Диссертация (1149494), страница 12
Текст из файла (страница 12)
// Перевод сангл. – М: «Мир», 1983.[9] Райков А.А., Орлов В.В., и Бекетов О.Б. О неоднородностях в пространственном распределении гамма-всплесков. // Астрофизика. – 2010. – Т. 53.– C.441.[10] Райков А.А., Орлов В.В., and Герасим Р.В. Определение фрактальной размерности крупномасштабной структуры по сверхновым типа Ia методомпопарных расстояний. // Астрофизика.
– 2014. – Т. 57. – C.309.[11] Решетников В.П. Обзоры неба и глубокие поля наземных и космическихтелескопов. // УФН. – 2005. – Т. 175. – C.1163.84[12] Теханович Д.И., Барышев Ю.В. Глобальная структура Локальной Вселенной согласно обзору 2MRS. // АБ САО РАН. – 2016. – Т. 71. – C.167.[13] Широков С.И., Барышев Ю.В., Теханович Д.И. Флуктуации пространственного распределения галактик в глубоком поле COSMOS на масштабахв гигапарсеки. // Вестник СПбГУ. – 2014. – Т. 59. – C.659.[14] Широков С.И., Ловягин Н.Ю., Барышев Ю.В., Горохов В.Л. Крупномасштабные флуктуации плотности галактик в независимых обзорах глубокихполей. // Астрон.Ж.
– 2016. – Т. 93. – C.546.[15] Широков С.И., Райков А.А., Барышев Ю.В. Свойства пространственного распределения источников гамма-всплесков. // Астрофизика. – 2017. –Т. 60. – C.527.[16] Balázs L.G., Bagoly Z., Hakkila J.E., Horváth I., Kóbori J., Rácz I.I., TóthL.V. A giant ring-like structure at 0.78 < z < 0.86 displayed by GRBs. //Mon.Not.Roy.Astron.Soc. – 2015.
– V. 452. – P.2236.[17] Baryshev Yu.V. and Teerikorpi P. Fundamental questions of practicalcosmology. // Springer Science, Dordrecht, Astrophysics and Space ScienceLibrary, V. 383, 2012. – 332 p.[18] Bhowmick A.K., Matteo T.Di, Feng Y., Lanusse F. The clustering ofz>7 galaxies: Predictions from the BLUETIDES simulation. //Mon.Not.Roy.Astron.Soc. – 2018. – V. 474.
– I. 4. P.5393.[19] Brusa M., et al. The XMM-Newton Wide-Field Survey in the COSMOS field(XMM-COSMOS): demography and multiwavelength properties of obscuredand unobscured luminous AGN. // Astrophys.J. – 2010. – V. 716. – P.348.[20] Chiang Yi-Kuan, et al. Discovery of a Large Number of CandidateProtoclusters Traced by ∼ 15 Mpc-scale Galaxy Overdensities in COSMOS.// Astrophys.J.Lett.
– 2014. – V. 782. – L3.[21] Clowes R.G., Harris K.A., Raghunathan Sr., Campusano L. E., Söchting I. K.,Graham M. J. Two close large quasar groups of size ∼ 350 Mpc at z ∼ 1.2. //Mon.Not.Roy.Astron.Soc. – 2012. – V. 419. – P.556.85[22] Clowes R.G., Harris K.A., Raghunathan Sr., Campusano L. E., SöchtingI. K., Graham M. J. A structure in the early Universe at z ∼ 1.3that exceeds the homogeneity scale of the R-W concordance cosmology. //Mon.Not.Roy.Astron.Soc. – 2013.
– V. 429. – P.2910.[23] Einasto M., Tago E., Lietzen H. Tracing a high redshift cosmic web with quasarsystems. // Astron.Astrophys. – 2014. – V. 568. – A46.[24] Einasto M., et al. Sloan Great Wall as a complex of superclusters with collapsingcores. // Astron.Astrophys. – 2016.
