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

  1. Nov 2026 to Nov 2027 HPC

    FCT Advanced Computing Project 2026.08382.CPCA.A1: JANUS on Deucalion, Gaia DR3

    2026.08382.CPCA.A1 · FCT I.P. · principal investigator · co-responsible investigator T. L. Campante

    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.
  2. Nov 2026 to Nov 2027 HPC

    FCT Advanced Computing Project 2026.08362.CPCA.A2: JANUS on MareNostrum 5, Gaia DR4

    2026.08362.CPCA.A2 · FCT I.P. · principal investigator · co-responsible investigator T. L. Campante

    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.
  3. Sep 2026 to Aug 2027 fellowship

    PhD research fellowship under the FCT project ArqueoGal

    CIAAUP-17/2026-BI-D · FCT, through project 2024.15303.PEX, hosted at IA · PI Tiago L. Campante

  4. May 2026 proposal

    PLATO noise estimates for a blue-straggler guest-observer proposal (34 open clusters)

    Co-investigator

    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.
  5. May 2026 proposal

    PLATO noise estimates for the NGC 1851 red-giant guest-observer proposal

    Co-investigator

    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

      Co-investigator

      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

      2024.15303.PEX · Fundação para a Ciência e a Tecnologia · Co-Investigator (team member) · PI Tiago L. Campante

      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

      2025.00007.HPCVLAB.UPORTO · FCT I.P., High Performance Computing Virtual Laboratory · team member

      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

      2025.01843.BD · Fundação para a Ciência e a Tecnologia

    • Sep 2021 to Mar 2022 fellowship

      MSc research fellowship, BreakStarS project

      CIAAUP-08/2021-BI-M · Fundação para a Ciência e a Tecnologia, through IA/CAUP

      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

    1. Sep 2022 to present degree

      PhD in Astronomy

      Faculdade de Ciências da Universidade do Porto and IA/CAUP · Porto, Portugal

      Thesis: Machine Learning Applied to Galactic Archaeology. Advisors: Tiago L. Campante, Diego Bossini, Andrea Miglio.

    2. Sep 2020 to Dec 2022 degree

      MSc in Astronomy and Astrophysics

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

      Thesis: Determination of Age and Mass for Seismic Stars in the Ariel Input Catalog.

    3. 2017 to Nov 2020 degree

      BSc in Physics (Astrophysics branch)

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

    Positions

    1. Sep 2025 to Mar 2026 abroad

      Visiting PhD Student, INAF Osservatorio di Astrofisica e Scienza dello Spazio

      INAF-OAS Bologna · Bologna, Italy

      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.
    2. Sep 2022 to present position

      PhD Researcher, Stellar Astrophysics Group

      IA/CAUP · Porto, Portugal

      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.
    3. Sep 2021 to Mar 2022 position

      MSc Research Fellow, BreakStarS project

      IA/CAUP · Porto, Portugal

      Implemented the small-frequency-separation routine in the stellar characterisation code PARAM.

    Observing and schools

    1. Jul 2024 school

      Porto Summer School on Asteroseismology, From Pixels to Stellar Ages

      Vila do Conde, Portugal

    2. May 2024 observing

      Visiting astronomer, ESPRESSO at the VLT, ESO Paranal Observatory

      Paranal, Chile

      Visitor-mode run 113.26FX.002 on GJ 570 A for PI T. L. Campante: six nights allocated, five usable.

    Awards

    1. 2023 award

      Best Master's Student in Astronomy and Astrophysics

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

    Memberships

    1. 2022 to present consortium

      Affiliate, TESS Asteroseismic Science Operations Centre (TASOC)

    2. 2022 to present consortium

      Member, Kepler Asteroseismic Science Consortium (KASOC), Red-Giant Oscillations working group

    3. 2021 to present consortium

      Member, ESA Ariel Science Consortium, Stellar Characterisation working group (Age, Mass and Radius sub-group)

    Service

    1. Jul 2024 organiser

      Local Organising Committee member, TASC8/KASC15 workshop

      TASC8/KASC15, 8th TESS and 15th Kepler Asteroseismic Science Consortium Workshop · Porto, Portugal

    2. Dec 2023 chair

      Chair of the Local Organising Committee, IA Stars Day

      IA Stars Day · Porto, Portugal

    3. 2022 organiser

      Local Organising Committee member, IA Stars Day

      IA Stars Day · Porto, Portugal

    Teaching and supervision

    1. Aug 2025 teaching

      Tutor, Escola de Verão de Física 2025

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

      One-week summer school for secondary-school students.

    2. Jun 2025 teaching

      Supervisor, IA Summer Programme 2025

      IA/CAUP · Porto, Portugal

      Three-week supervision of university students on Galactic archaeology and machine learning with synthetic data.

    3. Aug 2024 teaching

      Tutor, Escola de Verão de Física 2024

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

      One-week summer school for secondary-school students.

    4. Jul 2024 teaching

      Supervisor, IA Summer Programme 2024

      IA/CAUP · Porto, Portugal

      Three-week supervision of university students on Galactic archaeology and machine learning with synthetic data.

    5. Aug 2023 teaching

      Tutor, Escola de Verão de Física 2023 (The Colours of the Sun)

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal

      One-week summer school for secondary-school students.

    Outreach

    1. Feb 2023 to present outreach

      Physics-demonstrations monitor for visiting school groups

      Faculdade de Ciências da Universidade do Porto · Porto, Portugal