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Camille Bonvin

Has grant

Associate Professor

University of Geneva

Switzerland

Research Interests

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About

Camille Bonvin is an Associate Professor at the University of Geneva, Switzerland. Her research focuses on cosmology and astrophysics, particularly in areas such as dark energy, relativistic effects in galaxy clusters, and testing general relativity using galaxy observations. Recent articles reflect her interest in large-scale galaxy clustering and its impact on cosmological models.

Recent Grants

Grant: Close

Testing the law of gravity with novel large-scale structure observables

Open Date: 2020-11-01

Close Date: 2024-10-31

Grant: Close

Testing the law of gravity with novel large-scale structure observables

Open Date: 2020-11-01

Close Date: 2025-10-31

Grant: Close

Testing Gravity with large-scale structure

Open Date: 2016-06-01

Close Date: 2020-10-31

Articles (26)

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2022

Collaborators (118)

Daniel Holz

University of Chicago

UNITED STATES

Camille Bonvin

Research Interests

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About

Recent Grants

Articles (26)

Euclid. I. Overview of the Euclid mission

Testing the equivalence principle across the Universe: A model-independent approach with galaxy multitracing

Euclid: Relativistic effects in the dipole of the two-point correlation function

Reconstructing the dark energy density in light of DESI BAO observations

Gravitational redshift from galaxy clusters — a relativistic approach

The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: numerical results

The impact of large-scale galaxy clustering on the variance of the Hellings-Downs correlation: theoretical framework

Euclid preparation

Fast and spurious: a robust determination of our peculiar velocity with future galaxy surveys

Gravitational redshift constraints on the effective theory of interacting dark energy

Testing General Relativity through the EG Statistic Using the Weyl Potential and Galaxy Velocities

Using relativistic effects in large-scale structure to constrain astrophysical properties of galaxy populations

Disentangling modified gravity from a dark force with gravitational redshift

Cosmology with the Laser Interferometer Space Antenna

A case study for measuring the relativistic dipole of a galaxy cross-correlation with the Dark Energy Spectroscopic Instrument

Aberration of gravitational waveforms by peculiar velocity

Combining gravitational lensing and gravitational redshift to measure the anisotropic stress with future galaxy surveys

Model-independent test for gravity using intensity mapping and galaxy clustering

Detection and estimation of the cosmic dipole with the einstein telescope and cosmic explorer

Modified Einstein versus modified Euler for dark matter

Nonlinear redshift-space distortions on the full sky

Combining chirp mass, luminosity distance, and sky localization from gravitational wave events to detect the cosmic dipole

Can cosmology distinguish a dark force from a modification of gravity?

Euclid preparation

Measuring the distortion of time with relativistic effects in large-scale structure

Rescuing constraints on modified gravity using gravitational redshift in large-scale structure

Collaborators (118)

Daniel Holz

Graham Smith

Barry Wardell

Carlton Baugh

Victoria Yankelevich

Sebastien Clesse

Nelson Nunes

Matteo Calabrese

Michele Fumagalli

Ben Dryer

Javier Graciá Carpio

Mikael Granvik

Geraldine Servant

Azadeh Moradinezhad Dizgah

C J A P Martins

Rafael Rebolo

Saeed Rastgoo

Sotiria Fotopoulou

Isobel Hook

Savvas Koushiappas

Sergio Di Domizio

Luigi Pilo

Azadeh Maleknejad

Marco Peloso

Alexandre Refregier

Jorge Carretero

Fabio La Franca

Jussi Valiviita

Antonio da Silva

Per Lilje

Matteo Fossati

Hannu Kurki-Suonio

Stefano Camera

Ken Osato

chiara mancini

S Foffa

Santiago Avila

Andrei Lazanu

Jon Loveday

Kimmo Kiiveri

Tiago Barreiro

Mike Hudson

Benedict Bahr-Kalus

Sune Toft

Mikko Pöntinen

Elina Keihänen