Open Access

Table 1.

Properties of type 2 AGNs.

SDSS ObjID RAa Deca Redshift E(B − V)b log L[O III]c log Mstard Tidal featuree
1237661812812349452 186.44468 12.66188 0.00862 0.55 41.57 10.7 Y
1237660024523849823 45.95464 -1.10373 0.01363 0.62 40.85 10.9 Y
1237667142857916600 119.91716 15.38682 0.01552 0.62 41.16 10.5 N
1237662530065465417 212.67229 13.55800 0.01622 0.91 40.97 10.3 Y
1237649920576258107 14.91714 15.33098 0.01829 0.39 40.92 10.6 N
1237664836462182621 124.90783 21.11430 0.01848 0.49 41.01 10.9 N
1237652949068284053 13.37466 -8.76779 0.01898 0.48 41.38 10.6 N
1237661068722372615 175.57032 14.06660 0.02074 0.21 41.13 10.2 N
1237667323784593449 161.24281 26.09143 0.02094 0.37 41.03 9.8 N
1237665532252323890 222.65772 22.73434 0.02095 0.18 41.51 10.1 N
1237668624630611992 203.02007 17.04897 0.02165 0.28 40.86 10.7 N
1237659348026589196 200.05655 7.90781 0.02169 0.40 40.82 9.9 N
1237668297138045048 203.48241 18.30590 0.02247 0.50 40.85 10.4 N
1237663277925990500 356.00858 0.51661 0.02251 0.93 41.26 10.6 N
1237667915955634219 181.12362 20.31630 0.02262 0.37 41.58 10.7 N

Notes. The full table is available at the CDS.

(a)

RA and Dec are in degrees.

(b)

The color excess E(B − V) derived from the Balmer decrement.

(c)

The logarithmic luminosity of the [O III] λ5007 emission line. Here, L[O III] is corrected for internal extinction derived from the Balmer decrement. L[O III] is expressed in units of erg s−1.

(d)

The logarithmic stellar mass obtained from the MPA–JHU catalog. Mstar is expressed in solar masses (M).

e

The presence of tidal features in the host galaxy: Y = present, N = absent.

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