Standard

Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys. / Nabokov, N.V.; Baryshev, Yu. V.

In: Astrophysics, Vol. 53, No. 1, 2010, p. 101 - 111.

Research output: Contribution to journal › Article › peer-review

Harvard

Nabokov, NV & Baryshev, YV 2010, 'Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys', Astrophysics, vol. 53, no. 1, pp. 101 - 111. https://doi.org/10.1007/s10511-010-9103-3

APA

Nabokov, N. V., & Baryshev, Y. V. (2010). Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys. Astrophysics, 53(1), 101 - 111. https://doi.org/10.1007/s10511-010-9103-3

Vancouver

Nabokov NV, Baryshev YV. Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys. Astrophysics. 2010;53(1):101 - 111. https://doi.org/10.1007/s10511-010-9103-3

Author

Nabokov, N.V. ; Baryshev, Yu. V. / Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys. In: Astrophysics. 2010 ; Vol. 53, No. 1. pp. 101 - 111.

BibTeX

@article{7a43fd5e7b704168ac8e346794da99e6,
title = "Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys",
abstract = "Using the deep fields of COSMOS, FDF, HUDF, and HDF-N as an example, we discuss the prospects for and limitations on the method for searching for superlarge structures in the spatial distribution of galaxies proposed in the preceding article of this series. An analysis of the distribution N(z) of photometric redshifts in a grid of the deep fields of HUDF-FDF-COSMOS-HDFN reveals the possible existence of superlarge structures with a contrast dN/N˜50% and tangential and radial dimensions of about 1000 Mpc. The reality of the detected candidate superlarge structures in the universe can be verified by further observations with a finer grid of deep fields. The influence of systematic errors can be reduced by observing the same deep fields with several 3-10 meter telescopes and utilizing different methods for determining the photometric redshifts.",
keywords = "cosmology, deep fields, distant galaxies, large scale structure of the universe",
author = "N.V. Nabokov and Baryshev, {Yu. V.}",
year = "2010",
doi = "10.1007/s10511-010-9103-3",
language = "English",
volume = "53",
pages = "101 -- 111",
journal = "Astrophysics",
issn = "0571-7256",
publisher = "Wolters Kluwer",
number = "1",

}

RIS

TY - JOUR

T1 - Method for analyzing the spatial distribution of galaxies on gigaparsec scales. II. Application to a grid of the HUDF-FDF-COSMOS-HDF surveys

AU - Nabokov, N.V.

AU - Baryshev, Yu. V.

PY - 2010

Y1 - 2010

N2 - Using the deep fields of COSMOS, FDF, HUDF, and HDF-N as an example, we discuss the prospects for and limitations on the method for searching for superlarge structures in the spatial distribution of galaxies proposed in the preceding article of this series. An analysis of the distribution N(z) of photometric redshifts in a grid of the deep fields of HUDF-FDF-COSMOS-HDFN reveals the possible existence of superlarge structures with a contrast dN/N˜50% and tangential and radial dimensions of about 1000 Mpc. The reality of the detected candidate superlarge structures in the universe can be verified by further observations with a finer grid of deep fields. The influence of systematic errors can be reduced by observing the same deep fields with several 3-10 meter telescopes and utilizing different methods for determining the photometric redshifts.

AB - Using the deep fields of COSMOS, FDF, HUDF, and HDF-N as an example, we discuss the prospects for and limitations on the method for searching for superlarge structures in the spatial distribution of galaxies proposed in the preceding article of this series. An analysis of the distribution N(z) of photometric redshifts in a grid of the deep fields of HUDF-FDF-COSMOS-HDFN reveals the possible existence of superlarge structures with a contrast dN/N˜50% and tangential and radial dimensions of about 1000 Mpc. The reality of the detected candidate superlarge structures in the universe can be verified by further observations with a finer grid of deep fields. The influence of systematic errors can be reduced by observing the same deep fields with several 3-10 meter telescopes and utilizing different methods for determining the photometric redshifts.

KW - cosmology

KW - deep fields

KW - distant galaxies

KW - large scale structure of the universe

U2 - 10.1007/s10511-010-9103-3

DO - 10.1007/s10511-010-9103-3

M3 - Article

VL - 53

SP - 101

EP - 111

JO - Astrophysics

JF - Astrophysics

SN - 0571-7256

IS - 1

ER -

ID: 5377933