Dr
Romain
Thomas
School of Computer Science
Head of Research Software Engineering
romain.thomas@sheffield.ac.uk
Regent Court (CS)
Full contact details
Dr Romain Thomas
School of Computer Science
Regent Court (CS)
School of Computer Science
Regent Court (CS)
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
- STON: SofTware for petrOgraphic visualisatioN. Journal of Open Source Software, 10(115), 8144-8144.
- 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
- 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.
Preprints
- The less and the more IGM transmitted galaxies from z~2.7 to z~6 from
VANDELS and VUDS.
- The Intergalactic medium transmission towards z>4 galaxies with VANDELS
and the impact of dust attenuation.
- The most massive, passive, and oldest galaxies at 0.5 < z < 2.1:
Downsizing signature from galaxies selected from MgUV index.
- The VIMOS Ultra-Deep Survey (VUDS): IGM transmission towards galaxies
with 2.5
- STON: SofTware for petrOgraphic visualisatioN. Journal of Open Source Software, 10(115), 8144-8144.