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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” |
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