Browse by author
Lookup NU author(s): Dr Chris HarrisonORCiD
This is the final published version of an article that has been published in its final definitive form by Oxford University Press, 2016.
For re-use rights please refer to the publisher's terms and conditions.
© 2016 The Authors. Published by Oxford University Press on behalf of The Royal Astronomical Society.We present the stellar mass (M*), and K-corrected K-band absolute magnitude (MK) Tully- Fisher relations (TFRs) for subsamples of the 584 galaxies spatially resolved in H α emission by the KMOS Redshift One Spectroscopic Survey (KROSS). We model the velocity field of each of the KROSS galaxies and extract a rotation velocity, V80 at a radius equal to the major axis of an ellipse containing 80 per cent of the total integrated H α flux. The large sample size of KROSS allowed us to select 210 galaxies with well-measured rotation speeds. We extract from this sample a further 56 galaxies that are rotationally supported, using the stringent criterion V80/s σ > 3, where s is the flux weighted average velocity dispersion. We find the MK and M* TFRs for this subsample to be MK/mag = (-7.3 ± 0.9) × [(log(V80/km s-1) - 2.25] - 23.4 ± 0.2, and log(M*/M⊙) = (4.7 ± 0.4) × [(log(V80/km s-1) - 2.25] + 10.0 ± 0.3, respectively. We find an evolution of the M* TFR zero-point of -0.41 ± 0.08 dex over the last ~8 billion years. However, we measure no evolution in the MK TFR zero-point over the same period. We conclude that rotationally supported galaxies of a given dynamical mass had less stellar mass at z ~ 1 than the present day, yet emitted the same amounts of K-band light. The ability of KROSS to differentiate, using integral field spectroscopy with KMOS, between those galaxies that are rotationally supported and those that are not explains why our findings are at odds with previous studies without the same capabilities.
Author(s): Tiley AL, Stott JP, Swinbank AM, Bureau M, Harrison CM, Bower R, Johnson HL, Bunker AJ, Jarvis MJ, Magdis G, Sharples R, Smail I, Sobral D, Best P
Publication type: Article
Publication status: Published
Journal: Monthly Notices of the Royal Astronomical Society
Year: 2016
Volume: 460
Issue: 1
Pages: 103-129
Print publication date: 21/07/2016
Online publication date: 21/04/2016
Acceptance date: 19/04/2016
Date deposited: 04/02/2020
ISSN (print): 0035-8711
ISSN (electronic): 1365-2966
Publisher: Oxford University Press
URL: https://doi.org/10.1093/mnras/stw936
DOI: 10.1093/mnras/stw936
Altmetrics provided by Altmetric
