KROSS-SAMI: a direct IFS comparison of the Tully-Fisher relation across 8 Gyr since z approximate to 1

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Tiley, A. L., Bureau, M., Cortese, L., Harrison, C. M., Johnson, H. L., Stott, J. P., Swinbank, A. M., Smail, I., Sobral, D., Bunker, A. J., Glazebrook, K., Bower, R. G., Obreschkow, D., Bryant, J. J., Jarvis, M. J., Bland-Hawthorn, J., Magdis, G., Medling, A. M., Sweet, S. M., Tonini, C., Turner, O. J., Sharples, R. M., Croom, S. M., Goodwin, M., Konstantopoulos, I. S., Lorente, N. P. F., Lawrence, J. S., Mould, J., Owers, M. S., Richards, S. N.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Oxford University Press 2019
• Subjects: Galaxies: evolution; Galaxies: general; Galaxies: kinematics and dynamics; Galaxies: star formation; Kross; Zero Point; sami
• Online Access: https://espace.library.uq.edu.au/view/UQ:5cf490a/thumbnail_UQ5cf490a_OA_t.jpg; https://espace.library.uq.edu.au/view/UQ:5cf490a/UQ5cf490a_OA.pdf; https://espace.library.uq.edu.au/view/UQ:5cf490a

We construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially-resolved H alpha emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at z approximate to 1. We compare these to data from the Sydney-Australian-Astronomical-...