EDGES-3: Instrument Design and Commissioning

EDGES-3 is the third iteration of the Experiment to Detect the Global EoR Signature (EDGES) experiment, designed to measure the predicted global absorption feature in the radio spectrum produced by neutral hydrogen gas at cosmic dawn, a critical observation determining when and how the first stars populated the universe. The EDGES-3 instrument has been redesigned to include both the analog and digital electronics within the antenna, allowing for in-situ calibration and removal of the lossy balun found in EDGES-2. EDGES-3 has been on multiple deployments in the past 4 yr; to Oregon, Devon Island, Adak Island, and is currently installed and taking data in the outback of Western Australia. This paper provides an accounting of the challenges inherent in the detection of the global, cosmological 21 cm signal, the strategies EDGES employs to mitigate each of these challenges, a description of the instrument, and a report on the Western Australia deployment along with observational data.

Authors

Publication Details

Journal
Apollo (University of Cambridge)
Published
2025-12-01
DOI
https://doi.org/10.17863/cam.126131
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

EDGES-3: Instrument Design and Commissioning

Chris Eckert, Rigel Cappallo, John P. Barrett, Kenneth Wilson et al.
Apollo (University of Cambridge)
Radio Astronomy Observations and Technology
article

EDGES-3: Instrument Design and Commissioning

Chris Eckert, Rigel Cappallo, John P. Barrett, Kenneth Wilson, Raúl A. Monsalve, Nivedita Mahesh, Alan EE Rogers, Akshatha K Vydula, Judd D Bowman, Steven G Murray, Peter Sims, Parker Steen, Colin J Lonsdale
article en

Abstract

EDGES-3 is the third iteration of the Experiment to Detect the Global EoR Signature (EDGES) experiment, designed to measure the predicted global absorption feature in the radio spectrum produced by neutral hydrogen gas at cosmic dawn, a critical observation determining when and how the first stars populated the universe. The EDGES-3 instrument has been redesigned to include both the analog and digital electronics within the antenna, allowing for in-situ calibration and removal of the lossy balun found in EDGES-2. EDGES-3 has been on multiple deployments in the past 4 yr; to Oregon, Devon Island, Adak Island, and is currently installed and taking data in the outback of Western Australia. This paper provides an accounting of the challenges inherent in the detection of the global, cosmological 21 cm signal, the strategies EDGES employs to mitigate each of these challenges, a description of the instrument, and a report on the Western Australia deployment along with observational data.

Apollo (University of Cambridge)
Openalex Percentile: Top 23%
Radio Astronomy Observations and Technology
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.