Utilizza questo identificativo per citare o creare un link a questo documento:
http://hdl.handle.net/20.500.12386/27415
Campo DC | Valore | Lingua |
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dc.contributor.author | A. Saro | en_US |
dc.contributor.author | S. Bocquet | en_US |
dc.contributor.author | E. Rozo | en_US |
dc.contributor.author | B. A. Benson | en_US |
dc.contributor.author | J. Mohr | en_US |
dc.contributor.author | E. S. Rykoff | en_US |
dc.contributor.author | M. Soares-Santos | en_US |
dc.contributor.author | L. Bleem | en_US |
dc.contributor.author | S. Dodelson | en_US |
dc.contributor.author | P. Melchior | en_US |
dc.contributor.author | F. Sobreira | en_US |
dc.contributor.author | V. Upadhyay | en_US |
dc.contributor.author | J. Weller | en_US |
dc.contributor.author | T. Abbott | en_US |
dc.contributor.author | F. B. Abdalla | en_US |
dc.contributor.author | S. Allam | en_US |
dc.contributor.author | R. Armstrong | en_US |
dc.contributor.author | M. Banerji | en_US |
dc.contributor.author | A. H. Bauer | en_US |
dc.contributor.author | M. Bayliss | en_US |
dc.contributor.author | A. Benoit-Levy | en_US |
dc.contributor.author | G. M. Bernstein | en_US |
dc.contributor.author | E. Bertin | en_US |
dc.contributor.author | M. Brodwin | en_US |
dc.contributor.author | D. Brooks | en_US |
dc.contributor.author | E. Buckley-Geer | en_US |
dc.contributor.author | D. L. Burke | en_US |
dc.contributor.author | J. E. Carlstrom | en_US |
dc.contributor.author | R. Capasso | en_US |
dc.contributor.author | D. Capozzi | en_US |
dc.contributor.author | A. Carnero Rosell | en_US |
dc.contributor.author | M. Carrasco Kind | en_US |
dc.contributor.author | I. Chiu | en_US |
dc.contributor.author | R. Covarrubias | en_US |
dc.contributor.author | T. M. Crawford | en_US |
dc.contributor.author | M. Crocce | en_US |
dc.contributor.author | C. B. D'Andrea | en_US |
dc.contributor.author | L. N. da Costa | en_US |
dc.contributor.author | D. L. DePoy | en_US |
dc.contributor.author | S. Desai | en_US |
dc.contributor.author | T. de Haan | en_US |
dc.contributor.author | H. T. Diehl | en_US |
dc.contributor.author | J. P. Dietrich | en_US |
dc.contributor.author | P. Doel | en_US |
dc.contributor.author | C. E Cunha | en_US |
dc.contributor.author | T. F. Eifler | en_US |
dc.contributor.author | A. E. Evrard | en_US |
dc.contributor.author | A. Fausti Neto | en_US |
dc.contributor.author | E. Fernandez | en_US |
dc.contributor.author | B. Flaugher | en_US |
dc.contributor.author | P. Fosalba | en_US |
dc.contributor.author | J. Frieman | en_US |
dc.contributor.author | C. Gangkofner | en_US |
dc.contributor.author | E. Gaztanaga | en_US |
dc.contributor.author | D. Gerdes | en_US |
dc.contributor.author | D. Gruen | en_US |
dc.contributor.author | R. A. Gruendl | en_US |
dc.contributor.author | N. Gupta | en_US |
dc.contributor.author | C. Hennig | en_US |
dc.contributor.author | W. L. Holzapfel | en_US |
dc.contributor.author | K. Honscheid | en_US |
dc.contributor.author | B. Jain | en_US |
dc.contributor.author | D. James | en_US |
dc.contributor.author | K. Kuehn | en_US |
dc.contributor.author | N. Kuropatkin | en_US |
dc.contributor.author | O. Lahav | en_US |
dc.contributor.author | T. S. Li | en_US |
dc.contributor.author | H. Lin | en_US |
dc.contributor.author | M. A. G. Maia | en_US |
dc.contributor.author | M. March | en_US |
dc.contributor.author | J. L. Marshall | en_US |
dc.contributor.author | Paul Martini | en_US |
dc.contributor.author | M. McDonald | en_US |
dc.contributor.author | C. J. Miller | en_US |
dc.contributor.author | R. Miquel | en_US |
dc.contributor.author | B. Nord | en_US |
dc.contributor.author | R. Ogando | en_US |
dc.contributor.author | A. A. Plazas | en_US |
dc.contributor.author | C. L. Reichardt | en_US |
