Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/26984
DC Field | Value | Language |
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dc.contributor.author | Pierre, M. | en_US |
dc.contributor.author | Adami, C. | en_US |
dc.contributor.author | Birkinshaw, M. | en_US |
dc.contributor.author | CHIAPPETTI, LUCIO | en_US |
dc.contributor.author | ETTORI, STEFANO | en_US |
dc.contributor.author | Evrard, A. | en_US |
dc.contributor.author | Faccioli, L. | en_US |
dc.contributor.author | GASTALDELLO, FABIO | en_US |
dc.contributor.author | Giles, P. | en_US |
dc.contributor.author | Horellou, C. | en_US |
dc.contributor.author | IOVINO, Angela | en_US |
dc.contributor.author | Valtchanov, I. | en_US |
dc.contributor.author | Veropalumbo, A. | en_US |
dc.contributor.author | Ascaso, B. | en_US |
dc.contributor.author | Barnes, D. | en_US |
dc.contributor.author | De Petris, M. | en_US |
dc.contributor.author | Durret, F. | en_US |
dc.contributor.author | Donahue, M. | en_US |
dc.contributor.author | Ithana, M. | en_US |
dc.contributor.author | Jarvis, M. | en_US |
dc.contributor.author | Johnston-Hollitt, M. | en_US |
dc.contributor.author | Kay, S. | en_US |
dc.contributor.author | Kalfountzou, E. | en_US |
dc.contributor.author | La Franca, F. | en_US |
dc.contributor.author | Okabe, N. | en_US |
dc.contributor.author | Muzzin, A. | en_US |
dc.contributor.author | Rettura, A. | en_US |
dc.contributor.author | Ricci, F. | en_US |
dc.contributor.author | Ridl, J. | en_US |
dc.contributor.author | Risaliti, G. | en_US |
dc.contributor.author | Takizawa, M. | en_US |
dc.contributor.author | Thomas, P. | en_US |
dc.contributor.author | Koulouridis, E. | en_US |
dc.contributor.author | Truong, N. | en_US |
dc.contributor.author | Lidman, C. | en_US |
dc.contributor.author | Le Brun, A. | en_US |
dc.contributor.author | Maughan, B. | en_US |
dc.contributor.author | Maurogordato, S. | en_US |
dc.contributor.author | McCarthy, I. | en_US |
dc.contributor.author | Miyazaki, S. | en_US |
dc.contributor.author | Pacaud, F. | en_US |
dc.contributor.author | Paltani, S. | en_US |
dc.contributor.author | Plionis, M. | en_US |
dc.contributor.author | Reiprich, T. | en_US |
dc.contributor.author | Sadibekova, T. | en_US |
dc.contributor.author | Smolcic, V. | en_US |
dc.contributor.author | Snowden, S. | en_US |
dc.contributor.author | Surdej, J. | en_US |
dc.contributor.author | Tsirou, M. | en_US |
dc.contributor.author | Vignali, C. | en_US |
dc.contributor.author | Willis, J. | en_US |
dc.contributor.author | Alis, S. | en_US |
dc.contributor.author | Altieri, B. | en_US |
dc.contributor.author | Baran, N. | en_US |
dc.contributor.author | Benoist, C. | en_US |
dc.contributor.author | BONGIORNO, ANGELA | en_US |
dc.contributor.author | Bremer, M. | en_US |
dc.contributor.author | Butler, A. | en_US |
dc.contributor.author | CAPPI, Alberto | en_US |
dc.contributor.author | Caretta, C. | en_US |
dc.contributor.author | CILIEGI, Paolo | en_US |
dc.contributor.author | Clerc, N. | en_US |
dc.contributor.author | Corasaniti, P. S. | en_US |
dc.contributor.author | Coupon, J. | en_US |
dc.contributor.author | Delhaize, J. | en_US |
dc.contributor.author | DELVECCHIO, IVAN | en_US |
dc.contributor.author | Democles, J. | en_US |
dc.contributor.author | Desai, Sh. | en_US |
dc.contributor.author | Devriendt, J. | en_US |
dc.contributor.author | Dubois, Y. | en_US |
dc.contributor.author | Eckert, D. | en_US |
dc.contributor.author | Elyiv, A. | en_US |
dc.contributor.author | Farahi, A. | en_US |
dc.contributor.author | Ferraril, C. | en_US |
dc.contributor.author | Fotopoulou, S. | en_US |
dc.contributor.author | Forman, W. | en_US |
dc.contributor.author | Georgantopoulos, I. | en_US |
dc.contributor.author | Guglielmo, V. | en_US |
dc.contributor.author | Huynh, M. | en_US |
dc.contributor.author | Jerlin, N. | en_US |
dc.contributor.author | Jones, Ch. | en_US |
dc.contributor.author | Lavoie, S. | en_US |
dc.contributor.author | Le Fevre, J. -P. | en_US |
dc.contributor.author | Lieu, M. | en_US |
dc.contributor.author | Kilbinger, M. | en_US |
dc.contributor.author | MaruIli, F. | en_US |
dc.contributor.author | Mantz, A. | en_US |
