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 <br /> you downloaded it from elsewhere, please send me an <br /> email (magnusp@vilhelm.nu).</p> <p>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).</p> <p>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.</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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