Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies

T. Poutanen, P. Natoli, G. Polenta, J.G. Bartlett, M. Bucher, J.-F. Cardoso, A. Catalano, J. Delabrouille, K. Ganga, Y. Giraud-Héraud, G. Patanchon, M. Piat, M. Remazeilles, C. Rosset, G.F. Smoot, R. Stompor, M. Ashdown, M. Hobson, A. Lasenby, V. StolyarovR. Bhatia, R. Kneissl, L. Bonavera, K. Blagrave, J.R. Bond, P. Martin, M.-A. Miville-Deschênes, A.J. Banday, J.-P. Bernard, O. Forni, M. Giard, C. Leroy, L. Montier, E. Pointecouteau, I. Ristorcelli, J.J. Bock, O. Doré, G. Helou, S.R. Hildebrandt, G. Prézeau, G. Rocha, M.D. Seiffert, P.B. Lilje, A. Challinor, P. Shellard, J.-L. Starck, D. Yvon, Michael Linden-Vørnle, Hans Ulrik Nørgaard-Nielsen, L. Toffolatti, C.B. Netterfield, D. Pinheiro Gonçalves, D. Scott, S. Oliver, M. Juvela, E. Keihänen, R. Keskitalo, H. Kurki-Suonio, T. Poutanen, C. Chiang, W.C. Jones, L. Cayón, G.F. Smoot, M. White, L. Knox, R. Leonardi, P.M. Lubin, A. Zonca, B.D. Wandelt, S. Matarrese, P. De Bernardis, S. Masi, A. Melchiorri, F. Piacentini, M. Bersanelli, D. Maino, A. Mennella, M. Tomasi, A. Gregorio, P. Natoli, A. Balbi, P. Cabella, G. De Gasperis, P. Mazzotta, N. Vittorio, P.R. Christensen, P. Naselsky, J.A. Rubiño-Martín, R. Kneissl, X. Dupac, R. Leonardi, L. Mendes, G. Giardino, R.J. Laureijs, R. Leonardi, J.A. Tauber, H. Kurki-Suonio, T. Poutanen, G. Umana, A. Bonaldi, G. De Zotti, G. Polenta, M. Frailis, S. Galeotta, M. Maris, A. Mennella, F. Pasian, A. Zacchei, C. Burigana, F. Cuttaia, A. De Rosa, F. Finelli, E. Franceschi, A. Gruppuso, N. Mandolesi, G. Morgante, P. Natoli, S. Ricciardi, M. Sandri, L. Terenzi, L. Valenziano, F. Villa, M. Bersanelli, S. Donzelli, D. Maino, M. Tomasi, F. Stivoli, F.-X. Désert, A. Chamballu, D.L. Clements, A.H. Jaffe, D. Mortlock, D. Novikov, M. Rowan-Robinson, K. Ganga, B. Rusholme, A. Benoît, N. Aghanim, J. Aumont, H. Dole, M. Douspis, J. Grain, G. Lagache, C. Leroy, M.-A. Miville-Deschênes, F. Pajot, N. Ponthieu, J.-L. Puget, J.-P. Torre, K. Benabed, F.R. Bouchet, J.-F. Cardoso, S. Colombi, J.-M. Delouis, E. Hivon, A. Moneti, S. Prunet, J.-F. Sygnet, B.D. Wandelt, P. Fosalba, L.-Y. Chiang, A. Challinor, G. Efstathiou, S. Gratton, D. Harrison, D. Munshi, S. Donzelli, H.K. Eriksen, F.K. Hansen, P.B. Lilje, S.R. Hildebrandt, R.J. Hoyland, J.A. Rubiño-Martín, R.B. Barreiro, D. Herranz, M. López-Caniego, E. Martínez-González, P. Vielva, J.G. Bartlett, J.J. Bock, B.P. Crill, O. Doré, K.M. Górski, W.A. Holmes, R. Keskitalo, C.R. Lawrence, S. Mitra, I.J. O'Dwyer, G. Prézeau, G. Rocha, M.D. Seiffert, L.A. Wade, R.D. Davies, R.J. Davis, B. Maffei, M. Ashdown, A. Challinor, S. Gratton, D. Harrison, A. Lasenby, C.J. MacTavish, A. Catalano, A. Coulais, J.-M. Lamarre, M. Arnaud, J.-L. Starck, J.-F. Cardoso, S.R. Hildebrandt, J.F. MacÍas-Pérez, L. Perotto, C. Renault, D. Santos, F. Couchot, S. Henrot-Versillé, O. Perdereau, S. Plaszczynski, M. Tristram, J. Borrill, T.S. Kisner, G.F. Smoot, A.J. Banday, U. Dörl, T.A. Enßlin, W. Hovest, F. Matthai, J.P. Rachen, M. Reinecke, T. Riller, R. Sunyaev, J. Tuovinen, F.J. Lockman, A. Murphy, P.R. Christensen, P. Naselsky, I. Novikov, B.P. Crill, G. Savini, C. Baccigalupi, L. Bonavera, L. Danese, 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, A.J. Banday, J.-P. Bernard, O. Forni, M. Giard, C. Leroy, L. Montier, E. Pointecouteau, I. Ristorcelli, W.T. Reach, E. Battaner, K.M. Huffenberger, K.M. Górski

