The fitted parameters for the spectra from squares 5 and 6. The numbered columns are as follows: [1] the square number, [2] the mean flux density, [3] the number of Gaussian components fitted, [4] the peak optical depth assuming a covering factor of 1, [5] the integrated optical depth, also assuming a covering factor of 1, [6] the velocity shift with respect to the systemic velocity, [7] the FWHM of the absorption line, [8] the H i column density, where Ts is the spin temperature, [9] the Bayesian significance of the line, see Allison et al. (2012).
| Square . | Sv . | Nu.Gau. . | τpeak . | τint . | v . | FWHM . | NHI . | |${\rm ln}\, B$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$\rm mJy\, beam^{-1}$| . | . | . | . | km s−1 . | km s−1 . | atoms cm−2 . | . |
| 5 | 30.07 | 1 | |$0.14_{-0.01}^{+0.01}$| | |$28.16_{-1.97}^{+1.99}$| | |$-11_{-6}^{+6}$| | |$200_{-14}^{+16}$| | |$5.13_{-0.36}^{+0.36}\times 10^{19}T_{\rm s}$| | 145 |
| 6 | 9.84 | 1 | |$0.07_{-0.02}^{+0.02}$| | |$43.03_{-8.89}^{+9.05}$| | |$-148_{-63}^{+62}$| | |$581_{-103}^{+124}$| | |$7.83_{-1.61}^{+1.65}\times 10^{19}T_{\rm s}$| | 9 |
| Square . | Sv . | Nu.Gau. . | τpeak . | τint . | v . | FWHM . | NHI . | |${\rm ln}\, B$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$\rm mJy\, beam^{-1}$| . | . | . | . | km s−1 . | km s−1 . | atoms cm−2 . | . |
| 5 | 30.07 | 1 | |$0.14_{-0.01}^{+0.01}$| | |$28.16_{-1.97}^{+1.99}$| | |$-11_{-6}^{+6}$| | |$200_{-14}^{+16}$| | |$5.13_{-0.36}^{+0.36}\times 10^{19}T_{\rm s}$| | 145 |
| 6 | 9.84 | 1 | |$0.07_{-0.02}^{+0.02}$| | |$43.03_{-8.89}^{+9.05}$| | |$-148_{-63}^{+62}$| | |$581_{-103}^{+124}$| | |$7.83_{-1.61}^{+1.65}\times 10^{19}T_{\rm s}$| | 9 |
The fitted parameters for the spectra from squares 5 and 6. The numbered columns are as follows: [1] the square number, [2] the mean flux density, [3] the number of Gaussian components fitted, [4] the peak optical depth assuming a covering factor of 1, [5] the integrated optical depth, also assuming a covering factor of 1, [6] the velocity shift with respect to the systemic velocity, [7] the FWHM of the absorption line, [8] the H i column density, where Ts is the spin temperature, [9] the Bayesian significance of the line, see Allison et al. (2012).
| Square . | Sv . | Nu.Gau. . | τpeak . | τint . | v . | FWHM . | NHI . | |${\rm ln}\, B$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$\rm mJy\, beam^{-1}$| . | . | . | . | km s−1 . | km s−1 . | atoms cm−2 . | . |
| 5 | 30.07 | 1 | |$0.14_{-0.01}^{+0.01}$| | |$28.16_{-1.97}^{+1.99}$| | |$-11_{-6}^{+6}$| | |$200_{-14}^{+16}$| | |$5.13_{-0.36}^{+0.36}\times 10^{19}T_{\rm s}$| | 145 |
| 6 | 9.84 | 1 | |$0.07_{-0.02}^{+0.02}$| | |$43.03_{-8.89}^{+9.05}$| | |$-148_{-63}^{+62}$| | |$581_{-103}^{+124}$| | |$7.83_{-1.61}^{+1.65}\times 10^{19}T_{\rm s}$| | 9 |
| Square . | Sv . | Nu.Gau. . | τpeak . | τint . | v . | FWHM . | NHI . | |${\rm ln}\, B$| . |
|---|---|---|---|---|---|---|---|---|
| . | |$\rm mJy\, beam^{-1}$| . | . | . | . | km s−1 . | km s−1 . | atoms cm−2 . | . |
| 5 | 30.07 | 1 | |$0.14_{-0.01}^{+0.01}$| | |$28.16_{-1.97}^{+1.99}$| | |$-11_{-6}^{+6}$| | |$200_{-14}^{+16}$| | |$5.13_{-0.36}^{+0.36}\times 10^{19}T_{\rm s}$| | 145 |
| 6 | 9.84 | 1 | |$0.07_{-0.02}^{+0.02}$| | |$43.03_{-8.89}^{+9.05}$| | |$-148_{-63}^{+62}$| | |$581_{-103}^{+124}$| | |$7.83_{-1.61}^{+1.65}\times 10^{19}T_{\rm s}$| | 9 |
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