black hole pairs through AGN photometric variability astro-ph.HE · 2026 · author #5
- Identification of periodicities with arbitrary shapes in AGN light curves astro-ph.GA · 2025 · author #6
- Can a time evolving, asymmetric broad line region mimic a massive black hole binary? astro-ph.GA · 2025 · author #6
- ESPRESSO reveals a single but perturbed broad-line region in the supermassive black hole binary candidate PG 1302-102 astro-ph.GA · 2025 · author #4
- Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations astro-ph.GA · 2024 · author #4
- An effective model for the tidal disruption of satellites undergoing minor mergers with axisymmetric primaries astro-ph.GA · 2024 · author #2
- Size matters: are we witnessing super-Eddington accretion in high-redshift black holes from JWST? astro-ph.HE · 2024 · author #4
- A quasar-galaxy merger at $z\sim 6.2$: rapid host growth via accretion of two massive satellite galaxies astro-ph.GA · 2024 · author #4
- Repeating partial disruptions and two-body relaxation astro-ph.HE · 2024 · author #5
- Partial alignment between jets and megamasers: Coherent versus selective accretion astro-ph.GA · 2024 · author #1
- BANG-MaNGA: A census of kinematic discs and bulges across mass and star formation in the local Universe astro-ph.GA · 2024 · author #5
- A quasar-galaxy merger at $z\sim6.2$: black hole mass and quasar properties from the NIRSpec spectrum astro-ph.GA · 2024 · author #17
- Astrophysical and relativistic modeling of the recoiling black-hole candidate in quasar 3C 186 astro-ph.GA · 2024 · author #4
- On the connection between AGN radiative feedback and massive black hole spin astro-ph.GA · 2023 · author #3
- A fast test for the identification and confirmation of massive black hole binaries astro-ph.HE · 2023 · author #1
- The fragility of thin discs in galaxies -- II. Thin discs as tracers of the assembly history of galaxies astro-ph.GA · 2023 · author #4
- Decomposing galaxies with BANG: an automated morpho-kinematical decomposition of the SDSS-DR17 MaNGA survey astro-ph.GA · 2023 · author #2
- Quasi-periodic eruptions from impacts between the secondary and a rigidly precessing accretion disc in an extreme mass-ratio inspiral system astro-ph.HE · 2023 · author #7
- Gravitational waves from an eccentric population of primordial black holes orbiting Sgr A$^{\star}$ astro-ph.GA · 2023 · author #6
- The fragility of thin discs in galaxies -- I. Building tailored N-body galaxy models astro-ph.GA · 2023 · author #4
- Dynamical evolution of massive black hole pairs in the presence of spin-dependent radiative feedback astro-ph.GA · 2022 · author #3
- Morphological decomposition of TNG50 galaxies: methodology and catalogue astro-ph.GA · 2022 · author #4
- Maximally informed Bayesian modelling of disc galaxies astro-ph.GA · 2022 · author #2
- Extreme mass ratio inspirals and tidal disruption events in nuclear clusters. I. Time dependent rates astro-ph.GA · 2022 · author #5
- Optical follow-up of the tick-tock massive black hole binary candidate astro-ph.HE · 2022 · author #1
- Extreme Mass Ratio Inspirals triggered by Massive Black Hole Binaries: from Relativistic Dynamics to Cosmological Rates astro-ph.GA · 2022 · author #5
- Re-weighting dark matter in disc galaxies: a new general relativistic observational test astro-ph.GA · 2022 · author #3
- Disc instability and bar formation: view from the IllustrisTNG simulations astro-ph.GA · 2022 · author #7
- Astrophysics with the Laser Interferometer Space Antenna gr-qc · 2022 · author #38
- On the detectability of gravitational waves from primordial black holes orbiting Sgr A* gr-qc · 2022 · author #5
- Dual AGN in the Horizon-AGN simulation and their link to galaxy and massive black hole mergers, with an excursus on multiple AGN astro-ph.GA · 2021 · author #4
- The evolution of the barred galaxy population in the TNG50 simulation astro-ph.GA · 2021 · author #3
- Circumbinary disc self-gravity governing supermassive black hole binary mergers astro-ph.HE · 2021 · author #3
- Stellar hardening of massive black hole binaries: the impact of the host rotation astro-ph.GA · 2021 · author #3
- Binary black hole signatures in polarized light curves astro-ph.HE · 2021 · author #1
- The role of bars on the dynamical-friction driven inspiral of massive perturbers astro-ph.GA · 2021 · author #3
- Non-isotropic feedback from accreting spinning black holes astro-ph.GA · 2020 · author #5
- Black hole spin evolution in warped accretion discs astro-ph.GA · 2020 · author #5
- Dynamical evolution of massive perturbers in realistic multi-component galaxy models I: implementation and validation astro-ph.GA · 2020 · author #4
- Unveiling sub-parsec supermassive black hole binary candidates in active galactic nuclei astro-ph.HE · 2020 · author #9
- Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations astro-ph.GA · 2020 · author #7
- Global torques and stochasticity as the drivers of massive black hole pairing in the young Universe astro-ph.GA · 2020 · author #6
- Dynamical friction-driven orbital circularisation in rotating discs: a semi-analytical description astro-ph.GA · 2020 · author #4
- From galactic nuclei to the halo outskirts: tracing supermassive black holes across cosmic history and environments astro-ph.GA · 2020 · author #3
- The Quest for Dual and Binary Supermassive Black Holes: A Multi-Messenger View astro-ph.GA · 2020 · author #6
- Real galaxy mergers from galaxy pair catalogs astro-ph.GA · 2020 · author #2
- On the eccentricity evolution of massive black hole binaries in stellar backgrounds astro-ph.GA · 2020 · author #4
- The buildup of strongly barred galaxies in the TNG100 simulation astro-ph.GA · 2019 · author #3
- ALMA and HST kiloparsec-scale imaging of a quasar-galaxy merger at $z\approx 6.2$ astro-ph.GA · 2019 · author #2
- Testing the blast-wave AGN feedback scenario in MCG-03-58-007 astro-ph.GA · 2019 · author #5
- Neutron star binary orbits in their host potential: effect on early r-process enrichment astro-ph.HE · 2019 · author #3
- Multi-Messenger Astrophysics with Pulsar Timing Arrays astro-ph.HE · 2019 · author #10
