Standard
Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5. / Sokolov, Ilya V.; Castro-Tirado, A.J.; Verkhodanov, O.V.; Zhelenkova, O.P.; Baryshev, Yu.V.
Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia,. 2016. стр. 111-120.
Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции
Harvard
Sokolov, IV, Castro-Tirado, AJ, Verkhodanov, OV, Zhelenkova, OP
& Baryshev, YV 2016,
Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5. в
Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia,. стр. 111-120. <
http://adsabs.harvard.edu/abs/2016qptc.conf..111S>
APA
Sokolov, I. V., Castro-Tirado, A. J., Verkhodanov, O. V., Zhelenkova, O. P.
, & Baryshev, Y. V. (2016).
Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5. в
Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia, (стр. 111-120)
http://adsabs.harvard.edu/abs/2016qptc.conf..111SVancouver
Sokolov IV, Castro-Tirado AJ, Verkhodanov OV, Zhelenkova OP
, Baryshev YV.
Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5. в Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia,. 2016. стр. 111-120
Author
Sokolov, Ilya V. ; Castro-Tirado, A.J. ; Verkhodanov, O.V. ; Zhelenkova, O.P.
; Baryshev, Yu.V. /
Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5. Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia,. 2016. стр. 111-120
BibTeX
@inproceedings{d41b0db1e13c4ec2815f888d75d93a12,
title = "Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5",
abstract = "In this report we test for reliability any signatures of field galaxies clustering in the GRB 021004 line of sight. The first signature is the BTA and Hubble GRB 021004 field photometric redshift distribution with a peak at z ~ 0.5 estimated from multicolor photometry. The second signature is the MgII 2796,2803 absorption doublet at z ~ 0.5 in the GRB 021004 afterglow spectrum. The third signature is some inhomogeneity in Plank + GRB 021004 fields. And the fourth signature may be the galaxy clustering with an effective redshift of z = 0.5 from the Baryon Oscillation Spectroscopic Survey (BOSS), which is a part of the Sloan Digital Sky Survey III (SDSS-III)",
keywords = "Galaxy Clustering, Gamma-Ray Bursts, Multicolor Photometry",
author = "Sokolov, {Ilya V.} and A.J. Castro-Tirado and O.V. Verkhodanov and O.P. Zhelenkova and Yu.V. Baryshev",
year = "2016",
language = "English",
pages = "111--120",
booktitle = "Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: {"}Sneg{"}, Pyatigorsk, Russia,",
}
RIS
TY - GEN
T1 - Clustering of galaxies around the GRB 021004 sight-line at z ~ 0.5
AU - Sokolov, Ilya V.
AU - Castro-Tirado, A.J.
AU - Verkhodanov, O.V.
AU - Zhelenkova, O.P.
AU - Baryshev, Yu.V.
PY - 2016
Y1 - 2016
N2 - In this report we test for reliability any signatures of field galaxies clustering in the GRB 021004 line of sight. The first signature is the BTA and Hubble GRB 021004 field photometric redshift distribution with a peak at z ~ 0.5 estimated from multicolor photometry. The second signature is the MgII 2796,2803 absorption doublet at z ~ 0.5 in the GRB 021004 afterglow spectrum. The third signature is some inhomogeneity in Plank + GRB 021004 fields. And the fourth signature may be the galaxy clustering with an effective redshift of z = 0.5 from the Baryon Oscillation Spectroscopic Survey (BOSS), which is a part of the Sloan Digital Sky Survey III (SDSS-III)
AB - In this report we test for reliability any signatures of field galaxies clustering in the GRB 021004 line of sight. The first signature is the BTA and Hubble GRB 021004 field photometric redshift distribution with a peak at z ~ 0.5 estimated from multicolor photometry. The second signature is the MgII 2796,2803 absorption doublet at z ~ 0.5 in the GRB 021004 afterglow spectrum. The third signature is some inhomogeneity in Plank + GRB 021004 fields. And the fourth signature may be the galaxy clustering with an effective redshift of z = 0.5 from the Baryon Oscillation Spectroscopic Survey (BOSS), which is a part of the Sloan Digital Sky Survey III (SDSS-III)
KW - Galaxy Clustering
KW - Gamma-Ray Bursts
KW - Multicolor Photometry
M3 - Conference contribution
SP - 111
EP - 120
BT - Quark Phase Transition in Compact Objects and Multimessenger Astronomy: Neutrino Signals, Supernovae and Gamma-Ray Bursts. Proceeings of the conference held 7-14 October, 2015 at the Special Astrophysical Observatory of Russian Academy of Sciences (SAO RAS) and Baksan Neutrino Observatory of Institute for Nuclear Research of Russian Academy of Sciences (BNO INR RAS). Edited by V.V. Sokolov et al. Publisher: "Sneg", Pyatigorsk, Russia,
ER -
