Astronomy-General
Published March 7, 2016 | Version v1
Dataset Open

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

Creators

  • 1. Leiden Observatory

Description

This archive is currently hosted at zenodo.com by Magnus Persson. If 
you downloaded it from elsewhere, please send me an 
email (magnusp@vilhelm.nu).

This data was observed at the IRAM Plateau de Bure Interferometer 
(now NOEMA). Any publication arising from this data should have the 
appropriate notice that is provided by the IRAM instititue (see 
http://iram.fr).

This dataset currently contains the continuum subtracted UV-tables, 
in GILDAS u-v and UVFITS AIPS format for the sources NGC 1333 IRAS 
2A, NGC 1333 IRAS 4A, and NGC 1333 IRAS 4B at 203.4 GHz and 225.9 
GHz observed in the B and C configuration at PdBI (NOEMA). The 
target lines for the publicated project are the H218O line at 203 
GHz and the HDO line at 226 GHz. In addition to this there is also 
the 241 GHz HDO line for NGC 133 IRAS 2A observed in the C 
configuration.

Notes

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.

Files

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Additional details

Related works

Is supplement to
10.1051/0004-6361/201117917 (DOI)
10.1051/0004-6361/201322845 (DOI)