Table 1.
MUSE-ALMA Haloes number of targets covered by various observing campaigns.
| Facility | # quasar | # absorbers | # associated |
|---|---|---|---|
| fields | galaxies | ||
| HST spectroscopy | 19 | 32 | – |
| UVES/hiRES spec | 18 | 31 | – |
| VLT/MUSE | 19 | 32 | 79 |
| HST imaging | 18 | 30 | 79 |
| ALMA | 17 | 25a | 60b |
Notes. The table summarises the number of quasar fields, total number of absorbers in all quasar fields, and galaxies associated with the absorbers in all quasar fields observed by each facility. The quasar fields were initially selected from HST UV spectroscopy, with additional or follow-up observations from the ground with either Keck or the VLT. The associated galaxies were identified with MUSE and HST imaging, while to optimise the survey strategy given the size of the primary beams, ALMA observations targeted a subset of the known galaxies. a 17 (out of 25) absorbers were observed as part of the ALMA Large Programme. b 39 (out of 60) associated galaxies were observed as part of the ALMA Large Programme.
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.