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)

This archive is currently hosted at zenodo.com by Magnus Persson. If <br> you downloaded it from elsewhere, please send me an <br> email ([e-mail]). This data was observed at the IRAM Plateau de Bure Interferometer <br> (now NOEMA), Atacama Large (sub-)Millimeter Array (ALMA) and <br> SubMillimter Array (SMA). Any publication arising from this data <br> should have the appropriate notice that is provided by the <br> instititue in question (see http://iram.fr, http://almascience.org <br> or http://sma1.sma.hawaii.edu/). The data is provided as is, however, with this data it is possible <br> to reproduce the results presented in the paper(s) : "Constraining <br> the physical structure of the inner few 100 AU scales of <br> deeply-embedded low-mass protostars.", Authors: M. V. Persson, D. <br> Harsono, J. J. Tobin, E. F. van Dishoeck, J. K. Jørgensen, N. <br> Murillo, and S.-P. Lai, journal Astronomy &amp; Astrohpysics <br> This dataset currently contains the continuum subtracted UV-tables, <br> in UVFITS format written by GILDAS MAPPING for the sources NGC 1333 <br> IRAS 2A (203 GHz), NGC 1333 IRAS 4A (335), NGC 1333 IRAS 4B (203), <br> and VLA 1623 (219).