Search Results - "Casagrande, Luca"
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Connecting the Local Stellar Halo and Its Dark Matter Density to Dwarf Galaxies via Blue Stragglers
Published in The Astrophysical journal (01-06-2020)“…The Gaia H-R diagram shows the presence of apparently young stars at high tangential velocities. Using a simple analytical model, I show that these stars are…”
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The SkyMapper-Gaia RVS view of the Gaia–Enceladus–Sausage – an investigation of the metallicity and mass of the Milky Way’s last major merger
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT We characterize the Gaia–Enceladus–Sausage kinematic structure recently discovered in the Galactic halo using photometric metallicities from the…”
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3
The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood
Published in The Astrophysical journal (20-09-2018)“…The compositions of stars are a critical diagnostic tool for many topics in astronomy such as the evolution of our Galaxy, the formation of planets, and the…”
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M dwarfs: effective temperatures, radii and metallicities
Published in Monthly notices of the Royal Astronomical Society (11-09-2008)“…We empirically determine effective temperatures and bolometric luminosities for a large sample of nearby M dwarfs, for which high accuracy optical and infrared…”
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On the alleged duality of the Galactic halo
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…We examine the kinematics of the Galactic halo based on SDSS/SEGUE data by Carollo et al. We find that their claims of a counter-rotating halo are the result…”
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Absolute Calibration. III. Improved Absolute Calibration for the Visible through the Mid-infrared
Published in The Astronomical journal (01-03-2023)“…Abstract We propose Sirius as an improved zero-point-defining star and calibrate its spectrum to an accuracy of ∼0.6% in both the visible and infrared. This…”
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The GALAH survey: effective temperature calibration from the InfraRed Flux Method in the Gaia system
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT In order to accurately determine stellar properties, knowledge of the effective temperature of stars is vital. We implement Gaia and 2MASS photometry…”
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Interstellar extinction curve variations towards the inner Milky Way: a challenge to observational cosmology
Published in Monthly notices of the Royal Astronomical Society (01-03-2016)“…We investigate interstellar extinction curve variations towards ∼4 deg2 of the inner Milky Way in VIJKs photometry from the OGLE-III (third phase of the…”
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Standing on the Shoulders of Dwarfs: the Kepler Asteroseismic LEGACY Sample. I. Oscillation Mode Parameters
Published in The Astrophysical journal (01-02-2017)“…The advent of space-based missions like Kepler has revolutionized the study of solar-type stars, particularly through the measurement and modeling of their…”
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The EMBLA survey – metal-poor stars in the Galactic bulge
Published in Monthly notices of the Royal Astronomical Society (21-07-2016)“…Cosmological models predict the oldest stars in the Galaxy should be found closest to the centre of the potential well, in the bulge. The Extremely Metal-poor…”
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SEGUE-2: Old Milky Way Stars Near and Far
Published in The Astrophysical journal. Supplement series (01-04-2022)“…Abstract The Sloan Extension for Galactic Understanding and Exploration 2 (SEGUE-2) obtained 128,288 low-resolution spectra ( R ∼ 1800) of 118,958 unique stars…”
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The RAVE-on Catalog of Stellar Atmospheric Parameters and Chemical Abundances for Chemo-dynamic Studies in the Gaia Era
Published in The Astrophysical journal (01-05-2017)“…The orbits, atmospheric parameters, chemical abundances, and ages of individual stars in the Milky Way provide the most comprehensive illustration of galaxy…”
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Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
Published in The Astrophysical journal (01-05-2021)“…Abstract We combine asteroseismology, optical high-resolution spectroscopy, and kinematic analysis for 26 halo red giant branch stars in the Kepler field in…”
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14
GRACES observations of young [α/Fe]-rich stars
Published in Monthly notices of the Royal Astronomical Society (11-06-2016)“…We measure chemical abundance ratios and radial velocities in four massive (i.e. young) [α/Fe]-rich red giant stars using high-resolution high-S/N spectra from…”
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Unveiling systematic biases in the 1D LTE excitation-ionization balance of Fe for FGK stars: a novel approach to determination of stellar parameters
Published in Monthly notices of the Royal Astronomical Society (11-02-2013)“…We present a comprehensive analysis of different techniques available for the spectroscopic analysis of FGK stars and provide a recommended methodology which…”
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Asteroseismic masses of retired planet-hosting A-stars using SONG
Published in Monthly notices of the Royal Astronomical Society (01-12-2017)“…Abstract To better understand how planets form, it is important to study planet occurrence rates as a function of stellar mass. However, estimating masses of…”
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DOES SEGUE/SDSS INDICATE A DUAL GALACTIC HALO?
Published in The Astrophysical journal (09-04-2014)Get full text
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An analytic-geospatial approach for sustainable water resource management: a case study in the province of Perugia
Published in Journal of agricultural engineering (Pisa, Italy) (01-09-2013)“…Water is a strategic, but also highly vulnerable, natural resource. This because the increasing demand from multiple uses, in many cases competing amongst…”
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Selecting accreted populations: metallicity, elemental abundances, and ages of the Gaia-Sausage-Enceladus and Sequoia populations
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT Identifying stars found in the Milky Way as having formed in situ or accreted can be a complex and uncertain undertaking. We use Gaia kinematics and…”
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The SAGA so far: reading the history of the Galaxy with asteroseismology
Published in EPJ Web of conferences (01-01-2015)“…Asteroseismology has the capability of delivering stellar properties which would otherwise be inaccessible, such as radii, masses and thus ages of stars. When…”
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