Reddening Independent Quasar Selection from a Wide Field Optical and Near-IR Imaging Survey
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We present preliminary results from a wide field near-IR imaging survey that uses the Cambridge InfraRed Survey Instrument (CIRSI) on the 2.5m Isaac Newton Telescope (INT). CIRSI is a JH-band mosaic imager that contains 4 Rockwell 1024$^{2}$ HgCdTe detectors (the largest IR camera in existence), allowing us to survey approximately 4 deg^2 per night to H ~ 19. Combining CIRSI observations with the deep optical imaging from the INT Wide Field Survey, we demonstrate a reddening independent quasar selection technique based on the (g - z) / (z - H) color diagram.
To appear in Proceedings of the New Era of Wide Field Astronomy conference, Preston, England, August 2000
To appear in Proceedings of the New Era of Wide Field Astronomy conference, Preston, England, August 2000