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Journal Article

The CGM and IGM at z ̃ 5: metal budget and physical connection

MPS-Authors

Codoreanu,  Alex
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Ryan-Weber,  Emma V.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

García,  Luz Ángela
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Crighton,  Neil H. M.
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Becker,  George
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Pettini,  Max
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Madau,  Piero
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

Venemans,  Bram
Max Planck Institute for Astronomy, Max Planck Society and Cooperation Partners;

External Resource

https://ui.adsabs.harvard.edu/abs/2018MNRAS.481.4940C
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Citation

Codoreanu, A., Ryan-Weber, E. V., García, L. Á., Crighton, N. H. M., Becker, G., Pettini, M., et al. (2018). The CGM and IGM at z ̃ 5: metal budget and physical connection. Monthly Notices of the Royal Astronomical Society, 481, 4940-4959.


Cite as: https://hdl.handle.net/21.11116/0000-0005-CE68-F
Abstract
We present further results of a survey for absorption line systems in the spectra of four high redshift quasars (5.79 ≤ zem ≤ 6.13) obtained with the ESO Very Large Telescope X-Shooter. We identify 36 C