Table 3.

Best-fitting parameters for the Perseus MC and W 43 with polarization.*

Perseus MCW |$43$|
|$T \:(\mbox{K})$|16.67±0.0720.14±0.06
|$\tau _{250}\ (\times 10^{-4})$|4.25±0.0659.3±0.5
|$f_\mathrm{TLS}$|0.0136±0.00040.0293±0.04
|$\Delta _0^\mathrm{max}/h \:(\mbox{GHz})$|14.8±0.211.3±0.1
|$R_\Delta$|0.619±0.0220.913±0.007
|$\tau _+ \ (\times 10^{-11} \:\mbox{s})$||$2.28^{+0.10}_{-0.09}$|2.89±0.05
|$L_\mathrm{min}$|0.193±0.0030.318±0.001
EM (⁠|$\mbox{cm}^{-6}\:\mbox{pc}$|⁠)28.2±2.44097±29
dof2732
|$\chi ^2/\mathrm{dof}$|3.597.65
Perseus MCW |$43$|
|$T \:(\mbox{K})$|16.67±0.0720.14±0.06
|$\tau _{250}\ (\times 10^{-4})$|4.25±0.0659.3±0.5
|$f_\mathrm{TLS}$|0.0136±0.00040.0293±0.04
|$\Delta _0^\mathrm{max}/h \:(\mbox{GHz})$|14.8±0.211.3±0.1
|$R_\Delta$|0.619±0.0220.913±0.007
|$\tau _+ \ (\times 10^{-11} \:\mbox{s})$||$2.28^{+0.10}_{-0.09}$|2.89±0.05
|$L_\mathrm{min}$|0.193±0.0030.318±0.001
EM (⁠|$\mbox{cm}^{-6}\:\mbox{pc}$|⁠)28.2±2.44097±29
dof2732
|$\chi ^2/\mathrm{dof}$|3.597.65

*The errors are |$1 \sigma $|⁠.

Table 3.

Best-fitting parameters for the Perseus MC and W 43 with polarization.*

Perseus MCW |$43$|
|$T \:(\mbox{K})$|16.67±0.0720.14±0.06
|$\tau _{250}\ (\times 10^{-4})$|4.25±0.0659.3±0.5
|$f_\mathrm{TLS}$|0.0136±0.00040.0293±0.04
|$\Delta _0^\mathrm{max}/h \:(\mbox{GHz})$|14.8±0.211.3±0.1
|$R_\Delta$|0.619±0.0220.913±0.007
|$\tau _+ \ (\times 10^{-11} \:\mbox{s})$||$2.28^{+0.10}_{-0.09}$|2.89±0.05
|$L_\mathrm{min}$|0.193±0.0030.318±0.001
EM (⁠|$\mbox{cm}^{-6}\:\mbox{pc}$|⁠)28.2±2.44097±29
dof2732
|$\chi ^2/\mathrm{dof}$|3.597.65
Perseus MCW |$43$|
|$T \:(\mbox{K})$|16.67±0.0720.14±0.06
|$\tau _{250}\ (\times 10^{-4})$|4.25±0.0659.3±0.5
|$f_\mathrm{TLS}$|0.0136±0.00040.0293±0.04
|$\Delta _0^\mathrm{max}/h \:(\mbox{GHz})$|14.8±0.211.3±0.1
|$R_\Delta$|0.619±0.0220.913±0.007
|$\tau _+ \ (\times 10^{-11} \:\mbox{s})$||$2.28^{+0.10}_{-0.09}$|2.89±0.05
|$L_\mathrm{min}$|0.193±0.0030.318±0.001
EM (⁠|$\mbox{cm}^{-6}\:\mbox{pc}$|⁠)28.2±2.44097±29
dof2732
|$\chi ^2/\mathrm{dof}$|3.597.65

*The errors are |$1 \sigma $|⁠.

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