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Table 3.
Description of the I components for each source and the associated saturation rates.
| Star | rms | v | Flux | Δv | S/N | TB | R | R/Γ |
|---|---|---|---|---|---|---|---|---|
| (mJy) | (km s−1) | (Jy) | (km s−1) | (107 K) | (s−1) | |||
| R Aql | 43 | 45.2 | 1.7 | 1.2 | 14 | 0.8−1.4 | 0.2−0.4 | 0.04−0.08 |
| 46.9 | 3.9 | 0.7 | 32 | 1.7−3.1 | 0.5−0.9 | 0.1−0.2 | ||
| 48.7 | 10.1 | 1.8 | 83 | 4.5−8.1 | 1.3−2.3 | 0.3−0.5 | ||
| 48.9 | 10.4 | 1.0 | 85 | 4.6−8.4 | 1.3−2.3 | 0.3−0.5 | ||
| 52.0 | 3.9 | 0.7 | 32 | 1.7−3.1 | 0.5−0.9 | 0.1−0.2 | ||
| μ Cep | 46 | 26.0 | 3.3 | 0.4 | 25.0 | 4.1−89.9 | 1.1−25 | 0.2−5 |
| 26.4 | 4.0 | 1.4 | 31 | 5.0−109.0 | 1.4−30.3 | 0.3−6.1 | ||
| 28.2 | 6.0 | 1.5 | 46 | 7.5−163.4 | 2.1−45.4 | 0.4−9.1 | ||
| 29.5 | 2.1 | 0.3 | 16 | 2.6−57.2 | 0.7−15.9 | 0.1−3.2 | ||
| 30.5 | 4.3 | 1.1 | 33 | 5.4−117.1 | 1.5−32.5 | 0.3−6.5 | ||
| 33.3 | 1.9 | 0.3 | 15 | 2.4−51.8 | 0.7−14.4 | 0.1−2.9 | ||
| 34.5 | 4.6 | 1.4 | 35 | 5.8−125.3 | 1.6−34.8 | 0.3−7.0 | ||
| 34.9 | 2.2 | 0.5 | 17 | 2.8−59.9 | 0.8−16.6 | 0.2−3.3 | ||
| o Ceti | 36 | 44.8 | 26.2 | 0.6 | 260 | 2.5 | 0.7 | 0.1 |
| 46.8 | 68.7 | 0.4 | 682 | 6.5 | 1.8 | 0.4 | ||
| 47.0 | 26.5 | 1.0 | 263 | 2.5 | 0.7 | 0.1 | ||
| 47.9 | 37.4 | 0.4 | 372 | 3.6 | 1.0 | 0.2 | ||
| 49.2 | 93.8 | 0.9 | 932 | 8.9 | 2.5 | 0.5 | ||
| 49.3 | 93.7 | 0.5 | 931 | 8.9 | 2.5 | 0.5 | ||
| χ Cyg | 38 | 7.1 | 39.4 | 1.2 | 366 | 10.5 | 2.9 | 0.6 |
| 9.1 | 290.2 | 0.5 | 2693 | 77.6 | 21.6 | 4.3 | ||
| 9.3 | 172.7 | 1.1 | 1603 | 46.2 | 12.8 | 2.6 | ||
| 11.2 | 64.2 | 1.2 | 596 | 17.2 | 4.9 | 1.0 | ||
| 11.7 | 124.3 | 0.5 | 1154 | 33.2 | 9.3 | 1.9 | ||
| 13.6 | 15.1 | 1.2 | 140 | 4.0 | 1.1 | 0.2 | ||
| U Her | 45 | –20.1 | 3.7 | 1.3 | 29 | 2.2 | 0.6 | 0.1 |
| (March) | –17.7 | 30.2 | 1.0 | 240 | 18.3 | 5.1 | 1.0 | |
| –16.0 | 31.9 | 1.0 | 254 | 19.3 | 5.4 | 1.1 | ||
| –14.0 | 6.9 | 1.3 | 55 | 4.2 | 1.2 | 0.2 | ||
| –10.4 | 2.1 | 2.0 | 17 | 1.3 | 0.4 | 0.1 | ||
| U Her | 140 | –19.7 | 2.9 | 0.9 | 73 | 1.8 | 0.5 | 0.1 |
| (May) | –17.4 | 29.0 | 0.6 | 731 | 17.5 | 4.9 | 1.0 | |
| –17.0 | 32.9 | 1.3 | 830 | 19.9 | 5.5 | 1.1 | ||
| –16.2 | 19.6 | 0.6 | 495 | 11.9 | 3.3 | 0.7 | ||
| –14.2 | 3.2 | 1.5 | 81 | 1.0 | 0.3 | 0.1 | ||
| R Leo | 29 | –5.2 | 15.8 | 0.7 | 196 | 1.3 | 0.4 | 0.1 |
| –3.8 | 47.2 | 0.5 | 587 | 3.9 | 1.1 | 0.2 | ||
| –1.2 | 137.6 | 0.7 | 1710 | 11.3 | 3.1 | 0.6 | ||
| –0.2 | 162.3 | 2.3 | 2018 | 13.4 | 3.7 | 0.7 | ||
| 0.6 | 117.9 | 0.8 | 1465 | 9.7 | 2.7 | 0.5 | ||
| 2.7 | 21.6 | 0.4 | 268 | 1.8 | 0.5 | 0.1 | ||
| 3.5 | 51.3 | 1.5 | 637 | 4.2 | 1.2 | 0.2 |
Notes. We considered two different distances for μ Cep and R Aql (see Table 1).
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