Table 5.

The RT-22 measurements in 2003–2023: MJD (Column 1), yyyy.mm.dd (Column 2), flux densities at 37 GHz and their errors, Jy (Column 3). The full version is available as online supplementary material.

MJDyyyy.mm.dd|$S_{37}$|⁠, |$\sigma$|⁠, Jy
123
526792003.02.08|$1.42\pm 0.06$|
526812003.02.09|$1.32\pm 0.08$|
526932003.02.22|$1.49\pm 0.15$|
526952003.02.24|$1.43\pm 0.16$|
526972003.02.26|$1.55\pm 0.12$|
MJDyyyy.mm.dd|$S_{37}$|⁠, |$\sigma$|⁠, Jy
123
526792003.02.08|$1.42\pm 0.06$|
526812003.02.09|$1.32\pm 0.08$|
526932003.02.22|$1.49\pm 0.15$|
526952003.02.24|$1.43\pm 0.16$|
526972003.02.26|$1.55\pm 0.12$|
Table 5.

The RT-22 measurements in 2003–2023: MJD (Column 1), yyyy.mm.dd (Column 2), flux densities at 37 GHz and their errors, Jy (Column 3). The full version is available as online supplementary material.

MJDyyyy.mm.dd|$S_{37}$|⁠, |$\sigma$|⁠, Jy
123
526792003.02.08|$1.42\pm 0.06$|
526812003.02.09|$1.32\pm 0.08$|
526932003.02.22|$1.49\pm 0.15$|
526952003.02.24|$1.43\pm 0.16$|
526972003.02.26|$1.55\pm 0.12$|
MJDyyyy.mm.dd|$S_{37}$|⁠, |$\sigma$|⁠, Jy
123
526792003.02.08|$1.42\pm 0.06$|
526812003.02.09|$1.32\pm 0.08$|
526932003.02.22|$1.49\pm 0.15$|
526952003.02.24|$1.43\pm 0.16$|
526972003.02.26|$1.55\pm 0.12$|
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