Table 2
Sources detected in MMIRS survey.
| Objects | #targeted | #detected | #emission line | #continuum |
| detected | detected | |||
|
|
||||
| LAE | 27 | 4 | 4 | 1 |
| DB | 13 | 3 | 3 | 0 |
| BX | 29 | 6 | 6 | 0 |
| LBG | 1 | 1 | 1 | 0 |
| BzK | 6 | 1 | 1 | 1 |
| AGN | 11 | 2 | 2 | 2 |
| low-z | 5 | 5 | 0 | 3 |
| slit stars | 3 | 2 | 0 | 2 |
Notes. In this table we show the number of objects detected versus the ones targeted for each category of objects in the masks. The object name corresponds to the original category of the sources, as explained in Sect. 2. “low-z” are galaxies, whose BzK colors predict them to be at z < 1.4. They appeared bright in the observed H + K band and showed continua in MMIRS spectra. Together with slit stars these are useful to test the sensitivity and throughput of MMIRS.
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.