A Per-Baseline, Delay-Spectrum Technique for Accessing the 21cm Cosmic Reionization Signature
arXiv:1204.4749 · doi:10.1088/0004-637X/756/2/165
Abstract
A critical challenge in measuring the power spectrum of 21cm emission from cosmic reionization is compensating for the frequency dependence of an interferometer's sampling pattern, which can cause smooth-spectrum foregrounds to appear unsmooth and degrade the separation between foregrounds and the target signal. In this paper, we present an approach to foreground removal that explicitly accounts for this frequency dependence. We apply the delay transformation introduced in Parsons & Backer (2009) to each baseline of an interferometer to concentrate smooth-spectrum foregrounds within the bounds of the maximum geometric delays physically realizable on that baseline. By focusing on delay-modes that correspond to image-domain regions beyond the horizon, we show that it is possible to avoid the bulk of smooth-spectrum foregrounds. We map the point-spread function of delay-modes to k-space, showing that delay-modes that are uncorrupted by foregrounds also represent samples of the three-dimensional power spectrum, and can be used to constrain cosmic reionization. Because it uses only spectral smoothness to differentiate foregrounds from the targeted 21cm signature, this per-baseline analysis approach relies on spectrally- and spatially-smooth instrumental responses for foreground removal. For sufficient levels of instrumental smoothness relative to interfering foregrounds, this technique substantially reduces the level of calibration previously thought necessary to detect 21cm reionization. As a result, this approach places fewer constraints on antenna configuration within an array, facilitating the adoption of configurations optimized for power-spectrum sensitivity. Under these assumptions, we demonstrate the potential for PAPER to detect 21cm reionization at an amplitude of 10 mK^2 near k~0.2h Mpc^-1 with 132 dipoles in 7 months of observing.
33 Pages, 11 figures, accepted to ApJ
References in corpus (14)
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- The morphology of HII regions during reionization
- Bright Source Subtraction Requirements For Redshifted 21 cm Measurements
- Four Fundamental Foreground Power Spectrum Shapes for 21 cm Cosmology Observations
- Foreground simulations for the LOFAR - Epoch of Reionization Experiment
- Radiative transfer simulations of cosmic reionization I: methodology and initial results
- Imaging the Epoch of Reionization: limitations from foreground confusion and imaging algorithms
- A lower limit of dz > 0.06 for the duration of the reionization epoch
- A Sensitivity and Array-Configuration Study for Measuring the Power Spectrum of 21cm Emission from Reionization
- The GMRT-EoR Experiment: A new upper limit on the neutral hydrogen power spectrum at z~8.6
- A Method for 21cm Power Spectrum Estimation in the Presence of Foregrounds
- Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array
- The EoR Sensitivity of the Murchison Widefield Array
- Polarised foreground removal at low radio frequencies using rotation measure synthesis: uncovering the signature of hydrogen reionisation
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