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20122022
most citedThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Analysis of potential systematics

279 citations · 866 across the 11 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

math.NA2018★ 51 cited

Convergence of Lobatto-type Runge-Kutta methods for partitioned differential-algebraic systems of index 2

Rodrigo Takuro Sato Martín de Almagro

In this paper we propose a numerical scheme for partitioned systems of index 2 DAEs, such as those arising from nonholonomic mechanical problems and prove the order of a certain cl…

astro-ph.GA2018★ 15 cited

Variable Stars in Local Group Galaxies. IV. RR Lyrae stars in the central regions of the low-density galaxy Crater II

M. Monelli, A. R. Walker, C. E. Martìnez-Vàzquez +9

We present a search and analysis of variable stars in the recently discovered Crater~II dwarf galaxy. Based on , , data collected with the Isaac Newton Telescope (FoV$\si…

astro-ph.CO2018★ 78 cited

Comparing approximate methods for mock catalogues and covariance matrices III: Bispectrum

Manuel Colavincenzo, Emiliano Sefusatti, Pierluigi Monaco +19

We compare the measurements of the bispectrum and the estimate of its covariance obtained from a set of different methods for the efficient generation of approximate dark matter ha…

astro-ph.CO2018★ 86 cited

Comparing approximate methods for mock catalogues and covariance matrices II: Power spectrum multipoles

Linda Blot, Martin Crocce, Emiliano Sefusatti +19

We study the accuracy of several approximate methods for gravitational dynamics in terms of halo power spectrum multipoles and their estimated covariance matrix. We propagate the d…

astro-ph.CO2018★ 84 cited

Comparing approximate methods for mock catalogues and covariance matrices I: correlation function

Martha Lippich, Ariel G. Sánchez, Manuel Colavincenzo +19

This paper is the first in a set that analyses the covariance matrices of clustering statistics obtained from several approximate methods for gravitational structure formation. We…