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Large-scale clustering measurements with photometric redshifts: comparing the dark matter haloes of X-ray AGN, star-forming and passive galaxies at z ≈ 1

MPS-Authors
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Georgakakis,  A.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Salvato,  M.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Rosario,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Lutz,  D.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Nandra,  K.
High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society;

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Berta,  S.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Magnelli,  B.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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Popesso,  P.
Infrared and Submillimeter Astronomy, MPI for Extraterrestrial Physics, Max Planck Society;

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引用

Georgakakis, A., Mountrichas, G., Salvato, M., Rosario, D., Pérez-González, P. G., Lutz, D., Nandra, K., Coil, A., Cooper, M. C., Newman, J. A., Berta, S., Magnelli, B., Popesso, P., & Pozzi, F. (2014). Large-scale clustering measurements with photometric redshifts: comparing the dark matter haloes of X-ray AGN, star-forming and passive galaxies at z ≈ 1. Monthly Notices of the Royal Astronomical Society, 443(4), 3327-3340. doi:10.1093/mnras/stu1326.


引用: https://hdl.handle.net/11858/00-001M-0000-0025-73B1-3
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