Research output: Contribution to journalJournal articleResearchpeer-review

Abstract

Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg2, we determine the angular power spectra of cosmic infrared background (CIB) anisotropies from multipole = 200 to = 2000 at 217, 353, 545 and 857 GHz. We use 21-cm observations of Hi as a tracer of thermal dust emission to reduce the already low level of Galactic dust emission and use the 143 GHz Planck maps in these fields to clean out cosmic microwave background anisotropies. Both of these cleaning processes are necessary to avoid significant contamination of the CIB signal. We measure correlated CIB structure across frequencies. As expected, the correlation decreases with increasing frequency separation, because the contribution of high-redshift galaxies to CIB anisotropies increases with wavelengths. We find no significant difference between the frequency spectrum of the CIB anisotropies and the CIB mean, with ΔI / I = 15% from 217 to 857 GHz. In terms of clustering properties, the Planck data alone rule out the linear scale- and redshift-independent bias model. Non-linear corrections are significant. Consequently, we develop an alternative model that couples a dusty galaxy, parametric evolution model with a simple halo-model approach. It provides an excellent fit to the measured anisotropy angular power spectra and suggests that a different halo occupation distribution is required at each frequency, which is consistent with our expectation that each frequency is dominated by contributions from different redshifts. In our best-fit model, half of the anisotropy power at = 2000 comes from redshifts z <0.8 at 857 GHz and z <1.5 at 545 GHz, while about 90% come from redshifts z > 2 at 353 and 217 GHz, respectively. © ESO, 2011.
Original languageEnglish
JournalAstronomy & Astrophysics
Volume536
Pages (from-to)A18
ISSN0004-6361
DOIs
Publication statusPublished - 2011

