Table 3
HINSA parameters fit using method 2.
| Source(1) | n |  |
VLSR | Δ V | Tab | S∕N(Tab) | S∕Nc | N(HINSA) |
|---|---|---|---|---|---|---|---|---|
| (km s−1) | (km s−1) | (K) | (1018 cm−2) | |||||
| G159.2-20A1 | 1 | 0.01(1) | 6.48(8) | 0.8(1) | 0.55(5) | – | – | 0.10(8) |
| 2 | 0.03(1) | 4.24(5) | 1.1(1) | 1.30(5) | 26 | 23 | 0.5(2) | |
| G160.51-17.07 | 1 | 0.01(1) | 10.45(8) | 0.4(1) | 0.40(4) | – | – | 0.08(5) |
| G165.6-09A1 | 1 | 0.02(1) | −0.6(1) | 0.7(1) | 0.6(1) | 7 | 9 | 0.4(2) |
| G170.88-10.92* | 1 | 0.09(1) | 5.95(6) | 0.89(7) | 3.88(4) | 91 | 30 | 1.4(1) |
| G172.8-14A1* | 1 | 0.10(1) | 5.60(5) | 0.89(1) | 3.1(1) | 31 | 30 | 1.7(3) |
| 2 | 0.24(1) | 6.50(5) | 0.93(7) | 7.87(8) | 78 | 52 | 4.2(3) | |
| G173.3-16A1* | 1 | 0.26(1) | 6.36(5) | 1.26(6) | 7.88(5) | 138 | 92 | 4.4(1) |
| G174.06-15A1* | 1 | 0.20(1) | 6.15(6) | 0.94(7) | 4.52(5) | 82 | 52 | 2.6(1) |
| G174.08-13.2* | 1 | 0.60(1) | 5.09(5) | 0.92(5) | 16.1(7) | 230 | 79 | 8.0(1) |
| G174.4-15A1 | 1 | 0.17(1) | 5.10(5) | 1.39(5) | 5.0(1) | 38 | 67 | 3.4(2) |
| 2 | 0.12(1) | 6.80(5) | 1.41(5) | 3.8(1) | 20 | 83 | 2.8(2) | |
| G175.34-10.8* | 1 | 0.07(1) | 5.35(6) | 0.70(1) | 2.79(6) | 43 | 14 | 1.0(1) |
| G178.98-06.7* | 1 | 0.22(1) | 7.52(5) | 0.82(6) | 8.93(8) | 108 | 40 | 3.1(1) |
| G192.2-11A2 | 1 | 0.07(1) | 10.2(1) | 1.4(1) | 2.63(9) | 34 | 77 | 1.9(3) |
| L1489E | 1 | (0.01) | – | – | – | – | – | – |
| L1521B* | 1 | 0.07(1) | 6.21(6) | 0.95(7) | 2.27(4) | 58 | 28 | 1.4(2) |
| 05413-0104 | 1 | (0.01) | – | – | – | – | – | – |
| HH25 MMS | 1 | 0.12(1) | 10.05(7) | 1.3(1) | 4.73(9) | 50 | 68 | 4.1(4) |
| CB34 | 1 | 0.05(0.01) | 0.81(4) | 1.3(1) | 3.50(8) | 43 | 46 | – |
Notes. (1) The superscript “*” means HINSA feature can be extracted using method 1 from the H I 21 cm spectrum of the corresponding source. (2) If τ0 is 0.01, the corresponding fitting result is unreliable (see Eq. (31) in Sect. 5.2.5). A number in parentheses indicates the 1σ uncertainty in the last digit.
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