Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters

J.G. Bartlett; J. Delabrouille; K. Ganga; Y. Giraud-Héraud; M. Le Jeune; M. Piat; M. Remazeilles; C. Rosset; G.F. Smoot; T. Poutanen; I. Bikmaev; P. Natoli; G. Polenta; N. Mandolesi; M. Ashdown; P. Carvalho; M. Hobson; A. Lasenby; R. Kneissl; J.R. Bond; M.-A. Miville-Deschênes; A.J. Banday; J.-P. Bernard; I. Flores-Cacho; O. Forni; D.J. Marshall; E. Pointecouteau; O. Doré; S.R. Hildebrandt; S. Mei; G. Rocha; H. Dahle; P.B. Lilje; A. Da Silva; C. Hernández-Monteagudo; J. Borrill; J.-B. Melin; R. Piffaretti; D. Yvon; Allan Hornstrup; Michael Linden-Vørnle; Hans Ulrik Nørgaard-Nielsen; M. Frommert; M. Kunz; L. Toffolatti; I. Bikmaev; D. Scott; E. Pierpaoli; A. Liddle; M. Juvela; H. Kurki-Suonio; T. Poutanen; A.-S. Suur-Uski; W.C. Jones; G.F. Smoot; L. Knox; A. Stanford; P.R. Meinhold; A. Zonca; B.D. Wandelt; L. Cayón; S. Matarrese; P. De Bernardis; S. Masi; A. Melchiorri; F. Nati; F. Piacentini; M. Bersanelli; D. Maino; A. Mennella; M. Rossetti; S. Borgani; A. Gregorio; C. Burigana; P. Natoli; A. Balbi; G. De Gasperis; P. Mazzotta; N. Vittorio; P. Cabella; P.R. Christensen; P. Naselsky; A. Hempel; J.A. Rubiño-Martín; R. Kneissl; R. González-Riestra; X. Dupac; T. Jagemann; R. Leonardi; L. Mendes; J.A. Tauber; S. Mei; H. Kurki-Suonio; T. Poutanen; A.-S. Suur-Uski; G. De Zotti; S. Colafrancesco; G. Polenta; S. Borgani; M. Frailis; S. Galeotta; A. Gregorio; M. Maris; A. Zacchei; M. Massardi; C. Burigana; R.C. Butler; F. Cuttaia; F. Finelli; E. Franceschi; A. Gruppuso; N. Mandolesi; G. Morgante; P. Natoli; D. Paoletti; S. Ricciardi; M. Sandri; L. Terenzi; L. Valenziano; F. Villa; M. Bersanelli; S. Donzelli; D. Maino; A. Mennella; M. Rossetti; M. Tomasi; A. Melchiorri; F. Stivoli; F.-X. Désert; S. Mitra; A. Chamballu; D.L. Clements; A.H. Jaffe; D. Mortlock; R.-R. Chary; B. Rusholme; A. Benoît; H. Dole; N. Aghanim; J. Aumont; H. Dole; M. Douspis; M. Kunz; G. Lagache; M.-A. Miville-Deschênes; F. Pajot; J.-L. Puget; M. Remazeilles; N. Welikala; K. Benabed; F.R. Bouchet; S. Colombi; E. Hivon; A. Moneti; S. Prunet; J.-F. Sygnet; B.D. Wandelt; L. Popa; F. Marleau; L.-Y. Chiang; D. Harrison; D. Sutton; H. Dahle; H.K. Eriksen; F.K. Hansen; P.B. Lilje; R.T. Génova-Santos; A. Hempel; J.A. Rubiño-Martín; R.B. Barreiro; J.M. Diego; J. González-Nuevo; D. Herranz; M. López-Caniego; E. Martínez-González; L. Toffolatti; P. Vielva; P. Platania; J.G. Bartlett; B.P. Crill; O. Doré; K.M. Górski; W.A. Holmes; C.R. Lawrence; S. Mitra; G. Rocha; L.A. Wade; A. Bonaldi; M.L. Brown; R.J. Davis; F. Noviello; M. Ashdown; D. Harrison; A. Lasenby; D. Sutton; S. Henrot-Versillé; G. Luzzi; O. Perdereau; S. Plaszczynski; M. Tristram; A. Catalano; A. Coulais; J.-M. Lamarre; M. Arnaud; J. Démoclès; R. Piffaretti; G.W. Pratt; A. Catalano; G. Hurier; J.F. MacÍas-Pérez; C. Renault; B. Van Tent; G.F. Smoot; K. Dolag; T.A. Enßlin; C. Hernández-Monteagudo; W. Hovest; J. Knoche; M. Reinecke; R. Sunyaev; S.D.M. White; H. Böhringer; G. Chon; P.R. Christensen; P. Naselsky; B.P. Crill; G. Savini; C. Baccigalupi; G. De Zotti; J. González-Nuevo; S. Leach; F. Perrotta; R. Mann; P.A.R. Ade; D. Munshi; R. Sudiwala; R. Sunyaev; J. Borrill; S. Osborne; K. Benabed; F.R. Bouchet; S. Colombi; E. Hivon; S. Prunet; B.D. Wandelt; S. Mei; A.J. Banday; I. Flores-Cacho; O. Forni; D.J. Marshall; E. Pointecouteau; K. Dolag; J. Weller; E. Battaner; K.M. Huffenberger; K.M. Górski