Cite this

Poutanen, T., Natoli, P., Polenta, G., Bartlett, J. G., Bucher, M., Cardoso, J-F., ... Górski, K. M. (2011). Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies. Astronomy & Astrophysics, 536, A18. https://doi.org/10.1051/0004-6361/201116461
Poutanen, T. ; Natoli, P. ; Polenta, G. ; Bartlett, J.G. ; Bucher, M. ; Cardoso, J.-F. ; Catalano, A. ; Delabrouille, J. ; Ganga, K. ; Giraud-Héraud, Y. ; Patanchon, G. ; Piat, M. ; Remazeilles, M. ; Rosset, C. ; Smoot, G.F. ; Stompor, R. ; Ashdown, M. ; Hobson, M. ; Lasenby, A. ; Stolyarov, V. ; Bhatia, R. ; Kneissl, R. ; Bonavera, L. ; Blagrave, K. ; Bond, J.R. ; Martin, P. ; Miville-Deschênes, M.-A. ; Banday, A.J. ; Bernard, J.-P. ; Forni, O. ; Giard, M. ; Leroy, C. ; Montier, L. ; Pointecouteau, E. ; Ristorcelli, I. ; Bock, J.J. ; Doré, O. ; Helou, G. ; Hildebrandt, S.R. ; Prézeau, G. ; Rocha, G. ; Seiffert, M.D. ; Lilje, P.B. ; Challinor, A. ; Shellard, P. ; Starck, J.-L. ; Yvon, D. ; Linden-Vørnle, Michael ; Nørgaard-Nielsen, Hans Ulrik ; Toffolatti, L. ; Netterfield, C.B. ; Pinheiro Gonçalves, D. ; Scott, D. ; Oliver, S. ; Juvela, M. ; Keihänen, E. ; Keskitalo, R. ; Kurki-Suonio, H. ; Poutanen, T. ; Chiang, C. ; Jones, W.C. ; Cayón, L. ; Smoot, G.F. ; White, M. ; Knox, L. ; Leonardi, R. ; Lubin, P.M. ; Zonca, A. ; Wandelt, B.D. ; Matarrese, S. ; De Bernardis, P. ; Masi, S. ; Melchiorri, A. ; Piacentini, F. ; Bersanelli, M. ; Maino, D. ; Mennella, A. ; Tomasi, M. ; Gregorio, A. ; Natoli, P. ; Balbi, A. ; Cabella, P. ; De Gasperis, G. ; Mazzotta, P. ; Vittorio, N. ; Christensen, P.R. ; Naselsky, P. ; Rubiño-Martín, J.A. ; Kneissl, R. ; Dupac, X. ; Leonardi, R. ; Mendes, L. ; Giardino, G. ; Laureijs, R.J. ; Leonardi, R. ; Tauber, J.A. ; Kurki-Suonio, H. ; Poutanen, T. ; Umana, G. ; Bonaldi, A. ; De Zotti, G. ; Polenta, G. ; Frailis, M. ; Galeotta, S. ; Maris, M. ; Mennella, A. ; Pasian, F. ; Zacchei, A. ; Burigana, C. ; Cuttaia, F. ; De Rosa, A. ; Finelli, F. ; Franceschi, E. ; Gruppuso, A. ; Mandolesi, N. ; Morgante, G. ; Natoli, P. ; Ricciardi, S. ; Sandri, M. ; Terenzi, L. ; Valenziano, L. ; Villa, F. ; Bersanelli, M. ; Donzelli, S. ; Maino, D. ; Tomasi, M. ; Stivoli, F. ; Désert, F.-X. ; Chamballu, A. ; Clements, D.L. ; Jaffe, A.H. ; Mortlock, D. ; Novikov, D. ; Rowan-Robinson, M. ; Ganga, K. ; Rusholme, B. ; Benoît, A. ; Aghanim, N. ; Aumont, J. ; Dole, H. ; Douspis, M. ; Grain, J. ; Lagache, G. ; Leroy, C. ; Miville-Deschênes, M.-A. ; Pajot, F. ; Ponthieu, N. ; Puget, J.-L. ; Torre, J.-P. ; Benabed, K. ; Bouchet, F.R. ; Cardoso, J.-F. ; Colombi, S. ; Delouis, J.-M. ; Hivon, E. ; Moneti, A. ; Prunet, S. ; Sygnet, J.-F. ; Wandelt, B.D. ; Fosalba, P. ; Chiang, L.-Y. ; Challinor, A. ; Efstathiou, G. ; Gratton, S. ; Harrison, D. ; Munshi, D. ; Donzelli, S. ; Eriksen, H.K. ; Hansen, F.K. ; Lilje, P.B. ; Hildebrandt, S.R. ; Hoyland, R.J. ; Rubiño-Martín, J.A. ; Barreiro, R.B. ; Herranz, D. ; López-Caniego, M. ; Martínez-González, E. ; Vielva, P. ; Bartlett, J.G. ; Bock, J.J. ; Crill, B.P. ; Doré, O. ; Górski, K.M. ; Holmes, W.A. ; Keskitalo, R. ; Lawrence, C.R. ; Mitra, S. ; O'Dwyer, I.J. ; Prézeau, G. ; Rocha, G. ; Seiffert, M.D. ; Wade, L.A. ; Davies, R.D. ; Davis, R.J. ; Maffei, B. ; Ashdown, M. ; Challinor, A. ; Gratton, S. ; Harrison, D. ; Lasenby, A. ; MacTavish, C.J. ; Catalano, A. ; Coulais, A. ; Lamarre, J.-M. ; Arnaud, M. ; Starck, J.-L. ; Cardoso, J.-F. ; Hildebrandt, S.R. ; MacÍas-Pérez, J.F. ; Perotto, L. ; Renault, C. ; Santos, D. ; Couchot, F. ; Henrot-Versillé, S. ; Perdereau, O. ; Plaszczynski, S. ; Tristram, M. ; Borrill, J. ; Kisner, T.S. ; Smoot, G.F. ; Banday, A.J. ; Dörl, U. ; Enßlin, T.A. ; Hovest, W. ; Matthai, F. ; Rachen, J.P. ; Reinecke, M. ; Riller, T. ; Sunyaev, R. ; Tuovinen, J. ; Lockman, F.J. ; Murphy, A. ; Christensen, P.R. ; Naselsky, P. ; Novikov, I. ; Crill, B.P. ; Savini, G. ; Baccigalupi, C. ; Bonavera, L. ; Danese, L. ; De Zotti, G. ; González-Nuevo, J. ; Leach, S. ; Perrotta, F. ; Mann, R. ; Ade, P.A.R. ; Munshi, D. ; Sudiwala, R. ; Sunyaev, R. ; Borrill, J. ; Osborne, S. ; Banday, A.J. ; Bernard, J.-P. ; Forni, O. ; Giard, M. ; Leroy, C. ; Montier, L. ; Pointecouteau, E. ; Ristorcelli, I. ; Reach, W.T. ; Battaner, E. ; Huffenberger, K.M. ; Górski, K.M. / Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies. In: Astronomy & Astrophysics. 2011 ; Vol. 536. pp. A18.
@article{0c5ff95b44b14d358f5434b87edc448f,
title = "Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies",
abstract = "Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg2, we determine the angular power spectra of cosmic infrared background (CIB) anisotropies from multipole = 200 to = 2000 at 217, 353, 545 and 857 GHz. We use 21-cm observations of Hi as a tracer of thermal dust emission to reduce the already low level of Galactic dust emission and use the 143 GHz Planck maps in these fields to clean out cosmic microwave background anisotropies. Both of these cleaning processes are necessary to avoid significant contamination of the CIB signal. We measure correlated CIB structure across frequencies. As expected, the correlation decreases with increasing frequency separation, because the contribution of high-redshift galaxies to CIB anisotropies increases with wavelengths. We find no