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  • 1708.08461v1

    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/aa8768 © Copyright 2017 IOP Publishing

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Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies

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

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Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies. / Barisic, Ivana; van der Wel, Arjen; Bezanson, Rachel et al.
In: The Astrophysical Journal, Vol. 847, No. 1, 72, 21.09.2017.

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

Harvard

Barisic, I, van der Wel, A, Bezanson, R, Pacifici, C, Noeske, K, Munoz-Mateos, JC, Franx, M, Smolcic, V, Bell, EF, Brammer, G, Calhau, J, Chauke, P, van Dokkum, PG, van Houdt, J, Gallazzi, A, Labbe, I, Maseda, MV, Muzzin, A, Sobral, D, Straatman, C & Wu, P-F 2017, 'Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies', The Astrophysical Journal, vol. 847, no. 1, 72. https://doi.org/10.3847/1538-4357/aa8768

APA

Barisic, I., van der Wel, A., Bezanson, R., Pacifici, C., Noeske, K., Munoz-Mateos, J. C., Franx, M., Smolcic, V., Bell, E. F., Brammer, G., Calhau, J., Chauke, P., van Dokkum, P. G., van Houdt, J., Gallazzi, A., Labbe, I., Maseda, M. V., Muzzin, A., Sobral, D., ... Wu, P-F. (2017). Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies. The Astrophysical Journal, 847(1), Article 72. https://doi.org/10.3847/1538-4357/aa8768

Vancouver

Barisic I, van der Wel A, Bezanson R, Pacifici C, Noeske K, Munoz-Mateos JC et al. Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies. The Astrophysical Journal. 2017 Sept 21;847(1):72. doi: 10.3847/1538-4357/aa8768

Author

Barisic, Ivana ; van der Wel, Arjen ; Bezanson, Rachel et al. / Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies. In: The Astrophysical Journal. 2017 ; Vol. 847, No. 1.

Bibtex

@article{f6296fe788f8421e9fd90fbabe99b0fb,
title = "Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies",
abstract = "We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L-3 GHz > 10(23) W Hz(-1)) at 0.6 175 kms(-1), corresponding to black hole masses in excess of 10(8) M-circle dot. Furthermore, we confirm that at a fixed stellar mass the fraction of radio-loud AGN at z similar to 1 is five to 10 times higher than in the local universe, suggesting that quiescent, massive galaxies at z similar to 1 switch on as radio AGN on average once every Gyr. Our results strengthen the existing evidence for a link between high black hole masses, radio loudness, and quiescence at z similar to 1.",
keywords = "galaxies: evolution, galaxies: fundamental parameters, galaxies: high-redshift, galaxies: jets, galaxies: star formation, ACTIVE GALACTIC NUCLEI, SUPERMASSIVE BLACK-HOLES, GHZ LARGE PROJECT, AGN FEEDBACK, COSMIC EVOLUTION, FORMING GALAXIES, HOST GALAXIES, MASSIVE GALAXIES, POPULATION, CATALOG",
author = "Ivana Barisic and {van der Wel}, Arjen and Rachel Bezanson and Camilla Pacifici and Kai Noeske and Munoz-Mateos, {Juan C.} and Marijn Franx and Vernesa Smolcic and Bell, {Eric F.} and Gabriel Brammer and Joao Calhau and Priscilla Chauke and {van Dokkum}, {Pieter G.} and {van Houdt}, Josha and Anna Gallazzi and Ivo Labbe and Maseda, {Michael V.} and Adam Muzzin 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/aa8768 {\textcopyright} Copyright 2017 IOP Publishing",
year = "2017",
month = sep,
day = "21",
doi = "10.3847/1538-4357/aa8768",
language = "English",
volume = "847",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "1",

}

RIS

TY - JOUR

T1 - Stellar Dynamics and Star Formation Histories of z similar to 1 Radio-loud Galaxies

AU - Barisic, Ivana

AU - van der Wel, Arjen

AU - Bezanson, Rachel

AU - Pacifici, Camilla

AU - Noeske, Kai

AU - Munoz-Mateos, Juan C.

AU - Franx, Marijn

AU - Smolcic, Vernesa

AU - Bell, Eric F.

AU - Brammer, Gabriel

AU - Calhau, Joao

AU - Chauke, Priscilla

AU - van Dokkum, Pieter G.

AU - van Houdt, Josha

AU - Gallazzi, Anna

AU - Labbe, Ivo

AU - Maseda, Michael V.

AU - Muzzin, Adam

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/aa8768 © Copyright 2017 IOP Publishing

PY - 2017/9/21

Y1 - 2017/9/21

N2 - We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L-3 GHz > 10(23) W Hz(-1)) at 0.6 175 kms(-1), corresponding to black hole masses in excess of 10(8) M-circle dot. Furthermore, we confirm that at a fixed stellar mass the fraction of radio-loud AGN at z similar to 1 is five to 10 times higher than in the local universe, suggesting that quiescent, massive galaxies at z similar to 1 switch on as radio AGN on average once every Gyr. Our results strengthen the existing evidence for a link between high black hole masses, radio loudness, and quiescence at z similar to 1.

AB - We investigate the stellar kinematics and stellar populations of 58 radio-loud galaxies of intermediate luminosities (L-3 GHz > 10(23) W Hz(-1)) at 0.6 175 kms(-1), corresponding to black hole masses in excess of 10(8) M-circle dot. Furthermore, we confirm that at a fixed stellar mass the fraction of radio-loud AGN at z similar to 1 is five to 10 times higher than in the local universe, suggesting that quiescent, massive galaxies at z similar to 1 switch on as radio AGN on average once every Gyr. Our results strengthen the existing evidence for a link between high black hole masses, radio loudness, and quiescence at z similar to 1.

KW - galaxies: evolution

KW - galaxies: fundamental parameters

KW - galaxies: high-redshift

KW - galaxies: jets

KW - galaxies: star formation

KW - ACTIVE GALACTIC NUCLEI

KW - SUPERMASSIVE BLACK-HOLES

KW - GHZ LARGE PROJECT

KW - AGN FEEDBACK

KW - COSMIC EVOLUTION

KW - FORMING GALAXIES

KW - HOST GALAXIES

KW - MASSIVE GALAXIES

KW - POPULATION

KW - CATALOG

U2 - 10.3847/1538-4357/aa8768

DO - 10.3847/1538-4357/aa8768

M3 - Journal article

VL - 847

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 72

ER -