most cited2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering

13 citations · 25 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20235 cited

Unraveling emission line galaxy conformity at z~1 with DESI early data

Sihan Yuan, Risa H. Wechsler, Yunchong Wang +32

Emission line galaxies (ELGs) are now the preeminent tracers of large-scale structure at z>0.8 due to their high density and strong emission lines, which enable accurate redshift m…

astro-ph.CO20231 cited

Robust cosmological inference from non-linear scales with k-th nearest neighbor statistics

Sihan Yuan, Tom Abel, Risa H. Wechsler

We present the methodology for deriving accurate and reliable cosmological constraints from non-linear scales (<50Mpc/h) with k-th nearest neighbor (kNN) statistics. We detail our…

astro-ph.CO2023

Cosmological constraints from density-split clustering in the BOSS CMASS galaxy sample

Enrique Paillas, Carolina Cuesta-Lazaro, Will J. Percival +13

We present a clustering analysis of the BOSS DR12 CMASS galaxy sample, combining measurements of the galaxy two-point correlation function and density-split clustering down to a sc…

astro-ph.CO20231 cited

SUNBIRD: A simulation-based model for full-shape density-split clustering

Carolina Cuesta-Lazaro, Enrique Paillas, Sihan Yuan +13

Combining galaxy clustering information from regions of different environmental densities can help break cosmological parameter degeneracies and access non-Gaussian information fro…

astro-ph.CO20235 cited

Synthetic light cone catalogues of modern redshift and weak lensing surveys with AbacusSummit

Boryana Hadzhiyska, Sihan Yuan, Chris Blake +32

The joint analysis of different cosmological probes, such as galaxy clustering and weak lensing, can potentially yield invaluable insights into the nature of the primordial Univers…

astro-ph.CO202313 cited

2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering

Sihan Yuan, Alvaro Zamora, Tom Abel

Beyond standard summary statistics are necessary to summarize the rich information on non-linear scales in the era of precision galaxy clustering measurements. For the first time,…