significant difference between the frequency spectrum of the CIB anisotropies and the CIB mean, with ΔI / I = 15{\%} from 217 to 857 GHz. In terms of clustering properties, the Planck data alone rule out the linear scale- and redshift-independent bias model. Non-linear corrections are significant. Consequently, we develop an alternative model that couples a dusty galaxy, parametric evolution model with a simple halo-model approach. It provides an excellent fit to the measured anisotropy angular power spectra and suggests that a different halo occupation distribution is required at each frequency, which is consistent with our expectation that each frequency is dominated by contributions from different redshifts. In our best-fit model, half of the anisotropy power at = 2000 comes from redshifts z <0.8 at 857 GHz and z <1.5 at 545 GHz, while about 90{\%} come from redshifts z > 2 at 353 and 217 GHz, respectively. {\circledC} ESO, 2011.",
author = "T. Poutanen and P. Natoli and G. Polenta and J.G. Bartlett and M. Bucher and J.-F. Cardoso and A. Catalano and J. Delabrouille and K. Ganga and Y. Giraud-Héraud and G. Patanchon and M. Piat and M. Remazeilles and C. Rosset and G.F. Smoot and R. Stompor and M. Ashdown and M. Hobson and A. Lasenby and V. Stolyarov and R. Bhatia and R. Kneissl and L. Bonavera and K. Blagrave and J.R. Bond and P. Martin and M.-A. Miville-Deschênes and A.J. Banday and J.-P. Bernard and O. Forni and M. Giard and C. Leroy and L. Montier and E. Pointecouteau and I. Ristorcelli and J.J. Bock and O. Doré and G. Helou and S.R. Hildebrandt and G. Prézeau and G. Rocha and M.D. Seiffert and P.B. Lilje and A. Challinor and P. Shellard and J.-L. Starck and D. Yvon and Michael Linden-V{\o}rnle and N{\o}rgaard-Nielsen, {Hans Ulrik} and L. Toffolatti and C.B. Netterfield and {Pinheiro Gonçalves}, D. and D. Scott and S. Oliver and M. Juvela and E. Keihänen and R. Keskitalo and H. Kurki-Suonio and T. Poutanen and C. Chiang and W.C. Jones and L. Cayón and G.F. Smoot and M. White and L. Knox and R. Leonardi and P.M. Lubin and A. Zonca and B.D. Wandelt and S. Matarrese and {De Bernardis}, P. and S. Masi and A. Melchiorri and F. Piacentini and M. Bersanelli and D. Maino and A. Mennella and M. Tomasi and A. Gregorio and P. Natoli and A. Balbi and P. Cabella and {De Gasperis}, G. and P. Mazzotta and N. Vittorio and P.R. Christensen and P. Naselsky and J.A. Rubiño-Martín and R. Kneissl and X. Dupac and R. Leonardi and L. Mendes and G. Giardino and R.J. Laureijs and R. Leonardi and J.A. Tauber and H. Kurki-Suonio and T. Poutanen and G. Umana and A. Bonaldi and {De Zotti}, G. and G. Polenta and M. Frailis and S. Galeotta and M. Maris and A. Mennella and F. Pasian and A. Zacchei and C. Burigana and F. Cuttaia and {De Rosa}, A. and F. Finelli and E. Franceschi and A. Gruppuso and N. Mandolesi and G. Morgante and P. Natoli 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 M. Tomasi and F. Stivoli and F.-X. Désert and A. Chamballu and D.L. Clements and A.H. Jaffe and D. Mortlock and D. Novikov and M. Rowan-Robinson and K. Ganga and B. Rusholme and A. Benoît and N. Aghanim and J. Aumont and H. Dole and M. Douspis and J. Grain and G. Lagache and C. Leroy and M.-A. Miville-Deschênes and F. Pajot and N. Ponthieu and J.-L. Puget and J.-P. Torre and K. Benabed and F.R. Bouchet and J.-F. Cardoso and S. Colombi and J.-M. Delouis and E. Hivon and A. Moneti and S. Prunet and J.-F. Sygnet and B.D. Wandelt and P. Fosalba and L.-Y. Chiang and A. Challinor and G. Efstathiou and S. Gratton and D. Harrison and D. Munshi and S. Donzelli and H.K. Eriksen and F.K. Hansen and P.B. Lilje and S.R. Hildebrandt and R.J. Hoyland and J.A. Rubiño-Martín and R.B. Barreiro and D. Herranz and M. López-Caniego and E. Martínez-González and P. Vielva and J.G. Bartlett and J.J. Bock and B.P. Crill and O. Doré and K.M. Górski and W.A. Holmes and R. Keskitalo and C.R. Lawrence and S. Mitra and I.J. O'Dwyer and G. Prézeau and G. Rocha and M.D. Seiffert and L.A. Wade and R.D. Davies and R.J. Davis and B. Maffei and M. Ashdown and A. Challinor and S. Gratton and D. Harrison and A. Lasenby and C.J. MacTavish and A. Catalano and A. Coulais and J.-M. Lamarre and M. Arnaud and J.-L. Starck and J.-F. Cardoso and S.R. Hildebrandt and J.F. MacÍas-Pérez and L. Perotto and C. Renault and D. Santos and F. Couchot and S. Henrot-Versillé and O. Perdereau and S. Plaszczynski and M. Tristram and J. Borrill and T.S. Kisner and G.F. Smoot and A.J. Banday and U. Dörl and T.A. En{\ss}lin and W. Hovest and F. Matthai and J.P. Rachen and M. Reinecke and T. Riller and R. Sunyaev and J. Tuovinen and F.J. Lockman and A. Murphy and P.R. Christensen and P. Naselsky and I. Novikov and B.P. Crill and G. Savini and C. Baccigalupi and L. Bonavera and L. Danese and {De Zotti}, G. and J. González-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 A.J. Banday and J.-P. Bernard and O. Forni and M. Giard and C. Leroy and L. Montier and E. Pointecouteau and I. Ristorcelli and W.T. Reach and E. Battaner and K.M. Huffenberger and K.M. Górski",
year = "2011",
doi = "10.1051/0004-6361/201116461",
language = "English",
volume = "536",
pages = "A18",
journal = "Astronomy & Astrophysics",
issn = "0004-6361",
publisher = "E D P Sciences",

