Tiziana Di Matteo
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Tiziana Di Matteophysics Degrees
Physics
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#11766
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Cosmology
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Astrophysics
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Physics
Tiziana Di Matteo's Degrees
- PhD Physics University of Padua
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(Suggest an Edit or Addition)Tiziana Di Matteo's Published Works
Published Works
- A Unified, Merger-driven Model of the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes, and Galaxy Spheroids (2005) (1369)
- Black Holes in Galaxy Mergers: The Formation of Red Elliptical Galaxies (2004) (615)
- Black Holes in Galaxy Mergers: Evolution of Quasars (2005) (477)
- Direct Cosmological Simulations of the Growth of Black Holes and Galaxies (2007) (421)
- A Merger-driven Scenario for Cosmological Disk Galaxy Formation (2005) (420)
- A Physical Model for the Origin of Quasar Lifetimes (2005) (309)
- The Kinematic Structure of Merger Remnants (2006) (308)
- Formation of z~6 Quasars from Hierarchical Galaxy Mergers (2006) (259)
- Accretion onto the Supermassive Black Hole in M87 (2002) (256)
- Neutrino Trapping and Accretion Models for Gamma-Ray Bursts (2002) (256)
- COLD FLOWS AND THE FIRST QUASARS (2011) (197)
- Radio Foregrounds for the 21 Centimeter Tomography of the Neutral Intergalactic Medium at High Redshifts (2001) (176)
- THE FUNDAMENTAL PLANE OF ACCRETION ONTO BLACK HOLES WITH DYNAMICAL MASSES (2009) (159)
- THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY: THE QUASAR LUMINOSITY FUNCTION FROM DATA RELEASE NINE (2012) (147)
- Luminosity-dependent Quasar Lifetimes: A New Interpretation of the Quasar Luminosity Function (2005) (121)
- Possible Evidence for Truncated Thin Disks in the Low-Luminosity Active Galactic Nuclei M81 and NGC 4579 (1999) (118)
- How Rapidly Do Supermassive Black Hole “Seeds” Grow at Early Times? (2007) (107)
- Resolving the Composite Fe Kα Emission Line in the Galactic Black Hole Cygnus X-1 with Chandra (2002) (95)
- Low-Luminosity States of the Black Hole Candidate GX 339–4. I. ASCA and Simultaneous Radio/RXTE Observations (1999) (94)
- The Evolution in the Faint-End Slope of the Quasar Luminosity Function (2005) (85)
- Hydrodynamic Simulation of the Cosmological X-Ray Background (2000) (84)
- The Role of Galactic Winds on Molecular Gas Emission from Galaxy Mergers (2007) (78)
- Instabilities in the Time-Dependent Neutrino Disk in Gamma-Ray Bursts (2007) (76)
- Luminosity-dependent Quasar Lifetimes: Reconciling the Optical and X-Ray Quasar Luminosity Functions (2005) (70)
- Accretion onto Nearby Supermassive Black Holes: Chandra Constraints on the Dominant Cluster Galaxy NGC 6166 (2000) (59)
- Limits on the Accretion Rates onto Massive Black Holes in Nearby Galaxies (2000) (45)
- The Nature of CO Emission from z ∼ 6 Quasars (2007) (40)
- Quasi-Periodic Variability and the Inner Radii of Thin Accretion Disks in Galactic Black Hole Systems (1999) (39)
- Feedback-driven Evolution of the Far-Infrared Spectral Energy Distributions of Luminous and Ultraluminous Infrared Galaxies (2006) (35)
- Angular Anisotropies in the Cosmic Gamma-Ray Background as a Probe of Its Origin (2007) (29)
- Iron Kα Emission from the Low-Luminosity Active Galaxies M81 and NGC 4579 (2004) (25)
- A CHANDRA SURVEY OF SUPERMASSIVE BLACK HOLES WITH DYNAMICAL MASS MEASUREMENTS (2012) (22)
- The Cosmological Evolution of Metal Enrichment in Quasar Host Galaxies (2003) (20)
- GROWTH OF EARLY SUPERMASSIVE BLACK HOLES AND THE HIGH-REDSHIFT EDDINGTON RATIO DISTRIBUTION (2012) (19)
- TERAPIXEL IMAGING OF COSMOLOGICAL SIMULATIONS (2011) (13)
- Synchrotron Emission from Hot Accretion Flows and the Cosmic Microwave Background Anisotropy (2000) (9)
- Vortex dynamics and pinning properties analysis of MgB2 bulk samples by ac susceptibility measurements (2002) (9)
- Hard X-Ray Emission from Elliptical Galaxies and Its Contribution to the X-Ray Background (1999) (7)
- Massive black hole mergers with orbital information: predictions from the ASTRID simulation (2021) (4)
- X-Ray Images of Hot Accretion Flows (2001) (0)
- Ultramassive Black Holes Formed by Triple Quasar Mergers at z ∼ 2 (2022) (0)
- Stress transmission in granular matter (2002) (0)
- A close quasar pair in a disk–disk galaxy merger at z = 2.17 (2022) (0)
- Orbital and Radiative Properties of Wandering Intermediate-Mass Black Holes in the ASTRID Simulation (2022) (0)
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