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We perform the first population study of luminous, but heavily-reddened quasars in the rest-frame UV at z = 1.5 – 2.7 – a peak epoch of both star formation and black hole accretion. We find resolved, blue emission in the DES imaging, consistent with a star forming host galaxy. Via SED fitting, we derive instantaneous SFRs for the sample and find a trend between quasar luminosity and SFR.
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