The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8
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The Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS) Band 6 scan (212-272 GHz) covers potential [C ii] emission in galaxies at 6 2.0 x 10(8) L (circle dot) (5 sigma) to be less than 1.8 x 10(-4) Mpc(-3) (90% confidence level). At this luminosity depth and volume coverage, we present an observed evolution of the [C ii] luminosity function from z = 6-8 to z similar to 0 by comparing the ASPECS measurement to literature results at lower redshift.
Originalsprog | Engelsk |
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Artikelnummer | 67 |
Tidsskrift | Astrophysical Journal |
Vol/bind | 912 |
Udgave nummer | 1 |
Antal sider | 12 |
ISSN | 0004-637X |
DOI | |
Status | Udgivet - 1 maj 2021 |
Links
- https://arxiv.org/pdf/2102.10706.pdf
Indsendt manuskript
ID: 262795103