Imagen de Portada

The multimessenger view of Pulsar Timing Array black holes with the Horizon-AGN simulation

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Leclere, Hippolyte Quelquejay, Li, Kunyang, Volonteri, Marta, Babak, Stanislav, Beckmann, Ricarda S., Dubois, Yohan, Laigle, Clotilde, Webb, Natalie A.
Formato:	Preprint
Publicado:	2025
Materias:	Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Probing Supermassive Black Hole Mergers with Pulsar Timing Arrays
por: Leclere, Hippolyte Quelquejay
Publicado: (2026)

Tracking on-the-fly massive black hole binary evolution and coalescence in galaxy simulations: RAMCOAL
por: Li, Kunyang, et al.
Publicado: (2024)

Wandering and escaping: recoiling massive black holes in cosmological simulations
por: Dong-Páez, Chi An, et al.
Publicado: (2024)

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN
por: Leonova, Ecaterina, et al.
Publicado: (2026)

From eccentric binaries to nonstationary gravitational wave backgrounds
por: Falxa, Mikel, et al.
Publicado: (2024)

Statistics of the projected angles between the black-hole spin and the host-galaxy rotation axes from NewHorizon
por: Peirani, Sebastien, et al.
Publicado: (2025)

Supermassive black hole growth in hierarchically merging nuclear star clusters
por: Kritos, Konstantinos, et al.
Publicado: (2024)

Black hole spin evolution across cosmic time from the NewHorizon simulation
por: Beckmann, Ricarda S., et al.
Publicado: (2024)

Cosmic evolution of black hole-spin and galaxy orientations: clues from the NewHorizon and Galactica simulations
por: Peirani, Sebastien, et al.
Publicado: (2024)

Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
por: Toubiana, A., et al.
Publicado: (2024)

Massive black holes and their galaxies
por: Beckmann, Ricarda S., et al.
Publicado: (2026)

Effective-one-body modelling of eccentric supermassive black hole binaries for Pulsar Timing Array
por: Manzini, Sara, et al.
Publicado: (2025)

Distinguish dark matter theories with the cosmic web and next-generation surveys I: an alternative theory of gravity
por: Boldrini, Pierre, et al.
Publicado: (2024)

The impact of superradiance on the spin evolution of variably accreting massive black holes
por: Nandakumar, Adithya, et al.
Publicado: (2025)

Assembly of the Intracluster Light in the Horizon-AGN Simulation
por: Brown, Harley J., et al.
Publicado: (2024)

Large-scale dual AGN in large-scale cosmological hydrodynamical simulations
por: Puerto-Sánchez, Clara, et al.
Publicado: (2024)

How complex are galaxies? A non-parametric estimation of the intrinsic dimensionality of wide-band photometric data
por: Cadiou, Corentin, et al.
Publicado: (2024)

Forecasting the sensitivity of Pulsar Timing Arrays to gravitational wave backgrounds
por: Babak, Stanislav, et al.
Publicado: (2024)

A catalogue of candidate milli-parsec separation massive black hole binaries from long term optical photometric monitoring
por: Foustoul, Vincent, et al.
Publicado: (2025)

Primordial gravitational wave backgrounds from phase transitions with next generation ground based detectors
por: Caprini, Chiara, et al.
Publicado: (2024)

Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations
por: Dubois, Yohan, et al.
Publicado: (2024)

Star-Gas Misalignment in Galaxies: II. Origins Found from the Horizon-AGN Simulation
por: Khim, Donghyeon J., et al.
Publicado: (2020)

Probing supermassive black hole scalarization with Pulsar Timing Arrays
por: Smarra, Clemente, et al.
Publicado: (2025)

Star-gas misalignment in galaxies: I. The properties of galaxies from the Horizon-AGN simulation and comparisons to SAMI
por: Khim, Donghyeon J., et al.
Publicado: (2019)

The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe
por: Antoniadis, J., et al.
Publicado: (2023)

Off-center black hole seed formation? Implications for high and low redshift massive black holes
por: Izquierdo-Villalba, David, et al.
Publicado: (2025)

Hydrodynamic simulations of black hole evolution in AGN discs I: orbital alignment of highly inclined satellites
por: Rowan, Connar, et al.
Publicado: (2025)

Hydrodynamic simulations of black hole evolution in AGN discs II: inclination damping for partially embedded satellites
por: Whitehead, Henry, et al.
Publicado: (2025)

Test of Cosmic Web-feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
por: Ko, Eunhee, et al.
Publicado: (2024)

Size matters: are we witnessing super-Eddington accretion in high-redshift black holes from JWST?
por: Lupi, Alessandro, et al.
Publicado: (2024)

A Square Kilometre Array Pulsar Census
por: Keane, E. F., et al.
Publicado: (2025)

Searching for unresolved massive black hole pairs through AGN photometric variability
por: Bertassi, Lorenzo, et al.
Publicado: (2026)

Binary black holes in magnetized AGN disks
por: Joshi, Raj Kishor, et al.
Publicado: (2025)

Primordial black holes in cosmological simulations: growth prospects for supermassive black holes
por: Prole, Lewis R., et al.
Publicado: (2025)

The role of migration traps in the formation of binary black holes in AGN disks
por: Vaccaro, Maria Paola, et al.
Publicado: (2025)

Gravitational Wave Phase shifts of black hole mergers in AGN Disks
por: Tagawa, Hiromichi, et al.
Publicado: (2025)

Gravitational wave mergers of accreting binary black holes in AGN discs
por: Ishibashi, W., et al.
Publicado: (2024)

Conditions for Super-Eddington Accretion onto the First Black Holes
por: Gordon, Simone T., et al.
Publicado: (2024)

On the Origin of Star Formation Quenching of Galaxies in Group Environments using the NewHorizon simulation
por: Rhee, Jinsu, et al.
Publicado: (2024)

The SKAO Pulsar Timing Array
por: Shannon, Ryan M., et al.
Publicado: (2025)