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Table 5

Distribution of sources across AGNs-majority cells of the SOM.

Cell LS US
[1] [2] [3] [4] [5] [6] [7]
(0,0) 19 (150.4183, 2.0851672) AGN* 10 (150.25323,1.9661424) AGN
(1,0) 28 (150.20827, 1.8754041) AGN* 4 (150.2556,2.3534932) AGN
(2,0) 44 + 2 GAL (149.77417, 2.6741626) AGN 49 (149.79821, 2.3900828) EmG*
(0,1) 55 (149.73895, 2.2206892) AGN* 5 (149.77079, 1.7466647) AGN
(1,1) 46 (150.45356, 2.5279411) AGN* 4 (150.47956, 2.2531361) AGN
(2,1) 13 + 2 STAR (150.34245, 2.2262767) AGN* 9 (150.53943,1.9236345) AGN
(1,2) 42 (150.44369, 2.0491065) AGN* 7 (149.77293, 2.5557609) SN/AGN
(2,7) 1 (150.07368, 2.346843) AGN 51 (150.55828, 2.6438238) GAL*
(5,7) 1 (150.04032, 2.4712367) AGN 81 (150.38622, 1.8416973) GAL*

Notes. Column [1] identifies the cell involved, Column [2] shows the number of source for which we know the classification from the Labeled Sources (LS): they are all AGN with the exception of cells (2,0) and (2,1), for which we report also the contaminants (galaxies or stars). In Column [3] we report the coordinates in the format (RA, Dec) of the closest labeled sources to the prototype of the given cell, and Column [4] shows how this source is labeled. Analogously, Column [5] reports the number of unlabeled sources falling into the given cell, Column [6] the coordinates of the closest unlabeled object to the prototype, and in Column [7] we report the classification (if available) from Simbad database; the classes are abbreviated in the following way: active galactic nucleus (AGN), emission-line galaxy (EmG), galaxy (GAL), supernova (SN). Labels in Columns [4] and [7] marked with an asterisk indicate whether the corresponding source is the closest to the prototype when considering both the LS and US.

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