J162556.1-243014  New radio detection. Probable counterpart is infrared source
J162556.1-243014   no.11 in Table 2 of Wilking et al.  (1989ApJ...340..823W).
J162603.0-242336  Emission at 6cm is left circularly polarized (LCP) with a
J162603.0-242336   detection significance S/N=16 in Stokes V maps and a
J162603.0-242336   fractional circular polarization computed from peak Stokes V
J162603.0-242336   and I fluxes of {pi}_c_=-0.059 (LCP).
J162615.5-243428  Possible double radio source, but source structure is
J162615.5-243428   uncertain due to beam elongation at low source elevation.
J162622.4-242252  Peak flux increased by a factor of ~5 during the time interval
J162622.4-242252   0629-0931UT.
J162624.0-241613  New radio detection. Probable counterpart is H{alpha}
J162624.0-241613   emission-line star no. 31 in Table 1 of Wilking et al.
J162624.0-241613   (1987AJ.....94..106W), which is cross-listed as Elias-24
J162624.0-241613   Elias (1978ApJ...224..453E).
J162630.5-242256  The peak flux density at 3.6cm is comparable to that at 6cm,
J162630.5-242256   suggesting a flat spectral energy distribution and possible
J162630.5-242256   nonthermal radio emission.
J162632.7-242245  Marginal detection (S/N=5.1).
J162634.1-242328  Stokes I emission is extended. Emission at 6cm is left
J162634.1-242328   circularly polarized (LCP) with a detection significance
J162634.1-242328   S/N=9 in Stokes V maps and a fractional circular polarization
J162634.1-242328   {pi}_c_=-0.046 (LCP). Stokes V maps with Oph S1 located near
J162634.1-242328   phase center give peak fluxes V(6cm)=-330({+/-}38){mu}Jy and
J162634.1-242328   V(3.5cm)=-390({+/-}30){mu}Jy, where the minus sign denotes
J162634.1-242328   LCP. The peak flux ratios V/I give fractional circular
J162634.1-242328   polarizations {pi}_{c}(6cm)=-0.046 (LCP) and
J162634.1-242328   {pi}_c_(3.5 cm)=-0.062 (LCP). The Stokes V map at 20cm has an
J162634.1-242328   rms noise of 65{mu}Jy/beam, giving a 3{sigma} upper limit
J162634.1-242328   V(20 cm)<=95{mu}Jy and {pi}_c_(20 cm)<=0.0035. The 6-cm
J162634.1-242328   Stokes V flux given above is consistent with the value
J162634.1-242328   V(6cm)=-280({+/-}50){mu}Jy obtained with the VLA on
J162634.1-242328   1987 Aug 6 Andre et al. (1988ApJ...335..940A).
J162643.8-241632  The infrared counterpart is offset by 3.2" from the radio peak
J162643.8-241632   position making the identification uncertain.
J162700.0-242640  Emission at 6cm is right circularly polarized with a detection
J162700.0-242640   significance S/N=34 in Stokes V maps and a fractional
J162700.0-242640   circular polarization computed from peak Stokes V and I
J162700.0-242640   fluxes of {pi}_c_=+0.034.  Corresponds to #20 (BZ6) in
J162700.0-242640   Table II of Stine et al. (1988AJ.....96.1394S), who argue
J162700.0-242640   that it is extragalactic.