MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years

Anastasia A. Ponomareva; Wanga Mulaudzi; Natasha Maddox; Bradley S. Frank; Matt J. Jarvis; Enrico M. Di Teodoro; Marcin Glowacki; Renée C. Kraan-Korteweg; Tom A. Oosterloo; Elizabeth A. K. Adams; Hengxing Pan; Isabella Prandoni; Sambatriniaina H. A. Rajohnson; Francesco Sinigaglia; Nathan J. Adams; Ian Heywood; Rebecca A. A. Bowler; Peter W. Hatfield; Jordan D. Collier; Srikrishna Sekhar

doi:10.1093/mnras/stab2654

MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years

Anastasia A. Ponomareva^*, Wanga Mulaudzi, Natasha Maddox, Bradley S. Frank, Matt J. Jarvis, Enrico M. Di Teodoro, Marcin Glowacki, Renée C. Kraan-Korteweg, Tom A. Oosterloo, Elizabeth A. K. Adams, Hengxing Pan, Isabella Prandoni, Sambatriniaina H. A. Rajohnson, Francesco Sinigaglia, Nathan J. Adams, Ian Heywood, Rebecca A. A. Bowler, Peter W. Hatfield, Jordan D. Collier, Srikrishna Sekhar

^*Corresponding author voor dit werk

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Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H I-based baryonic Tully-Fisher relation (bTFr), covering a period of ~1 billion years (0 ≤ z ≤ 0.081). We consider the bTFr based on two different rotational velocity measures: the width of the global H I profile and V_out, measured as the outermost rotational velocity from the resolved H I rotation curves. Both relations exhibit very low intrinsic scatter orthogonal to the best-fitting relation (σ_⊥ = 0.07 ± 0.01), comparable to the SPARC sample at z ≃ 0. The slopes of the relations are similar and consistent with the z ≃ 0 studies ($3.66^{+0.35}_{-0.29}$ for W₅₀ and $3.47^{+0.37}_{-0.30}$ for V_out). We find no evidence that the bTFr has evolved over the last billion years, and all galaxies in our sample are consistent with the same relation independent of redshift and the rotational velocity measure. Our results set-up a reference for all future studies of the H I-based bTFr as a function of redshift that will be conducted with the ongoing deep SKA pathfinders surveys.

Originele taal-2	English
Pagina's (van-tot)	1195-1205
Aantal pagina's	11
Tijdschrift	Monthly Notices of the Royal Astronomical Society
Volume	508
DOI's	https://doi.org/10.1093/mnras/stab2654
Status	Published - 1-nov.-2021

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10.1093/mnras/stab2654

MIGHTEE-HI: the baryonic Tully–Fisher relation over the last billionyearsFinal publisher's version, 1,43 MBLicentie: Taverne

https://ui.adsabs.harvard.edu/abs/2021MNRAS.508.1195P

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The bTFr of MIGHTEE-H I spiral galaxies
Ponomareva, A. (Creator), Mulaudzi, W. (Creator), Maddox, N. (Creator), Frank, B. S. (Creator), Jarvis, M. J. (Creator), Di Teodoro, E. M. (Creator), Glowacki, M. (Creator), Kraan-Korteweg, R. C. (Creator), Oosterloo, T. A. (Creator), Adams, E. A. K. (Creator), Pan, H. (Creator), Prandoni, I. (Creator), Rajohnson, S. H. A. (Contributor), Sinigaglia, F. (Creator), Adams, N. J. (Creator), Heywood, I. (Creator), Bowler, R. A. A. (Contributor), Hatfield, P. W. (Creator), Collier, J. D. (Creator) & Sekhar, S. (Creator), Centre de Donnees Strasbourg (CDS), 11-sep.-2024
DOI: 10.26093/cds/vizier.75081195
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Ponomareva, A. A., Mulaudzi, W., Maddox, N., Frank, B. S., Jarvis, M. J., Teodoro, E. M. D., Glowacki, M., Kraan-Korteweg, R. C., Oosterloo, T. A., Adams, E. A. K., Pan, H., Prandoni, I., Rajohnson, S. H. A., Sinigaglia, F., Adams, N. J., Heywood, I., Bowler, R. A. A., Hatfield, P. W., Collier, J. D., & Sekhar, S. (2021). MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years. Monthly Notices of the Royal Astronomical Society, 508, 1195-1205. https://doi.org/10.1093/mnras/stab2654

@article{5dd258cf7dd2408cb89f0d91924f76ed,

title = "MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years",

abstract = "Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H I-based baryonic Tully-Fisher relation (bTFr), covering a period of ~1 billion years (0 ≤ z ≤ 0.081). We consider the bTFr based on two different rotational velocity measures: the width of the global H I profile and Vout, measured as the outermost rotational velocity from the resolved H I rotation curves. Both relations exhibit very low intrinsic scatter orthogonal to the best-fitting relation (σ⊥ = 0.07 ± 0.01), comparable to the SPARC sample at z ≃ 0. The slopes of the relations are similar and consistent with the z ≃ 0 studies ($3.66^{+0.35}_{-0.29}$ for W50 and $3.47^{+0.37}_{-0.30}$ for Vout). We find no evidence that the bTFr has evolved over the last billion years, and all galaxies in our sample are consistent with the same relation independent of redshift and the rotational velocity measure. Our results set-up a reference for all future studies of the H I-based bTFr as a function of redshift that will be conducted with the ongoing deep SKA pathfinders surveys.",

