The density field of the 10k zCOSMOS galaxies
K. Kovac, S. J. Lilly, O. Cucciati, C. Porciani, A. Iovino, G., Zamorani, P. Oesch, M. Bolzonella, C. Knobel, A. Finoguenov, Y. Peng, C. M., Carollo, L. Pozzetti, K. Caputi, J. D. Silverman, L. Tasca, M. Scodeggio, D., Vergani, E. Zucca, T. Contini, J.-P. Kneib, O. Le Fevre

TL;DR
This paper constructs high-resolution three-dimensional density maps of galaxies up to redshift 1 using spectroscopic data and innovative algorithms, revealing large-scale structures consistent with mock catalogues.
Contribution
It introduces the ZADE algorithm to incorporate photometric redshifts into density field reconstruction, enhancing environment sampling and reducing noise.
Findings
Reconstructed large-scale galaxy structures up to z~1.
Good agreement between observed and mock catalogues.
Density maps correlate well with virialized groups and clusters.
Abstract
We use the current sample of ~10,000 zCOSMOS spectra of sources selected with I(AB) < 22.5 to define the density field out to z~1, with much greater resolution in the radial dimension than has been possible with either photometric redshifts or weak lensing. We apply new algorithms that we have developed (ZADE) to incorporate objects not yet observed spectroscopically by modifying their photometric redshift probability distributions using the spectroscopic redshifts of nearby galaxies. This strategy allows us to probe a broader range of galaxy environments and reduce the Poisson noise in the density field. The reconstructed overdensity field of the 10k zCOSMOS galaxies consists of cluster-like patterns surrounded by void-like regions, extending up to z~1. Some of these structures are very large, spanning the ~50 Mpc/h transverse direction of the COSMOS field and extending up to Delta…
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