70 citations · 202 across the 8 of their papers we have counts for
7 papers
Euclid preparation. XCV. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation
Euclid Collaboration, S. Joudaki, V. Pettorino +345
We provide a description of the code implementation and structure of Cosmology Likelihood for Observables in Euclid (CLOE), developed by members of the Euclid Consortium. CLOE is a…
MUSCLE-UPS: Improved Approximations of the Matter Field with the Extended Press-Schechter Formalism and Lagrangian Perturbation Theory
Federico Tosone, Mark C. Neyrinck, Benjamin R. Granett +2
Lagrangian algorithms to simulate the evolution of cold dark matter (CDM) are invaluable tools to generate large suites of mock halo catalogues. In this paper, we first show that t…
Beyond the Lognormal Approximation: a General Simulation Scheme
Federico Tosone, Mark C. Neyrinck, Benjamin R. Granett +2
We present a public code to generate random fields with an arbitrary probability distribution function (PDF) and an arbitrary correlation function. The algorithm is cosmology-indep…
The Multi-Tracer Optimal Estimator applied to VIPERS
Antonio D. Montero-Dorta, L. Raul Abramo, Benjamin R. Granett +2
We use mock galaxy data from the VIMOS Public Extragalactic Redshift Survey (VIPERS) to test the performance of the Multi-Tracer Optimal Estimator (MTOE) of Abramo et al. as a tool…
Euclid Mission: building of a Reference Survey
J. Amiaux, R. Scaramella, Y. Mellier +28
Euclid is an ESA Cosmic-Vision wide-field-space mission which is designed to explain the origin of the acceleration of Universe expansion. The mission will investigate at the same…
Constraints on Massive Neutrinos from the CFHTLS Angular Power Spectrum
Jun-Qing Xia, Benjamin R. Granett, Matteo Viel +6
We use the galaxy angular power spectrum at from the Canada-France-Hawaii-Telescope Legacy Survey Wide fields (CFHTLS-Wide) to constrain separately the total neutrin…
Empirical H-alpha emitter count predictions for dark energy surveys
J. E. Geach, A. Cimatti, W. Percival +12
Future galaxy redshift surveys aim to measure cosmological quantities from the galaxy power spectrum. A prime example is the detection of baryonic acoustic oscillations (BAOs), pro…