Table C.2
Observed parameters of HCN laser lines towards CIT 6, Y CVn, S Cep, IRC+50096, V Cyg, II Lup, and CRL 3068.
| Line | Obs. date | ϕ | Vpk | Vrange | ∫ S dv | Spk | LHCN | σ @ Vch |
|---|---|---|---|---|---|---|---|---|
| (GHz) | (yyyy-mm-ss) | (km s−1) | (km s−1) | (Jy k km s−1) | (Jy) | (photons s−1) | (Jy @ km s−1) | |
| CIT 6 | ||||||||
| 805 | 2012–06-16 | 0.21 | −6.7 | [−10.0, −0.6] | 2501.4 | 463.7 | 3.2 × 1044 | 27.3 @ 0.19 |
| 891 | 2012–05-04 | 0.14 | −4.8 | [−10.0, 0.0] | 12185.4 | 2909.8 | 1.6 × 1045 | 28.1 @ 0.17 |
| 964 | 2012-05-04 | 0.14 | −4.7 | [−10.0, 0.0] | 6608.6 | 1633.4 | 8.4 × 1044 | 49.3 @ 0.16 |
| 2018-12-17 | 0.92 | −5.6 | [−7.6, −1.2] | 6689.1 | 2308.4 | 8.5 × 1044 | 172.1 @ 0.30 | |
| 968 | 2012-05-04 | 0.14 | −4.6 | [−10.0, −0.7] | 4167.7 | 760.2 | 5.3 × 1044 | 45.5 @ 0.15 |
| 2018-12-17 | 0.92 | −4.9 | [−7.8, −1.1] | 3796.0 | 890.4 | 4.8 × 1044 | 171.8 @ 0.30 | |
| 1055 | 2012-05-04 | 0.14 | −4.1 | [−7.6, −1.4] | 2098.0 | 786.5 | 2.7 × 1044 | 98.7 @ 0.14 |
| Y CVn | ||||||||
| 805 | 2012-06-16 | +19.9 | [+14.2, +25.4] | 1446.5 | 245.4 | 4.2 × 1043 | 28.4 @ 0.19 | |
| 891 | 2012-06-14 | +21.1 | [+14.8,+28.0] | 4877.9 | 825.8 | 1.4 × 1044 | 27.6 @ 0.17 | |
| 964 | 2012-06-15 | … | … | … | <152.1 | … | 50.7 @ 0.16 | |
| 2018-12-17 | +20.8 | [+18.4, +21.6] | 1342.6 | 534.0 | 3.9 × 1043 | 103.8 @ 0.30 | ||
| 968 | 2012-06-15 | +21.0 | [+15.4, +25.6] | 2238.6 | 387.6 | 6.5 × 1043 | 66.1 @ 0.15 | |
| 2018-12-17 | +18.4 | [+15.1, +23.0] | 3238.2 | 989.1 | 9.4 × 1043 | 149.7 @ 0.30 | ||
| 1055 | 2012-05-18 | … | … | … | <310.9 | … | 103.6 @ 0.14 | |
| S Cep | ||||||||
| 805 | 2012-05-23 | 0.40 | −16.8 | [−22.2, −9.4] | 2729.3 | 547.1 | 2.4 × 1044 | 29.5 @ 0.19 |
| 891 | 2012-05-24 | 0.40 | −15.2 | [−22.0, −10.0] | 9272.6 | 1983.0 | 8.1 × 1044 | 26.6 @ 0.17 |
| 964 | 2012-05-24 | 0.40 | −16.7 | [−20.4, −11.6] | 4417.5 | 1077.8 | 3.8 × 1044 | 50.7 @ 0.16 |
| 2018-12-17 | 0.35 | −17.5 | [−19.6, −14.2] | 4132.0 | 1401.3 | 3.6 × 1044 | 135.5 @ 0.30 | |
| 968 | 2012-05-24 | 0.40 | −13.8 | [−20.4, −11.2] | 2071.2 | 407.4 | 1.8 × 1044 | 61.0 @ 0.15 |
| 2018-12-17 | 0.35 | −15.9 | [−18.3, −12.4] | 2132.6 | 640.3 | 1.9 × 1044 | 152.6 @ 0.60 | |
