Separation of the maser disk from the continuum sources.
|Galaxy||δ RA||δ Dec||Reference|
|Mrk 0001||4.5 ± 1.0||0.4 ± 1.0||1|
|Mrk 1419||1.5 ± 10.0||1.5 ± 10.0||2|
|NGC 2273||22.5 ± 10.0||3.3 ± 10.0||2|
Notes. Column 1: name of galaxy. Columns 2 and 3: separation of the maser disk from the center of the 5 GHz nuclear continuum source and the uncertainties. For Mrk 0001 the separation is for our first observation and with respect to the continuum source in the northwest of the image. Column 4: references for maser disk positions. (1) Kuo et al., in prep.; (2) Kuo et al. (2011).
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