– V. 595. – A70.[25] Gabrielli A., Sylos Labini F., Joice M., Pietronero L. Statistical physics forcosmic structures. // Springer, Berlin, 2005. – 424 p.[26] Gnedin Yu.N., Mikhailov A.G., Piotrovich M.Yu. The most distant quasar atz = 7.08: Probable retrograde rotation of an accreting supermassive black hole.// Astron.Nachr. – 2015. – V. 336. – I. 3. – P.312.[27] Gott III J.R., Juric M., and Schlegel D. A Map of the Universe. // Astrophys.J.– 2005. – V. 624.
– P.463.[28] Grassberger P., Procaccia I. Characterization of strange attractors. //Phys.Rev.Lett. – 1983. – V. 50. – P.346.[29] Grassberger P., Procaccia I. Measuring the strangeness of strange attractors.// Physica D: Nonlinear Phenom. – 1983. – V. 9. – P.189.[30] Guzzo L., Massey R., et al. The Cosmic Evolution Survey (COSMOS): A LargeScale Structure at z=0.73 and the Relation of Galaxy Morphologies to LocalEnvironment. // Astrophys.J.Suppl.Ser.
– 2007. – V. 172. – P.254.[31] Ilbert O., Capak P., et al. COSMOS photometric redshifts with 30-bands for2-deg2 . // Astrophys.J. – 2009. – V. 690. – P.1236.[32] Ryabinkov A.I., Kaurov A.A., Kaminker A.D. Quasi-periodical features in thedistribution of Luminous Red Galaxies // Astrophys.Space Sci. – 2013 – V. 344.– I. 1.
– P.219.86[33] Kendall M.G. and Moran P.A.P. Geometrical Probability. // Griffin, London,1963.[34] Kocevski D. and Petrosian V. On the Lack of Time Dilation Signatures inGamma-Ray Burst Light Curves. // Astrophys.J. – 2013. – V. 765. – P.116.[35] Komberg B.V., Kravtsov A.V., Lukash V.N. The search for and investigationof large quasar groups. // Mon.Not.Roy.Astron.Soc. – 1996. – V. 282. – P.713.[36] Koprowski M., et al.
A reassessment of the redshift distribution and physicalproperties of luminous (sub-)millimetre galaxies. // Mon.Not.Roy.Astron.Soc.– 2014. – V. 444. – I.1. – P.117.[37] Kovac K., et al. The Density Field of the 10k zCOSMOS Galaxies. //Astrophys.J. – 2010. – V. 708. – P.505.[38] Kroupa P., et al. The Failures of the Standard Model of Cosmology Require aNew Paradigm.
// Int.J.Mod.Phys.D. – 2012. – V. 21. – I. 14. – 1230003.[39] Li Ming-Hua and Lin Hai-Nan. Testing the homogeneity of the Universe usinggamma-ray bursts. // Astron.Astrophys. – 2015. – V. 582. – A111.[40] Lietzen H., Tempel E., Liivamägi L.J., et al. Discovery of a massive superclustersystem at z ∼ 0.47. // Astron.Astrophys. – 2016.
– V. 588. – L4.[41] Liske J. On the cosmological distance and redshift between any two objects. //Mon.Not.Roy.Astron.Soc. – 2000. – V. 319. – P.557.[42] Mainieri V., et al. Black hole accretion and host galaxies of obscured quasarsin XMM-COSMOS. // Astron.Astrophys. – 2011. – V. 535 – A80.[43] Makarov D., Karachentsev I. Galaxy groups and clouds in the Local (z ∼ 0.01)universe // Mon.Not.Roy.Astron.Soc.
– 2011. – V. 412. – I. 4. – P.2498.[44] Massey R., Rhodes J., Ellis R., et al. Dark matter maps reveal cosmicscaffolding. // Nature. – 2007. – V. 445. – P.286.[45] Massey R., Rhodes J., Leauthaud A., et al. COSMOS: Three-dimensional WeakLensing and the Growth of Structure. // Astrophys.J. – 2007. – V. 172. – P.239.87[46] Meneux B., et al. The zCOSMOS survey. The dependence of clustering onluminosity and stellar mass at z = 0.2 − 1.