doi:10.1051/0004-6361/201219519

Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters

J.G. Bartlett, J. Delabrouille, K. Ganga, Y. Giraud-Héraud, M. Le Jeune, M. Piat, M. Remazeilles, C. Rosset, G.F. Smoot, T. Poutanen, I. Bikmaev, P. Natoli, G. Polenta, N. Mandolesi, M. Ashdown, P. Carvalho, M. Hobson, A. Lasenby, R. Kneissl, J.R. BondM.-A. Miville-Deschênes, A.J. Banday, J.-P. Bernard, I. Flores-Cacho, O. Forni, D.J. Marshall, E. Pointecouteau, O. Doré, S.R. Hildebrandt, S. Mei, G. Rocha, H. Dahle, P.B. Lilje, A. Da Silva, C. Hernández-Monteagudo, J. Borrill, J.-B. Melin, R. Piffaretti, D. Yvon, Allan Hornstrup, Michael Linden-Vørnle, Hans Ulrik Nørgaard-Nielsen, M. Frommert, M. Kunz, L. Toffolatti, I. Bikmaev, D. Scott, E. Pierpaoli, A. Liddle, M. Juvela, H. Kurki-Suonio, T. Poutanen, A.-S. Suur-Uski, W.C. Jones, G.F. Smoot, L. Knox, A. Stanford, P.R. Meinhold, A. Zonca, B.D. Wandelt, L. Cayón, S. Matarrese, P. De Bernardis, S. Masi, A. Melchiorri, F. Nati, F. Piacentini, M. Bersanelli, D. Maino, A. Mennella, M. Rossetti, S. Borgani, A. Gregorio, C. Burigana, P. Natoli, A. Balbi, G. De Gasperis, P. Mazzotta, N. Vittorio, P. Cabella, P.R. Christensen, P. Naselsky, A. Hempel, J.A. Rubiño-Martín, R. Kneissl, R. González-Riestra, X. Dupac, T. Jagemann, R. Leonardi, L. Mendes, J.A. Tauber, S. Mei, H. Kurki-Suonio, T. Poutanen, A.-S. Suur-Uski, G. De Zotti, S. Colafrancesco, G. Polenta, S. Borgani, M. Frailis, S. Galeotta, A. Gregorio, M. Maris, A. Zacchei, M. Massardi, C. Burigana, R.C. Butler, F. Cuttaia, F. Finelli, E. Franceschi, A. Gruppuso, N. Mandolesi, G. Morgante, P. Natoli, D. Paoletti, S. Ricciardi, M. Sandri, L. Terenzi, L. Valenziano, F. Villa, M. Bersanelli, S. Donzelli, D. Maino, A. Mennella, M. Rossetti, M. Tomasi, A. Melchiorri, F. Stivoli, F.-X. Désert, S. Mitra, A. Chamballu, D.L. Clements, A.H. Jaffe, D. Mortlock, R.-R. Chary, B. Rusholme, A. Benoît, H. Dole, N. Aghanim, J. Aumont, H. Dole, M. Douspis, M. Kunz, G. Lagache, M.-A. Miville-Deschênes, F. Pajot, J.-L. Puget, M. Remazeilles, N. Welikala, K. Benabed, F.R. Bouchet, S. Colombi, E. Hivon, A. Moneti, S. Prunet, J.-F. Sygnet, B.D. Wandelt, L. Popa, F. Marleau, L.-Y. Chiang, D. Harrison, D. Sutton, H. Dahle, H.K. Eriksen, F.K. Hansen, P.B. Lilje, R.T. Génova-Santos, A. Hempel, J.A. Rubiño-Martín, R.B. Barreiro, J.M. Diego, J. González-Nuevo, D. Herranz, M. López-Caniego, E. Martínez-González, L. Toffolatti, P. Vielva, P. Platania, J.G. Bartlett, B.P. Crill, O. Doré, K.M. Górski, W.A. Holmes, C.R. Lawrence, S. Mitra, G. Rocha, L.A. Wade, A. Bonaldi, M.L. Brown, R.J. Davis, F. Noviello, M. Ashdown, D. Harrison, A. Lasenby, D. Sutton, S. Henrot-Versillé, G. Luzzi, O. Perdereau, S. Plaszczynski, M. Tristram, A. Catalano, A. Coulais, J.-M. Lamarre, M. Arnaud, J. Démoclès, R. Piffaretti, G.W. Pratt, A. Catalano, G. Hurier, J.F. MacÍas-Pérez, C. Renault, B. Van Tent, G.F. Smoot, K. Dolag, T.A. Enßlin, C. Hernández-Monteagudo, W. Hovest, J. Knoche, M. Reinecke, R. Sunyaev, S.D.M. White, H. Böhringer, G. Chon, P.R. Christensen, P. Naselsky, B.P. Crill, G. Savini, C. Baccigalupi, G. De Zotti, J. González-Nuevo, S. Leach, F. Perrotta, R. Mann, P.A.R. Ade, D. Munshi, R. Sudiwala, R. Sunyaev, J. Borrill, S. Osborne, K. Benabed, F.R. Bouchet, S. Colombi, E. Hivon, S. Prunet, B.D. Wandelt, S. Mei, A.J. Banday, I. Flores-Cacho, O. Forni, D.J. Marshall, E. Pointecouteau, K. Dolag, J. Weller, E. Battaner, K.M. Huffenberger, K.M. Górski