- The erratic dynamical life of black hole seeds in high-redshift galaxies astro-ph.GA · 2019 · author #4
- Barred galaxies in cosmological zoom-in simulations: the importance of feedback astro-ph.GA · 2018 · author #3
- Black holes, gravitational waves and fundamental physics: a roadmap gr-qc · 2018 · author #94
- On the orientation of Narrow Line Seyfert I astro-ph.GA · 2018 · author #2
- Bar resilience to flybys in a cosmological framework astro-ph.GA · 2018 · author #2
- AGN mass estimates in large spectroscopic surveys: the effect of host galaxy light astro-ph.GA · 2018 · author #4
- $r$-process nucleosynthesis in the early Universe through fast mergers of compact binaries in triple systems astro-ph.HE · 2018 · author #4
- The influence of Massive Black Hole Binaries on the Morphology of Merger Remnants astro-ph.GA · 2017 · author #3
- The birth of a supermassive black hole binary astro-ph.GA · 2017 · author #6
- External versus internal triggers of bar formation in cosmological zoom-in simulations astro-ph.GA · 2017 · author #2
- Bars as seen by Herschel & Sloan astro-ph.GA · 2017 · author #2
- A survey of dual active galactic nuclei in simulations of galaxy mergers: frequency and properties astro-ph.GA · 2016 · author #2
- Shocks and angular momentum flips: a different path to feeding the nuclear regions of merging galaxies astro-ph.GA · 2016 · author #2
- Bar-driven evolution and quenching of spiral galaxies in cosmological simulations astro-ph.GA · 2016 · author #3
- Retrograde binaries of massive black holes in circum-binary accretion discs astro-ph.GA · 2016 · author #3
- Robust automatic photometry of local galaxies from SDSS Dissecting the color magnitude relation with color profiles astro-ph.GA · 2016 · author #4
- Nuclear discs as clocks for the assembly history of early-type galaxies: the case of NGC4458 astro-ph.GA · 2016 · author #5
- Quasi-periodicities at year-like timescales in Blazars astro-ph.GA · 2015 · author #3
- Massive black holes in merging galaxies astro-ph.GA · 2015 · author #3
- Massive black hole and gas dynamics in mergers of galaxy nuclei - II. Black hole sinking in star-forming nuclear discs astro-ph.GA · 2015 · author #3
- Overlapping inflows as catalysts of AGN activity - II: Relative importance of turbulence and inflow-disc interaction astro-ph.GA · 2015 · author #3
- Black hole accretion versus star formation rate: theory confronts observations astro-ph.GA · 2015 · author #5
- Growing black holes and galaxies: black hole accretion versus star formation rate astro-ph.GA · 2015 · author #5
- Linking the fate of massive black hole binaries to the active galactic nuclei luminosity function astro-ph.HE · 2015 · author #1
- Massive black hole and gas dynamics in galaxy nuclei mergers. I. Numerical implementation astro-ph.GA · 2014 · author #3
- New insights on the recoiling/binary black hole candidate J0927+2943 via molecular gas observations astro-ph.GA · 2014 · author #2
- Growth and activity of black holes in galaxy mergers with varying mass ratios astro-ph.GA · 2014 · author #3
- The nature of massive black hole binary candidates: II. Spectral energy distribution atlas astro-ph.GA · 2014 · author #3
- Linking the spin evolution of massive black holes to galaxy kinematics astro-ph.CO · 2014 · author #3
- Super-Critical Growth of Massive Black Holes from Stellar-Mass Seeds astro-ph.CO · 2014 · author #3
- Overlapping Inflow Events as Catalysts for Supermassive Black Hole Growth astro-ph.GA · 2013 · author #3
- Nuclear coups: dynamics of black holes in galaxy mergers astro-ph.CO · 2013 · author #4
- Red-channel (6000-8000 {\AA}) nuclear spectra of 376 local galaxies astro-ph.CO · 2013 · author #3
- The nature of massive black hole binary candidates: I. Spectral properties and evolution astro-ph.CO · 2013 · author #2
- Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. III. Nurture shapes up the Hubble sequence in the Great Wall astro-ph.CO · 2013 · author #4
- Effects Of Circum-nuclear Disk Gas Evolution And The Spin Of Central Black Holes astro-ph.HE · 2012 · author #2
- Evolution of binary black holes in self gravitating discs: dissecting the torques astro-ph.CO · 2012 · author #3
- Gravitational Recoil From Accretion-Aligned Black-Hole Binaries gr-qc · 2012 · author #3
- Observability of Dual Active Galactic Nuclei in Merging Galaxies astro-ph.CO · 2011 · author #4
- Massive black hole binary plane reorientation in rotating stellar systems astro-ph.GA · 2011 · author #2
- Massive black hole binary eccentricity in rotating stellar systems astro-ph.GA · 2011 · author #3
- Limiting eccentricity of sub-parsec massive black hole binaries surrounded by self-gravitating gas discs astro-ph.CO · 2011 · author #2
- Geometry and inclination of the broad line region in blazars astro-ph.CO · 2010 · author #2
- Massive black holes in stellar systems: 'quiescent' accretion and luminosity astro-ph.GA · 2010 · author #2
- The peculiar optical spectrum of 4C+22.25: Imprint of a massive black hole binary? astro-ph.CO · 2010 · author #2
- Gravitational recoil: effects on massive black hole occupation fraction over cosmic time astro-ph.CO · 2010 · author #3
- Double quasars: probes of black hole scaling relationships and merger scenarios astro-ph · 2008 · author #3
Mentions
- 2411.16876 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2504.06331 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2403.18002 #1 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2311.07576 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2406.18652 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2406.06697 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2406.17847 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2403.09812 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2404.05786 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2402.08740 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2402.13319 #17 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2303.12868 #6 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2310.06896 #1 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2305.03762 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2304.00775 #7 