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    Rights statement: This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated versionA L Tiley, M Bureau, L Cortese, C M Harrison, H L Johnson, J P Stott, A M Swinbank, I Smail, D Sobral, A J Bunker, K Glazebrook, R G Bower, D Obreschkow, J J Bryant, M J Jarvis, J Bland-Hawthorn, G Magdis, A M Medling, S M Sweet, C Tonini, O J Turner, R M Sharples, S M Croom, M Goodwin, I S Konstantopoulos, N P F Lorente, J S Lawrence, J Mould, M S Owers, S N Richards; KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1, Monthly Notices of the Royal Astronomical Society, Volume 482, Issue 2, 11 January 2019, Pages 2166–2188, https://doi.org/10.1093/mnras/sty2794 is available online at: https://academic.oup.com/mnras/article/482/2/2166/5134162

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

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

In: Monthly Notices of the Royal Astronomical Society, Vol. 482, No. 2, 11.01.2019, p. 2166–2188.

Research output: Contribution to journalJournal article

Harvard

Tiley, AL, Bureau, M, Cortese, L, Harrison, CM, Johnson, HL, Stott, JP, Swinbank, AM, Smail, I, Sobral, D, Bunker, AJ, Glazebrook, K, Bower, RG, Obreschkow, D, Bryant, JJ, Jarvis, MJ, Bland-Hawthorn, J, Magdis, G, Medling, AM, Sweet, SM, Tonini, C, Turner, OJ, Sharples, RM, Croom, SM, Goodwin, M, Konstantopoulos, IS, Lorente, NPF, Lawrence, JS, Mould, J, Owers, MS & Richards, SN 2019, 'KROSS-SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1', Monthly Notices of the Royal Astronomical Society, vol. 482, no. 2, pp. 2166–2188. https://doi.org/10.1093/mnras/sty2794

APA

Tiley, A. L., Bureau, M., Cortese, L., Harrison, C. M., Johnson, H. L., Stott, J. P., ... Richards, S. N. (2019). KROSS-SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1. Monthly Notices of the Royal Astronomical Society, 482(2), 2166–2188. https://doi.org/10.1093/mnras/sty2794

Vancouver

Tiley AL, Bureau M, Cortese L, Harrison CM, Johnson HL, Stott JP et al. KROSS-SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1. Monthly Notices of the Royal Astronomical Society. 2019 Jan 11;482(2):2166–2188. https://doi.org/10.1093/mnras/sty2794

Author

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. / KROSS-SAMI : a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 482, No. 2. pp. 2166–2188.

Bibtex

@article{3c7f8a792c3940459be8f9bf0f01ba78,
title = "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 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.",
keywords = "astro-ph.GA",
author = "Tiley, {A. L.} and M. Bureau and L. Cortese and Harrison, {C. M.} and Johnson, {H. L.} and Stott, {J. P.} and Swinbank, {A. M.} and I. Smail and D. Sobral and Bunker, {A. J.} and K. Glazebrook and Bower, {R. G.} and D. Obreschkow and Bryant, {J. J.} and Jarvis, {M. J.} and J. Bland-Hawthorn and G. Magdis and Medling, {A. M.} and Sweet, {S. M.} and C. Tonini and Turner, {O. J.} and Sharples, {R. M.} and Croom, {S. M.} and M. Goodwin and Konstantopoulos, {I. S.} and Lorente, {N. P. F.} and Lawrence, {J. S.} and J. Mould and Owers, {M. S.} and Richards, {S. N.}",
note = "This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated versionA L Tiley, M Bureau, L Cortese, C M Harrison, H L Johnson, J P Stott, A M Swinbank, I Smail, D Sobral, A J Bunker, K Glazebrook, R G Bower, D Obreschkow, J J Bryant, M J Jarvis, J Bland-Hawthorn, G Magdis, A M Medling, S M Sweet, C Tonini, O J Turner, R M Sharples, S M Croom, M Goodwin, I S Konstantopoulos, N P F Lorente, J S Lawrence, J Mould, M S Owers, S N Richards; KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1, Monthly Notices of the Royal Astronomical Society, Volume 482, Issue 2, 11 January 2019, Pages 2166–2188, https://doi.org/10.1093/mnras/sty2794 is available online at: https://academic.oup.com/mnras/article/482/2/2166/5134162",
year = "2019",
month = "1",
day = "11",
doi = "10.1093/mnras/sty2794",
language = "English",
volume = "482",
pages = "2166–2188",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "2",

}

RIS

TY - JOUR

T1 - KROSS-SAMI

T2 - a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1

AU - Tiley, A. L.

AU - Bureau, M.

AU - Cortese, L.

AU - Harrison, C. M.

AU - Johnson, H. L.

AU - Stott, J. P.

AU - Swinbank, A. M.

AU - Smail, I.

AU - Sobral, D.

AU - Bunker, A. J.

AU - Glazebrook, K.

AU - Bower, R. G.

AU - Obreschkow, D.

AU - Bryant, J. J.

AU - Jarvis, M. J.

AU - Bland-Hawthorn, J.

AU - Magdis, G.

AU - Medling, A. M.

AU - Sweet, S. M.

AU - Tonini, C.

AU - Turner, O. J.

AU - Sharples, R. M.

AU - Croom, S. M.

AU - Goodwin, M.

AU - Konstantopoulos, I. S.

AU - Lorente, N. P. F.

AU - Lawrence, J. S.

AU - Mould, J.

AU - Owers, M. S.

AU - Richards, S. N.

N1 - This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated versionA L Tiley, M Bureau, L Cortese, C M Harrison, H L Johnson, J P Stott, A M Swinbank, I Smail, D Sobral, A J Bunker, K Glazebrook, R G Bower, D Obreschkow, J J Bryant, M J Jarvis, J Bland-Hawthorn, G Magdis, A M Medling, S M Sweet, C Tonini, O J Turner, R M Sharples, S M Croom, M Goodwin, I S Konstantopoulos, N P F Lorente, J S Lawrence, J Mould, M S Owers, S N Richards; KROSS–SAMI: a direct IFS comparison of the Tully–Fisher relation across 8 Gyr since z ≈ 1, Monthly Notices of the Royal Astronomical Society, Volume 482, Issue 2, 11 January 2019, Pages 2166–2188, https://doi.org/10.1093/mnras/sty2794 is available online at: https://academic.oup.com/mnras/article/482/2/2166/5134162

PY - 2019/1/11

Y1 - 2019/1/11

N2 - 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.

AB - 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.

KW - astro-ph.GA

U2 - 10.1093/mnras/sty2794

DO - 10.1093/mnras/sty2794

M3 - Journal article

VL - 482

SP - 2166

EP - 2188

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 2

ER -