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Abstract

We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. The candidates were selected using ancillary data flags derived from the ROSAT All Sky Survey (RASS) and Digitized Sky Survey all-sky maps, with the aim of pushing into the low SZ flux, high-z regime and testing RASS flags as indicators of candidate reliability. Fourteen new clusters were detected by XMM-Newton, ten single clusters and two double systems. Redshifts from X-ray spectroscopy lie in the range 0.2 to 0.9, with six clusters at z > 0.5. Estimated masses (M500) range from 2.5 × 1014 to 8 × 1014 MM·. We discuss our results in the context of the full XMM-Newton validation programme, in which 51 new clusters have been detected. This includes four double and two triple systems, some of which are chance projections on the sky of clusters at different redshifts. We find thatassociation with a source from the RASS-Bright Source Catalogue is a robust indicator of the reliability of a candidate, whereas association with a source from the RASS-Faint Source Catalogue does not guarantee that the SZ candidate is a bona fide cluster. Nevertheless, most Planck clusters appear in RASS maps, with a significance greater than 2σ being a good indication that the candidate is a real cluster. Candidate validation from association with SDSS galaxy overdensity at z > 0.5 is also discussed. The full sample gives a Planck sensitivity threshold of Y500 4 × 10-4 arcmin2, with indication for Malmquist bias in the Y X-Y500 relation below this threshold. The corresponding mass threshold depends on redshift. Systems with M500 > 5 × 1014 MM at z > 0.5 are easily detectable with Planck. The newly-detected clusters follow the YX-Y500 relation derived from X-ray selected samples. Compared to X-ray selected clusters, the new SZ clusters have a lower X-ray luminosity on average for their mass. There is no indication of departure from standard self-similar evolution in the X-ray versus SZ scaling properties. In particular, there is no significant evolution of the YX/Y500 ratio. © ESO, 2013.

Original language	English
Journal	Astronomy and Astrophysics
Volume	550
Pages (from-to)	A130
Number of pages	19
ISSN	0004-6361
DOIs	https://doi.org/10.1051/0004-6361/201219519
Publication status	Published - 2013

Keywords

Surveys
X ray spectroscopy
Galaxies

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10.1051/0004-6361/201219519

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Bartlett, J. G., Delabrouille, J., Ganga, K., Giraud-Héraud, Y., Le Jeune, M., Piat, M., Remazeilles, M., Rosset, C., Smoot, G. F., Poutanen, T., Bikmaev, I., Natoli, P., Polenta, G., Mandolesi, N., Ashdown, M., Carvalho, P., Hobson, M., Lasenby, A., Kneissl, R., ... Górski, K. M. (2013). Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters. Astronomy and Astrophysics, 550, A130. https://doi.org/10.1051/0004-6361/201219519

@article{bc87b6128eaf4bd8b15e47f39ae08fe3,

title = "Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters",

abstract = "We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. The candidates were selected using ancillary data flags derived from the ROSAT All Sky Survey (RASS) and Digitized Sky Survey all-sky maps, with the aim of pushing into the low SZ flux, high-z regime and testing RASS flags as indicators of candidate reliability. Fourteen new clusters were detected by XMM-Newton, ten single clusters and two double systems. Redshifts from X-ray spectroscopy lie in the range 0.2 to 0.9, with six clusters at z > 0.5. Estimated masses (M500) range from 2.5 × 1014 to 8 × 1014 MM·. We discuss our results in the context of the full XMM-Newton validation programme, in which 51 new clusters have been detected. This includes four double and two triple systems, some of which are chance projections on the sky of clusters at different redshifts. We find thatassociation with a source from the RASS-Bright Source Catalogue is a robust indicator of the reliability of a candidate, whereas association with a source from the RASS-Faint Source Catalogue does not guarantee that the SZ candidate is a bona fide cluster. Nevertheless, most Planck clusters appear in RASS maps, with a significance greater than 2σ being a good indication that the candidate is a real cluster. Candidate validation from association with SDSS galaxy overdensity at z > 0.5 is also discussed. The full sample gives a Planck sensitivity threshold of Y500 4 × 10-4 arcmin2, with indication for Malmquist bias in the Y X-Y500 relation below this threshold. The corresponding mass threshold depends on redshift. Systems with M500 > 5 × 1014 MM at z > 0.5 are easily detectable with Planck. The newly-detected clusters follow the YX-Y500 relation derived from X-ray selected samples. Compared to X-ray selected clusters, the new SZ clusters have a lower X-ray luminosity on average for their mass. There is no indication of departure from standard self-similar evolution in the X-ray versus SZ scaling properties. In particular, there is no significant evolution of the YX/Y500 ratio. {\textcopyright} ESO, 2013.",

