The HETDEX Survey: Emission Line Exploration and Source Classification
Dustin Davis, Karl Gebhardt, Erin Mentuch Cooper, Robin Ciardullo,, Maximilian Fabricius, Daniel J. Farrow, John J. Feldmeier, Steven L., Finkelstein, Eric Gawiser, Caryl Gronwall, Gary J. Hill, Ulrich Hopp, Lindsay, R. House, Donghui Jeong, Wolfram Kollatschny, Eiichiro Komatsu

TL;DR
The paper presents the HETDEX survey's goal to map over a million galaxies using emission lines, and introduces ELiXer, a classification tool that effectively distinguishes Lyα emitters from interlopers with high accuracy and low contamination.
Contribution
It introduces ELiXer, a novel classification method that improves galaxy identification accuracy in the HETDEX survey, enabling precise large-scale structure measurements.
Findings
ELiXer achieves 98.1% accuracy in distinguishing LAEs from foreground galaxies.
Contamination rate of Lyα by [OII] is estimated at 1.2%.
Lyα recovery rate using ELiXer is 99.1%.
Abstract
The Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) is an untargeted spectroscopic survey that aims to measure the expansion rate of the Universe at to 1% precision for both and . HETDEX is in the process of mapping in excess of one million Lyman Alpha emitting (LAE) galaxies and a similar number of lower-z galaxies as a tracer of the large-scale structure. The success of the measurement is predicated on the post-observation separation of galaxies with Ly emission from the lower- interloping galaxies, primarily [OII], with low contamination and high recovery rates. The Emission Line eXplorer (ELiXer) is the principal classification tool for HETDEX, providing a tunable balance between contamination and completeness as dictated by science needs. By combining multiple selection criteria, ELiXer improves upon the 20 Angstrom rest-frame…
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Taxonomy
TopicsCCD and CMOS Imaging Sensors · Particle Detector Development and Performance · Astronomy and Astrophysical Research
