Persson, Magnus
2016-03-07
<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>
The data is provided as is, however, with this data it is possible
to reproduce the results presented in the paper(s) :
"The deuterium fractionation of water on solar-system scales in
deeply- embedded low-mass protostars" - Persson et al. (2014)
DOI link : http://dx.doi.org/10.1051/0004-6361/201322845
"Subarcsecond resolution observations of warm water toward three
deeply embedded low-mass protostars" - Persson et al. (2014)
DOI link: http://dx.doi.org/10.1051/0004-6361/201117917
If any publication is planned that will use this particular dataset,
I would greatly appreciate a "heads up", as I am very interested in
the re-use and further analysis of this data.
https://doi.org/10.5281/zenodo.47123
oai:zenodo.org:47123
Zenodo
https://doi.org/10.1051/0004-6361/201117917
https://doi.org/10.1051/0004-6361/201322845
https://zenodo.org/communities/astronomy-general
https://doi.org/
info:eu-repo/semantics/openAccess
Creative Commons Zero v1.0 Universal
https://creativecommons.org/publicdomain/zero/1.0/legalcode
astronomy
observations
PdBI
protostars
star formation
Observations of H218O at 203.4 GHz and HDO at 225 GHz (and 241 GHz) toward IRAS 2A, IRAS 4A and IRAS 4B
info:eu-repo/semantics/other