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Table I.1.

ALMA 2017 Sgr A* light curves, in total flux, polarized intensity, and Stokes V.

Day UT Duration Parameter Spectral Window Samples Flux (Jy) Modulation max-min
(2017) (h) (h) label Frequency (GHz) (Jy)
April 6 8:24 - 14:33 6.15 Stokes I B1 212.1 − 214.1 2324 2.88 ± 0.13 0.044 0.41
B2 214.1 − 216.1 2331 2.87 ± 0.12 0.043 0.41
B3 226.1 − 228.1 2319 2.89 ± 0.13 0.044 0.48
B4 228.1 − 230.1 2329 2.89 ± 0.13 0.044 0.42
P B1 212.1 − 214.1 2324 0.22 ± 0.06 0.27 0.22
B2 214.1 − 216.1 2331 0.22 ± 0.06 0.27 0.22
B3 226.1 − 228.1 2319 0.22 ± 0.05 0.25 0.21
B4 228.1 − 230.1 2329 0.23 ± 0.06 0.25 0.22
Stokes V B1 212.1 − 214.1 2324 −0.037 ± 0.015 0.41 0.055
B2 214.1 − 216.1 2331 −0.037 ± 0.015 0.40 0.056
B3 226.1 − 228.1 2319 −0.037 ± 0.016 0.42 0.058
B4 228.1 − 230.1 2329 −0.040 ± 0.015 0.38 0.053

April 7 4:02 - 14:25 10.37 Stokes I B1 212.1 − 214.1 3771 2.61 ± 0.18 0.069 0.73
B2 214.1 − 216.1 3765 2.61 ± 0.18 0.068 0.73
B3 226.1 − 228.1 3721 2.61 ± 0.18 0.069 0.71
B4 228.1 − 230.1 3727 2.62 ± 0.19 0.071 0.75
P B1 212.1 − 214.1 3771 0.18 ± 0.06 0.31 0.27
B2 214.1 − 216.1 3765 0.18 ± 0.06 0.31 0.27
B3 226.1 − 228.1 3721 0.19 ± 0.06 0.31 0.28
B4 228.1 − 230.1 3727 0.20 ± 0.06 0.33 0.29
Stokes V B1 212.1 − 214.1 3771 −0.030 ± 0.013 0.43 0.058
B2 214.1 − 216.1 3765 −0.030 ± 0.013 0.43 0.060
B3 226.1 − 228.1 3721 −0.029 ± 0.012 0.41 0.056
B4 228.1 − 230.1 3727 −0.030 ± 0.012 0.41 0.059

April 11 9:00 - 14:03 2.82 Stokes I B1 212.1 − 214.1 1378 2.73 ± 0.33 0.119 1.15
B2 214.1 − 216.1 1377 2.72 ± 0.33 0.121 1.16
B3 226.1 − 228.1 1370 2.69 ± 0.34 0.125 1.20
B4 228.1 − 230.1 1362 2.69 ± 0.34 0.125 1.19
P B1 212.1 − 214.1 1378 0.21 ± 0.05 0.26 0.23
B2 214.1 − 216.1 1377 0.21 ± 0.05 0.26 0.23
B3 226.1 − 228.1 1370 0.21 ± 0.06 0.26 0.24
B4 228.1 − 230.1 1362 0.22 ± 0.06 0.27 0.25
Stokes V B1 212.1 − 214.1 1378 −0.033 ± 0.007 0.20 0.032
B2 214.1 − 216.1 1377 −0.030 ± 0.007 0.23 0.031
B3 226.1 − 228.1 1370 −0.028 ± 0.006 0.23 0.029
B4 228.1 − 230.1 1362 −0.027 ± 0.007 0.25 0.030

Notes. Stokes V reported values are tentative, as the detected levels fall below ALMA’s guaranteed CP accuracy.

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