VizieR Online Data Catalog: Polarization data toward the protostar Serpens SMM1 (Hull+, 2017)

We present ALMA 343GHz (Band 7; 870um) polarization observations toward the very embedded intermediate-mass protostar Serpens SMM1. We complement these observations with new Submillimeter Array (SMA) 345GHz (880um) dust polarization observations as well as with archival polarization maps obtained with the James Clerk Maxwell Telescope (JCMT; 850um) and the Combined Array for Research in Millimeter-wave Astronomy (CARMA; 1.3mm).

The 870um ALMA dust polarization observations that we present were taken on 2015 June 3 and 7, and have a synthesized beam (resolution element) of ~0.33", corresponding to a linear resolution of ~140au at a distance of 436pc. We also present 1.3mm (Band 6) ALMA spectral-line data, which were taken in two different array configurations on 2014 August 18 (~0.3" angular resolution) and 2015 April 06 (~1" resolution). Finally, we present 1.3mm ALMA continuum data with ~0.1" resolution (R. Pokhrel et al. 2017, in preparation), observed on 2016 September 10, 13, and 2016 October 31.

The SMA polarization observations (Figure 1(c)) were taken on 2012 May 25 (compact configuration) and 2012 September 2 and 3 (extended configuration), and have a synthesized beam of ~0.8".

The archival JCMT SCUBA polarization data (Figure 1(a)) were obtained from supplementary data provided by Matthews+ (2009, J/ApJS/182/143).

The CARMA polarization data (Figure 1(b)) were taken between 2011 and 2013 as part of the TADPOL survey (Hull+ 2014, J/ApJS/213/13). The data were taken using the 1.3mm polarization receiver system in the C, D, and E arrays at CARMA, which correspond to angular resolutions at 1.3mm of approximately 1", 2", and 4", respectively.

(2 data files).