Integrated fringe data and analytical results obtained using Quick-Look Data Analysis (Takefuji et al. 2007). The fringe data were standardized by the noise dispersion and were processed five points moving average. Left: the steady source CGCG 502-027. Hardly any flux variability was observed in the 1970s. The flux density is 2635.7 mJy according to the NVSS catalog. Center: the steady source 4C +32.60. Hardly any flux variability was observed in the 1970s. The flux density is 625.7 mJy according to the NVSS catalog. Right: a Fermi LAT bright source B2 1846+32A. The flux density detected by us was stronger than the values observed in the 1980s and 1990s. A flux density of at least 1200 mJy and 1600 mJy was detected in 2004 and in 2005, respectively. In the 1980s and 1990s, the flux density was about 500 mJy.