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The XXL Survey. VII. A supercluster of galaxies at z = 0.43
Astronomy and Astrophysics, 592 (2016); A6. https://doi.org/10.1051/0004-6361/201527142
Pompei, E.; Adami, C.; Eckert, D.; Gastaldello, F.; Lavoie, S.; Poggianti, B.; Altieri, B.; Alis, S.; Baran, Nikola; Benoist, C.; Jaffé, Y. L.; Koulouridis, E.; Maurogordato, S.; Pacaud, F.; Pierre, M.; Sadibekova, T.; Smolčić, Vernesa; Valtchanov, I. Više autora...

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Pompei, E., Adami, C., Eckert, D., Gastaldello, F., Lavoie, S., Poggianti, B. ... Valtchanov, I. (2016). The XXL Survey. VII. A supercluster of galaxies at z = 0.43. Astronomy and Astrophysics, 592.. doi: 10.1051/0004-6361/201527142

Pompei, E., et al. "The XXL Survey. VII. A supercluster of galaxies at z = 0.43." Astronomy and Astrophysics, vol. 592, 2016. https://doi.org/10.1051/0004-6361/201527142

Pompei, E., C. Adami, D. Eckert, F. Gastaldello, S. Lavoie, B. Poggianti, B. Altieri, et al. "The XXL Survey. VII. A supercluster of galaxies at z = 0.43." Astronomy and Astrophysics 592 (2016). https://doi.org/10.1051/0004-6361/201527142

Pompei, E., et al. (2016) 'The XXL Survey. VII. A supercluster of galaxies at z = 0.43', Astronomy and Astrophysics, 592. doi: 10.1051/0004-6361/201527142

Pompei E, Adami C, Eckert D, Gastaldello F, Lavoie S, Poggianti B, i sur.. The XXL Survey. VII. A supercluster of galaxies at z = 0.43. Astronomy and Astrophysics [Internet]. 2016. [pristupljeno 27.12.2024.];592. doi: 10.1051/0004-6361/201527142

E. Pompei, et al., "The XXL Survey. VII. A supercluster of galaxies at z = 0.43", Astronomy and Astrophysics, vol. 592, 2016. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:205002. [Citirano: 27.12.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:205002
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Naslov (engleski)The XXL Survey. VII. A supercluster of galaxies at z = 0.43
AutorE. Pompei
AutorC. Adami
AutorD. Eckert
AutorF. Gastaldello
AutorS. Lavoie
AutorB. Poggianti
AutorB. Altieri
AutorS. Alis
AutorNikola Baran
AutorC. Benoist
AutorY. L. Jaffé
AutorE. Koulouridis
AutorS. Maurogordato
AutorF. Pacaud
AutorM. Pierre
AutorT. Sadibekova
AutorVernesa Smolčić
MBZ: 336180
AutorI. Valtchanov
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
The XXL Survey is the largest homogeneous and contiguous survey carried out with XMM-Newton. Covering an area of 50 deg2 distributed over two fields, it primarily investigates the large-scale structures of the Universe using the distribution of galaxy clusters and active galactic nuclei as tracers of the matter distribution. Given its depth and sky coverage, XXL is particularly suited to systematically unveiling the clustering of X-ray clusters and to identifying superstructures in a homogeneous X- ray sample down to the typical mass scale of a local massive cluster. A friends-of-friends algorithm in three-dimensional physical space was run to identify large-scale structures. In this paper we report the discovery of the highest redshift supercluster of galaxies found in the XXL Survey. We describe the X-ray properties of the clusters members of the structure and the optical follow- up. The newly discovered supercluster is composed of six clusters of galaxies at a median redshift z ~ 0.43 and distributed across ~30′× 15′ (10 × 5 Mpc) on the sky. This structure is very compact with all the clusters residing in one XMM pointing ; for this reason this is the first supercluster discovered with the XXL Survey. Photometric redshifts from the CFHTLS (Canada-France-Hawaii Telescope Legacy Survey) data release T0007 placed the supercluster at an approximate redshift of zphot ~ 0.45 ; subsequent spectroscopic follow-up with WHT (William Herschel Telescope) and NTT (New Technology Telescope) confirmed a median redshift of z ~ 0.43. An estimate of the X-ray mass and luminosity of this supercluster returns values of 1.7 × 1015 M⊙ and of 1.68 × 1044 erg s-1, respectively, and a total gas mass of Mgas = 9.3 × 1013 M⊙. These values put XLSSC-e at the average mass range of superclusters ; its appearance, with two members of equal size, is quite unusual with respect to other superclusters and provides a unique view of the formation process of a massive structure.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaAstronomy and Astrophysics
Brojčani podacivol. 592, A6
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201527142
URN:NBNurn:nbn:hr:217:205002
Datum objave publikacije2016
URL dokumentahttps://www.aanda.org/articles/aa/abs/2016/08/aa27142-15/aa27142-15.html
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© ESO 2016. Received 7 August 2015. Accepted 27 October 2015. Published online 15 June 2016.
RepozitorijRepozitorij Prirodoslovno-matematičkog fakulteta
Datum i vrijeme pohrane2020-02-23 18:35:50