EZOA: Nançay H

We present follow-up 21 cm H <ns0:sc>I</ns0:sc> line observations made with the Nançay Radio Telescope (NRT) of 99 weak or potential detections of galaxies from the EZOA catalogue in the northern Zone of Avoidance (ZoA), which were extracted from the shallow version of the EBHIS blind H <ns0:sc>I</ns0:sc> survey performed with the Effelsberg radio telescope. The new NRT observations are on average almost three times as sensitive as those from EBHIS. Of the 99 observed sources, we confirmed 72, while three yielded inconclusive results. We find that the quality assessment of the EZOA catalogue entries correlates well with the NRT recovery rate; for instance, only four of the 22 potential detections could be confirmed. Due to the higher sensitivity as well as the large north-south extent of the NRT beam, the NRT observations also yielded five serendipitous detections, which we include here. We updated the EZOA catalogue with the improved H <ns0:sc>I</ns0:sc> parameters and detections. To test the mitigation of radio frequency interference signals, we also observed selected sources using a dedicated receiver and data processing system.

Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-03-07
DOI
https://doi.org/10.1051/0004-6361/202453250/pdf
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
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article

EZOA: Nançay H

Springer Link (Chiba Institute of Technology)
Galaxies: Formation, Evolution, Phenomena
article

EZOA: Nançay H

article en

Abstract

We present follow-up 21 cm H <ns0:sc>I</ns0:sc> line observations made with the Nançay Radio Telescope (NRT) of 99 weak or potential detections of galaxies from the EZOA catalogue in the northern Zone of Avoidance (ZoA), which were extracted from the shallow version of the EBHIS blind H <ns0:sc>I</ns0:sc> survey performed with the Effelsberg radio telescope. The new NRT observations are on average almost three times as sensitive as those from EBHIS. Of the 99 observed sources, we confirmed 72, while three yielded inconclusive results. We find that the quality assessment of the EZOA catalogue entries correlates well with the NRT recovery rate; for instance, only four of the 22 potential detections could be confirmed. Due to the higher sensitivity as well as the large north-south extent of the NRT beam, the NRT observations also yielded five serendipitous detections, which we include here. We updated the EZOA catalogue with the improved H <ns0:sc>I</ns0:sc> parameters and detections. To test the mitigation of radio frequency interference signals, we also observed selected sources using a dedicated receiver and data processing system.

Springer Link (Chiba Institute of Technology)
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