Table 2.

Key observational characteristics of the FAST-H i COSMOS data. Note that the total sky coverage is |$\sim$|2 deg|$^2$| where the centre sensitive area is |$\sim$|1.2 deg|$^2$|⁠.

Key parametersFAST
Centre coordinate10h00m, +02d14m
Area covered|$\sim$|2 deg|$^2$|
Obs. time11 h
Frequency range|$1310{\!-\!}1420$| MHz
Channel width22.9 kHz
Pixel size60|$^{\prime \prime }$|
Median H i channel rms noise|$\sim$|385 μJy beam|$^{-1}$|
Beam174|$^{\prime \prime }$||$\times$| 174|$^{\prime \prime }$| (⁠|$z=0$|⁠)
|$N_\mathrm{H\,{{\small I}}}$| sensitivity (⁠|$3\sigma$|⁠)|${\sim} 2\times 10^{17}$||$\mathrm{cm}^{-2}$|
Key parametersFAST
Centre coordinate10h00m, +02d14m
Area covered|$\sim$|2 deg|$^2$|
Obs. time11 h
Frequency range|$1310{\!-\!}1420$| MHz
Channel width22.9 kHz
Pixel size60|$^{\prime \prime }$|
Median H i channel rms noise|$\sim$|385 μJy beam|$^{-1}$|
Beam174|$^{\prime \prime }$||$\times$| 174|$^{\prime \prime }$| (⁠|$z=0$|⁠)
|$N_\mathrm{H\,{{\small I}}}$| sensitivity (⁠|$3\sigma$|⁠)|${\sim} 2\times 10^{17}$||$\mathrm{cm}^{-2}$|
Table 2.

Key observational characteristics of the FAST-H i COSMOS data. Note that the total sky coverage is |$\sim$|2 deg|$^2$| where the centre sensitive area is |$\sim$|1.2 deg|$^2$|⁠.

Key parametersFAST
Centre coordinate10h00m, +02d14m
Area covered|$\sim$|2 deg|$^2$|
Obs. time11 h
Frequency range|$1310{\!-\!}1420$| MHz
Channel width22.9 kHz
Pixel size60|$^{\prime \prime }$|
Median H i channel rms noise|$\sim$|385 μJy beam|$^{-1}$|
Beam174|$^{\prime \prime }$||$\times$| 174|$^{\prime \prime }$| (⁠|$z=0$|⁠)
|$N_\mathrm{H\,{{\small I}}}$| sensitivity (⁠|$3\sigma$|⁠)|${\sim} 2\times 10^{17}$||$\mathrm{cm}^{-2}$|
Key parametersFAST
Centre coordinate10h00m, +02d14m
Area covered|$\sim$|2 deg|$^2$|
Obs. time11 h
Frequency range|$1310{\!-\!}1420$| MHz
Channel width22.9 kHz
Pixel size60|$^{\prime \prime }$|
Median H i channel rms noise|$\sim$|385 μJy beam|$^{-1}$|
Beam174|$^{\prime \prime }$||$\times$| 174|$^{\prime \prime }$| (⁠|$z=0$|⁠)
|$N_\mathrm{H\,{{\small I}}}$| sensitivity (⁠|$3\sigma$|⁠)|${\sim} 2\times 10^{17}$||$\mathrm{cm}^{-2}$|
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