Design, operation and performance of the PAON4 prototype transit interferometer

• Published in: Monthly notices of the Royal Astronomical Society Vol. 493; no. 2; pp. 2965 - 2980
• Main Authors: Ansari, R, Campagne, J E, Charlet, D, Moniez, M, Pailler, C, Perdereau, O, Taurigna, M, Martin, J M, Rigaud, F, Colom, P, Abbon, Ph, Magneville, Ch, Pezzani, J, Viou, C, Torchinsky, S A, Huang, Q, Zhang, J
• Format: Journal Article
• Language: English
• Published: Oxford University Press 01.04.2020; Oxford University Press (OUP): Policy P - Oxford Open Option A
• Subjects: Astrophysics; Instrumentation and Detectors; Physics; radio continuum: general; radio lines: galaxies; cosmology: observations, large-scale structure of Universe; methods: observational; instrumentation: interferometers; techniques: interferometric; large-scale structure of Universe; cosmology: observations
• ISSN: 0035-8711; 1365-2966
• DOI: 10.1093/mnras/staa345

ABSTRACT PAON4 is an L-band (1250–1500 MHz) small interferometer operating in transit mode deployed at the Nançay observatory in France, designed as a prototype instrument for intensity mapping. It features four 5 m diameter dishes in a compact triangular configuration, with a total geometric collecting area of ${\sim} 75\, \mathrm{m^2}$, and is equipped with dual polarization receivers. A total of 36 visibilities are computed from the eight independent RF signals by the software correlator over the full 250 MHz RF band. The array operates in transit mode, with the dishes pointed toward a fixed declination, while the sky drifts across the instrument. Sky maps for each frequency channel are then reconstructed by combining the time-dependent visibilities from the different baselines observed at different declinations. This paper presents an overview of the PAON4 instrument design and goals, as a prototype for dish arrays to map the large-scale structure in radio, using intensity mapping of the atomic hydrogen 21 cm line. We operated PAON4 over several years and use data from observations at different periods to assess the array performance. We present a preliminary analysis of a large fraction of these data and discuss crucial issues for this type of instrument, such as the calibration strategy, instrument response stability and noise behaviour.