Design, operation and performance of the PAON4 prototype transit interferometer
arXiv:1910.07956 · 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~meter diameter dishes in a compact triangular configuration, with a total geometric collecting area of , and equipped with dual polarization receivers. A total of 36 visibilities are computed from the 8 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 line. We operated PAON4 over several years and use data from observations in different periods to assess the array performance. We present preliminary analysis of a large fraction of this data and discuss crucial issues for this type of instrument, such as the calibration strategy, instrument response stability, and noise behaviour.
arXiv comment17 pages, 16 figures, accepted to MNRAS
References in corpus (52)
- Planck 2015 results. XIII. Cosmological parameters
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- LOFAR: The LOw-Frequency ARray
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
- A Population of Fast Radio Bursts at Cosmological Distances
- The direct localization of a fast radio burst and its host
- Beyond CDM: Problems, solutions, and the road ahead
- The Precision Array for Probing the Epoch of Reionization: 8 Station Results
- An Accurate Flux Density Scale from 50 MHz to 50 GHz
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization
- Measurement of 21 cm brightness fluctuations at z ~ 0.8 in cross-correlation
- Late-time cosmology with 21cm intensity mapping experiments
- The International Pulsar Timing Array: Second data release
- LOFAR facet calibration
- Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
- Revisiting the radio interferometer measurement equation. I. A full-sky Jones formalism
- HI intensity mapping : a single dish approach
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
- Radio interferometric gain calibration as a complex optimization problem
- Evolution of the 21 cm signal throughout cosmic history
- The Green Bank Northern Celestial Cap Pulsar Survey - I: Survey Description, Data Analysis, and Initial Results
- Dark Energy Survey Year 1 Results: Measurement of the Baryon Acoustic Oscillation scale in the distribution of galaxies to redshift 1
- All-Sky Interferometry with Spherical Harmonic Transit Telescopes
- Coaxing Cosmic 21cm Fluctuations from the Polarized Sky using m-mode Analysis
- Twenty-one centimeter tomography with foregrounds
- The Tianlai project: a 21cm cosmology experiment
- Baryonic Acoustic Oscillations in 21cm Emission: A Probe of Dark Energy out to High Redshifts
- Observables and unobservables in dark energy cosmologies
- The Fast Fourier Transform Telescope
- Radio Interferometric Calibration Using The SAGE Algorithm
- Cosmological Constraints from Multiple Probes in the Dark Energy Survey
- The effect of foreground subtraction on cosmological measurements from Intensity Mapping
- Fundamental Limitations on the Calibration of Redundant 21 cm Cosmology Instruments and Implications for HERA and the SKA
- Probing dark energy with baryonic oscillations and future radio surveys of neutral Hydrogen
- Simulations for single-dish intensity mapping experiments
- Fast gain calibration in radio astronomy using alternating direction implicit methods: Analysis and applications
- 21 cm observation of LSS at z~1 Instrument sensitivity and foreground subtraction
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Angular clustering tomography and its cosmological implications
- The BINGO telescope: a new instrument exploring the new 21-cm cosmology window
- Sky reconstruction from transit visibilities: PAON-4 and Tianlai Dish Array
- Sky reconstruction for the Tianlai cylinder array
- 21 cm Intensity Mapping
- BAORadio: A digital pipeline for radio interferometry and 21 cm mapping of large scale structures
- Reconstruction of HI power spectra with radio-interferometers to study dark energy
- Characterization of a dense aperture array for radio astronomy
- HI intensity mapping with FAST
- Progress in the Construction and Testing of the Tianlai Radio Interferometers
- A Digital Broadband Beamforming Architecture for 2-PAD
- On sky characterization of the BAORadio wide band digital backend: Search for HI emission in Abell85, Abell1205 and Abell2440 galaxy clusters