Article
Astronomy & Astrophysics
Emmanuel Schaan, Martin White
Summary: Line intensity mapping proposes an efficient method for observing distant faint galaxies and mapping the matter density field at high redshift. By measuring mean intensity and redshift-space power spectra, degeneracies between cosmology and astrophysics in LIM can be highlighted. LIM contains information about galaxies too faint to detect in high-noise or high-confusion regimes, making it a valuable tool for exploring the universe.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Yonadav Barry Ginat, Vincent Desjacques, Donghui Jeong, Fabian Schmidt
Summary: The study introduces a fully non-linear and relativistically covariant expression for the observed galaxy density contrast, ensuring the accurate consideration of the galaxy over-density field. This decomposition method is expected to be useful for future research on non-linearities in galaxy number counts, such as deriving the relativistic expression for the galaxy bispectrum. Additionally, the results are specialized to conformal Newtonian gauge, highlighting the importance of different contributions to the observed monopole of the galaxy density.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Maresuke Shiraishi, Teppei Okumura, Kazuyuki Akitsu
Summary: The study considers the benefits of measuring cosmic statistical anisotropy using redshift-space correlators without adopting the plane-parallel (PP) approximation. By decomposing correlators using the general tripolar spherical harmonic (TripoSH) basis, the study achieves superior detectability of anisotropic signatures.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Goran Jelic-Cizmek, Francesca Lepori, Camille Bonvin, Ruth Durrer
Summary: The study emphasizes the importance of including gravitational lensing in spectroscopic surveys for accurate galaxy number counts. Neglecting lensing can lead to significant shifts in cosmological parameters. The analysis also suggests potential improvements in spectroscopic survey analysis by incorporating cross-correlations between different redshift bins and utilizing complementary information from photometric surveys.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Maresuke Shiraishi, Teppei Okumura, Kazuyuki Akitsu
Summary: In this study, the galaxy intrinsic alignment is used to test the cosmic isotropy along with galaxy number density and peculiar velocity. The impacts of isotropy breaking on the configuration-space two-point correlation functions (2PCFs) are analyzed, and it is found that anisotropic distortions appear and have shapes determined by a preferred direction causing the isotropy violation. The study also suggests that the plane parallel (PP) approximation may not be valid in certain cases, and an accurate test for cosmic isotropy requires a formulation of 2PCF that does not rely on this approximation.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Roy Maartens, Sheean Jolicoeur, Obinna Umeh, Eline M. De Weerd, Chris Clarkson
Summary: Next-generation galaxy and 21cm intensity mapping surveys will rely on high-precision measurements of primordial non-Gaussianity using a combination of power spectrum and bispectrum. Theoretical precision at the same level is essential for these measurements. Incorporating a consistent general relativistic model of galaxy bias at second order extends the theoretical understanding of the galaxy bispectrum. The influence of primordial non-Gaussianity on the bispectrum goes beyond galaxy bias and dark matter density, and includes effects from redshift-space distortions.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
L. Raul Abramo, Joao Vitor Dinarte Ferri, Ian Lucas Tashiro
Summary: The general expressions for the multi-tracer Fisher matrix are derived, assuming that the cross-spectra are constrained by the auto-spectra and allowing for independent degrees of freedom in the cross-spectra. It is shown that the independent degrees of freedom of the cross-spectra are not constrained by cosmic variance, similar to the ratios of power spectra. Moreover, the uncertainties in the independent degrees of freedom of the cross-spectra decrease even faster than the uncertainties in the ratios of power spectra with increasing number density of the tracers. Simple expressions for the optimal number of tracers in a survey are also derived.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
William L. Matthewson, Ruth Durrer
Summary: This paper investigates how small-scale effects influence the angular-redshift power spectrum. It is found that spectroscopic surveys with high redshift resolution are already affected by small-scale features on large angular scales, particularly at low multipoles. Therefore, it is important to consider the non-linearities on small scales when studying the angular power spectrum with spectroscopic redshift resolution, even at low multipoles. The use of the correlation function in relatively wide redshift bins, which is not affected by large-scale non-linearities, may be preferred over the angular power spectrum. The extent to which small-scale effects become visible on large scales is quantified in detail, with a focus on bin auto-correlations.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Emanuele Castorina, Enea Di Dio
Summary: Measurements of galaxy clustering in Fourier space provide insights into the early Universe and the effects of Primordial Non Gaussianities. Relativistic effects can complicate the interpretation of data and may diverge in the Infra-Red. This work calculates the ensemble average of a commonly used Fourier space estimator, considering all general relativistic effects. The study finds that once the individual divergent GR terms are taken into account, there is no Infra-Red sensitivity in the observable. Additionally, the importance of GR effects, including lensing magnification, in interpreting the galaxy power spectrum multipoles is investigated, revealing them to be generally small corrections to the leading redshift space distortions term.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Joseph DeRose, Shi-Fan Chen, Nickolas Kokron, Martin White
Summary: Numerical simulations in cosmology require trade-offs between volume, resolution, and run-time, leading to sample variance in predictions of ensemble-average quantities. We extend the technique of Zel'dovich control variates to reduce the sample variance in measurements of 2-point statistics of biased tracers in redshift space. This allows improved predictions for the clustering of astronomical objects at very modest computational expense.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Florian Beutler, Patrick McDonald
Summary: Recent developments in galaxy redshift surveys have led to the proposal of a matrix-based analysis framework for galaxy power spectrum multipoles, providing deconvolved power spectrum results for several datasets. The use of deconvolved power spectrum multipoles allows for a data analysis independent of survey-specific aspects, such as the window function. This alternative analysis method has been shown to yield similar results to standard analysis in the case of the BOSS dataset, with various analysis components and a Python toolbox provided for convenience.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
L. Raul Abramo, Joao Vitor Dinarte Ferri, Ian Lucas Tashiro, Arthur Loureiro
Summary: This paper presents a method to predict the constraining power of galaxy surveys using the multi-tracer Fisher matrix based on angular power spectra in the linear regime of structure formation, avoiding the impracticality of deriving the Fisher matrix from numerically evaluated covariance matrices.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2022)
Article
Astronomy & Astrophysics
Byeonghee Yu, Uros Seljak, Yin Li, Sukhdeep Singh
Summary: We present growth of structure constraints from the cosmological analysis of the power spectrum multipoles of SDSS-III BOSS DR12 galaxies. We use a galaxy power spectrum model that decomposes galaxies into halo mass bins and combines perturbation theory and halo model to model halo clustering. By constraining a single parameter f sigma 8 to Planck+BAO prior, we reduce the effects of prior volume and mismodeling. Our analysis yields tight constraints on f sigma 8 and discusses the sensitivity of cosmological parameter estimation to various factors.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2023)
Article
Astronomy & Astrophysics
Biswajit Pandey, Suman Sarkar
Summary: The study investigates the issue of cosmic homogeneity in galaxies from the SDSS using Renyi entropy and divergence. It finds that the scale of homogeneity is underestimated in smaller samples, but can be improved with the use of independent voxels and larger samples. The analysis concludes that the galaxy distribution in the SDSS becomes homogeneous on a length scale beyond 140 h(-1) Mpc.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)
Article
Astronomy & Astrophysics
Lawrence Dam, Krzysztof Bolejko, Geraint F. Lewis
Summary: This paper explores the effect of redshift-space distortions (RSD) on the apparent peculiar motions of tracers, focusing on the estimation of the velocity power spectrum. The study shows that RSD introduces a dissipative correction leading to damping on relatively large, quasilinear scales. The research provides essential modeling ingredients for density-velocity multi-tracer analysis proposed for upcoming redshift surveys.
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
(2021)