Observations Of H218O At 203.4 Ghz And Hdo At 225 Ghz (And 241 Ghz) Toward Iras 2A, Iras 4A And Iras 4B
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This archive is currently hosted at zenodo.com by Magnus Persson. If <br> you downloaded it from elsewhere, please send me an <br> email (magnusp@vilhelm.nu). This data was observed at the IRAM Plateau de Bure Interferometer <br> (now NOEMA). Any publication arising from this data should have the <br> appropriate notice that is provided by the IRAM instititue (see <br> http://iram.fr). This dataset currently contains the continuum subtracted UV-tables, <br> in GILDAS u-v <strong>and</strong> UVFITS AIPS format for the sources NGC 1333 IRAS <br> 2A, NGC 1333 IRAS 4A, and NGC 1333 IRAS 4B at 203.4 GHz and 225.9 <br> GHz observed in the B and C configuration at PdBI (NOEMA). The <br> target lines for the publicated project are the H<sub>2</sub><sup>18</sup>O line at 203 <br> GHz and the HDO line at 226 GHz. In addition to this there is also <br> the 241 GHz HDO line for NGC 133 IRAS 2A observed in the C <br> configuration.