| 1055 | 2012-05-24 | 0.40 | −16.5 | [−17.8, −12.4] | 2121.8 | 581.9 | 1.8 × 1044 | 90.4 @ 0.14 |
| IRC+50096 | ||||||||
| 805 | 2012-08-25 | 0.84 | −12.1 | [−21.0, −10.0] | 916.3 | 156.7 | 1.7 × 1044 | 30.0 @ 0.19 |
| 891 | 2012-08-11 | 0.81 | −18.6 | [−23.0, −7.0] | 4391.2 | 790.4 | 8.3 × 1044 | 29.4 @ 0.17 |
| 964 | 2012-08-16 | 0.82 | −18.4 | [−20.2, −8.0] | 1874.0 | 346.8 | 3.5 × 1044 | 52.2 @ 0.16 |
| 968 | 2012-08-16 | 0.82 | … | … | … | <153.9 | … | 51.3 @ 0.15 |
| 1055 | 2012-08-25 | 0.82 | … | … | … | <291.3 | … | 97.1 @ 0.14 |
| V Cyg | ||||||||
| 805 | 2012-05-23 | 0.56 | +14.3 | [+6.8, +21.4] | 2292.8 | 471.8 | 1.9 × 1044 | 29.3 @ 0.19 |
| 891 | 2012-05-24 | 0.57 | +11.0 | [+8.0,+21.0] | 10737.9 | 2215.4 | 8.7 × 1044 | 28.8 @ 0.17 |
| 964 | 2012-05-03 | 0.52 | +11.2 | [+9.0, +21.4] | 5975.4 | 1321.8 | 4.8 × 1044 | 56.1 @ 0.16 |
| 968 | 2012-05-03 | 0.52 | +14.5 | [+7.5, +19.6] | 2182.9 | 464.8 | 1.8 × 1044 | 52.1 @ 0.15 |
| 1055 | 2012-06-21 | 0.63 | +15.1 | [+8.3, +18.2] | 2093.1 | 527.3 | 1.7 × 1044 | 97.6 @ 0.14 |
| II Lup | ||||||||
| 805 | 2012-09-12 | 0.43 | −15.9 | [−19.0, −11.0] | 447.1 | 148.6 | 1.1 × 1044 | 7.2 @ 0.19 |
| 891 | 2012-09-18 | 0.45 | −16.1 | [−20.4, −11.0] | 3830.4 | 1042.5 | 9.5 × 1044 | 11.8 @ 0.17 |
| 964 | 2012-09-07 | 0.42 | −14.6 | [−18.6, −11.0] | 2275.7 | 739.4 | 5.6 × 1044 | 12.0 @ 0.16 |
| 968 | 2012-09-07 | 0.42 | −15.9 | [−18.0, −12.0] | 654.7 | 190.2 | 1.6 × 1044 | 13.0 @ 0.15 |
| 1055 | 2012-09-21 | 0.46 | −14.6 | [−16.4, −12.4] | 324.1 | 120.9 | 8.0 × 1043 | 20.3 @ 0.14 |
| CRL 3068 | ||||||||
| 805 | 2012-06-21 | … | … | … | <69.3 | … | 23.1 @ 0.19 | |
| 891 | 2012-05-24 | … | … | … | <76.2 | … | 25.4 @ 0.17 | |
| 964 | 2012-05-31 | … | … | … | <179.7 | … | 59.9 @ 0.16 | |
| 968 | 2012-05-31 | … | … | … | <139.8 | … | 46.6 @ 0.15 | |
| 1055 | 2012-06-21 | … | … | … | <277.8 | … | 92.6 @ 0.14 | |
Notes. The descriptions of the table are the same as in Table C.1. For the non-detection, the upper limits of the peak intensity (<3 σ) are given. No ephemeris information for Y CVn, II Lup and CRL 3068 are provided by AAVSO. We additionally adopted the data from Feast et al. (2003) for II Lup to estimate their stellar phases for the observing dates.
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