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Table 1.

Observation parameters.

AGC name On-source Phase calibrator Peak. coords Major Minor PA FINT Fpeak rms L1.4 GHz
(min) (J2000) (″) (″) (°) (mJy) (mJy beam−1) (mJy beam−1) (W Hz−1)
102708 62 2340+266 < 0.066 0.022 < 21.7
102850 62 0040+331 - < 0.096 0.032 < 21.9
114732 50 0119+084 < 0.084 0.028 < 21.8
115713 50 0141+138 014135.19+165730.51 1.6 ± 0.3 1.2 ± 0.3 32 1.7 ± 0.1 1.25 0.055 23.1
115018 62 0149+059 < 0.078 0.026 < 22.0
124351 57 0224+069 < 0.087 0.029 < 21.9
749309SE 69 1013+248 101103.21+273924.36 5.2 ± 0.2 0.5 ± 0.4 173 2.9 ± 0.1 1.09 0.058 23.5
749309NW ... ... 101100.41+274036.52 3.4 ± 0.4 3.2 ± 0.4 132 1.2 ± 0.1 0.44 0.058 23.1
219835 70 1156+314 113033.97+322149.19 364 ± 22 80.8 0.293 25.3
249507 65 1407+284 140340.33+295456.48 2.1 ± 0.1 1.4 ± 0.1 50 3.0 ± 0.1 1.86 0.025 23.4
322231 50 2232+117 < 0.090 0.030 < 21.8

Notes. Column 1: AGC name given by Haynes et al. (2018). Columns 2–3: On-source time and phase calibrator for this project. Columns 4–9: Fitted parameters of the radio continuum emission including the peak coordinates, Gaussian component size, peak, and integrated flux densities. Column 10: 1σ noise level. Column 11: Radio luminosity of the radio continuum emission. The redshift for AGC 249507 is sourced from the LAMOST survey, while the redshift for other galaxies was derived based on the peak frequency of the potential OH 1667 MHz line as reported in Haynes et al. (2018).

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