activity
20232026
most citedEuclid. I. Overview of the Euclid mission

550 citations · 560 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.CO2026

Euclid preparation: Testing multi-field inflation with galaxy power spectrum and bispectrum

Euclid Collaboration, D. Linde, A. Moradinezhad Dizgah +281

Primordial non-Gaussianity (PNG) is a powerful probe of the origin of cosmic structure. Stage-IV surveys like \Euclid will measure galaxy - and -point clustering at high sign…

astro-ph.CO2026

Euclid preparation. Galaxy power spectrum and bispectrum modelling

Euclid Collaboration, K. Pardede, A. Eggemeier +306

Higher-order correlation functions of the large-scale galaxy distribution offer access to information beyond that contained in standard 2-point statistics such as the power spectru…

astro-ph.CO2026

Testing parity with composite-field spectra of BOSS and DESI luminous red galaxies

Zucheng Gao, Marina S. Cagliari, Azadeh Moradinezhad Dizgah +1

Detection of parity violation on cosmological scales would have profound implications for fundamental physics. Motivated in part by recent measurements of parity-odd four-point cor…

astro-ph.CO2026★ 1 cited

Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks

Iñigo Sáez-Casares, Matteo Calabrese, Davide Bianchi +4

The possibility to constrain cosmological parameters from galaxy surveys using field-level machine learning methods that bypass traditional summary statistics analyses, depends cru…

astro-ph.CO2025

Hierarchical summaries for primordial non-Gaussianities

M. S. Cagliari, A. Bairagi, B. Wandelt

The advent of Stage IV galaxy redshift surveys such as DESI and Euclid marks the beginning of an era of precision cosmology, with one key objective being the detection of primordia…

astro-ph.CO2025

Disentangling Target Lines from Interlopers and Continuum with Neural Networks: A SPHEREx Intensity Mapping Case Study

Marina S. Cagliari, Zucheng Gao, Azadeh Moradinezhad Dizgah

Line-intensity mapping (LIM) traces the large-scale distribution of matter by measuring fluctuations in aggregate line emission from unresolved galaxies and the intergalactic mediu…

astro-ph.CO2025

Correcting for interloper contamination in the power spectrum with neural networks

Marina S. Cagliari, Azadeh Moradinezhad Dizgah, Francisco Villaescusa-Navarro

Modern slitless spectroscopic surveys, such as Euclid and the Roman Space Telescope, collect vast numbers of galaxy spectra but suffer from low signal-to-noise ratios. This often l…

astro-ph.CO2025★ 5 cited

Bispectrum constraints on Primordial non-Gaussianities with the eBOSS DR16 quasars

Marina S. Cagliari, Matilde Barberi-Squarotti, Kevin Pardede +2

We present constraints on , the parameter quantifying the amplitude of local Primordial Non-Gaussianities (PNG), from a combined analysis of the tree-level power spectr…

astro-ph.CO2024★ 550 cited

Euclid. I. Overview of the Euclid mission

Euclid Collaboration, Y. Mellier, Abdurro'uf +1134

The current standard model of cosmology successfully describes a variety of measurements, but the nature of its main ingredients, dark matter and dark energy, remains unknown. Eucl…

astro-ph.CO2024★ 3 cited

Euclid: Testing photometric selection of emission-line galaxy targets

M. S. Cagliari, B. R. Granett, L. Guzzo +144

Multi-object spectroscopic galaxy surveys typically make use of photometric and colour criteria to select targets. Conversely, the Euclid NISP slitless spectrograph will record spe…

astro-ph.CO2023★ 1 cited

Optimal constraints on Primordial non-Gaussianity with the eBOSS DR16 quasars in Fourier space

Marina S. Cagliari, Emanuele Castorina, Marco Bonici +1

We present constraints on the amplitude of local Primordial Non-Gaussianities (PNG), , using the quasar sample in the Sloan Digital Sky Survey IV extended Baryon Oscill…