Dataset Open Access

Continuum u-v tables for NGC 1333 IRAS 2A (PdBI, 203 GHz), NGC 1333 IRAS 4A (SMA, 335), NGC 1333 IRAS 4B (PdBI, 203), and VLA 1623 (ALMA, 219)

Persson, Magnus

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), Atacama Large (sub-)Millimeter Array (ALMA) and 
SubMillimter Array (SMA). Any publication arising from this data 
should have the appropriate notice that is provided by the 
instititue in question (see http://iram.fr, http://almascience.org 
or http://sma1.sma.hawaii.edu/).

The data is provided as is, however, with this data it is possible 
to reproduce the results presented in the paper(s) : "Constraining 
the physical structure of the inner few 100 AU scales of 
deeply-embedded low-mass protostars.", Authors: M. V. Persson, D. 
Harsono, J. J. Tobin, E. F. van Dishoeck, J. K. Jørgensen, N. 
Murillo, and S.-P. Lai, journal Astronomy & Astrohpysics


This dataset currently contains the continuum subtracted UV-tables, 
in UVFITS format written by GILDAS MAPPING for the sources NGC 1333 
IRAS 2A (203 GHz), NGC 1333 IRAS 4A (335), NGC 1333 IRAS 4B (203), 
and VLA 1623 (219).

 

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. This work has benefited from research funding from the European Community's sixth Framework Programme under RadioNet R113CT 2003 5058187. This paper made use of the following ALMA data: ADS/JAO.ALMA 2013.1.01004.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.
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