© 2019 Novel Probes Collaboration


Queen Mary University London, t.baker "at" qmul.ac.uk

Cosmological aspects of modified gravity; observational probes

Alex Barreira

Max Planck Institute for Astrophysics, barreira "at" mpa-garching.mpg.de

Weak lensing & large scale structure probes of gravity; modified gravity simulations

University of Oxford, harry.desmond "at" physics.ox.ac.uk

Tests of modified gravity in galaxies; galaxy dynamics; the galaxy-halo connection; baryonic effects

University of Oxford, p.ferreira1 "at" physics.ox.ac.uk

Interplay between theoretical and observational cosmology; the dark sector; cosmological modified gravity

University of Pennsylvania, bjain "at" physics.upenn.edu

Weak lensing; astrophysical probes of modified gravity and tests with galaxy surveys

ICG Portsmouth, Kazuya.Koyama "at" port.ac.uk

Theoretical cosmology; early universe and structure formation; accelerated cosmic expansion

University of Durham, baojiu.li "at" durham.ac.uk

Cosmological tests of gravity; large scale structure; weak lensing; modified gravity simulations

University of Geneva, lucas.lombriser "at" unige.ch

Cosmological modified gravity; nonlinear structure formation

Princeton University, anicola'at'astro.princeton.edu

Cosmological probes; surveys

University of Pennsylvania, sakstein "at" sas.upenn.edu

Theoretical aspects of modified gravity; screening mechanisms; novel probes with stars and galaxies

Max Planck Institute for Astrophysics, fabians "at" mpa-garching.mpg.de

Cosmological modified gravity; large-scale structure; modified gravity simulations; the early universe; gravitational lensing

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LBNL, evlinder "at" lbl.gov

Dark energy and cosmic acceleration; tests of General Relativity; CMB; inflation

Cornell University, rachel.bean "at" cornell.edu

Large scale structure; cosmological tests of modified gravity; inflation; weak lensing

ICG Portsmouth, gong-bo.zhao "at" port.ac.uk

Modified gravity simulations; consistency tests of GR and dark energy; structure formation; CMB; weak lensing

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