Free Access
Table 4.
Descriptions of the ID_flag keyword in the final catalogues used to indicate the origin of the possible association and optical/IR identification, or lack thereof.
| ID_flag | Description |
|---|---|
| 0 | No identification is possible – in cases of extended diffuse emission |
| 1 | The identification (or lack thereof) is made through the LR method |
| 2 | The identification, and possible association, is made based on a match to a bright optical/IR galaxy |
| 22 | The identification is made based on a match to a bright optical/IR galaxy after classification, and possible association, in LGZ as “host broken up” |
| 31 | The possible association and identification (or lack thereof) is made through LGZ |
| 32 | The possible association and identification (or lack thereof) is made after further processing when classified as “too zoomed in” in LGZ (on branch B of the decision tree) |
| 41 | The source and identification (or lack thereof) comes from the deblending workflow based on the “M” source decision tree |
| 42 | The source and identification (or lack thereof) comes from the deblending workflow after classification in LGZ as “blend” |
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.