Search Results - "Andrea, V."
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Cold dark matter haloes in the Planck era: evolution of structural parameters for Einasto and NFW profiles
Published in Monthly notices of the Royal Astronomical Society (11-07-2014)“…We present the evolution of the structure of relaxed cold dark matter (CDM) haloes in the cosmology from the Planck satellite. Our simulations cover five…”
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NIHAO project – I. Reproducing the inefficiency of galaxy formation across cosmic time with a large sample of cosmological hydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (21-11-2015)“…We introduce project Nihao (Numerical Investigation of a Hundred Astrophysical Objects), a set of 100 cosmological zoom-in hydrodynamical simulations performed…”
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Non-linear evolution of cosmological structures in warm dark matter models
Published in Monthly notices of the Royal Astronomical Society (01-07-2012)“…The dark energy dominated warm dark matter (WDM) model is a promising alternative cosmological scenario. We explore large-scale structure formation in this…”
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NIHAO XV: the environmental impact of the host galaxy on galactic satellite and field dwarf galaxies
Published in Monthly notices of the Royal Astronomical Society (11-02-2019)Get full text
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Constraints on the Relationship between Stellar Mass and Halo Mass at Low and High Redshift
Published in The Astrophysical journal (20-02-2010)“…We use a statistical approach to determine the relationship between the stellar masses of galaxies and the masses of the dark matter halos in which they…”
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NIHAO IX: the role of gas inflows and outflows in driving the contraction and expansion of cold dark matter haloes
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…We use ∼100 cosmological galaxy formation ‘zoom-in’ simulations using the smoothed particle hydrodynamics code gasoline to study the effect of baryonic…”
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NIHAO – IV: core creation and destruction in dark matter density profiles across cosmic time
Published in Monthly notices of the Royal Astronomical Society (11-03-2016)“…We use the NIHAO (Numerical Investigation of Hundred Astrophysical Objects) cosmological simulations to investigate the effects of baryonic physics on the time…”
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Formation of ultra-diffuse galaxies in the field and in galaxy groups
Published in Monthly notices of the Royal Astronomical Society (21-08-2019)“…We study ultra-diffuse galaxies (UDGs) in zoom in cosmological simulations, seeking the origin of UDGs in the field versus galaxy groups. We find that while…”
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Concentration, spin and shape of dark matter haloes as a function of the cosmological model: WMAP1, WMAP3 and WMAP5 results
Published in Monthly notices of the Royal Astronomical Society (21-12-2008)“…We investigate the effects of changes in the cosmological parameters between the Wilkinson Microwave Anisotropy Probe (WMAP) 1st, 3rd and 5th year results on…”
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NIHAO – XI. Formation of ultra-diffuse galaxies by outflows
Published in Monthly notices of the Royal Astronomical Society. Letters (21-03-2017)“…Abstract We address the origin of ultra-diffuse galaxies (UDGs), which have stellar masses typical of dwarf galaxies but effective radii of Milky Way-sized…”
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NIHAO – XXIII. Dark matter density shaped by black hole feedback
Published in Monthly notices of the Royal Astronomical Society. Letters (11-06-2020)“…ABSTRACT We present a systematic analysis of the reaction of dark matter distribution to galaxy formation across more than eight orders of magnitude in stellar…”
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Cores in warm dark matter haloes: a Catch 22 problem
Published in Monthly notices of the Royal Astronomical Society (01-08-2012)“…Abstract The free streaming of warm dark matter particles dampens the fluctuation spectrum, flattens the mass function of haloes and sets a fine-grained phase…”
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The dependence of dark matter profiles on the stellar-to-halo mass ratio: a prediction for cusps versus cores
Published in Monthly notices of the Royal Astronomical Society (01-01-2014)“…We use a suite of 31 simulated galaxies drawn from the MaGICC project to investigate the effects of baryonic feedback on the density profiles of dark matter…”
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NIHAO-UHD: The properties of MW-like stellar disks in high resolution cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…Simulating thin and extended galactic disks has long been a challenge in computational astrophysics. We introduce the NIHAO-UHD suite of cosmological…”
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An observational test for star formation prescriptions in cosmological hydrodynamical simulations
Published in Monthly notices of the Royal Astronomical Society (11-06-2019)“…Abstract State-of-the-art cosmological hydrodynamical simulations of galaxy formation have reached the point at which their outcomes result in galaxies with…”
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NIHAO project II: halo shape, phase-space density and velocity distribution of dark matter in galaxy formation simulations
Published in Monthly notices of the Royal Astronomical Society (11-10-2016)“…We use the NIHAO (Numerical Investigation of Hundred Astrophysical Objects) cosmological simulations to study the effects of galaxy formation on key properties…”
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Community-acquired bloodstream infections in Africa: a systematic review and meta-analysis
Published in The Lancet infectious diseases (01-06-2010)“…Summary Data on the prevalence and causes of community-acquired bloodstream infections in Africa are scarce. We searched three databases for studies that…”
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Systemic sclerosis-associated interstitial lung disease
Published in The lancet respiratory medicine (01-03-2020)“…Systemic sclerosis is an autoimmune connective tissue disease, which is characterised by immune dysregulation and progressive fibrosis that typically affects…”
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Stars Behind Bars. I. The Milky Way's Central Stellar Populations
Published in The Astrophysical journal (10-07-2018)“…We show for the first time that a fully cosmological hydrodynamical simulation can reproduce key properties of the innermost region of the Milky Way (MW). Our…”
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Panchromatic Simulated Galaxy Observations from the NIHAO Project
Published in The Astrophysical journal (01-11-2023)“…We present simulated galaxy spectral energy distributions (SEDs) from the far-ultraviolet (FUV) through the far-infrared (FIR), created using hydrodynamic…”
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