Pith. sign in

REVIEW

Reconstruction of HI power spectra with radio-interferometers to study dark energy

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 0807.3614 v1 pith:FBZT6DD2 submitted 2008-07-23 astro-ph

R. Ansari , J.-M. Le Goff , Ch. Magneville , M. Moniez , N. Palanque-Delabrouille , J. Rich , V. Ruhlmann-Kleider , Ch. Yèche This is my paper · ORCID
classification astro-ph
keywords darkenergydiscussoscillationspowerradio-interferometersacousticarrays
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

Among the tools available for the study of the dark energy driving the expansion of the Universe, Baryon Acoustic Oscillations (BAO) and their effects on the matter power spectrum are particularly attractive. It was recently proposed to study these oscillations by mapping the 21cm emission of the neutral hydrogen in the redshift range $0.5<z<3$. We discuss here the precision of such measurements using radio-interferometers consisting of arrays of dishes or north-south oriented cylinders. We then discuss the resulting uncertainties on the BAO scales and the sensitivity to the parameters of the Dark Energy equation of state.

Discussion (0). Continue with ORCID to comment.

Pith tools