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Found 7 papers, 3 papers with code
Probabilistic Mass Mapping with Neural Score Estimation
We introduce a novel methodology allowing for efficient sampling of the high-dimensional Bayesian posterior of the weak lensing mass-mapping problem, and relying on simulations for defining a fully non-Gaussian prior.
Angular clustering and host halo properties of [OII] emitters at $z >1$ in the Subaru HSC survey
From the constrained HOD model, the average mass of halos hosting the [OII] emitters is derived to be $\log{M_{eff}/(h^{-1}M_\odot)}=12. 70^{+0. 09}_{-0. 07}$ and $12. 61^{+0. 09}_{-0. 05}$ at z=1. 19 and 1. 47, respectively, which will become halos with the present-day mass, $M\sim 1. 5 \times 10^{13}h^{-1}M_\odot$.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
$κ$TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
The $\kappa$TNG suite includes 10, 000 realisations of $5 \times 5 \, \mathrm{deg}^2$ maps for 40 source redshifts up to $z_s = 2. 6$, well covering the range of interest for existing and upcoming weak lensing surveys.
Cosmology and Nongalactic Astrophysics
Super-sample covariance of the thermal Sunyaev-Zel'dovich effect
First, we study the impact of super sample covariance (SSC) on the tSZ power spectrum measurements, and find that the sample variance is dominated by the connected non-Gaussian (cNG) covariance arising mainly from Poisson number fluctuations of massive clusters in the survey volume.
Cosmology and Nongalactic Astrophysics
Power Spectrum of Intrinsic Alignments of Galaxies in IllustrisTNG
The shape of massive disk- and spheroid-galaxies tend to align with the tidal field.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
Perturbation theory challenge for cosmological parameters estimation - I. Matter power spectrum in real space
We study the accuracy with which cosmological parameters can be determined from real space power spectrum of matter density contrast at weakly nonlinear scales using analytical approaches.
Cosmology and Nongalactic Astrophysics
Full-sky Gravitational Lensing Simulation for Large-area Galaxy Surveys and Cosmic Microwave Background Experiments
The data sets include full-sky convergence and shear maps from redshifts $z=0. 05$ to $5. 3$ at intervals of $150 \, h^{-1}{\rm Mpc}$ comoving radial distance (corresponding to a redshift interval of $\Delta z \simeq 0. 05$ at the nearby universe), enabling the construction of a mock shear catalog for an arbitrary source distribution up to $z=5. 3$.
Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