keywords = "Surveys, X ray spectroscopy, Galaxies",

author = "J.G. Bartlett and J. Delabrouille and K. Ganga and Y. Giraud-H{\'e}raud and {Le Jeune}, M. and M. Piat and M. Remazeilles and C. Rosset and G.F. Smoot and T. Poutanen and I. Bikmaev and P. Natoli and G. Polenta and N. Mandolesi and M. Ashdown and P. Carvalho and M. Hobson and A. Lasenby and R. Kneissl and J.R. Bond and M.-A. Miville-Desch{\^e}nes and A.J. Banday and J.-P. Bernard and I. Flores-Cacho and O. Forni and D.J. Marshall and E. Pointecouteau and O. Dor{\'e} and S.R. Hildebrandt and S. Mei and G. Rocha and H. Dahle and P.B. Lilje and {Da Silva}, A. and C. Hern{\'a}ndez-Monteagudo and J. Borrill and J.-B. Melin and R. Piffaretti and D. Yvon and Allan Hornstrup and Michael Linden-V{\o}rnle and N{\o}rgaard-Nielsen, {Hans Ulrik} and M. Frommert and M. Kunz and L. Toffolatti and I. Bikmaev and D. Scott and E. Pierpaoli and A. Liddle and M. Juvela and H. Kurki-Suonio and T. Poutanen and A.-S. Suur-Uski and W.C. Jones and G.F. Smoot and L. Knox and A. Stanford and P.R. Meinhold and A. Zonca and B.D. Wandelt and L. Cay{\'o}n and S. Matarrese and {De Bernardis}, P. and S. Masi and A. Melchiorri and F. Nati and F. Piacentini and M. Bersanelli and D. Maino and A. Mennella and M. Rossetti and S. Borgani and A. Gregorio and C. Burigana and P. Natoli and A. Balbi and {De Gasperis}, G. and P. Mazzotta and N. Vittorio and P. Cabella and P.R. Christensen and P. Naselsky and A. Hempel and J.A. Rubi{\~n}o-Mart{\'i}n and R. Kneissl and R. Gonz{\'a}lez-Riestra and X. Dupac and T. Jagemann and R. Leonardi and L. Mendes and J.A. Tauber and S. Mei and H. Kurki-Suonio and T. Poutanen and A.-S. Suur-Uski and {De Zotti}, G. and S. Colafrancesco and G. Polenta and S. Borgani and M. Frailis and S. Galeotta and A. Gregorio and M. Maris and A. Zacchei and M. Massardi and C. Burigana and R.C. Butler and F. Cuttaia and F. Finelli and E. Franceschi and A. Gruppuso and N. Mandolesi and G. Morgante and P. Natoli and D. Paoletti and S. Ricciardi and M. Sandri and L. Terenzi and L. Valenziano and F. Villa and M. Bersanelli and S. Donzelli and D. Maino and A. Mennella and M. Rossetti and M. Tomasi and A. Melchiorri and F. Stivoli and F.-X. D{\'e}sert and S. Mitra and A. Chamballu and D.L. Clements and A.H. Jaffe and D. Mortlock and R.-R. Chary and B. Rusholme and A. Beno{\^i}t and H. Dole and N. Aghanim and J. Aumont and H. Dole and M. Douspis and M. Kunz and G. Lagache and M.-A. Miville-Desch{\^e}nes and F. Pajot and J.-L. Puget and M. Remazeilles and N. Welikala and K. Benabed and F.R. Bouchet and S. Colombi and E. Hivon and A. Moneti and S. Prunet and J.-F. Sygnet and B.D. Wandelt and L. Popa and F. Marleau and L.-Y. Chiang and D. Harrison and D. Sutton and H. Dahle and H.K. Eriksen and F.K. Hansen and P.B. Lilje and R.T. G{\'e}nova-Santos and A. Hempel and J.A. Rubi{\~n}o-Mart{\'i}n and R.B. Barreiro and J.M. Diego and J. Gonz{\'a}lez-Nuevo and D. Herranz and M. L{\'o}pez-Caniego and E. Mart{\'i}nez-Gonz{\'a}lez and L. Toffolatti and P. Vielva and P. Platania and J.G. Bartlett and B.P. Crill and O. Dor{\'e} and K.M. G{\'o}rski and W.A. Holmes and C.R. Lawrence and S. Mitra and G. Rocha and L.A. Wade and A. Bonaldi and M.L. Brown and R.J. Davis and F. Noviello and M. Ashdown and D. Harrison and A. Lasenby and D. Sutton and S. Henrot-Versill{\'e} and G. Luzzi and O. Perdereau and S. Plaszczynski and M. Tristram and A. Catalano and A. Coulais and J.-M. Lamarre and M. Arnaud and J. D{\'e}mocl{\`e}s and R. Piffaretti and G.W. Pratt and A. Catalano and G. Hurier and J.F. Mac{\'I}as-P{\'e}rez and C. Renault and {Van Tent}, B. and G.F. Smoot and K. Dolag and T.A. En{\ss}lin and C. Hern{\'a}ndez-Monteagudo and W. Hovest and J. Knoche and M. Reinecke and R. Sunyaev and S.D.M. White and H. B{\"o}hringer and G. Chon and P.R. Christensen and P. Naselsky and B.P. Crill and G. Savini and C. Baccigalupi and {De Zotti}, G. and J. Gonz{\'a}lez-Nuevo and S. Leach and F. Perrotta and R. Mann and P.A.R. Ade and D. Munshi and R. Sudiwala and R. Sunyaev and J. Borrill and S. Osborne and K. Benabed and F.R. Bouchet and S. Colombi and E. Hivon and S. Prunet and B.D. Wandelt and S. Mei and A.J. Banday and I. Flores-Cacho and O. Forni and D.J. Marshall and E. Pointecouteau and K. Dolag and J. Weller and E. Battaner and K.M. Huffenberger and K.M. G{\'o}rski",

