Our PapersΒΆ
Nature Astronomy (2024)
We apply the
SimBIG
to analyze the SDSS-III: BOSS CMASS galaxies using two clustering statistics beyond the standard power spectrum: the bispectrum and a summary of the galaxy field based on a convolutional neural network. We constrain the cosmic expansion (H0) and growth rate (S8) 1.5 and 1.9 times more tightly than power spectrum analyses.PRD accepted (2024)
We apply the
SimBIG
to analyze the masked power spectra of SDSS-III: BOSS CMASS galaxies.PRD 109, 3528 (2024)
We apply the
SimBIG
to analyze the skew spectra of SDSS-III: BOSS CMASS galaxies.PRD 109, 3534 (2024)
We apply the
SimBIG
to analyze the bispectrum of SDSS-III: BOSS CMASS galaxies.PRD 109, 3535 (2024)
We apply the
SimBIG
to analyze the wavelet scattering transform of SDSS-III: BOSS CMASS galaxies.PRD 109, 3536 (2024)
We apply the
SimBIG
to conduct a field-level inference of SDSS-III: BOSS CMASS galaxies based on convolutional neural networks.PNAS 120, 42 (2023)
We present the
SimBIG
framework and apply it to analyze the power spectrum of SDSS-III: BOSS CMASS galaxies. We demonstrate that we can rigorously analyze galaxy clustering down to non-scales (k=0.5 h/Mpc) and extract additional cosmological information beyondc current standard anlayses.JCAP 2023, 4 (2022)
We present the mock challenge used to validate the
SimBIG
framework. The mock challenge consists of 1,500 test simulations constructed using forward models with different N-body simulation, halo finder, and galaxy-halo connection. With these simulations, we rigorously validate the accuarcy and precision of the posteriors inferred from SimBIG