Compressing combined probes: redshift weights for joint lensing and clustering analyses
arXiv:2006.11297 · doi:10.1093/mnras/staa2537
Abstract
Combining different observational probes, such as galaxy clustering and weak lensing, is a promising technique for unveiling the physics of the Universe with upcoming dark energy experiments. Whilst this strategy significantly improves parameter constraints, decreasing the degeneracies of individual analyses and controlling the systematics, processing data from tens of millions of galaxies is not a trivial task. In this work we derive and test a new estimator for joint clustering and lensing data analysis, maximising the scientific return and decreasing the computational cost. Our estimator compresses the data by up-weighting the components most sensitive to the parameters of interest, with no loss of information, taking into account information from the cross-correlation between the two probes. We derive optimal redshift weights which may be applied to individual galaxies when testing a given statistic and cosmological model.
9 pages, 7 figures
References in corpus (25)
- LSST: from Science Drivers to Reference Design and Anticipated Data Products
- Cosmological parameters from CMB and other data: a Monte-Carlo approach
- The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
- Spectroscopic Target Selection for the Sloan Digital Sky Survey: The Luminous Red Galaxy Sample
- Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?
- Euclid Definition Study Report
- The Dark Energy Survey Data Release 1
- The Kilo-Degree Survey
- Massive Lossless Data Compression and Multiple Parameter Estimation from Galaxy Spectra
- CosmoLike - Cosmological Likelihood Analyses for Photometric Galaxy Surveys
- Joint Galaxy-Lensing Observables and the Dark Energy
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: a tomographic measurement of cosmic structure growth and expansion rate based on optimal redshift weights
- 4MOST - 4-metre Multi-Object Spectroscopic Telescope
- Simultaneous measurement of cosmology and intrinsic alignments using joint cosmic shear and galaxy number density correlations
- Combining cluster observables and stacked weak lensing to probe dark energy: Self-calibration of systematic uncertainties
- Comprehensive Two-Point Analyses of Weak Gravitational Lensing Surveys
- Redshift-weighted constraints on primordial non-Gaussianity from the clustering of the eBOSS DR14 quasars in Fourier space
- The effect of Limber and flat-sky approximations on galaxy weak lensing
- Joint Analysis of Gravitational Lensing, Clustering and Abundance: Toward the Unification of Large-Scale Structure Analysis
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: Measuring the anisotropic Baryon Acoustic Oscillations with redshift weights
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift space distortions between redshift 0.8 and 2.2
- Parameter Inference for Weak Lensing using Gaussian Processes and MOPED
- Optimal Redshift Weighting For Redshift Space Distortions
- The extended Baryon Oscillation Spectroscopic Survey (eBOSS): testing a new approach to measure the evolution of the structure growth
- Sheer shear: weak lensing with one mode