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KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1

Abstract:

We construct Tully–Fisher relations (TFRs), from large samples of galaxies with spatially resolved H α emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at z ≈ 1. We compare these to data from the Sydney-Australian-Astronomical-Observatory Multi-object Integral-Field Spectrograph (SAMI) Galaxy Survey at z ≈ 0. We stringently match the data quality of the latter to the former, and apply identical analysis methods and sub-sample selection c...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's Version

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Publisher copy:
10.1093/mnras/sty2794

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics
Subgroup:
Astrophysics
Oxford college:
Wadham College
ORCID:
0000-0003-4980-1012
Cortese, L More by this author
Harrison, CM More by this author
Johnson, HL More by this author
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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
482
Issue:
2
Pages:
2166–2188
Publication date:
2018-10-17
Acceptance date:
2018-10-15
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:935943
URN:
uri:e0dede57-7f4e-4bc8-81cf-616762e298dc
UUID:
uuid:e0dede57-7f4e-4bc8-81cf-616762e298dc
Local pid:
pubs:935943

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