}

Poutanen, T, Natoli, P, Polenta, G, Bartlett, JG, Bucher, M, Cardoso, J-F, Catalano, A, Delabrouille, J, Ganga, K, Giraud-Héraud, Y, Patanchon, G, Piat, M, Remazeilles, M, Rosset, C, Smoot, GF, Stompor, R, Ashdown, M, Hobson, M, Lasenby, A, Stolyarov, V, Bhatia, R, Kneissl, R, Bonavera, L, Blagrave, K, Bond, JR, Martin, P, Miville-Deschênes, M-A, Banday, AJ, Bernard, J-P, Forni, O, Giard, M, Leroy, C, Montier, L, Pointecouteau, E, Ristorcelli, I, Bock, JJ, Doré, O, Helou, G, Hildebrandt, SR, Prézeau, G, Rocha, G, Seiffert, MD, Lilje, PB, Challinor, A, Shellard, P, Starck, J-L, Yvon, D, Linden-Vørnle, M, Nørgaard-Nielsen, HU, Toffolatti, L, Netterfield, CB, Pinheiro Gonçalves, D, Scott, D, Oliver, S, Juvela, M, Keihänen, E, Keskitalo, R, Kurki-Suonio, H, Poutanen, T, Chiang, C, Jones, WC, Cayón, L, Smoot, GF, White, M, Knox, L, Leonardi, R, Lubin, PM, Zonca, A, Wandelt, BD, Matarrese, S, De Bernardis, P, Masi, S, Melchiorri, A, Piacentini, F, Bersanelli, M, Maino, D, Mennella, A, Tomasi, M, Gregorio, A, Natoli, P, Balbi, A, Cabella, P, De Gasperis, G, Mazzotta, P, Vittorio, N, Christensen, PR, Naselsky, P, Rubiño-Martín, JA, Kneissl, R, Dupac, X, Leonardi, R, Mendes, L, Giardino, G, Laureijs, RJ, Leonardi, R, Tauber, JA, Kurki-Suonio, H, Poutanen, T, Umana, G, Bonaldi, A, De Zotti, G, Polenta, G, Frailis, M, Galeotta, S, Maris, M, Mennella, A, Pasian, F, Zacchei, A, Burigana, C, Cuttaia, F, De Rosa, A, Finelli, F, Franceschi, E, Gruppuso, A, Mandolesi, N, Morgante, G, Natoli, P, Ricciardi, S, Sandri, M, Terenzi, L, Valenziano, L, Villa, F, Bersanelli, M, Donzelli, S, Maino, D, Tomasi, M, Stivoli, F, Désert, F-X, Chamballu, A, Clements, DL, Jaffe, AH, Mortlock, D, Novikov, D, Rowan-Robinson, M, Ganga, K, Rusholme, B, Benoît, A, Aghanim, N, Aumont, J, Dole, H, Douspis, M, Grain, J, Lagache, G, Leroy, C, Miville-Deschênes, M-A, Pajot, F, Ponthieu, N, Puget, J-L, Torre, J-P, Benabed, K, Bouchet, FR, Cardoso, J-F, Colombi, S, Delouis, J-M, Hivon, E, Moneti, A, Prunet, S, Sygnet, J-F, Wandelt, BD, Fosalba, P, Chiang, L-Y, Challinor, A, Efstathiou, G, Gratton, S, Harrison, D, Munshi, D, Donzelli, S, Eriksen, HK, Hansen, FK, Lilje, PB, Hildebrandt, SR, Hoyland, RJ, Rubiño-Martín, JA, Barreiro, RB, Herranz, D, López-Caniego, M, Martínez-González, E, Vielva, P, Bartlett, JG, Bock, JJ, Crill, BP, Doré, O, Górski, KM, Holmes, WA, Keskitalo, R, Lawrence, CR, Mitra, S, O'Dwyer, IJ, Prézeau, G, Rocha, G, Seiffert, MD, Wade, LA, Davies, RD, Davis, RJ, Maffei, B, Ashdown, M, Challinor, A, Gratton, S, Harrison, D, Lasenby, A, MacTavish, CJ, Catalano, A, Coulais, A, Lamarre, J-M, Arnaud, M, Starck, J-L, Cardoso, J-F, Hildebrandt, SR, MacÍas-Pérez, JF, Perotto, L, Renault, C, Santos, D, Couchot, F, Henrot-Versillé, S, Perdereau, O, Plaszczynski, S, Tristram, M, Borrill, J, Kisner, TS, Smoot, GF, Banday, AJ, Dörl, U, Enßlin, TA, Hovest, W, Matthai, F, Rachen, JP, Reinecke, M, Riller, T, Sunyaev, R, Tuovinen, J, Lockman, FJ, Murphy, A, Christensen, PR, Naselsky, P, Novikov, I, Crill, BP, Savini, G, Baccigalupi, C, Bonavera, L, Danese, L, De Zotti, G, González-Nuevo, J, Leach, S, Perrotta, F, Mann, R, Ade, PAR, Munshi, D, Sudiwala, R, Sunyaev, R, Borrill, J, Osborne, S, Banday, AJ, Bernard, J-P, Forni, O, Giard, M, Leroy, C, Montier, L, Pointecouteau, E, Ristorcelli, I, Reach, WT, Battaner, E, Huffenberger, KM & Górski, KM 2011, 'Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies', Astronomy & Astrophysics, vol. 536, pp. A18. https://doi.org/10.1051/0004-6361/201116461

Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies. / Poutanen, T.; Natoli, P.; Polenta, G.; Bartlett, J.G.; Bucher, M.; Cardoso, J.-F.; Catalano, A.; Delabrouille, J.; Ganga, K.; Giraud-Héraud, Y.; Patanchon, G.; Piat, M.; Remazeilles, M.; Rosset, C.; Smoot, G.F.; Stompor, R.; Ashdown, M.; Hobson, M.; Lasenby, A.; Stolyarov, V.; Bhatia, R.; Kneissl, R.; Bonavera, L.; Blagrave, K.; Bond, J.R.; Martin, P.; Miville-Deschênes, M.-A.; Banday, A.J.; Bernard, J.-P.; Forni, O.; Giard, M.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Bock, J.J.; Doré, O.; Helou, G.; Hildebrandt, S.R.; Prézeau, G.; Rocha, G.; Seiffert, M.D.; Lilje, P.B.; Challinor, A.; Shellard, P.; Starck, J.-L.; Yvon, D.; Linden-Vørnle, Michael; Nørgaard-Nielsen, Hans Ulrik; Toffolatti, L.; Netterfield, C.B.; Pinheiro Gonçalves, D.; Scott, D.; Oliver, S.; Juvela, M.; Keihänen, E.; Keskitalo, R.; Kurki-Suonio, H.; Poutanen, T.; Chiang, C.; Jones, W.C.; Cayón, L.; Smoot, G.F.; White, M.; Knox, L.; Leonardi, R.; Lubin, P.M.; Zonca, A.; Wandelt, B.D.; Matarrese, S.; De Bernardis, P.; Masi, S.; Melchiorri, A.; Piacentini, F.; Bersanelli, M.; Maino, D.; Mennella, A.; Tomasi, M.; Gregorio, A.; Natoli, P.; Balbi, A.; Cabella, P.; De Gasperis, G.; Mazzotta, P.; Vittorio, N.; Christensen, P.R.; Naselsky, P.; Rubiño-Martín, J.A.; Kneissl, R.; Dupac, X.; Leonardi, R.; Mendes, L.; Giardino, G.; Laureijs, R.J.; Leonardi, R.; Tauber, J.A.; Kurki-Suonio, H.; Poutanen, T.; Umana, G.; Bonaldi, A.; De Zotti, G.; Polenta, G.; Frailis, M.; Galeotta, S.; Maris, M.; Mennella, A.; Pasian, F.; Zacchei, A.; Burigana, C.; Cuttaia, F.; De Rosa, A.; Finelli, F.; Franceschi, E.; Gruppuso, A.; Mandolesi, N.; Morgante, G.; Natoli, P.; Ricciardi, S.; Sandri, M.; Terenzi, L.; Valenziano, L.; Villa, F.; Bersanelli, M.; Donzelli, S.; Maino, D.; Tomasi, M.; Stivoli, F.; Désert, F.-X.; Chamballu, A.; Clements, D.L.; Jaffe, A.H.; Mortlock, D.; Novikov, D.; Rowan-Robinson, M.; Ganga, K.; Rusholme, B.; Benoît, A.; Aghanim, N.; Aumont, J.; Dole, H.; Douspis, M.; Grain, J.; Lagache, G.; Leroy, C.; Miville-Deschênes, M.-A.; Pajot, F.; Ponthieu, N.; Puget, J.-L.; Torre, J.-P.; Benabed, K.; Bouchet, F.R.; Cardoso, J.-F.; Colombi, S.; Delouis, J.-M.; Hivon, E.; Moneti, A.; Prunet, S.; Sygnet, J.-F.; Wandelt, B.D.; Fosalba, P.; Chiang, L.-Y.; Challinor, A.; Efstathiou, G.; Gratton, S.; Harrison, D.; Munshi, D.; Donzelli, S.; Eriksen, H.K.; Hansen, F.K.; Lilje, P.B.; Hildebrandt, S.R.; Hoyland, R.J.; Rubiño-Martín, J.A.; Barreiro, R.B.; Herranz, D.; López-Caniego, M.; Martínez-González, E.; Vielva, P.; Bartlett, J.G.; Bock, J.J.; Crill, B.P.; Doré, O.; Górski, K.M.; Holmes, W.A.; Keskitalo, R.; Lawrence, C.R.; Mitra, S.; O'Dwyer, I.J.; Prézeau, G.; Rocha, G.; Seiffert, M.D.; Wade, L.A.; Davies, R.D.; Davis, R.J.; Maffei, B.; Ashdown, M.; Challinor, A.; Gratton, S.; Harrison, D.; Lasenby, A.; MacTavish, C.J.; Catalano, A.; Coulais, A.; Lamarre, J.-M.; Arnaud, M.; Starck, J.-L.; Cardoso, J.-F.; Hildebrandt, S.R.; MacÍas-Pérez, J.F.; Perotto, L.; Renault, C.; Santos, D.; Couchot, F.; Henrot-Versillé, S.; Perdereau, O.; Plaszczynski, S.; Tristram, M.; Borrill, J.; Kisner, T.S.; Smoot, G.F.; Banday, A.J.; Dörl, U.; Enßlin, T.A.; Hovest, W.; Matthai, F.; Rachen, J.P.; Reinecke, M.; Riller, T.; Sunyaev, R.; Tuovinen, J.; Lockman, F.J.; Murphy, A.; Christensen, P.R.; Naselsky, P.; Novikov, I.; Crill, B.P.; Savini, G.; Baccigalupi, C.; Bonavera, L.; Danese, L.; De Zotti, G.; González-Nuevo, J.; Leach, S.; Perrotta, F.; Mann, R.; Ade, P.A.R.; Munshi, D.; Sudiwala, R.; Sunyaev, R.; Borrill, J.; Osborne, S.; Banday, A.J.; Bernard, J.-P.; Forni, O.; Giard, M.; Leroy, C.; Montier, L.; Pointecouteau, E.; Ristorcelli, I.; Reach, W.T.; Battaner, E.; Huffenberger, K.M.; Górski, K.M.

