Multi-band EBL intensity mapping cross-correlated with cosmic shear and galaxy clustering recovers IHL, IGL, and EoR parameters with 10-35% smaller uncertainties than intensity mapping alone.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
fields
astro-ph.CO 3representative citing papers
Late-type galaxies dominate shape-shape alignments in the filaments of the Perseus-Pisces supercluster while early-types cluster near dense centers, indicating distinct tidal mechanisms out to 1 Mpc/h.
Cross-covariances and cross-correlations between Euclid spectroscopic and photometric probes have negligible impact on cosmological parameter constraints.
citing papers explorer
-
Euclid preparation. Decomposing components of the extragalactic background light using multi-band intensity mapping cross-correlations
Multi-band EBL intensity mapping cross-correlated with cosmic shear and galaxy clustering recovers IHL, IGL, and EoR parameters with 10-35% smaller uncertainties than intensity mapping alone.
-
Dissecting the Perseus-Pisces supercluster observed with CFHT-MegaCam: Exploring late-type galaxy shape alignments within the local cosmic web
Late-type galaxies dominate shape-shape alignments in the filaments of the Perseus-Pisces supercluster while early-types cluster near dense centers, indicating distinct tidal mechanisms out to 1 Mpc/h.
-
Euclid preparation: 6x2 pt analysis of Euclid's spectroscopic and photometric data sets
Cross-covariances and cross-correlations between Euclid spectroscopic and photometric probes have negligible impact on cosmological parameter constraints.