year = "2013",

doi = "10.1051/0004-6361/201219519",

language = "English",

volume = "550",

pages = "A130",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Bartlett, JG, Delabrouille, J, Ganga, K, Giraud-Héraud, Y, Le Jeune, M, Piat, M, Remazeilles, M, Rosset, C, Smoot, GF, Poutanen, T, Bikmaev, I, Natoli, P, Polenta, G, Mandolesi, N, Ashdown, M, Carvalho, P, Hobson, M, Lasenby, A, Kneissl, R, Bond, JR, Miville-Deschênes, M-A, Banday, AJ, Bernard, J-P, Flores-Cacho, I, Forni, O, Marshall, DJ, Pointecouteau, E, Doré, O, Hildebrandt, SR, Mei, S, Rocha, G, Dahle, H, Lilje, PB, Da Silva, A, Hernández-Monteagudo, C, Borrill, J, Melin, J-B, Piffaretti, R, Yvon, D, Hornstrup, A , Linden-Vørnle, M, Nørgaard-Nielsen, HU, Frommert, M, Kunz, M, Toffolatti, L, Bikmaev, I, Scott, D, Pierpaoli, E, Liddle, A, Juvela, M, Kurki-Suonio, H, Poutanen, T, Suur-Uski, A-S, Jones, WC, Smoot, GF, Knox, L, Stanford, A, Meinhold, PR, Zonca, A, Wandelt, BD, Cayón, L, Matarrese, S, De Bernardis, P, Masi, S, Melchiorri, A, Nati, F, Piacentini, F, Bersanelli, M, Maino, D, Mennella, A, Rossetti, M, Borgani, S, Gregorio, A, Burigana, C, Natoli, P, Balbi, A, De Gasperis, G, Mazzotta, P, Vittorio, N, Cabella, P, Christensen, PR, Naselsky, P, Hempel, A, Rubiño-Martín, JA, Kneissl, R, González-Riestra, R, Dupac, X, Jagemann, T, Leonardi, R, Mendes, L, Tauber, JA, Mei, S, Kurki-Suonio, H, Poutanen, T, Suur-Uski, A-S, De Zotti, G, Colafrancesco, S, Polenta, G, Borgani, S, Frailis, M, Galeotta, S, Gregorio, A, Maris, M, Zacchei, A, Massardi, M, Burigana, C, Butler, RC, Cuttaia, F, Finelli, F, Franceschi, E, Gruppuso, A, Mandolesi, N, Morgante, G, Natoli, P, Paoletti, D, Ricciardi, S, Sandri, M, Terenzi, L, Valenziano, L, Villa, F, Bersanelli, M, Donzelli, S, Maino, D, Mennella, A, Rossetti, M, Tomasi, M, Melchiorri, A, Stivoli, F, Désert, F-X, Mitra, S, Chamballu, A, Clements, DL, Jaffe, AH, Mortlock, D, Chary, R-R, Rusholme, B, Benoît, A, Dole, H, Aghanim, N, Aumont, J, Dole, H, Douspis, M, Kunz, M, Lagache, G, Miville-Deschênes, M-A, Pajot, F, Puget, J-L, Remazeilles, M, Welikala, N, Benabed, K, Bouchet, FR, Colombi, S, Hivon, E, Moneti, A, Prunet, S, Sygnet, J-F, Wandelt, BD, Popa, L, Marleau, F, Chiang, L-Y, Harrison, D, Sutton, D, Dahle, H, Eriksen, HK, Hansen, FK, Lilje, PB, Génova-Santos, RT, Hempel, A, Rubiño-Martín, JA, Barreiro, RB, Diego, JM, González-Nuevo, J, Herranz, D, López-Caniego, M, Martínez-González, E, Toffolatti, L, Vielva, P, Platania, P, Bartlett, JG, Crill, BP, Doré, O, Górski, KM, Holmes, WA, Lawrence, CR, Mitra, S, Rocha, G, Wade, LA, Bonaldi, A, Brown, ML, Davis, RJ, Noviello, F, Ashdown, M, Harrison, D, Lasenby, A, Sutton, D, Henrot-Versillé, S, Luzzi, G, Perdereau, O, Plaszczynski, S, Tristram, M, Catalano, A, Coulais, A, Lamarre, J-M, Arnaud, M, Démoclès, J, Piffaretti, R, Pratt, GW, Catalano, A, Hurier, G, MacÍas-Pérez, JF, Renault, C, Van Tent, B, Smoot, GF, Dolag, K, Enßlin, TA, Hernández-Monteagudo, C, Hovest, W, Knoche, J, Reinecke, M, Sunyaev, R, White, SDM, Böhringer, H, Chon, G, Christensen, PR, Naselsky, P, Crill, BP, Savini, G, Baccigalupi, C, De Zotti, G, González-Nuevo, J, Leach, S, Perrotta, F, Mann, R, Ade, PAR, Munshi, D, Sudiwala, R, Sunyaev, R, Borrill, J, Osborne, S, Benabed, K, Bouchet, FR, Colombi, S, Hivon, E, Prunet, S, Wandelt, BD, Mei, S, Banday, AJ, Flores-Cacho, I, Forni, O, Marshall, DJ, Pointecouteau, E, Dolag, K, Weller, J, Battaner, E, Huffenberger, KM & Górski, KM 2013, 'Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters', Astronomy and Astrophysics, vol. 550, pp. A130. https://doi.org/10.1051/0004-6361/201219519