In: Astronomy & Astrophysics, Vol. 536, 2011, p. A18.

Research output: Contribution to journalJournal articleResearchpeer-review

TY - JOUR

T1 - Planck early results. XVIII. The power spectrum of cosmic infrared background anisotropies

AU - Poutanen, T.

AU - Natoli, P.

AU - Polenta, G.

AU - Bartlett, J.G.

AU - Bucher, M.

AU - Cardoso, J.-F.

AU - Catalano, A.

AU - Delabrouille, J.

AU - Ganga, K.

AU - Giraud-Héraud, Y.

AU - Patanchon, G.

AU - Piat, M.

AU - Remazeilles, M.

AU - Rosset, C.

AU - Smoot, G.F.

AU - Stompor, R.

AU - Ashdown, M.

AU - Hobson, M.

AU - Lasenby, A.

AU - Stolyarov, V.

AU - Bhatia, R.

AU - Kneissl, R.

AU - Bonavera, L.

AU - Blagrave, K.

AU - Bond, J.R.

AU - Martin, P.

AU - Miville-Deschênes, M.-A.

AU - Banday, A.J.

AU - Bernard, J.-P.

AU - Forni, O.

AU - Giard, M.

AU - Leroy, C.

AU - Montier, L.

AU - Pointecouteau, E.

AU - Ristorcelli, I.

AU - Bock, J.J.

AU - Doré, O.

AU - Helou, G.

AU - Hildebrandt, S.R.

AU - Prézeau, G.

AU - Rocha, G.

AU - Seiffert, M.D.

AU - Lilje, P.B.

AU - Challinor, A.

AU - Shellard, P.

AU - Starck, J.-L.

AU - Yvon, D.

AU - Linden-Vørnle, Michael

AU - Nørgaard-Nielsen, Hans Ulrik

AU - Toffolatti, L.

AU - Netterfield, C.B.

AU - Pinheiro Gonçalves, D.

AU - Scott, D.

AU - Oliver, S.

AU - Juvela, M.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Chiang, C.

AU - Jones, W.C.

