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Table 3

Overview of the observed PO transitions.

Rms
Ω J′ − J Λ Line flux noise δν
(K km s-1) (mK) (MHz)

1/2 5/2−3/2 e 29.191 1.7 2.0
1/2 5/2−3/2 f 32.046 1.7 2.0
3/2 5/2−3/2 e 0.030 2.1 2.0
3/2 5/2−3/2 f 0.030 2.1 2.0
1/2 7/2−5/2 e 33.269 1.7 2.0
1/2 7/2−5/2 f 27.782 1.7 2.0
3/2 7/2−5/2 e 1.622 2.0 2.0
3/2 7/2−5/2 f 1.622 2.0 2.0

(Jy km s-1) (mJy)

1/2 13/2−11/2 e 1.528 33.4 2.4
1/2 13/2−11/2 f 1.183 33.4 2.4
3/2 13/2 − 11/2 e 0.471 27.8 2.4
3/2 13/2−11/2 f 0.471 27.8 2.4
1/2 15/2−13/2 e 0.657 48.8 2.4
1/2 15/2 − 13/2 f 0.133 48.8 2.4
3/2 15/2−13/2 e 0.196 50.6 2.4
3/2 15/2−13/2 f 0.196 50.6 2.4

Notes. The respective columns list the quantum number Ω, the rotational transition J′ − J, the Λ component, the velocity-integrated line flux, the rms noise, and the frequency resolution δν.

(†)

Component 1 (see Table 2) was not fitted in our analysis, because the noise was much higher owing to an optically thick line of terrestrial water at ~325 GHz. Instead, component 1 was assumed to have the same strength as component 6.

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