Heavy Element Absorption Systems at 5.0 < z < 6.8: Metal-poor Neutral Gas and a Diminishing Signature of Highly Ionized Circumgalactic Matter-Reference-Cited by-同舟云学术

Heavy Element Absorption Systems at 5.0 < z < 6.8: Metal-poor Neutral Gas and a Diminishing Signature of Highly Ionized Circumgalactic Matter

Published:2019-09-04 Issue:2 Volume:882 Page:77
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Cooper Thomas J.^ORCID,Simcoe Robert A.^ORCID,Cooksey Kathy L.,Bordoloi Rongmon^ORCID,Miller Daniel R.,Furesz Gabor,Turner Monica L.^ORCID,Bañados Eduardo^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab3402/pdf

Reference110 articles.

1. The Chemical Composition of the Sun

2. Statistical Tests for the Origin of Absorption Lines Observed in Quasi-Stellar Sources

3. THE PAN-STARRS1 DISTANT z > 5.6 QUASAR SURVEY: MORE THAN 100 QUASARS WITHIN THE FIRST GYR OF THE UNIVERSE

4. An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5

5. DISCOVERY OF EIGHTz∼ 6 QUASARS FROM Pan-STARRS1

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