The Galactic Plane Infrared Polarization Survey (GPIPS) covers 76 sq. deg in the Galactic midplane between 18° <= l <= 56° and -1° <= b <= +1°. It uses H-band (1.6 microns) linear polarimetry to determine magnetic field orientations in the plane of the sky near dense molecular clouds. The full GPIPS data set will contain almost 6 million stars, with about one million of those having high-quality photometry. The link to the homepage of the GPIPS survey can be found here.
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GPIPS_Polarimetry_Data_Access.pdf
GPIPS_Polarimetry_Data_Access.pdf
Sep 5, 2016 - GPIPS Extended Observations: Polarimetry (2D)
Adobe PDF - 29.1 KB - MD5: f35045fe1e6bcf355732e41ba836e62f
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