Search Results - "Maturi, Matteo"
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AMICO: optimized detection of galaxy clusters in photometric surveys
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We present Adaptive Matched Identifier of Clustered Objects (AMICO), a new algorithm for the detection of galaxy clusters in photometric surveys…”
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amico galaxy clusters in KiDS-DR3: sample properties and selection function
Published in Monthly notices of the Royal Astronomical Society (01-05-2019)Get full text
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AMICO galaxy clusters in KiDS-DR3: weak lensing mass calibration
Published in Monthly notices of the Royal Astronomical Society (01-04-2019)Get full text
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Exploring the Mass and Redshift Dependencies of the Cluster Pressure Profile with Stacks on Thermal Sunyaev–Zel’dovich Maps
Published in The Astrophysical journal. Supplement series (01-04-2023)“…We provide novel constraints on the parameters defining the universal pressure profile (UPP) within clusters of galaxies, and explore their dependencies on…”
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De-noising the galaxies in the Hubble XDF with EMPCA
Published in Monthly notices of the Royal Astronomical Society (01-10-2017)Get full text
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EasyCritics – I. Efficient detection of strongly lensing galaxy groups and clusters in wide-field surveys
Published in Monthly notices of the Royal Astronomical Society (11-01-2019)Get full text
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Properties and observables of massive galaxies in self-interacting dark matter cosmologies
Published in Monthly notices of the Royal Astronomical Society (04-07-2023)“…ABSTRACT We use hydrodynamic cosmological simulations to test the differences between cold and self-interacting dark matter models (CDM and SIDM) in the mass…”
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Detecting strongly lensed supernovae at z ∼ 5–7 with LSST
Published in Monthly notices of the Royal Astronomical Society (11-01-2020)“…Supernovae (SNe) could be powerful probes of the properties of stars and galaxies at high redshifts in future surveys. Wide fields and longer exposure times…”
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CoMaLit – VI. Intrinsic scatter in stacked relations. The weak lensing AMICO galaxy clusters in KiDS-DR3
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…Unbiased and precise mass calibration of galaxy clusters is crucial to fully exploit galaxy clusters as cosmological probes. Stacking of weak lensing (WL)…”
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AMICO galaxy clusters in KiDS-DR3: measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
Published in Monthly notices of the Royal Astronomical Society (08-02-2022)“…Galaxy clusters are biased tracers of the underlying matter density field. At very large radii beyond about 10 Mpc h−1, the shear profile shows evidence of a…”
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Galaxy cluster optical mass proxies from probabilistic memberships
Published in Monthly notices of the Royal Astronomical Society (10-10-2023)“…ABSTRACT Robust galaxy cluster mass estimates are fundamental for constraining cosmological parameters from counts. For this reason, it is essential to search…”
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INSPIRE: INvestigating Stellar Population In RElics – VII. The local environment of ultra-compact massive galaxies
Published in Monthly notices of the Royal Astronomical Society (03-10-2024)“…ABSTRACT Relic galaxies, the oldest ultra-compact massive galaxies (UCMGs), contain almost exclusively ‘pristine’ stars formed during an intense star formation…”
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AMICO galaxy clusters in KiDS-DR3: galaxy population properties and their redshift dependence
Published in Monthly notices of the Royal Astronomical Society (01-11-2020)“…ABSTRACT A catalogue of galaxy clusters was obtained in an area of 414 $\deg ^2$ up to a redshift z ∼ 0.8 from the Data Release 3 of the Kilo-Degree Survey…”
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Camouflaged Galactic cosmic microwave background polarization foregrounds: total and polarized contributions of the kinetic Sunyaev–Zeldovich effect
Published in Monthly notices of the Royal Astronomical Society (01-02-2008)“…We consider the role of the Galactic kinetic Sunyaev–Zeldovich (SZ) effect as a cosmic microwave background (CMB) polarization foreground. While the Galactic…”
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De-noising the galaxies in the Hubble XDF with EMPCA
Published 19-07-2016“…We present a method to model optical images of galaxies using Expectation Maximization Principal Components Analysis (EMPCA). The method relies on the data…”
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AMICO-COSMOS galaxy cluster and group catalogue up to $z = 2$: Sample properties and X-ray counterparts
Published 19-12-2023“…A&A 687, A56 (2024) We present a new galaxy cluster search in the COSMOS field through the use of the Adaptive Matched Identifier of Clustered Objects (AMICO)…”
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