keywords = "Galaxies: evolution, Galaxies: kinematics and dynamics, Galaxies: spiral, dark matter, Astrophysics - Astrophysics of Galaxies",

author = "Ponomareva, {Anastasia A.} and Wanga Mulaudzi and Natasha Maddox and Frank, {Bradley S.} and Jarvis, {Matt J.} and Teodoro, {Enrico M. Di} and Marcin Glowacki and Kraan-Korteweg, {Ren{\'e}e C.} and Oosterloo, {Tom A.} and Adams, {Elizabeth A. K.} and Hengxing Pan and Isabella Prandoni and Rajohnson, {Sambatriniaina H. A.} and Francesco Sinigaglia and Adams, {Nathan J.} and Ian Heywood and Bowler, {Rebecca A. A.} and Hatfield, {Peter W.} and Collier, {Jordan D.} and Srikrishna Sekhar",

year = "2021",

month = nov,

day = "1",

doi = "10.1093/mnras/stab2654",

language = "English",

volume = "508",

pages = "1195--1205",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

}

Ponomareva, AA, Mulaudzi, W, Maddox, N, Frank, BS, Jarvis, MJ, Teodoro, EMD, Glowacki, M, Kraan-Korteweg, RC, Oosterloo, TA , Adams, EAK, Pan, H, Prandoni, I, Rajohnson, SHA, Sinigaglia, F, Adams, NJ, Heywood, I, Bowler, RAA, Hatfield, PW, Collier, JD & Sekhar, S 2021, 'MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years', Monthly Notices of the Royal Astronomical Society, vol. 508, blz. 1195-1205. https://doi.org/10.1093/mnras/stab2654

TY - JOUR

T1 - MIGHTEE-H I

T2 - The baryonic Tully-Fisher relation over the last billion years

AU - Ponomareva, Anastasia A.

AU - Mulaudzi, Wanga

AU - Maddox, Natasha

AU - Frank, Bradley S.

AU - Jarvis, Matt J.

AU - Teodoro, Enrico M. Di

AU - Glowacki, Marcin

AU - Kraan-Korteweg, Renée C.

AU - Oosterloo, Tom A.

AU - Adams, Elizabeth A. K.

AU - Pan, Hengxing

AU - Prandoni, Isabella

AU - Rajohnson, Sambatriniaina H. A.

AU - Sinigaglia, Francesco

AU - Adams, Nathan J.

AU - Heywood, Ian

AU - Bowler, Rebecca A. A.

AU - Hatfield, Peter W.

AU - Collier, Jordan D.

AU - Sekhar, Srikrishna

PY - 2021/11/1

Y1 - 2021/11/1

N2 - Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H I-based baryonic Tully-Fisher relation (bTFr), covering a period of ~1 billion years (0 ≤ z ≤ 0.081). We consider the bTFr based on two different rotational velocity measures: the width of the global H I profile and Vout, measured as the outermost rotational velocity from the resolved H I rotation curves. Both relations exhibit very low intrinsic scatter orthogonal to the best-fitting relation (σ⊥ = 0.07 ± 0.01), comparable to the SPARC sample at z ≃ 0. The slopes of the relations are similar and consistent with the z ≃ 0 studies ($3.66^{+0.35}_{-0.29}$ for W50 and $3.47^{+0.37}_{-0.30}$ for Vout). We find no evidence that the bTFr has evolved over the last billion years, and all galaxies in our sample are consistent with the same relation independent of redshift and the rotational velocity measure. Our results set-up a reference for all future studies of the H I-based bTFr as a function of redshift that will be conducted with the ongoing deep SKA pathfinders surveys.

AB - Using a sample of 67 galaxies from the MeerKAT International GigaHertz Tiered Extragalactic Exploration Survey Early Science data, we study the H I-based baryonic Tully-Fisher relation (bTFr), covering a period of ~1 billion years (0 ≤ z ≤ 0.081). We consider the bTFr based on two different rotational velocity measures: the width of the global H I profile and Vout, measured as the outermost rotational velocity from the resolved H I rotation curves. Both relations exhibit very low intrinsic scatter orthogonal to the best-fitting relation (σ⊥ = 0.07 ± 0.01), comparable to the SPARC sample at z ≃ 0. The slopes of the relations are similar and consistent with the z ≃ 0 studies ($3.66^{+0.35}_{-0.29}$ for W50 and $3.47^{+0.37}_{-0.30}$ for Vout). We find no evidence that the bTFr has evolved over the last billion years, and all galaxies in our sample are consistent with the same relation independent of redshift and the rotational velocity measure. Our results set-up a reference for all future studies of the H I-based bTFr as a function of redshift that will be conducted with the ongoing deep SKA pathfinders surveys.

KW - Galaxies: evolution

KW - Galaxies: kinematics and dynamics

KW - Galaxies: spiral

KW - dark matter

KW - Astrophysics - Astrophysics of Galaxies

U2 - 10.1093/mnras/stab2654

DO - 10.1093/mnras/stab2654

M3 - Article

SN - 0035-8711

VL - 508

SP - 1195

EP - 1205

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

ER -

MIGHTEE-H I: The baryonic Tully-Fisher relation over the last billion years

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The bTFr of MIGHTEE-H I spiral galaxies

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