Four Planck-selected dusty star-forming galaxies are confirmed as strongly lensed at z≈2.3–3.3 via NOEMA CO line detections; a lens model for one source yields µ≈11.
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A pilot sample of Planck-selected strongly lensed sub-mm galaxies: NOEMA observations and physical characterisation
Four Planck-selected dusty star-forming galaxies are confirmed as strongly lensed at z≈2.3–3.3 via NOEMA CO line detections; a lens model for one source yields µ≈11.