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Francis Bernardeau (IPhT Saclay)20/03/2023 14:00
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Micol Bolzonella, Pablo Fosalba20/03/2023 16:30
- Presentation of the Flagship Wide by P. Fosalba
- Presentation of the Flagship Deep by M. Bolzonella
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Dr Santiago Casas (TTK, RWTH Aachen University)21/03/2023 09:00CLOE, status and performances
We expand and adjust the synthetic Euclid likelihoods of the MontePython software in order to match the exact recipes used
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in previous Euclid Fisher matrix forecasts for several probes: weak lensing cosmic shear, photometric galaxy clustering, the cross-
correlation between the latter observables, and spectroscopic galaxy clustering. We also establish which precision settings are
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ALAIN BLANCHARD (IRAP , OMP)21/03/2023 12:30
Euclid will have the unique feature of simultaneously having 2D probes with 3*2pt but also 3D data on the same areas of the sky. In this presentation I will discuss how to use this information in a cost-effective way and the type of gain that can be forecasted.
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Stefano Camera (U. Turin)21/03/2023 15:30
I present a new technique for the measurement of the growth of cosmic structures via the power spectrum of weak lensing cosmic shear, which can be straightforwardly combined to classic bias and growth measurements from clustering. It is based on a template-fitting approach, where a redshift-dependent amplitude of lensing modulates a fixed template power spectrum. To allow for tracking the...
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Lance Miller (Oxford University)21/03/2023 16:50PSF tool kit, status and performances
We describe the status of PSF modelling for SPV3, providing updates and features that may be used in multi-faceted investigations.
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M. Casey Cragg (U. Oxford)21/03/2023 17:10Weak Lensing End2End box, status and performances
We are currently working on propagating expected Euclid PSF errors into shear biases for the WL E2E box as part of the SPV3 exercise. Given some base and perturbed PSFs generated using the PSF Toolkit, we numerically estimate the multiplicative and additive shear biases for galaxies in the Flagship 2 mock catalogue. We currently consider two sources of PSF error: firstly, errors in the PSF...
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Konstantinos Tanidis (University of Oxford)22/03/2023 11:00PSF tool kit, status and performances
In this work, we study the effect of spatially-varying multiplicative bias on the cosmological parameter estimation in the combined photometric analysis of the 3x2pt statistics for a Euclid DR3 end-to-end forecast. To do so, we consider a spin-0 m-bias map characterized by a Gaussian profile angular power spectrum that has been studied in the literature. Also, we proceed with a conservative...
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William Hartley22/03/2023 15:00
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Andy Taylor22/03/2023 15:30
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Francis Bernardeau (IPhT Saclay)
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