Luca Casagrande

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Australian National University

Australia

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About

Associate Professor Luca Casagrande is a faculty member at the Australian National University. His research focuses on asteroseismology, stellar populations, and the chemical evolution of the Milky Way, as evidenced by his recent articles. Through his work, he utilizes data from advanced observational facilities, including GAIA and TESS, to enhance the understanding of stellar dynamics and ages in galactic contexts.

Recent Grants

Grant: Close

The milli-arcsecond cosmos: astrophysical imaging with Heimdallr

Open Date: 2022-01-01

Close Date: 2023-12-31

Grant: Close

A dedicated telescope to study the interiors of stars from their oscillations

Open Date: 2019-01-01

Close Date: 2019-12-31

Grant: Close

Interferometric Observations of Benchmark Stars for Calibrating Large Stellar Surveys of the Milky Way

Open Date: 2018-01-01

Close Date:

Grant: Close

The life-stories of galaxies from stellar fossils

Open Date: 2016-01-01

Close Date: 2019-12-31

Grant: Close

Dynamic stars: Atmospheres, evolution and asteroseismology

Open Date: 2015-01-01

Close Date: 2017-12-31

Articles (20)

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2025

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2022

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2022

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2022

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2022

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2021

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2021

Professor

Università degli Studi di Bologna Dipartimento di Fisica e Astronomia

ITALY

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Luca Casagrande

Research Interests

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About

Recent Grants

Articles (20)

Tracing the Milky Way: calibrating chemical ages with high-precision Kepler data

Advancing the accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary

Asteroseismology of the G8 subgiant β Aquilae with SONG-Tenerife, SONG-Australia and TESS

Internal dynamics of multiple populations in 28 Galactic globular clusters: a wide-field study with Gaia and the Hubble Space Telescope

Hunting for UVdim stars in Galactic open clusters. Clues from ultraviolet photometry

C3PO – IV. Co-natal stars depleted in refractories are magnetically more active – possible imprints of planets

The rise of the Milky Way Disk through EMP stars

Survey of extended main-sequence turn-offs in galactic open clusters: stellar rotations from Gaia RVS spectra

The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators: I. Data and Asteroseismic parameters

Spectrophotometry and radial distribution of multiple stellar populations in globular clusters from Gaia XP spectra

M giants with IGRINS

The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler

Absolute Calibration. III. Improved Absolute Calibration for the Visible through the Mid-infrared

Shell helium-burning hot subdwarf B stars as candidates for blue large-amplitude pulsators

Chromosome maps of globular clusters from wide-field ground-based photometry

The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission

Erratum “Milky Way Tomography with the SkyMapper Southern Survey. II. Photometric Recalibration of SMSS DR2” (2021, ApJ, 907, 68)

Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field

Distances, extinctions, and stellar parameters for stars in SkyMapper DR3

Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si. II. Application to the colour–magnitude diagrams of the globular clusters 47 Tuc, NGC 6362, M 5, M 3, M 55, and M92

Collaborators (12)

Alessandra Mastrobuono-Battisti

GIACOMO CORDONI

Claudia Reyes

D Yong

Dennis Stello

Luisa Fernanda Rodríguez Díaz

Tim Bedding

Sohee Jang

Mikkel Nørup Lund

A D Mackey

M Carlos

Andrea Miglio

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