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Alberto Sesana

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Associate Professor

University of Milano-Bicocca

Italy

Research Interests

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Grant: Close

Gravitational Wave Detection with Pulsar Timing Arrays

Open Date: 2015-01-01

Close Date: 2019-12-01

Articles (34)

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Collaborators (19)

Tamara Bogdanovic

Professor

Georgia Institute of Technology

UNITED STATES

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Alessia Franchini

Assistant Professor

University of Milano-Bicocca

ITALY

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Nils Hoyer

Max-Planck-Institut für Astronomie

GERMANY

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Hannah Middleton

University of Birmingham

UNITED KINGDOM

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Riccardo Buscicchio

Assistant professor

Gran Sasso Science Institute

ITALY

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Melanie Habouzit

Assistant Professor / Group Leader

University of Geneva

SWITZERLAND

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Astrid Lamberts

Université Côte d'Azur

FRANCE

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alberto vecchio

Professor of Astrophysics

University of Birmingham

UNITED KINGDOM

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Walter Dehnen

GERMANY

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Alexandre Toubiana

University of Milano-Bicocca

ITALY

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Justin I Read

Chair of Astrophysics, Early Career Researcher Lead

University of Surrey

UNITED KINGDOM

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Volker Springel

Max-Planck-Institut für Astronomie

GERMANY

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David Champion

Max-Planck-Institut für Radioastronomie

GERMANY

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Giulia Fumagalli

California Institute of Technology

UNITED STATES

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Taeho Ryu

Assistant Professor

University of Colorado Boulder

UNITED STATES

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Boris Goncharov

Senior Scientist

Max Planck Institute for Gravitational Physics

GERMANY

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Roberto Serafinelli

Istituto Nazionale di Astrofisica

ITALY

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Rosa Valiante

Sapienza University of Rome

ITALY

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Alessandro Lupi

Associate Professor

Università degli Studi dell'Insubria - Sede di Como

ITALY

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Alberto Sesana

Research Interests

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Recent Grants

Articles (34)

Constraints on the early growth of massive black holes from the PTA and JWST with L-GalaxiesBH

Assessing the performance of future space-based detectors: Astrophysical foregrounds and individual sources

Dissecting the nanohertz gravitational wave sky: Frequency-correlated anisotropy induced by eccentric supermassive black hole binaries

Data span and frequency coverage requirements for robust detection and inference in pulsar timing arrays

Identifying massive black hole binaries via light curve variability in optical time-domain surveys

The role of radiation pressure in accreting massive black hole binaries

Eccentricity distribution of extreme mass ratio inspirals

Lighting up the nanohertz gravitational wave sky: Opportunities and challenges of multimessenger astronomy with pulsar timing array experiments

The impact of outliers on pulsar timing array signals

Realistic consecutive galaxy mergers form eccentric pulsar timing array sources

Reading signatures of supermassive binary black holes in pulsar timing array observations

Off-centre black hole seed formation: Implications for high- and low-redshift massive black holes

Updated predictions for gravitational wave emission from tidal disruption events for next-generation observatories

Variability in the supermassive black hole binary candidate SDSS J2320+0024: No evidence of periodic modulation

Test for LISA foreground Gaussianity and stationarity: Extreme mass-ratio inspirals

Cyclostationary signals in LISA: A practical application to Milky Way satellites

Hanging on the cliff: Extreme mass ratio inspiral formation with local two-body relaxation and post-Newtonian dynamics

Impact of the observation frequency coverage on the significance of a gravitational wave background detection in pulsar timing array data

Separating deterministic and stochastic gravitational wave signals in realistic pulsar timing array datasets

Demographics of tidal disruption events with L-Galaxies

The behaviour of eccentric sub-pc massive black hole binaries embedded in massive discs

Neural networks unveiling the properties of gravitational wave background from supermassive black hole binaries

Repeating partial disruptions and two-body relaxation

Connecting low-redshift LISA massive black hole mergers to the nHz stochastic gravitational wave background

Emission signatures from sub-parsec post-Newtonian binaries embedded in circumbinary discs

Mass-redshift dependency of supermassive black hole binaries for the gravitational wave background

Testing strengths, limitations, and biases of current pulsar timing arrays’ detection analyses on realistic data

Correction to: Massive black hole binary systems and the NANOGrav 12.5 yr results

Resolving Massive Black Hole Binary Evolution via Adaptive Particle Splitting

Observing GW190521-like binary black holes and their environment with LISA

The Competing Effect of Gas and Stars in the Evolution of Massive Black Hole Binaries

Unveiling the gravitational universe at μ-Hz frequencies

Unveiling Sub-Pc supermassive black hole binary candidates in active galactic nuclei

Pulsar Timing Array Constraints on the Merger Timescale of Subparsec Supermassive Black Hole Binary Candidates

Collaborators (19)

Tamara Bogdanovic

Alessia Franchini

Nils Hoyer

Hannah Middleton

Riccardo Buscicchio

Melanie Habouzit

Astrid Lamberts

alberto vecchio

Walter Dehnen

Alexandre Toubiana

Justin I Read

Volker Springel

David Champion

Giulia Fumagalli

Taeho Ryu

Boris Goncharov

Roberto Serafinelli

Rosa Valiante

Alessandro Lupi

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