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2305.13442 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2302.03349 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2212.08669 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2205.06275 #1 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2204.05343 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2203.05663 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2206.04693 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2112.07193 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2205.06277 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2203.07734 #7 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2205.06819 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2110.04537 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2011.06606 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2011.06596 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2204.05143 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1908.00547 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2103.07486 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2103.14652 #1 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2104.14570 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2106.13253 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2010.08555 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2009.06662 #9 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2005.04902 #7 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2005.02409 #6 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2001.06293 #6 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2001.10548 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2002.04621 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2001.02231 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2001.02461 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1905.12016 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1906.00985 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1906.05308 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1806.05195 #94 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1810.07701 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1902.01297 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1903.07644 #10 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1803.08504 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1805.06459 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1805.03658 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1705.02348 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1801.03506 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1710.04658 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1706.04010 #6 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1611.09244 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1701.00364 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1610.08507 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1607.02141 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1604.01392 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1603.07753 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1601.03292 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1512.04561 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1509.09027 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1509.02920 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1508.00022 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1502.06363 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1502.03101 #1 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1410.0959 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1409.1585 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1409.0004 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1403.4931 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1402.6995 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1308.1400 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1305.4941 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1303.2374 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1203.1877 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1109.3707 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1105.0670 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1502.07076 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1104.3868 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1011.5879 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1011.4311 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1007.3738 #2 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1001.1743 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1402.7088 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1310.7581 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1312.2595 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1202.6063 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1201.1923 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1111.0223 #4 · arxiv_oai · confidence 0.70 Massimo Dotti
- 0812.1569 #3 · arxiv_oai · confidence 0.70 Massimo Dotti
- 2604.00101 #5 · arxiv_oai · confidence 0.70 Massimo Dotti
- 1509.09027 #3 · backfill · confidence 0.70 Massimo Dotti
- 1509.02920 #3 · backfill · confidence 0.70 Massimo Dotti
- 1508.00022 #3 · backfill · confidence 0.70 Massimo Dotti
- 1502.07076 #5 · backfill · confidence 0.70 Massimo Dotti
Frequent Coauthors
- Marta Volonteri 24 shared papers
- Alberto Sesana 22 shared papers
- Alessandro Lupi 22 shared papers
- Matteo Bonetti 20 shared papers
- Pedro R. Capelo 20 shared papers
- Francesco Haardt 18 shared papers
- Lucio Mayer 13 shared papers
- Elisa Bortolas 12 shared papers
- Monica Colpi 12 shared papers
- Roberto Decarli 12 shared papers
- Silvia Bonoli 11 shared papers
- Fabio Rigamonti 9 shared papers
- Tommaso Zana 8 shared papers
- Stefano Covino 7 shared papers
- David Izquierdo-Villalba 6 shared papers
- Hugo Pfister 6 shared papers
- Yetli Rosas-Guevara 6 shared papers
- Alessia Franchini 5 shared papers
- Carmen Montuori 5 shared papers
- Chiara Mazzucchelli 5 shared papers