TY - JOUR

T1 - Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters

AU - Bartlett, J.G.

AU - Delabrouille, J.

AU - Ganga, K.

AU - Giraud-Héraud, Y.

AU - Le Jeune, M.

AU - Piat, M.

AU - Remazeilles, M.

AU - Rosset, C.

AU - Smoot, G.F.

AU - Poutanen, T.

AU - Bikmaev, I.

AU - Natoli, P.

AU - Polenta, G.

AU - Mandolesi, N.

AU - Ashdown, M.

AU - Carvalho, P.

AU - Hobson, M.

AU - Lasenby, A.

AU - Kneissl, R.

AU - Bond, J.R.

AU - Miville-Deschênes, M.-A.

AU - Banday, A.J.

AU - Bernard, J.-P.

AU - Flores-Cacho, I.

AU - Forni, O.

AU - Marshall, D.J.

AU - Pointecouteau, E.

AU - Doré, O.

AU - Hildebrandt, S.R.

AU - Mei, S.

AU - Rocha, G.

AU - Dahle, H.

AU - Lilje, P.B.

AU - Da Silva, A.

AU - Hernández-Monteagudo, C.

AU - Borrill, J.

AU - Melin, J.-B.

AU - Piffaretti, R.

AU - Yvon, D.

AU - Hornstrup, Allan

AU - Linden-Vørnle, Michael

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Frommert, M.

AU - Kunz, M.

AU - Toffolatti, L.

AU - Bikmaev, I.

AU - Scott, D.

AU - Pierpaoli, E.

AU - Liddle, A.

AU - Juvela, M.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Suur-Uski, A.-S.

AU - Jones, W.C.

AU - Smoot, G.F.

AU - Knox, L.

AU - Stanford, A.

AU - Meinhold, P.R.

AU - Zonca, A.

AU - Wandelt, B.D.

AU - Cayón, L.

AU - Matarrese, S.

AU - De Bernardis, P.

AU - Masi, S.

AU - Melchiorri, A.

AU - Nati, F.

AU - Piacentini, F.

AU - Bersanelli, M.

AU - Maino, D.

AU - Mennella, A.

AU - Rossetti, M.

AU - Borgani, S.

AU - Gregorio, A.

AU - Burigana, C.

AU - Natoli, P.

AU - Balbi, A.

