Search Results - "Sesana, A."
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Systematic investigation of the expected gravitational wave signal from supermassive black hole binaries in the pulsar timing band
Published in Monthly notices of the Royal Astronomical Society. Letters (21-07-2013)“…In this Letter, we carry out the first systematic investigation of the expected gravitational wave (GW) background generated by supermassive black hole (SMBH)…”
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Massive black hole binary systems and the NANOGrav 12.5 yr results
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2021)“…ABSTRACT The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) recently reported evidence for the presence of a common stochastic signal…”
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LINKING THE SPIN EVOLUTION OF MASSIVE BLACK HOLES TO GALAXY KINEMATICS
Published in The Astrophysical journal (20-10-2014)“…We present the results of a semianalytical model that evolves the masses and spins of massive black holes together with the properties of their host galaxies…”
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Gas-driven massive black hole binaries: signatures in the nHz gravitational wave background
Published in Monthly notices of the Royal Astronomical Society (01-03-2011)“…Pulsar timing arrays (PTAs) measure nHz frequency gravitational waves (GWs) generated by orbiting massive black hole binaries (MBHBs) with periods between 0.1…”
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Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays
Published in Monthly notices of the Royal Astronomical Society (21-04-2009)“…Massive black holes are key components of the assembly and evolution of cosmic structures, and a number of surveys are currently on going or planned to probe…”
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The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays
Published in Monthly notices of the Royal Astronomical Society (11-10-2008)“…Massive black hole binary systems, with masses in the range ∼104–1010M⊙, are among the primary sources of gravitational waves in the frequency window ∼10−9–0.1…”
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Limiting eccentricity of subparsec massive black hole binaries surrounded by self-gravitating gas discs
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…We study the dynamics of supermassive black hole binaries embedded in circumbinary gaseous discs, with the smoothed particle hydrodynamics code gadget-2. The…”
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European Pulsar Timing Array limits on continuous gravitational waves from individual supermassive black hole binaries
Published in Monthly notices of the Royal Astronomical Society (11-01-2016)“…We have searched for continuous gravitational wave (CGW) signals produced by individually resolvable, circular supermassive black hole binaries (SMBHBs) in the…”
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Eccentricity evolution of PTA sources from cosmological initial conditions
Published in Monthly notices of the Royal Astronomical Society (01-07-2024)“…ABSTRACT Recent results from pulsar timing arrays (PTAs) show evidence for a gravitational wave background (GWB) consistent with a population of unresolved…”
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Cosmography with strong lensing of LISA gravitational wave sources
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…Laser Interferometer Space Antenna (LISA) might detect gravitational waves from mergers of massive black hole binaries strongly lensed by intervening galaxies…”
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Gravitational-Wave Physics and Astronomy in the 2020s and 2030s
Published in Nature reviews physics (14-04-2021)“…The 100 years since the publication of Albert Einstein’s theory of General Relativity saw significant development of the understanding of the theory, the…”
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High-precision timing of 42 millisecond pulsars with the European Pulsar Timing Array
Published in Monthly notices of the Royal Astronomical Society (21-05-2016)“…We report on the high-precision timing of 42 radio millisecond pulsars (MSPs) observed by the European Pulsar Timing Array (EPTA). This EPTA Data Release 1.0…”
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Predicting the hypervelocity star population in Gaia
Published in Monthly notices of the Royal Astronomical Society (01-06-2018)Get full text
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Multimessenger astronomy with pulsar timing and X-ray observations of massive black hole binaries
Published in Monthly notices of the Royal Astronomical Society (01-02-2012)“…In the decade of the dawn of gravitational wave astronomy, the concept of multimessenger astronomy, combining gravitational wave signals to conventional…”
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Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search
Published in Monthly notices of the Royal Astronomical Society (01-02-2022)“…ABSTRACT The European Pulsar Timing Array (EPTA) collaboration has recently released an extended data set for six pulsars (DR2) and reported evidence for a…”
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The imprint of massive black hole formation models on the LISA data stream
Published in Monthly notices of the Royal Astronomical Society (01-06-2007)“…The formation, merging and accretion history of massive black holes (MBHs) along the hierarchical build-up of cosmic structures leaves a unique imprint on the…”
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Gas-driven massive black hole binaries: signatures in the nHz gravitational wave background
Published in Monthly notices of the Royal Astronomical Society (01-03-2011)Get full text
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Strong lensing of gravitational waves as seen by LISA
Published in Physical review letters (17-12-2010)“…We discuss strong gravitational lensing of gravitational waves from the merging of massive black hole binaries in the context of the LISA mission. Detection of…”
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Massive Black Hole Binaries : Dynamical Evolution and Observational Signatures
Published in Advances in astronomy (01-01-2012)“…The study of the dynamical evolution of massive black hole pairs in mergers is crucial in the context of a hierarchical galaxy formation scenario. The…”
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Chasing supermassive black hole merging events with Athena and LISA
Published in Monthly notices of the Royal Astronomical Society (01-05-2023)“…ABSTRACT The European Space Agency is studying two large-class missions bound to operate in the decade of the 30s, and aiming at investigating the most…”
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