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Table 1

Spectral windows (spws) of our ALMA observations of W Hya.

spw Central frequency (GHz) Bandwidth (MHz) Velocity resolution (km s−1) Angular resolution (mas) RMS mJy/beam Continuum flux density (mJy)
1 250.727 468.75 1.17 19.7 × 16.5 0.57 267.7 ± 1.3
2 251.826 468.75 1.16 19.3 × 16.7 0.52 270.0 ± 1.4
3 252.471 468.75 1.16 19.3 × 16.7 0.47 271.8 ± 1.0
4 253.703 468.75 1.15 19.1 × 16.5 0.52 273.7 ± 1.4
5 265.886 468.75 1.10 18.4 × 15.8 0.59 301.5 ± 1.6
6 266.943 468.75 1.10 18.4 × 15.8 0.55 305.6 ± 1.5
7 267.198 468.75 1.10 18.3 × 15.8 0.60 306.0 ± 1.5
8 267.720 937.50 1.09 18.2 × 15.8 0.63 306.2 ± 1.3
9 268.168 937.50 1.09 18.1 × 15.7 0.65 307.8 ± 1.3

Notes. The velocity resolution corresponds to twice the channel width, with the Hanning smoothing at the correlator taken into account. The RMS noise is given for each spectral channel.

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