Submillimeter Array Polarimetry with Hertz

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Abstract
We describe the characteristics of the 350 μm polarimeter Hertz learned from laboratory tests and recent observations at the Caltech Submillimeter Observatory. Hertz contains a pair of 32 element arrays with 18'' pixel spacing and 20'' resolution. The instrument has been improved since initial observations in 1994 and 1995; the detector noise is now below the sky background noise. In excellent weather conditions on Mauna Kea, the noise-equivalent flux density (NEFD) for the measurement of polarized flux is 3-4 Jy Hz-1/2. The subtraction of correlated sky noise accomplished by the two-array design is crucial for achieving this performance. A method for analysis of our polarization data in the presence of the correlated noise is described. The instrumental polarization of Hertz is less than 0.5% across the detector array. Systematic errors in the measurement of polarization are less than 0.2%. We present a 350 μm polarization map of Sgr B2 with 140 detections at greater than 3 σ significance. For our current database of all 350 μm polarization measurements, the median polarization is 1.1%.

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