XXIV. Cosmology from Sunyaev-Zeldovich cluster counts

  title={XXIV. Cosmology from Sunyaev-Zeldovich cluster counts},
  author={P. Ade and N. Aghanim and M. Arnaud and M. Ashdown and J. Aumont and C. Baccigalupi and A. Banday and R. B. Barreiro and J. Bartlett and N. Bartolo and E. Battaner and R. Battye and K. Benabed and A. Benoit and A. Benoit-L{\'e}vy and J. Bernard and M. Bersanelli and P. Bielewicz and J. Bock and A. Bonaldi and L. Bonavera and J. Bond and J. Borrill and F. Bouchet and M. Bucher and C. Burigana and R. C. Butler and E. Calabrese and J. Cardoso and A. Catalano and A. Challinor and A. Chamballu and R. Chary and H. Chiang and P. Christensen and S. Church and D. Clements and S. Colombi and L. Colombo and C. Combet and B. Comis and F. Couchot and A. Coulais and B. Crill and A. Curto and F. Cuttaia and L. Danese and R. Davies and R. Davis and P. Bernardis and A. Rosa and G. Zotti and J. Delabrouille and F. D'esert and J. Diego and K. Dolag and H. Dole and S. Donzelli and O. Dor'e and M. Douspis and A. Ducout and X. Dupac and G. Efstathiou and F. Elsner and T. Ensslin and H. Eriksen and E. Falgarone and J. Fergusson and F. Finelli and O. Forni and M. Frailis and A. Fraisse and E. Franceschi and A. Frejsel and S. Galeotta and S. Galli and K. Ganga and M. Giard and Y. Giraud-H'eraud and E. Gjerl{\o}w and J. Gonz'alez-Nuevo and K. M. G'orski and S. Gratton and A. Gregorio and A. Gruppuso and J. Gudmundsson and F. Hansen and D. Hanson and D. Harrison and S. Henrot-Versill'e and C. Hern'andez-Monteagudo and D. Herranz and S. Hildebrandt and E. Hivon and M. Hobson and W. Holmes and A. Hornstrup and W. Hovest and K. Huffenberger and G. Hurier and A. Jaffe and T. Jaffe and W. Jones and M. Juvela and E. Keihanen and R. Keskitalo and T. Kisner and R. Kneissl and J. Knoche and M. Kunz and H. Kurki-Suonio and G. Lagache and A. Lahteenmaki and J. Lamarre and A. Lasenby and M. Lattanzi and C. Lawrence and R. Leonardi and J. Lesgourgues and F. L{\'e}vrier and M. Liguori and P. Lilje and M. Linden-Vornle and M. L'opez-Caniego and P. Lubin and J. Mac'ias-P'erez and G. Maggio and D. Maino and N. Mandolesi and A. Mangilli and M. Maris and P. Martin and E. Mart'inez-Gonz'alez and S. Masi and S. Matarrese and P. McGehee and P. Meinhold and A. Melchiorri and J. Melin and L. Mendes and A. Mennella and M. Migliaccio and S. Mitra and M. Miville-Desch{\^e}nes and A. Moneti and L. Montier and G. Morgante and D. Mortlock and A. Moss and D. Munshi and J. A. Murphy and P. Naselsky and F. Nati and P. Natoli and C. Netterfield and H. N{\o}rgaard-Nielsen and F. Noviello and D. Novikov and I. Novikov and C. A. Oxborrow and F. Paci and L. Pagano and F. Pajot and D. Paoletti and B. Partridge and F. Pasian and G. Patanchon and T. Pearson and O. Perdereau and L. Perotto and F. Perrotta and V. Pettorino and F. Piacentini and M. Piat and E. Pierpaoli and D. Pietrobon and S. Plaszczynski and E. Pointecouteau and G. Polenta and L. Popa and G. Pratt and G. Prezeau and S. Prunet and J. Puget and J. Rachen and R. Rebolo and M. Reinecke and M. Remazeilles and C. Renault and A. Renzi and I. Ristorcelli and G. Rocha and M. Roman and C. Rosset and M. Rossetti and G. Roudier and J. Rubino-Mart'in and B. Rusholme and M. Sandri and D. Santos and M. Savelainen and G. Savini and D. Scott and M. Seiffert and E. Shellard and L. Spencer and V. Stolyarov and R. Stompor and R. Sudiwala and R. Sunyaev and D. Sutton and A. Suur-Uski and J. Sygnet and J. Tauber and L. Terenzi and L. Toffolatti and M. Tomasi and M. Tristram and M. Tucci and J. Tuovinen and M. Turler and G. Umana and L. Valenziano and J. Valiviita and B. Tent and P. Vielva and F. Villa and L. Wade and B. Wandelt and I. Wehus and J. Weller and S. White and D. Yvon and A. Zacchei and A. Zonca},
  journal={Astronomy and Astrophysics},
We present cluster counts and corresponding cosmological constraints from the Planck full mission data set. Our catalogue consists of 439 clusters detected via their Sunyaev-Zeldovich (SZ) signal d ... 


Neutrinos and BBN (and the CMB)
The halo mass function through the cosmic ages
2009a), with excellent agreement
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independent of redshift). This was not the case for our 2013 paper (Planck Collaboration XX 2014) where we adopted the AHF fit with parameters varying with redshift in the first ArXiv version
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2010b) from the combination of the REXCESS
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J. Cosmol. Astropart
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A classic example is the Malmquist bias, where bright objects near the flux limit are preferentially detected. This effect is amplified by Eddington bias, the mass function dictating
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Right: ratio of each simulated Y500–M500 relation relative to Eq. A.9. The different scaling laws are taken from Kay et al. (2012b)
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