Table 3.
IRAM observations summary.
| PHz | Planck | N. targets |
N. at | |
|---|---|---|---|---|
| ID | ID | observed | detected (a) | similar z(b) |
| 57 | G176 | 5 | 2 | 2 |
| 70 | G223 | 1 | 0 | ... |
| 237 | G173 | 1 | 1 | ... |
| 343 | G162 | 1 | 0 | ... |
| 631 | G006 | 1 | 1 | ... |
| 712 | G237 (c) | 2 | 2 | 0 |
| 832 | G191 | 9 | 3(4) | 2(3) |
| 1473 | G088 | 1 | 0 | ... |
| 124051 | G059 | 2 | 2 | 2 |
| 124052 | G073 (d) | 2 | 2 | 0 |
| 124053 | G124 | 4 | 4(5) | 2(3) |
| 125002 | G072 | 1 | 0 | ... |
| 125018 | G112 | 1 | 1 | ... |
| 125026 | G143 | 1 | 1 | ... |
| 125027 | G131 | 2 | 2 | 0 |
| 125056 | G052 | 2 | 1 | ... |
| 125107 | G068 | 1 | 1 | ... |
| 125132 | G063 | 1 | 1(2) | ... |
| All | 38 | 24(27) | 8(10) | |
Notes.
We list in parentheses the number of CO detections at distinct redshifts. In three cases, we find two objects at different redshifts associated with the same SPIRE target, G191 07, G124 01, and G063 02.
The field G237 contains a spectroscopically confirmed protocluster at the redshift of one of the two CO-detected sources (Polletta et al. 2021; Koyama et al. 2021).
ALMA observations of both targets in G073 yielded continuum detections of five sources (three in G073 03, and two in G073 15), and a CO(3–2) line detection at z ∼ 1.51 − 1.54 in three of them (Kneissl et al. 2019; Hill, priv. comm.). Our EMIR observations detected only one CO line at these redshifts (see Kneissl et al. 2019), and one at a different redshift in G073 15.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.