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Deep Ecliptic Survey

Overview

The Deep Ecliptic Survey obtained deep images within a strip 13-degrees wide covering the full circumference of the ecliptic, using the Mosaic CCD cameras on the KPNO Mayall and CTIO Blanco 4-m telescopes. The primary goal was to identify faint Kuiper Belt Objects (KBOs) with the goal of mapping out the structure and population of the Kuiper Belt. To detect KBOs, each field was imaged twice within a single night. Exposures are typically 4 min. Data products include the reduced and calibrated survey images.

Deep Ecliptic Survey at a Glance

PI(s) Marc Buei
Proposal ID 2001B-0026
Years of Observation 2001-2005
Area covered: Sparse sampling of a 13-degree wide strip around the ecliptic
Bands VR-band (Broad filter that includes the V and R bands)
Median Depth (5σ) 23.4
Median Seeing 1.66 arcsec
Number of fields 4480