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Table 1:

G23.01-0.41: radio continuum emission.
          Peak positiona    
Telescope $\lambda$ HPBW PA Image rms RA(J2000) Dec(J2000) $F_{\rm peak}$ $F_{\rm int}$
  (cm) ( $'' \times ''$) ($^\circ$) (mJy beam-1) (h m s) ($^\circ$' '') (mJy beam-1) (mJy)
VLA-A 1.3 $0.131 \times 0.095$ -13 0.06 18 34 40.284 -09 00 38.31 0.72 0.98
VLA-C 1.3 $1.1 \times 0.8 $ 0 0.05 ... ... 1.31 1.44
VLA-A 3.6 $0.36 \times 0.24 $ -5 0.03 ... ... 0.47 0.59
VLA-C 3.6 $2.7 \times 1.9 $ 2 0.03 ... ... 0.52 0.50

Notes. (a) The absolute position of the VLA-A 1.3 cm emission peak, obtained aligning positions of persistent water maser spots between the VLA and VLBA observations, should be accurate to about $\pm$ $0\hbox{$.\!\!^{\prime\prime}$ }01$.


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