Curriculum vitae
The full public record, section by section. The two-page academic CV has the same facts in print form.
Academic CV, 2 pages (PDF) Publications Talks
Funding and computing allocations
- Nov 2026 to Nov 2027 HPC
FCT Advanced Computing Project 2026.08382.CPCA.A1: JANUS on Deucalion, Gaia DR3
Allocation to run JANUS on the Gaia DR3 XP spectra of about 220 million stars: 299,520 ARM core-hours (99,840 granted, tripled as a bonus), 1,500 A100 GPU-hours and 10 TB for 12 months.
- Approved under call FCT/CPCA/2025/01.
- Nov 2026 to Nov 2027 HPC
FCT Advanced Computing Project 2026.08362.CPCA.A2: JANUS on MareNostrum 5, Gaia DR4
Allocation to run JANUS on the Gaia DR4 XP spectra of about 1.8 billion stars: 1,002,400 core-hours, 1,000 H100 GPU-hours and 25 TB for 12 months.
- Approved under call FCT/CPCA/2025/01.
- Sep 2026 to Aug 2027 fellowship
PhD research fellowship under the FCT project ArqueoGal
- May 2026 proposal
PLATO noise estimates for a blue-straggler guest-observer proposal (34 open clusters)
Computed single-camera PLATO noise-to-signal ratios with the HAYDN Noise Estimator for blue stragglers in their host clusters, using Gaia DR3 fields and the PLATO camera configuration.
- 124 blue stragglers in 34 host clusters, plus two anchor globular clusters; the target list came from the proposing collaborator.
- The same Deucalion sweep covered all 36 clusters (34 hosts plus the anchors NGC 1851 and NGC 2298): one HNE run per cluster, 108 Slurm submissions including resubmissions.
- Delivered as a data package with per-cluster dashboards and combined Gaia, StarHorse and noise tables.
- Ran noise-to-signal simulations with the HAYDNsim pipeline, with the HAYDN Noise Estimator in its PLATO configuration.
- May 2026 proposal
PLATO noise estimates for the NGC 1851 red-giant guest-observer proposal
Computed PLATO noise-to-signal ratios for the red giants of the globular cluster NGC 1851 with the HAYDNsim pipeline and the HAYDN Noise Estimator in its PLATO configuration.
- May 2026 proposal
PLATO noise estimates for accreted-star candidates for a guest-observer proposal
Computed per-candidate PLATO noise-to-signal ratios and flux contamination for accreted-star candidates, each with its own Gaia DR3 field of contaminants.
- 4,086 candidates, each with a 63 arcsec Gaia DR3 cone to G = 18.5, StarHorse and GSP-Phot parameters and a dedicated noise run.
- Ran noise-to-signal simulations with the HAYDNsim pipeline, with the HAYDN Noise Estimator in its PLATO configuration.
- Feb 2026 to Aug 2027 project
FCT Exploratory Research Project ArqueoGal: Unraveling the evolutionary history of the Milky Way with Galactic Archaeology
Co-Investigator (team member) and developer of the project's machine-learning pipelines (Tasks 3, 5 and 6). PI T. L. Campante.
- Dec 2025 to Sep 2026 HPC
Deucalion development access, University of Porto HPCvLAB
JANUS development and HAYDNsim runs for the HAYDN proposal: 94,001 core-hours in about 250 jobs.
- Sep 2025 to Aug 2026 fellowship
FCT Doctoral Fellowship
- Sep 2021 to Mar 2022 fellowship
MSc research fellowship, BreakStarS project
Research fellowship "Study of the small separation as a constraint in the modelling of red giant stars" (CIAAUP-08/2021-BI-M), in the FCT project BreakStarS at IA Porto (PTDC/FIS-AST/30389/2017).
Education
- Sep 2022 to present degree
PhD in Astronomy
Thesis: Machine Learning Applied to Galactic Archaeology. Advisors: Tiago L. Campante, Diego Bossini, Andrea Miglio.
- Sep 2020 to Dec 2022 degree
MSc in Astronomy and Astrophysics
Thesis: Determination of Age and Mass for Seismic Stars in the Ariel Input Catalog.
- 2017 to Nov 2020 degree
BSc in Physics (Astrophysics branch)
Positions
- Sep 2025 to Mar 2026 abroad
Visiting PhD Student, INAF Osservatorio di Astrofisica e Scienza dello Spazio
Six-month secondment in A. Miglio's group building the HAYDNsim simulation pipeline for the proposed HAYDN mission, with regular visits to INAF Osservatorio Astronomico di Padova.
- Built the noise-estimation and synthetic-catalogue tools (TRILEGAL, King-profile sampling) for globular and open clusters.
- Ran the noise simulations on the Deucalion supercomputer and the University of Bologna clusters.
- Sep 2022 to present position
PhD Researcher, Stellar Astrophysics Group
Doctoral research on machine-learning methods for Galactic archaeology with Gaia, APOGEE and asteroseismic data.
- Developing JANUS, a neural network that predicts APOGEE-like stellar parameters and abundances from Gaia XP spectra, with a reliability score for each star.
- Released Starfold, an open-source package that finds stellar populations without labels and measures how often each one recurs.
- Developer of the machine-learning pipelines of the FCT exploratory project ArqueoGal (2024.15303.PEX), PI T. L. Campante.
- Built a characterisation pipeline that combines Gaia DR3, TESS, Kepler/K2 and 2MASS data with PARAM to estimate stellar ages.
- Sep 2021 to Mar 2022 position
MSc Research Fellow, BreakStarS project
Implemented the small-frequency-separation routine in the stellar characterisation code PARAM.
Observing and schools
- Jul 2024 school
Porto Summer School on Asteroseismology, From Pixels to Stellar Ages
- May 2024 observing
Visiting astronomer, ESPRESSO at the VLT, ESO Paranal Observatory
Visitor-mode run 113.26FX.002 on GJ 570 A for PI T. L. Campante: six nights allocated, five usable.
Awards
- 2023 award
Best Master's Student in Astronomy and Astrophysics
Memberships
- 2022 to present consortium
Affiliate, TESS Asteroseismic Science Operations Centre (TASOC)
- 2022 to present consortium
Member, Kepler Asteroseismic Science Consortium (KASOC), Red-Giant Oscillations working group
- 2021 to present consortium
Member, ESA Ariel Science Consortium, Stellar Characterisation working group (Age, Mass and Radius sub-group)
Service
- Jul 2024 organiser
Local Organising Committee member, TASC8/KASC15 workshop
- Dec 2023 chair
Chair of the Local Organising Committee, IA Stars Day
- 2022 organiser
Local Organising Committee member, IA Stars Day
Teaching and supervision
- Aug 2025 teaching
Tutor, Escola de Verão de Física 2025
One-week summer school for secondary-school students.
- Jun 2025 teaching
Supervisor, IA Summer Programme 2025
Three-week supervision of university students on Galactic archaeology and machine learning with synthetic data.
- Aug 2024 teaching
Tutor, Escola de Verão de Física 2024
One-week summer school for secondary-school students.
- Jul 2024 teaching
Supervisor, IA Summer Programme 2024
Three-week supervision of university students on Galactic archaeology and machine learning with synthetic data.
- Aug 2023 teaching
Tutor, Escola de Verão de Física 2023 (The Colours of the Sun)
One-week summer school for secondary-school students.
Outreach
- Feb 2023 to present outreach
Physics-demonstrations monitor for visiting school groups