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Observations of H218O at 203.4 GHz and HDO at 225 GHz (and 241 GHz) toward IRAS 2A, IRAS 4A and IRAS 4B

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

ShareScore

40/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
8
Harmonization
4
Access
16
Reuse readiness
8
Engagement
4

Topics

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