The ALMA Spectroscopic Survey in the HUDF: A Search for [C ii] Emitters at 6 ≤ z ≤ 8
Research output: Contribution to journal › Journal article › Research › peer-review
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.
| Original language | English |
|---|---|
| Article number | 67 |
| Journal | Astrophysical Journal |
| Volume | 912 |
| Issue number | 1 |
| Number of pages | 12 |
| ISSN | 0004-637X |
| DOIs | |
| Publication status | Published - 1 May 2021 |
Links
- https://arxiv.org/pdf/2102.10706.pdf
Submitted manuscript
ID: 262795103