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Measuring our peculiar velocity from spectroscopic redshift surveys
Mohamed Yousry Elkhashab, Cristiano Porciani, Daniele Bertacca
Our peculiar velocity imprints a dipole on galaxy density maps derived from redshift surveys. The dipole gives rise to an oscillatory signal in the multipole moments of the observe…
The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
Prachi Khatri, Emilio Romano-Díaz, Cristiano Porciani
The [C II] fine-structure line at 157.74 m is one of the brightest far-infrared emission lines and an important probe of galaxy properties like the star formation rate (SFR) and…
Euclid preparation. L. Calibration of the linear halo bias in CDM cosmologies
Euclid Collaboration, T. Castro, A. Fumagalli +253
The Euclid mission, designed to map the geometry of the dark Universe, presents an unprecedented opportunity for advancing our understanding of the cosmos through its photometric g…
Euclid preparation. XLIX. Selecting active galactic nuclei using observed colours
Euclid Collaboration, L. Bisigello, M. Massimo +244
Euclid will cover over 14000 with two optical and near-infrared spectro-photometric instruments, and is expected to detect around ten million active galactic nuclei (AGN)…
Euclid preparation. The Cosmic Dawn Survey (DAWN) of the Euclid Deep and Auxiliary Fields
Euclid Collaboration, C. J. R. McPartland, L. Zalesky +288
Euclid will provide deep NIR imaging to 26.5 AB magnitude over 59 deg in its deep and auxiliary fields. The Cosmic DAWN survey complements the deep Euclid data with…
The streaming model for the three-point correlation function and its connection to standard perturbation theory
Anna Pugno, Alexander Eggemeier, Cristiano Porciani +1
Redshift-space distortions present a significant challenge in building models for the three-point correlation function (3PCF). We compare two possible lines of attack: the streamin…