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Table 3

GBT observations: line intensities and spectral characteristics.

UT date (yyyy/mm/dd) Δ (au) rh (au) Line RMS(1) (mK channel−1 ) Area ()(2) (K km s−1) Width(3) (km s−1) Δυ(3) (km s−1) (km s−1)
2020/07/24.71 0.696 0.667 OH 1 665 12 0.428 ± 0.014 2.89 ± 0.11 −0.07 ± 0.05 2.32 ± 0.07
2020/08/11.88 1.078 1.053 OH 1 665 9 < 0.03
2020/07/24.71 0.696 0.667 OH 1 667 10 0.827 ± 0.012 2.95 ± 0.05 −0.05 ± 0.02 2.43 ± 0.04
2020/08/11.88 1.078 1.053 OH 1 667 9 −0.017 ± 0.005 0.67 ± 0.27 −0.53 ± 0.12
2020/07/24.81 0.696 0.669 NH3 (11 − 11) 48 < 0.017
2020/07/24.81 0.696 0.669 NH3 (22 − 22) 47 < 0.016
2020/07/24.81 0.696 0.669 NH3 (33 − 33) 47 < 0.016
2020/07/24.81 0.696 0.669 NH3 (44 − 44) 46 < 0.016
2020/07/24.81 0.696 0.669 NH3 (55 − 55) 46 < 0.016

Notes. (1)For a spectral channel width of ~0.005 km s−1 for the NH3 lines and ~0.3 km s−1 for the OH 1665 and 1667 MHz lines. (2)Velocity-integrated flux density (i.e., line area) in the scale or a 3σ upper limit. Considered velocity intervals are [−2.5, +2.5] km s−1 and [−1.5,1.5] km s−1 for the OH and NH3 lines, respectively. For the OH 1667 MHz line observed on 11.88 August 2020, the line area is that obtained from a Gaussian fit.(3) Velocity offset from a Gaussian fit. (4)Half lower bases of the fitted trapezia (Fig. 2).

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