<i>Planck</i>early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Ade, Peter A. R.; Aghanim, N.; Arnaud, M.; Ashdown, M.; Aumont, J.; Baccigalupi, C.; Balbi, A.; Banday, A. J.; Barreiro, R. B.; Bartelmann, Matthias; Bartlett, J. G.; Battaner, E.; Benabed, K.; Benoı̂t, A.; Bernard, J.-P.; Bersanelli, M.; Bhatia, R.; Bock, J. J.; Bonaldi, A.; Bond, J. R.; Borrill, J.; Bouchet, F. R.; Bourdin, H.; Brown, Michael L.; Bucher, M.; Burigana, C.; Cabella, P.; Cardoso, J.-F.; Catalano, A.; Cayón, L.; Challinor, A.; Chamballu, A.; Chiang, L.-Y; Chiang, C.; Chon, G.; Christensen, P. R.; Churazov, E.; Clements, D. L.; Colafrancesco, S.; Colombi, S.; Couchot, F.; Coulais, A.; Crill, B. P.; Cuttaia, F.; Silva, Antônio da; Dahle, H.; Danese, L.; Bernardis, P. de; Gasperis, G. de; Rosa, A. De; Zotti, G. de; Delabrouille, J.; Delouis, J.-M.; Désert, F.‐X.; Diego, J. M.; Dolag, K.; Donzelli, S.; Doré, O.; Dörl, U.; Douspis, M.; Dupac, X.; Efstathiou, G.; Enßlin, T. A.; Finelli⋆, F.; Flores-Cacho, I.; Forni, O.; Frailis, M.; Franceschi, E.; Fromenteau, S.; Galeotta, S.; Ganga, K.; Génova-Santos, R. T.; Giard, M.; Giardino, G.; Giraud‐Héraud, Y.; González‐Nuevo, J.; Górski, K. M.; Gratton, S.; Gregorio, A.; Gruppuso, A.; Harrison, D. L.; Henrot-Versillé, S.; Hernández-Monteagudo, C.; Herranz, D.; Hildebrandt, S. R.; Hivon, E.; Hobson, M.; Holmes, W. A.; Hovest, W.; Hoyland, R. J.; Huffenberger, K. M.; Jaffe, A. H.; Jones, W. C.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kisner, T. S.; Kneißl, R.; Knox, L.; Kurki-Suonio, H.; Lagache, G.; Lamarre, J.-M.; Lanoux, J.; Lasenby, A.; Laureijs, R. J.; Lawrence, C. R.; Leach, S.; Leonardi, R.; Liddle, Andrew R.; Lilje, P. B.; Linden-Vørnle, M.; López‐Caniego, M.; Lubin, P. M.; Macías-Pérez, J. F.; MacTavish, C. J.; Maffei, B.; Maino, D.; Mandolesi, N.; Mann, Robert; Maris, M.; Marleau, F.; Martínez-González, E.; Masi, S.; Matarrese, S.; Matthai, F.; Mazzotta, P.; Melchiorri, A.; Melin, J.-B.; Mendes, L.; Mennella, A.; Mitra, S.; Miville-Deschênes, M.-A.; Moneti, A.; Montier, L.; Morgante, G.; Mortlock, D.; Munshi, D.; Murphy, A.; Naselsky, P.; Natoli, P.; Netterfield, C. B.; Nørgaard-Nielsen, H. U.; Noviello, F.; Novikov, D.; Новиков, И. Д.; Osborne, S.; Pajot, F.; Pasian, F.; Patanchon, G.; Perdereau, O.; Perotto, L.; Perrotta, F.; Piacentini, F.; Piat, M.; Pierpaoli, E.; Piffaretti, R.; Plaszczynski, S.; Pointecouteau, É.; Polenta, G.; Ponthieu, N.; Poutanen, T.; Pratt, G. W.; Prézeau, G.; Prunet, S.; Puget, J.-L.; Rachen, J. P.; Rebolo, R.; Reinecke, M.; Renault, C.; Ricciardi, S.; Riller, T.; Ristorcelli, I.; Rocha, G.; Rosset, C.; Rubiño-Martín, J. A.; Rusholme, B.; Sandri, M.; Santos, D.; Savini, G.; Schaefer, B.; Scott, D.; Seiffert, M. D.; Shellard, P.; Smoot, George F.; Starck, Jean-Luc; Stivoli, F.; Stolyarov, V.; Sudiwala, R.; Sunyaev, R.; Sygnet, J.-F.; Tauber, J. A.; Terenzi, L.; Toffolatti, L.; Tomasi, M.; Torre, J. P.; Tristram, M.; Tuovinen, J.; Valenziano, L.; Vibert, L.; Vielva, P.; Villa, F.; Vittorio, N.; Wade, L. A.; Wandelt, B. D.; White, Simon D. M.; White, Martin; Yvon, D.; Zacchei, A.; Zonca, A.

doi:10.1051/0004-6361/201116458

Cited by 180 publications

(20 citation statements)

References 87 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Thus, the τ − y relation and its scatter reflect the difference in 1/(T e,∆ ) at fixed total gas pressure. This low-scatter correlation in the τ − y relation is not surprising given that the Planck satellite [62] and the Weighing the Giants collaboration [45] found tight correlations between Y and M gas . Previous X-ray measurements of clusters also showed a strong, low-scatter correlation between T X and M gas [e.g., 42,52,88].…”

