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Table C.2.

ALCHEMI tunings with discrepant amplitude calibration

SGa Array Flux Calibrators SpixAgeb c aid
B7d 7m J2258−2758,J0006−0623,J0522−3627 (3,-4,20),(-4,20),20 9.98 1.257
B3b 12mE J2258−2758 142,144 0.86 0.789
B7h 7m J2258−2758,J2253+1608,J0522−3627 (3,4),25,4 9.87 0.833
B6f 7m J2253+1608 -1,0,6 1.98 0.867
B3d 12mE J0006−0623 7 1.57 1.128
B3a 12mE J0006−0623 -5,4 0.05,0.68 1.108
B3c 12mE J0006−0623 -3,-6,0,1 0.48 1.107
B7o 7m J2253+1608,J0522−3627 (7,0,2,3),2 2.06 0.922
B3f 12mE J2258−2758,J2357−5311,J0006−0623 -27,-22,4 1.84 0.922
B6h 7m J2258−2758 5,-3,0,-2 3.71,1.03,1.20,4.30 0.924
B3a 12mC J0006−0623 23,27 0.24 0.937

Notes.

(a)

Refers to Science Goals within ALMA project nomenclature.

(b)

Number of days since the most recent ALMA-derived spectral index for a given calibrator. Multiple executions which used a given calibrator are grouped within parentheses. Negative values indicate spectral indices derived before a given calibrator measurement. Calibrator spectral indices are derived using measured Band 3 and Band 6 or Band 7 fluxes.

(c)

Normalized gain calibrator flux uncertainty averaged over all gain calibrator measurements for observation dates within five days. Multiple entries indicate multiple observation time ranges. Target for all gain calibration measurements was J0038−2459.

(d)

Amplitude scale factors are applied to the data as indicated by Equation 3.

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