dc.contributor.author | McGee, S. | en_US |
dc.contributor.author | Melin, J. -B. | en_US |
dc.contributor.author | Melnyk, O. | en_US |
dc.contributor.author | Moscardini, L. | en_US |
dc.contributor.author | Novak, M. | en_US |
dc.contributor.author | Piconcelli, E. | en_US |
dc.contributor.author | POGGIANTI, Bianca Maria | en_US |
dc.contributor.author | Pomarede, D. | en_US |
dc.contributor.author | Pompei, E. | en_US |
dc.contributor.author | Ponman, T. | en_US |
dc.contributor.author | Ramos Ceja, M. E. | en_US |
dc.contributor.author | Rana, P. | en_US |
dc.contributor.author | Rapetti, D. | en_US |
dc.contributor.author | Raychaudhury, S. | en_US |
dc.contributor.author | Ricci, M. | en_US |
dc.contributor.author | Rottgering, H. | en_US |
dc.contributor.author | Sahlen, M. | en_US |
dc.contributor.author | Sauvageot, J. -L. | en_US |
dc.contributor.author | Schimd, C. | en_US |
dc.contributor.author | Sereno, Mauro | en_US |
dc.contributor.author | Smith, G. P. | en_US |
dc.contributor.author | Umetsu, K. | en_US |
dc.contributor.author | Valageas, P. | en_US |
dc.contributor.author | Valotti, A. | en_US |
dc.date.accessioned | 2020-08-31T08:20:00Z | - |
dc.date.available | 2020-08-31T08:20:00Z | - |
dc.date.issued | 2017 | en_US |
dc.identifier.issn | 0004-6337 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/26984 | - |
dc.description.abstract | The XXL survey currently covers two 25 deg<SUP>2</SUP> patches with XMM observations of ∼10 ks. We summarize the scientific results associated with the first release of the XXL dataset, which occurred in mid-2016. We review several arguments for increasing the survey depth to 40 ks during the next decade of XMM operations. X-ray (z < 2) cluster, (z < 4) active galactic nuclei (AGN), and cosmic background survey science will then benefit from an extraordinary data reservoir. This, combined with deep multi-λ observations, will lead to solid standalone cosmological constraints and provide a wealth of information on the formation and evolution of AGN, clusters, and the X-ray background. In particular, it will offer a unique opportunity to pinpoint the z > 1 cluster density. It will eventually constitute a reference study and an ideal calibration field for the upcoming eROSITA and Euclid missions. | en_US |
dc.language.iso | eng | en_US |
dc.title | The XXL survey: First results and future | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1002/asna.201713352 | en_US |
dc.identifier.scopus | 2-s2.0-85016718482 | en_US |
dc.identifier.isi | 000400339900033 | en_US |
dc.identifier.url | https://onlinelibrary.wiley.com/doi/full/10.1002/asna.201713352 | en_US |
dc.identifier.url | https://arxiv.org/abs/1610.01781 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 338 | en_US |
dc.relation.issue | 334 | en_US |
dc.relation.firstpage | 334 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.international | sì | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | ASTRONOMISCHE NACHRICHTEN | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2017AN....338..334P | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | IASF Milano | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Roma | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | O.A. Brera | - |
crisitem.author.dept | O.A. Padova | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0001-7857-7908 | - |
crisitem.author.orcid | 0000-0003-4117-8617 | - |
crisitem.author.orcid | 0000-0002-9112-0184 | - |
crisitem.author.orcid | 0000-0001-6958-0304 | - |
crisitem.author.orcid | 0000-0002-0101-6624 | - |
crisitem.author.orcid | 0000-0002-9200-7167 | - |
crisitem.author.orcid | 0000-0002-0447-4620 | - |
crisitem.author.orcid | 0000-0001-8706-2252 | - |
crisitem.author.orcid | 0000-0001-8751-8360 | - |
crisitem.author.orcid | 0000-0003-0302-0325 | - |
crisitem.journal.journalissn | 0004-6337 | - |
crisitem.journal.ance | E016235 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
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j100arxiv.1610.01781.pdf | postprint | 3.33 MB | Adobe PDF | View/Open |
j100.pdf | [Administrators only] | 1.48 MB | Adobe PDF |
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