68 citations · 250 across the 7 of their papers we have counts for
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Impact of Simulated 1/f Noise for HI Intensity Mapping Experiments
Stuart Harper, Clive Dickinson, Richard Battye +5
Cosmology has entered an era where the experimental limitations are not due to instrumental sensitivity but instead due to inherent systematic uncertainties in the instrumentation…
Cosmological parameter forecasts for HI intensity mapping experiments using the angular power spectrum
L. C. Olivari, C. Dickinson, R. A. Battye +4
HI intensity mapping is a new observational technique to survey the large-scale structure of matter using the 21 cm emission line of atomic hydrogen (HI). In this work, we simulate…
Update on the BINGO 21cm intensity mapping experiment
Richard Battye, Ian Browne, Tianyue Chen +21
21cm intensity mapping is a novel approach aimed at measuring the power spectrum of density fluctuations and deducing cosmological information, notably from the Baryonic Acoustic O…
Simulated Effects of 1/f Noise on an SKA Intensity Mapping Survey
Stuart E. Harper, Clive Dickinson, Richard Battye +1
It has been proposed recently that the SKA1-MID could be used to conduct an HI intensity mapping survey that could rival upcoming Stage IV dark energy surveys. However, measuring t…
HI intensity mapping with FAST
Marie-Anne Bigot-Sazy, Yin-Zhe Ma, Richard A. Battye +7
We discuss the detectability of large-scale HI intensity fluctuations using the FAST telescope. We present forecasts for the accuracy of measuring the Baryonic Acoustic Oscillation…
Extracting HI cosmological signal with Generalized Needlet Internal Linear Combination
L. C. Olivari, M. Remazeilles, C. Dickinson
HI intensity mapping is a new observational technique to map fluctuations in the large-scale structure of matter using the 21 cm emission line of atomic hydrogen (HI). Sensitive ra…
Quintessence with Yukawa Interaction
André A. Costa, Lucas C. Olivari, E. Abdalla
We consider a quintessence model for dark energy interacting with dark matter via a Yukawa interaction. To put constraints on this model we use the CMB measurements from the Planck…