AU - De Gasperis, G.

AU - Mazzotta, P.

AU - Vittorio, N.

AU - Cabella, P.

AU - Christensen, P.R.

AU - Naselsky, P.

AU - Hempel, A.

AU - Rubiño-Martín, J.A.

AU - Kneissl, R.

AU - González-Riestra, R.

AU - Dupac, X.

AU - Jagemann, T.

AU - Leonardi, R.

AU - Mendes, L.

AU - Tauber, J.A.

AU - Mei, S.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Suur-Uski, A.-S.

AU - De Zotti, G.

AU - Colafrancesco, S.

AU - Polenta, G.

AU - Borgani, S.

AU - Frailis, M.

AU - Galeotta, S.

AU - Gregorio, A.

AU - Maris, M.

AU - Zacchei, A.

AU - Massardi, M.

AU - Burigana, C.

AU - Butler, R.C.

AU - Cuttaia, F.

AU - Finelli, F.

AU - Franceschi, E.

AU - Gruppuso, A.

AU - Mandolesi, N.

AU - Morgante, G.

AU - Natoli, P.

AU - Paoletti, D.

AU - Ricciardi, S.

AU - Sandri, M.

AU - Terenzi, L.

AU - Valenziano, L.

AU - Villa, F.

AU - Bersanelli, M.

AU - Donzelli, S.

AU - Maino, D.

AU - Mennella, A.

AU - Rossetti, M.

AU - Tomasi, M.

AU - Melchiorri, A.

AU - Stivoli, F.

AU - Désert, F.-X.

AU - Mitra, S.

AU - Chamballu, A.

AU - Clements, D.L.

AU - Jaffe, A.H.

AU - Mortlock, D.

AU - Chary, R.-R.

AU - Rusholme, B.

AU - Benoît, A.

AU - Dole, H.

AU - Aghanim, N.

AU - Aumont, J.

AU - Dole, H.

AU - Douspis, M.

AU - Kunz, M.

AU - Lagache, G.

AU - Miville-Deschênes, M.-A.

AU - Pajot, F.

AU - Puget, J.-L.

AU - Remazeilles, M.

AU - Welikala, N.

AU - Benabed, K.

AU - Bouchet, F.R.

AU - Colombi, S.

AU - Hivon, E.

AU - Moneti, A.

AU - Prunet, S.

AU - Sygnet, J.-F.

AU - Wandelt, B.D.

AU - Popa, L.

AU - Marleau, F.

AU - Chiang, L.-Y.

AU - Harrison, D.

AU - Sutton, D.

AU - Dahle, H.

AU - Eriksen, H.K.

AU - Hansen, F.K.

AU - Lilje, P.B.

AU - Génova-Santos, R.T.

AU - Hempel, A.

AU - Rubiño-Martín, J.A.

AU - Barreiro, R.B.

AU - Diego, J.M.

AU - González-Nuevo, J.

AU - Herranz, D.

AU - López-Caniego, M.

AU - Martínez-González, E.

AU - Toffolatti, L.

AU - Vielva, P.

AU - Platania, P.

AU - Bartlett, J.G.

AU - Crill, B.P.

AU - Doré, O.

AU - Górski, K.M.

AU - Holmes, W.A.

AU - Lawrence, C.R.

AU - Mitra, S.

AU - Rocha, G.

AU - Wade, L.A.

AU - Bonaldi, A.

AU - Brown, M.L.

AU - Davis, R.J.

AU - Noviello, F.

AU - Ashdown, M.

AU - Harrison, D.

AU - Lasenby, A.

AU - Sutton, D.

AU - Henrot-Versillé, S.

AU - Luzzi, G.

AU - Perdereau, O.

AU - Plaszczynski, S.

AU - Tristram, M.

AU - Catalano, A.

AU - Coulais, A.

AU - Lamarre, J.-M.

AU - Arnaud, M.

AU - Démoclès, J.

AU - Piffaretti, R.

AU - Pratt, G.W.

AU - Catalano, A.

AU - Hurier, G.

AU - MacÍas-Pérez, J.F.

AU - Renault, C.

AU - Van Tent, B.

AU - Smoot, G.F.

AU - Dolag, K.

AU - Enßlin, T.A.

AU - Hernández-Monteagudo, C.

AU - Hovest, W.

AU - Knoche, J.

AU - Reinecke, M.

AU - Sunyaev, R.

AU - White, S.D.M.

AU - Böhringer, H.

AU - Chon, G.

AU - Christensen, P.R.

AU - Naselsky, P.

AU - Crill, B.P.

AU - Savini, G.

AU - Baccigalupi, C.

AU - De Zotti, G.

AU - González-Nuevo, J.

AU - Leach, S.

AU - Perrotta, F.

AU - Mann, R.

AU - Ade, P.A.R.

AU - Munshi, D.

AU - Sudiwala, R.

AU - Sunyaev, R.

