A New Hardware Correlator in Korea: Performance Evaluation using KVN observations
Sang-Sung Lee (1,2), Chung Sik Oh (1), Duk-Gyoo Roh (1), Se-Jin Oh, (1), Jongsoo Kim (1,2), Jae-Hwan Yeom (1), Hyo Ryoung Kim (1), Dong-Gyu Jung, (1), Do-Young Byun (1), Taehyun Jung (1,2), Noriyuki Kawaguchi (3), Katsunori, M. Shibata (4), and Kiyoaki Wajima (1) ((1) KASI

TL;DR
This paper evaluates the performance of Korea's new Daejeon hardware correlator for VLBI observations, comparing it with a software correlator, and finds it produces consistent results suitable for continuum radio astronomy.
Contribution
The study presents the first performance assessment of the Daejeon hardware correlator, demonstrating its reliability and identifying minor differences with software correlator outputs.
Findings
Correlation outputs are consistent within 8%
Amplitude loss due to double-layer pattern is about 3%
Daejeon correlator is suitable for continuum observations
Abstract
We report results of the performance evaluation of a new hardware correlator in Korea, the Daejeon correlator, developed by the Korea Astronomy and Space Science Institute (KASI) and the National Astronomical Observatory of Japan (NAOJ). We conducted Very Long Baseline Interferometry (VLBI) observations at 22~GHz with the Korean VLBI Network (KVN) in Korea and the VLBI Exploration of Radio Astrometry (VERA) in Japan, and correlated the aquired data with the Daejeon correlator. For evaluating the performance of the new hardware correlator, we compared the correlation outputs from the Daejeon correlator for KVN observations with those from a software correlator, the Distributed FX (DiFX). We investigated the correlated flux densities and brightness distributions of extragalactic compact radio sources. The comparison of the two correlator outputs show that they are consistent with each…
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