AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis

@inproceedings{Ingoglia2022AMICOGC,
  title={AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis},
  author={Lorenzo Ingoglia and G. Covone and Mauro Sereno and Carlo Giocoli and Sandro Bardelli and Fabio Bellagamba and Gianluca Castignani and Samuel Farrens and Hendrik Hildebrandt and Shahab Joudaki and Eric Jullo and Denise Lanzieri and Giorgio F. Lesci and Federico Marulli and Matteo Maturi and Lauro Moscardini and Lorenza Nanni and Emanuela Puddu and Mario Radovich and Mauro Roncarelli and Feliciana Sapio and Carlo Schimd},
  year={2022}
}
Galaxy clusters are biased tracers of the underlying matter density field. At very large radii beyond about 10 Mpc/h, the shear profile shows evidence of a second-halo term. This is related to the correlated matter distribution around galaxy clusters and proportional to the so-called halo bias. We present an observational analysis of the halo bias-mass relation based on the AMICO galaxy cluster catalog, comprising around 7000 candidates detected in the third release of the KiDS survey.We split… 

Halo Properties and Mass Functions of Groups/Clusters from the DESI Legacy Imaging Surveys DR9

Based on a large group/cluster catalog recently constructed from the DESI Legacy Imaging Surveys DR9 using an extended halo-based group finder, we measure and model the group–galaxy weak-lensing

References

SHOWING 1-9 OF 9 REFERENCES

Large-scale structure in the Universe

A variety of observations constrain models of the origin of large-scale cosmic structures. Enough observational data have accumulated to constrain (and perhaps determine) the power spectrum of

Principles Of Physical Cosmology

TLDR
The principles of physical cosmology is universally compatible with any devices to read and is available in the book collection an online access to it is set as public so you can download it instantly.

THE MESSENGER

Recently NAFU SA and other role players expressed some criticism about government programmes. The criticism was not so much about the objectives and content of these programmes, but rather about

Measurement Error Models

  • A. Kukush
  • Computer Science
    International Encyclopedia of Statistical Science
  • 2011

33rdAdvancedSaas FeeCourse onGravitational Lensing: Strong, Weak, and Micro: Les Diablerets

  • Switzerland, April 7-12,
  • 2003

AMICO galaxy clusters in KiDS-DR3: constraints on cosmological parameters and on the mass-richness relation from the clustering of galaxy clusters

  • prep
  • 1996

Analysis Software and Systems XIV

  • 2005

The data underlying this article will be shared on reasonable request to the corresponding author