prikaz prve stranice dokumenta The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
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The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
Astronomy and Astrophysics, 620 (2018); A15. https://doi.org/10.1051/0004-6361/201732507
Guglielmo, V.; Poggianti, B. M.; Vulcani, B.; Moretti, A.; Fritz, J.; Gastaldello, F.; Adami, C.; Caretta, C. A.; Willis, J.; Koulouridis, E.; Ramos Ceja, M. E.; Giles, P.; Baldry, I.; Birkinshaw, M.; Bongiorno, A.; Brown, M.; Chiappetti, L.; Driver, S.; Elyiv, A.; Evrard, A.; Grootes, M.; Guennou, L.; Hopkins, A.; Horellou, C.; Iovino, A.; Maurogordato, S.; Owers, M.; Pacaud, F.; Paltani, S.; Pierre, M.; Plionis, M.; Ponman, T.; Robotham, A.; Sadibekova, T.; Smolčić, Vernesa; Tuffs, R.; Vignali, C Više autora...

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Guglielmo, V., Poggianti, B. M., Vulcani, B., Moretti, A., Fritz, J., Gastaldello, F. ... Vignali, C. (2018). The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations. Astronomy and Astrophysics, 620.. doi: 10.1051/0004-6361/201732507

Guglielmo, V., et al. "The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations." Astronomy and Astrophysics, vol. 620, 2018. https://doi.org/10.1051/0004-6361/201732507

Guglielmo, V., B. M. Poggianti, B. Vulcani, A. Moretti, J. Fritz, F. Gastaldello, C. Adami, et al. "The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations." Astronomy and Astrophysics 620 (2018). https://doi.org/10.1051/0004-6361/201732507

Guglielmo, V., et al. (2018) 'The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations', Astronomy and Astrophysics, 620. doi: 10.1051/0004-6361/201732507

Guglielmo V, Poggianti BM, Vulcani B, Moretti A, Fritz J, Gastaldello F, i sur.. The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations. Astronomy and Astrophysics [Internet]. 2018. [pristupljeno 19.03.2025.];620. doi: 10.1051/0004-6361/201732507

V. Guglielmo, et al., "The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations", Astronomy and Astrophysics, vol. 620, 2018. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:892772. [Citirano: 19.03.2025.]

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Naslov (engleski)The XXL Survey. XXX. Characterisation of the XLSSsC N01 supercluster and analysis of the galaxy stellar populations
AutorV. Guglielmo
AutorB. M. Poggianti
AutorB. Vulcani
AutorA. Moretti
AutorJ. Fritz
AutorF. Gastaldello
AutorC. Adami
AutorC. A. Caretta
AutorJ. Willis
AutorE. Koulouridis
AutorM. E. Ramos Ceja
AutorP. Giles
AutorI. Baldry
AutorM. Birkinshaw
AutorA. Bongiorno
AutorM. Brown
AutorL. Chiappetti
AutorS. Driver
AutorA. Elyiv
AutorA. Evrard
AutorM. Grootes
AutorL. Guennou
AutorA. Hopkins
AutorC. Horellou
AutorA. Iovino
AutorS. Maurogordato
AutorM. Owers
AutorF. Pacaud
AutorS. Paltani
AutorM. Pierre
AutorM. Plionis
AutorT. Ponman
AutorA. Robotham
AutorT. Sadibekova
AutorVernesa Smolčić
MBZ: 336180
AutorR. Tuffs
AutorC Vignali
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Astronomija i astrofizika
Sažetak (engleski)
Context. Superclusters form from the largest enhancements in the primordial density perturbation field and extend for tens of Mpc, tracing the large-scale structure of the Universe. X-ray detections and systematic characterisations of superclusters and the properties of their galaxies have only been possible in the last few years. Aims. We characterise XLSSsC N01, a rich supercluster at z ~ 0.3 detected in the XXL Survey, composed of X-ray clusters of different virial masses and X-ray... Više luminosities. As one of the first studies on this topic, we investigate the stellar populations of galaxies in different environments in the supercluster region. Methods. We study a magnitude-limited (r ≤ 20) and a mass-limited sample (log(M_∗/M_⊙) ≥ 10.8) of galaxies in the virialised region and in the outskirts of 11 XLSSsC N01 clusters, in high-density field regions, and in the low-density field. We compute the stellar population properties of galaxies using spectral energy distribution (SED) and spectral fitting techniques, and study the dependence of star formation rates (SFR), colours, and stellar ages on environment. Results. For r ≤ 20, the fraction of star-forming/blue galaxies, computed either from the specific-SFR (sSFR) or rest-frame colour, shows depletion within the cluster virial radii, where the number of galaxies with log(sSFR/yr^-1) > -12 and with (g - r)_restframe < 0.6 is lower than in the field. For log(M =M) 10:8, no trends with environment emerge, as massive galaxies are mostly already passive in all environments. No differences among low- and high- density field members and cluster members emerge in the sSFR-mass relation in the mass-complete regime. Finally, the luminosity- weighted age–mass relation of the passive populations within cluster virial radii show signatures of recent environmental quenching. Conclusions. The study of luminous and massive galaxies in this supercluster shows that while environment has a prominent role in determining the fractions of star-forming/blue galaxies, its effects on the star formation activity in star-forming galaxies are negligible. Sakrij dio sažetka
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. 620, A15
p-ISSN0004-6361
e-ISSN1432-0746
DOIhttps://doi.org/10.1051/0004-6361/201732507
URN:NBNurn:nbn:hr:217:892772
Datum objave publikacije2018
URL dokumentahttps://www.aanda.org/articles/aa/abs/2018/12/aa32507-17/aa32507-17.html
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Zaštićeno autorskim pravom.
Javna napomena© ESO 2018. Received 20 December 2017; Accepted 18 April 2018; Published online 20 November 2018.
Datum i vrijeme pohrane2020-03-01 18:23:53
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