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  • 1804.02402v1

    Rights statement: This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/aabc55

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Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies

Research output: Contribution to Journal/Magazine › Journal article › peer-review

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Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies. / Bezanson, Rachel; Wel, Arjen van der; Pacifici, Camilla et al.
In: The Astrophysical Journal, Vol. 858, No. 1, 60, 04.05.2018.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Bezanson, R, Wel, AVD, Pacifici, C, Noeske, K, Barišić, I, Bell, EF, Brammer, GB, Calhau, J, Chauke, P, Dokkum, PV, Franx, M, Gallazzi, A, Houdt, JV, Labbé, I, Maseda, MV, Muños-Mateos, JC, Muzzin, A, Sande, JVD, Sobral, D, Straatman, C & Wu, P-F 2018, 'Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies', The Astrophysical Journal, vol. 858, no. 1, 60. https://doi.org/10.3847/1538-4357/aabc55

APA

Bezanson, R., Wel, A. V. D., Pacifici, C., Noeske, K., Barišić, I., Bell, E. F., Brammer, G. B., Calhau, J., Chauke, P., Dokkum, P. V., Franx, M., Gallazzi, A., Houdt, J. V., Labbé, I., Maseda, M. V., Muños-Mateos, J. C., Muzzin, A., Sande, J. V. D., Sobral, D., ... Wu, P-F. (2018). Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies. The Astrophysical Journal, 858(1), Article 60. https://doi.org/10.3847/1538-4357/aabc55

Vancouver

Bezanson R, Wel AVD, Pacifici C, Noeske K, Barišić I, Bell EF et al. Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies. The Astrophysical Journal. 2018 May 4;858(1):60. doi: 10.3847/1538-4357/aabc55

Author

Bezanson, Rachel ; Wel, Arjen van der ; Pacifici, Camilla et al. / Spatially Resolved Stellar Kinematics from LEGA-C : Increased Rotational Support in z~0.8 Quiescent Galaxies. In: The Astrophysical Journal. 2018 ; Vol. 858, No. 1.

Bibtex

@article{3d70d40b085943beb8bd9656a0c38a7e,
title = "Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z~0.8 Quiescent Galaxies",
abstract = "We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at $z=0.6-1$ from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20kpc, or to an average of 2.7${\rm R_e}$. Combined with central stellar velocity dispersions ($\sigma_0$) this provides the first determination of the dynamical state of a sample selected by a lack of star formation activity at large lookback time. The most massive galaxies ($M_{\star}>2\times10^{11}\,M_{\odot}$) generally show no or little rotation measured at 5kpc ($|V_5|/\sigma_0",
keywords = "astro-ph.GA",
author = "Rachel Bezanson and Wel, {Arjen van der} and Camilla Pacifici and Kai Noeske and Ivana Bari{\v s}i{\'c} and Bell, {Eric F.} and Brammer, {Gabriel B.} and Joao Calhau and Priscilla Chauke and Dokkum, {Pieter van} and Marijn Franx and Anna Gallazzi and Houdt, {Josha van} and Ivo Labb{\'e} and Maseda, {Michael V.} and Mu{\~n}os-Mateos, {Juan Carlos} and Adam Muzzin and Sande, {Jesse van de} and David Sobral and Caroline Straatman and Po-Feng Wu",
note = "This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/aabc55",
year = "2018",
month = may,
day = "4",
doi = "10.3847/1538-4357/aabc55",
language = "English",
volume = "858",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Spatially Resolved Stellar Kinematics from LEGA-C

T2 - Increased Rotational Support in z~0.8 Quiescent Galaxies

AU - Bezanson, Rachel

AU - Wel, Arjen van der

AU - Pacifici, Camilla

AU - Noeske, Kai

AU - Barišić, Ivana

AU - Bell, Eric F.

AU - Brammer, Gabriel B.

AU - Calhau, Joao

AU - Chauke, Priscilla

AU - Dokkum, Pieter van

AU - Franx, Marijn

AU - Gallazzi, Anna

AU - Houdt, Josha van

AU - Labbé, Ivo

AU - Maseda, Michael V.

AU - Muños-Mateos, Juan Carlos

AU - Muzzin, Adam

AU - Sande, Jesse van de

AU - Sobral, David

AU - Straatman, Caroline

AU - Wu, Po-Feng

N1 - This is an author-created, un-copyedited version of an article accepted for publication/published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at doi: 10.3847/1538-4357/aabc55

PY - 2018/5/4

Y1 - 2018/5/4

N2 - We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at $z=0.6-1$ from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20kpc, or to an average of 2.7${\rm R_e}$. Combined with central stellar velocity dispersions ($\sigma_0$) this provides the first determination of the dynamical state of a sample selected by a lack of star formation activity at large lookback time. The most massive galaxies ($M_{\star}>2\times10^{11}\,M_{\odot}$) generally show no or little rotation measured at 5kpc ($|V_5|/\sigma_0

AB - We present stellar rotation curves and velocity dispersion profiles for 104 quiescent galaxies at $z=0.6-1$ from the Large Early Galaxy Astrophysics Census (LEGA-C) spectroscopic survey. Rotation is typically probed across 10-20kpc, or to an average of 2.7${\rm R_e}$. Combined with central stellar velocity dispersions ($\sigma_0$) this provides the first determination of the dynamical state of a sample selected by a lack of star formation activity at large lookback time. The most massive galaxies ($M_{\star}>2\times10^{11}\,M_{\odot}$) generally show no or little rotation measured at 5kpc ($|V_5|/\sigma_0

KW - astro-ph.GA

U2 - 10.3847/1538-4357/aabc55

DO - 10.3847/1538-4357/aabc55

M3 - Journal article

VL - 858

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 60

ER -