dc.contributor.author | A. K. Romer | en_US |
dc.contributor.author | A. Roodman | en_US |
dc.contributor.author | M. Sako | en_US |
dc.contributor.author | E. Sanchez | en_US |
dc.contributor.author | M. Schubnell | en_US |
dc.contributor.author | I. Sevilla | en_US |
dc.contributor.author | R. C. Smith | en_US |
dc.contributor.author | B. Stalder | en_US |
dc.contributor.author | A. A. Stark | en_US |
dc.contributor.author | STRAZZULLO, VERONICA | en_US |
dc.contributor.author | E. Suchyta | en_US |
dc.contributor.author | M. E. C. Swanson | en_US |
dc.contributor.author | G. Tarle | en_US |
dc.contributor.author | J. Thaler | en_US |
dc.contributor.author | D. Thomas | en_US |
dc.contributor.author | D. Tucker | en_US |
dc.contributor.author | V. Vikram | en_US |
dc.contributor.author | A. von der Linden | en_US |
dc.contributor.author | A. R. Walker | en_US |
dc.contributor.author | R. H. Wechsler | en_US |
dc.contributor.author | W. Wester | en_US |
dc.contributor.author | A. Zenteno | en_US |
dc.contributor.author | K. E. Ziegler | en_US |
dc.date.accessioned | 2020-09-16T11:33:26Z | - |
dc.date.available | 2020-09-16T11:33:26Z | - |
dc.date.issued | 2015 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27415 | - |
dc.description.abstract | We cross-match galaxy cluster candidates selected via their Sunyaev-Zel'dovich effect (SZE) signatures in 129.1 deg2 of the South Pole Telescope 2500d SPT-SZ survey with optically identified clusters selected from the Dark Energy Survey science verification data. We identify 25 clusters between 0.1 ≲ z ≲ 0.8 in the union of the SPT-SZ and redMaPPer (RM) samples. RM is an optical cluster finding algorithm that also returns a richness estimate for each cluster. We model the richness λ-mass relation with the following function <ln λ|M500> ∝ Bλln M500 + Cλln E(z) and use SPT-SZ cluster masses and RM richnesses λ to constrain the parameters. We find B_λ = 1.14^{+0.21}_{-0.18} and C_λ =0.73^{+0.77}_{-0.75}. The associated scatter in mass at fixed richness is σ _{ln M|λ } = 0.18^{+0.08}_{-0.05} at a characteristic richness λ = 70. We demonstrate that our model provides an adequate description of the matched sample, showing that the fraction of SPT-SZ-selected clusters with RM counterparts is consistent with expectations and that the fraction of RM-selected clusters with SPT-SZ counterparts is in mild tension with expectation. We model the optical-SZE cluster positional offset distribution with the sum of two Gaussians, showing that it is consistent with a dominant, centrally peaked population and a subdominant population characterized by larger offsets. We also cross-match the RM catalogue with SPT-SZ candidates below the official catalogue threshold significance ξ = 4.5, using the RM catalogue to provide optical confirmation and redshifts for 15 additional clusters with ξ ∈ [4, 4.5]. | en_US |
dc.language.iso | eng | en_US |
dc.title | Constraints on the richness-mass relation and the optical-SZE positional offset distribution for SZE-selected clusters | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/stv2141 | en_US |
dc.identifier.scopus | 2-s2.0-85040254034 | en_US |
dc.identifier.isi | 000368000400004 | en_US |
dc.identifier.url | http://arxiv.org/abs/1506.07814v1 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article/454/3/2305/1201112 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 454 | en_US |
dc.relation.issue | 3 | en_US |
dc.relation.firstpage | 2305 | en_US |
dc.relation.lastpage | 2319 | en_US |
dc.type.referee | REF_1 | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2015MNRAS.454.2305S | 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 | O.A. Trieste | - |
crisitem.author.orcid | 0000-0001-7975-2894 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
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