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Table 2

VLBI detected and undetected AGN and AGN candidates from the VLA+MERLIN 1.4 GHz survey (Muxlow et al. 2005).

Cat.numbera Nameb 1.4 GHz VLA flux density VLA classc VLBI detection

4 J123608+621035   217 μJy AGN yes
15 J123618+621635   47 μJy AGNC no
18 J123620+620844   123 μJy AGN no
21 J123622+621544   84 μJy AGNC no
24 J123623+621642   481 μJy AGNC yes
39 J123640+621009   87 μJy AGNC no
43 J123644+621133   1290 μJy AGN yes
47 J123646+621404   179 μJy AGN yes
56 J123652+621444   168 μJy AGN yes
64 J123700+620909 GN16 324 μJy AGNC yes
72 J123709+620837   72 μJy AGN no
73 J123709+620841   68 μJy AGNC no
74 J123711+621330   132 μJy AGNC no
78 J123714+620823   1350 μJy AGN yes
79 J123716+621512   187 μJy AGNC yes
81 J123716+621733   346 μJy AGNC yes
85 J123721+621129   383 μJy AGN yes
89 J123725+621128   5 mJy AGN no

Notes. Note that the VLBI in addition detected the starburst+AGN system J123642+621331 at z = 4.42 and the unclear identification J123642+621545 at z = 0.857. The VLBI sensitivity ranges from  ~50   μJy in the field center to  ~150   μJy at rphasecenter  >  6 arcmin (see text).


Number in VLA/MERLIN catalog (Muxlow et al. 2005), at increasing RA;


J2000 name of radio source (Muxlow et al. 2005);


the Muxlow et al. (2005) classification combines radio and infrared (ISO) information.

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