Section: τ Relationsmentioning

confidence: 74%

The tau of galaxy clusters

Battaglia

2016

J. Cosmol. Astropart. Phys.

106

161

View full text Add to dashboard Cite

The recent emergence of detections of the kinetic Sunyaev-Zel'dovich (kSZ) effect through crosscorrelation techniques is encouraging for the prospects of future cosmic microwave background (CMB) experiments. Extracting information on the large-scale velocity fields and constraining cosmological parameters from such kSZ measurements requires an understanding of the optical depth to CMB photons through halos. Using cosmological hydrodynamic simulations we find that there exists a low-scatter relation between the optical depth and thermal Sunyaev-Zel'dovich (tSZ) signal of halos within a physical aperture. We propose that such a relation can be used to break the degeneracy between optical depth and line-of-sight velocity in kSZ measurements. The limiting factors in our proposal are systematic uncertainties associated with the sub-grid physics models in the simulations, which we calculate to be less than 10 percent. We discuss future observational measurements that could potentially be used to mitigate the systematic uncertainties in this scaling relation.

show abstract

Section: τ Relationsmentioning

confidence: 74%

The tau of galaxy clusters

Battaglia

2016

J. Cosmol. Astropart. Phys.

106

161

View full text Add to dashboard Cite

show abstract

“…where ∆lnM is the cluster mass calibration offset relative to S 8,V 09 . We consider two mass calibration offset values, P11 = −0.12 ± 0.02 adopted by Planck team [77] and R12 = 0.11 ± 0.04 corresponding to the cluster mass scale employed in ref. [78].…”

Section: Jcap02(2014)012mentioning

confidence: 99%

“…Figure 4 presents the joint two-dimensional marginalized probability distributions in Ω m h 2 − N eff , Ω m h 2 − z eq , and Y P − ξ ν planes for the extensions of mΛCDM models involving leptonic asymmetry. When we transform N eff axis of the left [77] and R12 [78] (indicated by bands). Bottom: S 8 -H 0 joint confidence regions (at 68% and 95% CL) obtained from the same analysis.…”

Section: Degenerate Massive Neutrinosmentioning

confidence: 99%

Cosmological evidence for leptonic asymmetry after Planck

Caramete¹,

Popa²

2014

J. Cosmol. Astropart. Phys.

View full text Add to dashboard Cite

Recently, the Planck satellite found a larger and most precise value of the matter energy density, that impacts on the present values of other cosmological parameters such as the Hubble constant H 0 , the present cluster abundances S 8 , and the age of the Universe t U . The existing tension between Planck determination of these parameters in the frame of the base ΛCDM model and their determination from other measurements generated lively discussions, one possible interpretation being that some sources of systematic errors in cosmological measurements are not completely understood. An alternative interpretation is related to the fact that the CMB observations, that probe the high redshift Universe are interpreted in terms of cosmological parameters at present time by extrapolation within the base ΛCDM model that can be inadequate or incomplete. In this paper we quantify this tension by exploring several extensions of the base ΛCDM model that include the leptonic asymmetry. We set bounds on the radiation content of the Universe and neutrino properties by using the latest cosmological measurements, imposing also self-consistent BBN constraints on the primordial helium abundance. For all asymmetric cosmological models we find the preference of cosmological data for smaller values of active and sterile neutrino masses. This increases the tension between cosmological and short baseline neutrino oscillation data that favors a sterile neutrino with the mass of around 1 eV. For the case of degenerate massive neutrinos, we find that the discrepancies with the local determinations of H 0 , and t U are alleviated at ∼ 1.3σ level while S 8 is in agreement with its determination from CFHTLenS survey data at ∼ 1σ and with the prediction of cluster mass-observation relation at ∼ 0.5σ. We also find 2σ statistical preference of the cosmological data for the leptonic asymmetric models involving three massive neutrino species and neutrino direct mass hierarchy. We conclude that the current cosmological data favor the leptonic asymmetric extension of the base ΛCDM model and normal neutrino mass hierarchy over the models with additional sterile neutrino species and/or inverted neutrino mass hierarchy.

show abstract

“…The quantities Y X and Y S ZE were determined within the R 500 . The thermal pressure (P) of the intra-cluster medium for each galaxy cluster used in our analyses was modeled by Ade et al [55] via the universal pressure profile discussed by Arnaud et al [56]. This universal profile was obtained by comparing simulated data with observational data (a representative sample of nearby clusters covering the mass range 10 14 M < M 500 < 10 15 M ).…”

Section: A Datamentioning

confidence: 99%

On a possible cosmological evolution of galaxy cluster $Y_{\rm X}-Y_{\rm SZE}$ scaling relation

Holanda,

da Silva

2020

Preprint

View full text Add to dashboard Cite

An important result from self-similar models that describe the process of galaxy cluster formation is the simple scaling relationIn this ratio, Y S ZE is the integrated Sunyaev-Zel'dovich effect flux of a cluster, its X-ray counterpart is Y X , C XS ZE and C are constants and D A is the angular diameter distance to the cluster. In this paper, we consider the cosmic distance duality relation validity jointly with type Ia supernovae observations plus 61 Y S ZE D 2 A /C XS ZE Y X measurements as reported by the Planck Collaboration to explore if this relation is constant in the redshift range considered (z < 0.5). No one specific cosmological model is used. As basic result, although the data sets are compatible with no redshift evolution within 2σ c.l., a Bayesian analysis indicates that other C(z) functions analyzed in this work cannot be discarded. It is worth to stress that the observational determination of an universal C(z) function turns the Y S ZE D 2 A /C XS ZE Y X ratio in an useful cosmological tool to determine cosmological parameters. Moreover, the approach proposed here can also be used as a cross-check for those scaling relation calibration methods that use weak-lensing analyses.

show abstract

Planckearly results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations

Cited by 180 publications

References 87 publications

The tau of galaxy clusters

The tau of galaxy clusters

Cosmological evidence for leptonic asymmetry after Planck

On a possible cosmological evolution of galaxy cluster $Y_{\rm X}-Y_{\rm SZE}$ scaling relation

Contact Info

Product

Resources

About