Dr Romain Thomas
School of Computer Science
Head of Research Software Engineering
romain.thomas@sheffield.ac.uk
Regent Court (DCS)
Full contact details
Dr Romain Thomas
School of Computer Science
Regent Court (DCS)
211 Portobello
Sheffield
S1 4DP
School of Computer Science
Regent Court (DCS)
211 Portobello
Sheffield
S1 4DP
- Profile
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Dr Romain Thomas is the Head of Research Software Engineering at the University of Sheffield. His role is to lead a group of research software engineers (RSEs) who are collaborating with research groups at the University to deliver high quality research software.
Before coming to Sheffield, Romain was a Staff Astronomer at the European Southern Observatory (ESO) in Chile where he was leading software projects for data quality control at the Very Large Telescopes.
- Research interests
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Software, Open source, Open research, FAIR, Data
- Publications
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Journal articles
- Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey. Astronomy & Astrophysics, 666, A56-A56.
- The VIMOS Ultra Deep Survey: The reversal of the star-formation rate − density relation at 2 <z< 5. Astronomy & Astrophysics, 662, A33-A33.
- Less and more IGM-transmitted galaxies from z ∼ 2.7 to z ∼ 6 from VANDELS and VUDS. Astronomy & Astrophysics, 650, A63-A63.
- The VANDELS ESO public spectroscopic survey. Astronomy & Astrophysics, 647, A150-A150.
- SPARTAN: Maximizing the use of spectro-photometric observational data during template fitting. Astronomy and Computing, 34, 100427-100427.
- The ALPINE-ALMA [CII] survey. Astronomy & Astrophysics, 643, A1-A1.
- Spectroscopic observations of the machine-learning selected anomaly catalogue from the AllWISE Sky Survey. Astronomy & Astrophysics, 642, A103-A103.
- The intergalactic medium transmission towards z ≳ 4 galaxies with VANDELS and the impact of dust attenuation. Astronomy & Astrophysics, 634, A110-A110.
- SEDOBS: A tool to create simulated galaxy observations. Astronomy and Computing, 30, 100354-100354.
- The most massive, passive, and oldest galaxies at 0.5 < z < 2.1: Downsizing signature from galaxies selected from MgUV index. Astronomy & Astrophysics, 630, A145-A145.
- dfitspy: a dfits|fitsort implementation in python. Journal of Open Source Software, 4(35), 1249-1249.
- The progeny of a cosmic titan: a massive multi-component proto-supercluster in formation at z = 2.45 in VUDS. Astronomy & Astrophysics, 619, A49-A49.
- The VANDELS ESO public spectroscopic survey: Observations and first data release. Astronomy & Astrophysics, 616, A174-A174.
- The VIMOS Ultra-Deep Survey: Emerging from the dark, a massive proto-cluster at z ~ 4.57. Astronomy & Astrophysics, 615, A77-A77.
- The VIMOS Ultra Deep Survey. Astronomy & Astrophysics, 606, A19-A19.
- The extended epoch of galaxy formation: Age dating of ~3600 galaxies with 2 <z< 6.5 in the VIMOS Ultra-Deep Survey. Astronomy & Astrophysics, 602, A35-A35.
- New constraints on the average escape fraction of Lyman continuum radiation in z ~ 4 galaxies from the VIMOS Ultra Deep Survey (VUDS). Astronomy & Astrophysics, 601, A73-A73.
- The VIMOS Ultra Deep Survey first data release: Spectra and spectroscopic redshifts of 698 objects up to zspec ~ 6 in CANDELS. Astronomy & Astrophysics, 600, A110-A110.
- VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies with 2.5 < z < 5.5 and the colour selection of high-redshift galaxies. Astronomy & Astrophysics, 597, A88-A88.
- Effect of the star formation histories on theSFR-M∗relation atz≥ 2. Astronomy & Astrophysics, 593, A9-A9.
- The VIMOS Ultra Deep Survey: Lyαemission and stellar populations of star-forming galaxies at 2 < z < 2.5. Astronomy & Astrophysics, 588, A26-A26.
- Limits on the LyC signal fromz~ 3 sources with secure redshift and HST coverage in the E-CDFS field. Astronomy & Astrophysics, 587, A133-A133.
- The Lyman continuum escape fraction of galaxies atz= 3.3 in the VUDS-LBC/COSMOS field. Astronomy & Astrophysics, 585, A48-A48.
- Evolution of clustering length, large-scale bias, and host halo mass at 2 <z< 5 in the VIMOS Ultra Deep Survey (VUDS). Astronomy & Astrophysics, 583, A128-A128.
- The evolving star formation rate:M⋆relation and sSFR sincez≃ 5 from the VUDS spectroscopic survey. Astronomy & Astrophysics, 581, A54-A54.
- The VIMOS Ultra-Deep Survey: ~10 000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2 <z≃ 6. Astronomy & Astrophysics, 576, A79-A79.
- Stellar mass to halo mass relation from galaxy clustering in VUDS: a high star formation efficiency atz≃ 3. Astronomy & Astrophysics, 576, L7-L7.
- The VIMOS Ultra-Deep Survey (VUDS): fast increase in the fraction of strong Lyman-αemitters fromz= 2 toz= 6. Astronomy & Astrophysics, 573, A24-A24.
- VIMOS Ultra-Deep Survey (VUDS): Witnessing the assembly of a massive cluster atz~ 3.3. Astronomy & Astrophysics, 572, A41-A41.
- Discovery of a rich proto-cluster atz= 2.9 and associated diffuse cold gas in the VIMOS Ultra-Deep Survey (VUDS). Astronomy & Astrophysics, 570, A16-A16.
- Discovering extremely compact and metal-poor, star-forming dwarf galaxies out toz~ 0.9 in the VIMOS Ultra-Deep Survey. Astronomy & Astrophysics, 568, L8-L8.
- Mass assembly in quiescent and star-forming galaxies sincez≃ 4 from UltraVISTA. Astronomy & Astrophysics, 556, A55-A55.
- Gravitational Entropy of Black Holes and Wormholes. International Journal of Theoretical Physics, 51(3), 925-942.
- The VANDELS ESO public spectroscopic survey. Monthly Notices of the Royal Astronomical Society.
- Correction: Corrigendum: Analogues of primeval galaxies two billion years after the Big Bang. Nature Astronomy, 1(4).
- Analogues of primeval galaxies two billion years after the Big Bang. Nature Astronomy, 1(3).
Conference proceedings papers
- The SCUBA project: First layer of quality control at the Paranal Observatory. Observatory Operations: Strategies, Processes, and Systems VIII (pp 10-10), 14 December 2020 - 18 December 2020.
- Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey. Astronomy & Astrophysics, 666, A56-A56.