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• W2896774662 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 criteria to both to conduct a direct comparison of the absolute K-band magnitude and stellar mass TFRs at z ≈ 1 and 0. We find that matching the quality of the SAMI data to that of KROSS results in TFRs that differ significantly in slope, zero-point, and (sometimes) scatter in comparison to the corresponding original SAMI relations. These differences are in every case as large as or larger than the differences between the KROSS z ≈ 1 and matched SAMI z ≈ 0 relations. Accounting for these differences, we compare the TFRs at z ≈ 1 and 0. For disc-like, star-forming galaxies we find no significant difference in the TFR zero-points between the two epochs. This suggests the growth of stellar mass and dark matter in these types of galaxies is intimately linked over this ≈8 Gyr period." @default.
• W2896774662 created "2018-10-26" @default.
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• W2896774662 date "2018-10-17" @default.
• W2896774662 modified "2023-10-16" @default.
• W2896774662 title "KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since<i>z</i> ≈ 1" @default.
• W2896774662 cites W1607434071 @default.
• W2896774662 cites W1830177387 @default.
• W2896774662 cites W1911962099 @default.
• W2896774662 cites W1967037608 @default.
• W2896774662 cites W1970058472 @default.
• W2896774662 cites W1985952407 @default.
• W2896774662 cites W1986486448 @default.
• W2896774662 cites W1990491187 @default.
• W2896774662 cites W1994671833 @default.
• W2896774662 cites W1996537612 @default.
• W2896774662 cites W1998754913 @default.
• W2896774662 cites W2002482748 @default.
• W2896774662 cites W2004294893 @default.
• W2896774662 cites W2011437259 @default.
• W2896774662 cites W2015637674 @default.
• W2896774662 cites W2019198220 @default.
• W2896774662 cites W2019669573 @default.
• W2896774662 cites W2021590434 @default.
• W2896774662 cites W2025796785 @default.
• W2896774662 cites W2030326695 @default.
• W2896774662 cites W2032988955 @default.
• W2896774662 cites W2033690542 @default.
• W2896774662 cites W2034660746 @default.
• W2896774662 cites W2038101582 @default.
• W2896774662 cites W2052937506 @default.
• W2896774662 cites W2054460449 @default.
• W2896774662 cites W2056056926 @default.
• W2896774662 cites W2057101560 @default.
• W2896774662 cites W2064238820 @default.
• W2896774662 cites W2065550354 @default.
• W2896774662 cites W2065727797 @default.
• W2896774662 cites W2066675108 @default.
• W2896774662 cites W2068962850 @default.
• W2896774662 cites W2074259384 @default.
• W2896774662 cites W2082108152 @default.
• W2896774662 cites W2088034685 @default.
• W2896774662 cites W2095855161 @default.
• W2896774662 cites W2109510044 @default.
• W2896774662 cites W2110974947 @default.
• W2896774662 cites W2115023978 @default.
• W2896774662 cites W2119131940 @default.
• W2896774662 cites W2120241018 @default.
• W2896774662 cites W2121173473 @default.
• W2896774662 cites W2122471784 @default.
• W2896774662 cites W2123681429 @default.
• W2896774662 cites W2140887005 @default.
• W2896774662 cites W2142238829 @default.
• W2896774662 cites W2150331774 @default.
• W2896774662 cites W2152940085 @default.
• W2896774662 cites W2157389393 @default.
• W2896774662 cites W2162846384 @default.
• W2896774662 cites W2163814628 @default.
• W2896774662 cites W2167335950 @default.
• W2896774662 cites W2188589973 @default.
• W2896774662 cites W2239278317 @default.
• W2896774662 cites W2266791727 @default.
• W2896774662 cites W2335958557 @default.
• W2896774662 cites W2337947861 @default.
• W2896774662 cites W2471279288 @default.
• W2896774662 cites W2479052710 @default.
• W2896774662 cites W2493568130 @default.
• W2896774662 cites W2505702019 @default.
• W2896774662 cites W2580780033 @default.

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