Phone
226 089 847

Email
Tom.Scott@astro.up.pt

ORCID
0000-0002-3746-4859

Biographic Notes
Tom Scott obtained his bachelor, masters and PhD degrees from the University of Hertfordshire, in the UK and moved to Porto with a FCT Fellowship in 2015. Tom's research interests include the evolution of late-type galaxies in galaxy clusters, particularly the cold gas components (HI and molecular gas) and the formation and evolution of dwarf galaxies in different environments, especially tidal dwarf galaxies.

Lastest publications at IA (or with IA Researchers)T. C. Scott, E. Brinks, C. Sengupta, P. Lagos, 2024,
High-resolution HI mapping of nearby extremely metal-poor blue compact dwarf galaxies,
Astronomy & Astrophysics, 692, 16
>> AbstractY. Guo, C. Sengupta, T. C. Scott, P. Lagos, Y. Luo, 2024,
Catalogue of nearby blue and near-solar gas metallicity SDSS dwarf galaxies,
Monthly Notices of the Royal Astronomical Society, 528, 14
>> AbstractY. Guo, C. Sengupta, T. C. Scott, P. Lagos, Y. Luo, 2023,
H_ı in High Gas-phase Metallicity Dwarf Galaxy WISEA J230615.06+143927.9,
Research in Astronomy and Astrophysics, 24, 11
>> AbstractN. Deg, K. Spekkens, T. Westmeier, T. N. Reynolds, P. Venkataraman, S. Goliath, A. X. Shen, R. Halloran, A. Bosma, B. Catinella et al. (including: T. C. Scott), 2022,
WALLABY Pilot Survey: Public release of HI kinematic models for more than 100 galaxies from phase 1 of ASKAP pilot observations,
Publications of the Astronomical Society of Australia, 39
>> AbstractP. Lagos, S. I. Loubser, T. C. Scott, E. O'Sullivan, K. Kolokythas, A. Babul, A. Nigoche-Netro, V. Olivares, C. Sengupta, 2022,
Spatially resolved properties of early-type group-dominant galaxies with MUSE: gas content, ionization mechanisms, and metallicity gradients,
Monthly Notices of the Royal Astronomical Society, 516, 5487 - 5506
>> AbstractY. -F. Zhou, C. Sengupta, Y. Chandola, O. I. Wong, T. C. Scott, Y. -Z. Ma, H. Chen, 2022,
HIPASS study of southern ultradiffuse galaxies and low surface brightness galaxies,
Monthly Notices of the Royal Astronomical Society, 516, 1781 - 1787
>> Abstract