Wideband RFI Monitor Requirements, Design, and Commissioning at DRAO
Nicholas Bruce, Charl Baard, Stephen Harrison, Mohammad Islam, Abraham J. Otto, Dustin Lagoy, Robert Messing, Benoit Robert, Timothy Robishaw, Peter F. Driessen

TL;DR
This paper details the design, deployment, and commissioning of a wideband radio frequency interference monitor at DRAO, capable of high-resolution transient detection and long-term environment characterization.
Contribution
It introduces a novel RFI monitor with enhanced calibration, stability, and applications, including a new method to assess gain drift effects on data integration.
Findings
The monitor supports 2 GHz bandwidth with ~100 Hz channel resolution.
It operates as both a transient detector and environment characterization tool.
A new method for calculating gain drift effects was derived.
Abstract
In this paper, we introduce the radio frequency interference monitor deployed at the Dominion Radio Astrophysical Observatory. It provides 2 GHz of instantaneous bandwidth, supporting channel bandwidths as fine as ~100 Hz for 1 s integrations, or integration times as low as ~50 ms for the standard 3.33 kHz channel bandwidth. After operating as a prototype instrument for several years, the monitor was commissioned to improve the calibration method, analog section temperature, and gain stability. It now operates both as a transient detector and as a long-term radio environment characterization tool. We introduce novel applications for the monitor and derive a new method for calculating the effect of gain drift on integrated data.
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