Turnitin
降AI改写
早检测系统
早降重系统
Turnitin-UK版
万方检测-期刊版
维普编辑部版
Grammarly检测
Paperpass检测
checkpass检测
PaperYY检测
Physical models of galaxy formation in a cosmological framework
Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …
challenges in astrophysics today due to the vast range of scales and numerous physical …
Cosmology and fundamental physics with the Euclid satellite
Abstract Euclid is a European Space Agency medium-class mission selected for launch in
2020 within the cosmic vision 2015–2025 program. The main goal of Euclid is to understand …
2020 within the cosmic vision 2015–2025 program. The main goal of Euclid is to understand …
UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …
Too big to fail? The puzzling darkness of massive Milky Way subhaloes
We show that dissipationless Λ cold dark matter simulations predict that the majority of the
most massive subhaloes of the Milky Way are too dense to host any of its bright satellites …
most massive subhaloes of the Milky Way are too dense to host any of its bright satellites …
Semi-analytic galaxy evolution (SAGE): model calibration and basic results
This paper describes a new publicly available codebase for modeling galaxy formation in a
cosmological context, the" Semi-Analytic Galaxy Evolution" model, or sage for short. 5 sage …
cosmological context, the" Semi-Analytic Galaxy Evolution" model, or sage for short. 5 sage …
Small scale problems of the ΛCDM model: a short review
The ΛCDM model, or concordance cosmology, as it is often called, is a paradigm at its
maturity. It is clearly able to describe the universe at large scale, even if some issues remain …
maturity. It is clearly able to describe the universe at large scale, even if some issues remain …
From dwarf spheroidals to cD galaxies: simulating the galaxy population in a ΛCDM cosmology
We have updated and extended our semi-analytic galaxy formation modelling capabilities
and applied them simultaneously to the stored halo/subhalo merger trees of the Millennium …
and applied them simultaneously to the stored halo/subhalo merger trees of the Millennium …
The Milky Way's bright satellites as an apparent failure of ΛCDM
We use the Aquarius simulations to show that the most massive subhaloes in galaxy-mass
dark matter (DM) haloes in Λ cold dark matter (ΛCDM) are grossly inconsistent with the …
dark matter (DM) haloes in Λ cold dark matter (ΛCDM) are grossly inconsistent with the …
The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
We simulate the growth of galaxies and their central supermassive black holes by
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …
A comprehensive analysis of uncertainties affecting the stellar mass–halo mass relation for 0< z< 4
We conduct a comprehensive analysis of the relationship between central galaxies and their
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …
host dark matter halos, as characterized by the stellar mass–halo mass (SM–HM) relation …