AU - Borrill, J.

AU - Osborne, S.

AU - Benabed, K.

AU - Bouchet, F.R.

AU - Colombi, S.

AU - Hivon, E.

AU - Prunet, S.

AU - Wandelt, B.D.

AU - Mei, S.

AU - Banday, A.J.

AU - Flores-Cacho, I.

AU - Forni, O.

AU - Marshall, D.J.

AU - Pointecouteau, E.

AU - Dolag, K.

AU - Weller, J.

AU - Battaner, E.

AU - Huffenberger, K.M.

AU - Górski, K.M.

PY - 2013

Y1 - 2013

N2 - We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. The candidates were selected using ancillary data flags derived from the ROSAT All Sky Survey (RASS) and Digitized Sky Survey all-sky maps, with the aim of pushing into the low SZ flux, high-z regime and testing RASS flags as indicators of candidate reliability. Fourteen new clusters were detected by XMM-Newton, ten single clusters and two double systems. Redshifts from X-ray spectroscopy lie in the range 0.2 to 0.9, with six clusters at z > 0.5. Estimated masses (M500) range from 2.5 × 1014 to 8 × 1014 MM·. We discuss our results in the context of the full XMM-Newton validation programme, in which 51 new clusters have been detected. This includes four double and two triple systems, some of which are chance projections on the sky of clusters at different redshifts. We find thatassociation with a source from the RASS-Bright Source Catalogue is a robust indicator of the reliability of a candidate, whereas association with a source from the RASS-Faint Source Catalogue does not guarantee that the SZ candidate is a bona fide cluster. Nevertheless, most Planck clusters appear in RASS maps, with a significance greater than 2σ being a good indication that the candidate is a real cluster. Candidate validation from association with SDSS galaxy overdensity at z > 0.5 is also discussed. The full sample gives a Planck sensitivity threshold of Y500 4 × 10-4 arcmin2, with indication for Malmquist bias in the Y X-Y500 relation below this threshold. The corresponding mass threshold depends on redshift. Systems with M500 > 5 × 1014 MM at z > 0.5 are easily detectable with Planck. The newly-detected clusters follow the YX-Y500 relation derived from X-ray selected samples. Compared to X-ray selected clusters, the new SZ clusters have a lower X-ray luminosity on average for their mass. There is no indication of departure from standard self-similar evolution in the X-ray versus SZ scaling properties. In particular, there is no significant evolution of the YX/Y500 ratio. © ESO, 2013.

AB - We present the final results from the XMM-Newton validation follow-up of new Planck galaxy cluster candidates. We observed 15 new candidates, detected with signal-to-noise ratios between 4.0 and 6.1 in the 15.5-month nominal Planck survey. The candidates were selected using ancillary data flags derived from the ROSAT All Sky Survey (RASS) and Digitized Sky Survey all-sky maps, with the aim of pushing into the low SZ flux, high-z regime and testing RASS flags as indicators of candidate reliability. Fourteen new clusters were detected by XMM-Newton, ten single clusters and two double systems. Redshifts from X-ray spectroscopy lie in the range 0.2 to 0.9, with six clusters at z > 0.5. Estimated masses (M500) range from 2.5 × 1014 to 8 × 1014 MM·. We discuss our results in the context of the full XMM-Newton validation programme, in which 51 new clusters have been detected. This includes four double and two triple systems, some of which are chance projections on the sky of clusters at different redshifts. We find thatassociation with a source from the RASS-Bright Source Catalogue is a robust indicator of the reliability of a candidate, whereas association with a source from the RASS-Faint Source Catalogue does not guarantee that the SZ candidate is a bona fide cluster. Nevertheless, most Planck clusters appear in RASS maps, with a significance greater than 2σ being a good indication that the candidate is a real cluster. Candidate validation from association with SDSS galaxy overdensity at z > 0.5 is also discussed. The full sample gives a Planck sensitivity threshold of Y500 4 × 10-4 arcmin2, with indication for Malmquist bias in the Y X-Y500 relation below this threshold. The corresponding mass threshold depends on redshift. Systems with M500 > 5 × 1014 MM at z > 0.5 are easily detectable with Planck. The newly-detected clusters follow the YX-Y500 relation derived from X-ray selected samples. Compared to X-ray selected clusters, the new SZ clusters have a lower X-ray luminosity on average for their mass. There is no indication of departure from standard self-similar evolution in the X-ray versus SZ scaling properties. In particular, there is no significant evolution of the YX/Y500 ratio. © ESO, 2013.

KW - Surveys

KW - X ray spectroscopy

KW - Galaxies

U2 - 10.1051/0004-6361/201219519

DO - 10.1051/0004-6361/201219519

M3 - Journal article

SN - 0004-6361

VL - 550

SP - A130

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

ER -

Planck intermediate results: IV. the XMM-Newton validation programme for new Planck galaxy clusters

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