The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift

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The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift. / Lapi, A.; Raimundo, S.; Aversa, R.; Cai, Z.-Y.; Negrello, M.; Celotti, A.; De Zotti, G.; Danese, L.

In: Astrophysical Journal, Vol. 782, No. 2, 69, 01.02.2014.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Lapi, A, Raimundo, S, Aversa, R, Cai, Z-Y, Negrello, M, Celotti, A, De Zotti, G & Danese, L 2014, 'The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift', Astrophysical Journal, vol. 782, no. 2, 69. https://doi.org/10.1088/0004-637X/782/2/69

APA

Lapi, A., Raimundo, S., Aversa, R., Cai, Z-Y., Negrello, M., Celotti, A., De Zotti, G., & Danese, L. (2014). The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift. Astrophysical Journal, 782(2), [69]. https://doi.org/10.1088/0004-637X/782/2/69

Vancouver

Lapi A, Raimundo S, Aversa R, Cai Z-Y, Negrello M, Celotti A et al. The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift. Astrophysical Journal. 2014 Feb 1;782(2). 69. https://doi.org/10.1088/0004-637X/782/2/69

Author

Lapi, A. ; Raimundo, S. ; Aversa, R. ; Cai, Z.-Y. ; Negrello, M. ; Celotti, A. ; De Zotti, G. ; Danese, L. / The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift. In: Astrophysical Journal. 2014 ; Vol. 782, No. 2.

Bibtex

@article{e541c6e44c4446c88f8e3a08c9c1057b,
title = "The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift",
abstract = "We exploit the recent, wide samples of far-infrared (FIR) selected galaxies followed up in X-rays and of X-ray/optically selected active galactic nuclei (AGNs) followed up in the FIR band, along with the classic data on AGNs and stellar luminosity functions at high redshift z >~ 1.5, to probe different stages in the coevolution of supermassive black holes (BHs) and host galaxies. The results of our analysis indicate the following scenario: (1) the star formation in the host galaxy proceeds within a heavily dust-enshrouded medium at an almost constant rate over a timescale ",
keywords = "galaxies: elliptical and lenticular, cD, galaxies: evolution, galaxies: formation, galaxies: high-redshift, quasars: general",
author = "A. Lapi and S. Raimundo and R. Aversa and Z.-Y. Cai and M. Negrello and A. Celotti and {De Zotti}, G. and L. Danese",
year = "2014",
month = feb,
day = "1",
doi = "10.1088/0004-637X/782/2/69",
language = "English",
volume = "782",
journal = "Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - The Coevolution of Supermassive Black Holes and Massive Galaxies at High Redshift

AU - Lapi, A.

AU - Raimundo, S.

AU - Aversa, R.

AU - Cai, Z.-Y.

AU - Negrello, M.

AU - Celotti, A.

AU - De Zotti, G.

AU - Danese, L.

PY - 2014/2/1

Y1 - 2014/2/1

N2 - We exploit the recent, wide samples of far-infrared (FIR) selected galaxies followed up in X-rays and of X-ray/optically selected active galactic nuclei (AGNs) followed up in the FIR band, along with the classic data on AGNs and stellar luminosity functions at high redshift z >~ 1.5, to probe different stages in the coevolution of supermassive black holes (BHs) and host galaxies. The results of our analysis indicate the following scenario: (1) the star formation in the host galaxy proceeds within a heavily dust-enshrouded medium at an almost constant rate over a timescale

AB - We exploit the recent, wide samples of far-infrared (FIR) selected galaxies followed up in X-rays and of X-ray/optically selected active galactic nuclei (AGNs) followed up in the FIR band, along with the classic data on AGNs and stellar luminosity functions at high redshift z >~ 1.5, to probe different stages in the coevolution of supermassive black holes (BHs) and host galaxies. The results of our analysis indicate the following scenario: (1) the star formation in the host galaxy proceeds within a heavily dust-enshrouded medium at an almost constant rate over a timescale

KW - galaxies: elliptical and lenticular

KW - cD

KW - galaxies: evolution

KW - galaxies: formation

KW - galaxies: high-redshift

KW - quasars: general

U2 - 10.1088/0004-637X/782/2/69

DO - 10.1088/0004-637X/782/2/69

M3 - Journal article

VL - 782

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 69

ER -

ID: 230475393