M. Scalco
Physics and Astronomy · Indiana University
Publications
40
Citations
240
Est. group size
—
Recurring co-author estimate
Active years
10
Publishing since 2017
M. Scalco studies stars within dense star clusters and the faintest, coolest objects in our galaxy using space telescopes such as the Hubble Space Telescope (HST) and the James Webb Space Telescope (JWST). The work focuses on measuring the brightness and positions of stars in globular clusters, tracing how many stars form at different masses, and characterizing very low-mass and 'failed' stars like brown dwarfs and cool Y-dwarfs. This involves detailed photometry (measuring light) and astrometry (measuring precise positions and motions).
Publication activity has grown substantially over the past decade, rising from about one paper per year in the late 2010s to a peak of around a dozen in 2024, averaging seven per year over the last five years.
Generated by claude-opus-4-8 from public bibliographic data · Jul 11, 2026
- The mass functions of multiple stellar populations in 47 Tucanae
Barbara A. Mikulski Archive for Space Telescopes · 2026
- The mass functions of multiple stellar populations in 47 Tucanae
Barbara A. Mikulski Archive for Space Telescopes · 2026
- JWST observations of 47 Tucanae - I. The low-mass main sequence down to the hydrogen-burning limit
Barbara A. Mikulski Archive for Space Telescopes · 2026
- The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- III. Near-Infrared Photometry
arXiv (Cornell University) · 2026
- The Y Dwarf Population with HST: unlocking the secrets of our coolest neighbours -- III. Near-Infrared Photometry
arXiv (Cornell University) · 2026
- The Y-dwarf population with <i>HST</i> : unlocking the secrets of our coolest neighbours – III. Near-infrared photometry
Monthly Notices of the Royal Astronomical Society · 2026
- <scp> <i>JWST</i> </scp> Imaging of the Closest Globular Clusters— <scp>VI</scp> . The Lowest‐Mass Objects in M 4 and the Galactic Bulge
Astronomische Nachrichten · 2025
- JWST photometry and astrometry of 47 Tucanae. Discontinuity in the stellar sequence at the star/brown dwarf transition
arXiv (Cornell University) · 2025
- JWST Imaging of the Closest Globular Clusters -- V. The White Dwarfs Cooling Sequence of M4
arXiv (Cornell University) · 2025
- <i>James Webb Space Telescope</i> observations of the white dwarf cooling sequence of 47 Tucanæ
Monthly Notices of the Royal Astronomical Society · 2025
- <scp><i>JWST</i></scp> Imaging of the Closest Globular Clusters—V. The White Dwarfs Cooling Sequence of <scp>M4</scp>
Astronomische Nachrichten · 2025
- JWST photometry and astrometry of 47 Tucanæ
Astronomy and Astrophysics · 2025
- JWST Imaging of the Closest Globular Clusters -- I. Possible Infrared Excess Among White Dwarfs in NGC 6397
arXiv (Cornell University) · 2024
- The HST Large Programme on <i>ω</i> Centauri
Astronomy and Astrophysics · 2024
- <i>JWST</i> imaging of the closest globular clusters—I. Possible infrared excess among white dwarfs in NGC 6397
Astronomische Nachrichten · 2024
- arXiv (Cornell University)×12
- Monthly Notices of the Royal Astronomical Society×7
- Astronomy and Astrophysics×6
- Astronomische Nachrichten×5
- Barbara A. Mikulski Archive for Space Telescopes×3
This profile was generated automatically from public scholarly data (OpenAlex). Group size and activity levels are estimates derived from co-authorship patterns.
Last updated Jul 11, 2026.
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