Standard

Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields. / Shirokov, S.I.; Lovyagin, N.Y.; Baryshev, Y.V.; Gorokhov, V.L.

в: Astronomy Reports, Том 6, № 1, 2016, стр. 563-578.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Shirokov, SI, Lovyagin, NY, Baryshev, YV & Gorokhov, VL 2016, 'Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields', Astronomy Reports, Том. 6, № 1, стр. 563-578.

APA

Shirokov, S. I., Lovyagin, N. Y., Baryshev, Y. V., & Gorokhov, V. L. (2016). Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields. Astronomy Reports, 6(1), 563-578.

Vancouver

Shirokov SI, Lovyagin NY, Baryshev YV, Gorokhov VL. Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields. Astronomy Reports. 2016;6(1):563-578.

Author

Shirokov, S.I. ; Lovyagin, N.Y. ; Baryshev, Y.V. ; Gorokhov, V.L. / Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields. в: Astronomy Reports. 2016 ; Том 6, № 1. стр. 563-578.

BibTeX

@article{b8a17c40352e45f7951aa9f55b6b26d0,
title = "Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields",
abstract = "New arguments supporting the reality of large-scale fluctuations in the density of the visible matter in deep galaxy surveys are presented. A statistical analysis of the radial distributions of galaxies in the COSMOS and HDF-N deep fields is presented. Independent spectral and photometric surveys exist for each field, carried out in different wavelength ranges and using different observing methods. Catalogs of photometric redshifts in the optical (COSMOS-Zphot) and infrared (UltraVISTA) were used for the COSMOS field in the redshift interval 0.1 <z <3.5, as well as the zCOSMOS (10kZ) spectroscopic survey and the XMM-COSMOS and ALHAMBRA-F4 photometric redshift surveys. The HDFN-Zphot and ALHAMBRA-F5 catalogs of photometric redshifts were used for the HDF-N field. The Pearson correlation coefficient for the fluctuations in the numbers of galaxies obtained for independent surveys of the same deep field reaches R = 0.70 ± 0.16. The presence of this positive correlation supports the reality of fluctuations in th",
author = "S.I. Shirokov and N.Y. Lovyagin and Y.V. Baryshev and V.L. Gorokhov",
year = "2016",
language = "не определен",
volume = "6",
pages = "563--578",
journal = "Astronomy Reports",
issn = "1063-7729",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "1",

}

RIS

TY - JOUR

T1 - Large-scale fluctuations in the number density of galaxies in independent surveys of deep fields

AU - Shirokov, S.I.

AU - Lovyagin, N.Y.

AU - Baryshev, Y.V.

AU - Gorokhov, V.L.

PY - 2016

Y1 - 2016

N2 - New arguments supporting the reality of large-scale fluctuations in the density of the visible matter in deep galaxy surveys are presented. A statistical analysis of the radial distributions of galaxies in the COSMOS and HDF-N deep fields is presented. Independent spectral and photometric surveys exist for each field, carried out in different wavelength ranges and using different observing methods. Catalogs of photometric redshifts in the optical (COSMOS-Zphot) and infrared (UltraVISTA) were used for the COSMOS field in the redshift interval 0.1 <z <3.5, as well as the zCOSMOS (10kZ) spectroscopic survey and the XMM-COSMOS and ALHAMBRA-F4 photometric redshift surveys. The HDFN-Zphot and ALHAMBRA-F5 catalogs of photometric redshifts were used for the HDF-N field. The Pearson correlation coefficient for the fluctuations in the numbers of galaxies obtained for independent surveys of the same deep field reaches R = 0.70 ± 0.16. The presence of this positive correlation supports the reality of fluctuations in th

AB - New arguments supporting the reality of large-scale fluctuations in the density of the visible matter in deep galaxy surveys are presented. A statistical analysis of the radial distributions of galaxies in the COSMOS and HDF-N deep fields is presented. Independent spectral and photometric surveys exist for each field, carried out in different wavelength ranges and using different observing methods. Catalogs of photometric redshifts in the optical (COSMOS-Zphot) and infrared (UltraVISTA) were used for the COSMOS field in the redshift interval 0.1 <z <3.5, as well as the zCOSMOS (10kZ) spectroscopic survey and the XMM-COSMOS and ALHAMBRA-F4 photometric redshift surveys. The HDFN-Zphot and ALHAMBRA-F5 catalogs of photometric redshifts were used for the HDF-N field. The Pearson correlation coefficient for the fluctuations in the numbers of galaxies obtained for independent surveys of the same deep field reaches R = 0.70 ± 0.16. The presence of this positive correlation supports the reality of fluctuations in th

M3 - статья

VL - 6

SP - 563

EP - 578

JO - Astronomy Reports

JF - Astronomy Reports

SN - 1063-7729

IS - 1

ER -

ID: 7585238