Results 1 to 10 of about 166,709,059 (292)
Observed Evidence for the Primordial Origin of Galaxy Sizes
We present observational evidence supporting the scenario that the protogalactic angular momenta play an important role in molding the optical sizes of present galaxies. Analyzing the NASA-Sloan Atlas catalog in the redshift range of 0.02 ≤ z
Jun-Sung Moon, Jounghun Lee
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Large-scale structure (LSS) analysis in galaxy surveys is a powerful cosmological probe but is limited by tracer bias, which can obscure underlying information and weaken parameter constraints.
Zhujun Jiang +8 more
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Density-shear Baryon Acoustic Oscillation as a Cosmological Consistency Check
Tensions often arise between different data sets in cosmology, and consistency tests can serve as a powerful tool for diagnosing potential issues. Density-shear baryon acoustic oscillation (GI BAO) is the imprint of the BAO feature on the shear field ...
Kwan Chuen Chan +2 more
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Cross Correlation between the Thermal Sunyaev–Zeldovich Effect and the Integrated Sachs–Wolfe Effect
We present a joint cosmological analysis of the power spectra measurement of the Planck Compton parameter and the integrated Sachs–Wolfe (ISW) maps. We detect the statistical correlation between the Planck thermal Sunyaev–Zeldovich (tSZ) map and ISW data
Ayodeji Ibitoye +7 more
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From redshift to real space: Combining linear theory with neural networks
Context. Spectroscopic redshift surveys are key to tracing the large-scale structure (LSS) of the Universe and testing the Λ Cold Dark Matter model. However, redshifts as distance proxies introduce distortions in the 3D galaxy distribution.
Maragliano Edoardo +3 more
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We analyzed the distribution of spin parity in spiral galaxies using the HSC DR2 data. The spiral winding parity of disk galaxies, observed as S-spiral or Z-spiral projected onto the sky plane, provides robust information on the sign of the line-of-sight
Masanori Iye, Masafumi Yagi
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The DESI DR1 peculiar velocity survey: Growth rate measurements from the galaxy power spectrum
The large-scale structure of the Universe and its evolution encapsulate a wealth of cosmological information. A powerful means of unlocking this knowledge lies in measuring the auto-power spectrum and/or the cross-power spectrum of the galaxy density and
Qin F. +65 more
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Evolution of Cosmic Voids: Structure, Galaxies, and Dynamics
We investigate the structural, photometric, and dynamical evolution of cosmic voids and their galaxy populations from z = 2.09 to the present, focusing on void size as a key evolutionary parameter.
Saeed Tavasoli
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Assembly bias from nuisance to probe
Context. Two-halo galactic conformity is commonly interpreted as a manifestation of galaxy assembly bias, but its statistical structure and physical origin remain unclear. Aims.
Padilla Nelson, Lacerna Ivan, Paz Dante
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The large scale structure of the universe
Abstract Observational data on galaxies and clusters of galaxies are reviewed in the context of how they relate to the large scale structure of the Universe. Various methods of interpreting these data are discussed.
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