// Astron.Astrophys. – 2009. –V. 505. – P.463.[47] Molino A., et al. The ALHAMBRA Survey: Bayesian photometric redshifts with23 bands for 3 deg2 . // Mon.Not.Roy.Astron.Soc. – 2014. – V. 441. – I. 4. –P.2891.[48] Moster B., et al. A Cosmic Variance Cookbook. // Astrophys.J. – 2011. – V. 731.– P.113.[49] Muzzin A., at al. A public KS -selected catalog in the COSMOS / ULTRAVISTAfield: photometry, photometric redshifts and stellar population parameters. //Astrophys.J.Suppl.Ser.
– 2013. – V. 206. – N 1.[50] Park Changbom, Choi Yun-Young, Kim Juhan, Gott J. Richard III, KimSungsoo S., Kim Kap-Sung. The Challenge of the Largest Structures in theUniverse to Cosmology. // Astrophys.J.Lett. – 2012. – V. 759. – N 1.[51] Park Chan-Gyung, Hyun Hwasu, Noh Hyerim, Hwang Jai-chan. Thecosmological principle is not in the sky. // Mon.Not.Roy.Astron.Soc. – 2017.– V.
469. – P.1924.[52] Peebles P.J.E. Principles of Physical Cosmology. // Princeton Univ.Press, 1993.[53] Percival W.J., Robert N.C., Eisenstein D.J., et al. The Shape of the SloanDigital Sky Survey Data Release 5 Galaxy Power Spectrum. // Astrophys.J. –2006. – V. 657. – P.645.[54] Raikov A.A. and Orlov V.V. Method of pairwise separations and itsastronomical applications. // Mon.Not.Roy.Astron.Soc. – 2011. – V. 418. –P.2558.[55] Sokolov I.V., Castro-Tirado A.J., Verkhodanov O.V., Zhelenkova O.P.,Baryshev Yu.V. Clustering of galaxies around the GRB 021004 sight-line atz ∼ 0.5.
// Proceedings of the International Workshop on Quark PhaseTransition in Compact Objects and Multimessenger Astronomy: Neutrino88Signals, Supernovae and Gamma-Ray Bursts, KChR, Nizhnij Arkhyz (SAO),KBR, Terskol (BNO). – 2016. – P.111.[56] Sokolov V.V., et al. The core collapse supernovae, gamma-ray bursts and SN1987A. // in Proceedings of The International Conference “SN 1987A, QuarkPhase Transition in Compact Objects and Multimessenger Astronomy”, Russia,Terskol (BNO INR RAS), Nizhnij Arkhyz (SAO RAS), 2-8 July 2017. – 2018.https://www.sao.ru/hq/grb/conf_2017/program.html.[57] Somerville R., et al. Cosmic Variance in the Great Observatories Origins DeepSurvey.
// Astrophys.J. – 2004. – V. 600. – L171.[58] Sylos Labini F., Montuori M., Pietronero L. Scale-invariance of galaxyclustering. // Phys.Rept. – 1998. – V. 293 – P.61.[59] Sylos Labini F., Vasilyev N.L. Extension and estimation of correlations in colddark matter models. // Astron.Astrophys. – 2008.
– V. 477. – P.381.[60] Sylos Labini F., Baryshev Yu.V. Testing the Copernican and CosmologicalPrinciplesinthelocaluniversewithgalaxysurveys.//J.Cosmol.Astropart.Phys. – 2010. – I. 06. – id.021.[61] Sylos Labini F. Inhomogeneities in the universe. // Class.Quant.Grav. – 2011.– V. 28. – I. 16. – 164003.[62] Tasitsiomi A. The State of the Cold Dark Matter Models on Galactic andSubgalactic Scales. // Int.J.Mod.Phys.D. – 2003.