The galaxy bispectrum, measuring excess clustering of galaxy triplets, offers a probe of dark energy via baryon acoustic oscillations (BAOs). However up to now it has been severely underused due to the combinatorically explosive number of triangles. Here we exploit interference in the bispectrum to identify triangles that amplify BAOs. This approach reduces the computational cost of estimating covariance matrices, offers an improvement in BAO constraints equivalent to lengthening BOSS by 30% and simplifies adding bispectrum BAO information to future large-scale redshift survey analyses
We detect the peak of baryon acoustic oscillations (BAO) in the two-point correlation function of a ...
International audienceWe investigate if, for a fixed number density of targets and redshift, there i...
Bull P, Camera S, Raccanelli A, et al. Measuring baryon acoustic oscillations with future SKA survey...
The galaxy bispectrum, measuring excess clustering of galaxy triplets, offers a probe of dark energy...
The present spatial distribution of galaxies in the Universe is non-Gaussian, with 40% skewness in 5...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the Baryon Acoustic Oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
International audienceBaryon Acoustic Oscillations (BAOs) are a feature imprinted in the galaxy dist...
International audienceWe develop a methodology to optimize the measurement of baryon acoustic oscill...
Baryon acoustic oscillations (BAOs) are a powerful probe of the expansion history of our Universe an...
International audienceWe perform a tomographic baryon acoustic oscillations (BAO) analysis using the...
We detect the peak of baryon acoustic oscillations (BAO) in the two-point correlation function of a ...
International audienceWe investigate if, for a fixed number density of targets and redshift, there i...
Bull P, Camera S, Raccanelli A, et al. Measuring baryon acoustic oscillations with future SKA survey...
The galaxy bispectrum, measuring excess clustering of galaxy triplets, offers a probe of dark energy...
The present spatial distribution of galaxies in the Universe is non-Gaussian, with 40% skewness in 5...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the baryon acoustic oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
We analyse the Baryon Acoustic Oscillation (BAO) signal of the final Baryon Oscillation Spectroscopi...
International audienceBaryon Acoustic Oscillations (BAOs) are a feature imprinted in the galaxy dist...
International audienceWe develop a methodology to optimize the measurement of baryon acoustic oscill...
Baryon acoustic oscillations (BAOs) are a powerful probe of the expansion history of our Universe an...
International audienceWe perform a tomographic baryon acoustic oscillations (BAO) analysis using the...
We detect the peak of baryon acoustic oscillations (BAO) in the two-point correlation function of a ...
International audienceWe investigate if, for a fixed number density of targets and redshift, there i...
Bull P, Camera S, Raccanelli A, et al. Measuring baryon acoustic oscillations with future SKA survey...