AU - Cayón, L.

AU - Smoot, G.F.

AU - White, M.

AU - Knox, L.

AU - Leonardi, R.

AU - Lubin, P.M.

AU - Zonca, A.

AU - Wandelt, B.D.

AU - Matarrese, S.

AU - De Bernardis, P.

AU - Masi, S.

AU - Melchiorri, A.

AU - Piacentini, F.

AU - Bersanelli, M.

AU - Maino, D.

AU - Mennella, A.

AU - Tomasi, M.

AU - Gregorio, A.

AU - Natoli, P.

AU - Balbi, A.

AU - Cabella, P.

AU - De Gasperis, G.

AU - Mazzotta, P.

AU - Vittorio, N.

AU - Christensen, P.R.

AU - Naselsky, P.

AU - Rubiño-Martín, J.A.

AU - Kneissl, R.

AU - Dupac, X.

AU - Leonardi, R.

AU - Mendes, L.

AU - Giardino, G.

AU - Laureijs, R.J.

AU - Leonardi, R.

AU - Tauber, J.A.

AU - Kurki-Suonio, H.

AU - Poutanen, T.

AU - Umana, G.

AU - Bonaldi, A.

AU - De Zotti, G.

AU - Polenta, G.

AU - Frailis, M.

AU - Galeotta, S.

AU - Maris, M.

AU - Mennella, A.

AU - Pasian, F.

AU - Zacchei, A.

AU - Burigana, C.

AU - Cuttaia, F.

AU - De Rosa, A.

AU - Finelli, F.

AU - Franceschi, E.

AU - Gruppuso, A.

AU - Mandolesi, N.

AU - Morgante, G.

AU - Natoli, P.

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 - Tomasi, M.

AU - Stivoli, F.

AU - Désert, F.-X.

AU - Chamballu, A.

AU - Clements, D.L.

AU - Jaffe, A.H.

AU - Mortlock, D.

AU - Novikov, D.

AU - Rowan-Robinson, M.

AU - Ganga, K.

AU - Rusholme, B.

AU - Benoît, A.

AU - Aghanim, N.

AU - Aumont, J.

AU - Dole, H.

AU - Douspis, M.

AU - Grain, J.

AU - Lagache, G.

AU - Leroy, C.

AU - Miville-Deschênes, M.-A.

AU - Pajot, F.

AU - Ponthieu, N.

AU - Puget, J.-L.

AU - Torre, J.-P.

AU - Benabed, K.

AU - Bouchet, F.R.

AU - Cardoso, J.-F.

AU - Colombi, S.

AU - Delouis, J.-M.

AU - Hivon, E.

AU - Moneti, A.

AU - Prunet, S.

AU - Sygnet, J.-F.

AU - Wandelt, B.D.

AU - Fosalba, P.

AU - Chiang, L.-Y.

AU - Challinor, A.

AU - Efstathiou, G.

AU - Gratton, S.

AU - Harrison, D.

AU - Munshi, D.

AU - Donzelli, S.

AU - Eriksen, H.K.

AU - Hansen, F.K.

AU - Lilje, P.B.

AU - Hildebrandt, S.R.

AU - Hoyland, R.J.

AU - Rubiño-Martín, J.A.

AU - Barreiro, R.B.

AU - Herranz, D.

AU - López-Caniego, M.

AU - Martínez-González, E.

AU - Vielva, P.

AU - Bartlett, J.G.

AU - Bock, J.J.

AU - Crill, B.P.

AU - Doré, O.

AU - Górski, K.M.

AU - Holmes, W.A.

AU - Keskitalo, R.

AU - Lawrence, C.R.

AU - Mitra, S.

AU - O'Dwyer, I.J.

AU - Prézeau, G.

AU - Rocha, G.

AU - Seiffert, M.D.

AU - Wade, L.A.

AU - Davies, R.D.

AU - Davis, R.J.

AU - Maffei, B.

AU - Ashdown, M.

AU - Challinor, A.

AU - Gratton, S.

AU - Harrison, D.

AU - Lasenby, A.

AU - MacTavish, C.J.

AU - Catalano, A.

AU - Coulais, A.

AU - Lamarre, J.-M.

AU - Arnaud, M.

AU - Starck, J.-L.

AU - Cardoso, J.-F.

AU - Hildebrandt, S.R.

AU - MacÍas-Pérez, J.F.

AU - Perotto, L.

AU - Renault, C.

AU - Santos, D.

AU - Couchot, F.

AU - Henrot-Versillé, S.

AU - Perdereau, O.

AU - Plaszczynski, S.

AU - Tristram, M.

AU - Borrill, J.

AU - Kisner, T.S.

AU - Smoot, G.F.

AU - Banday, A.J.

AU - Dörl, U.

AU - Enßlin, T.A.

AU - Hovest, W.

AU - Matthai, F.

AU - Rachen, J.P.

AU - Reinecke, M.

AU - Riller, T.

AU - Sunyaev, R.

AU - Tuovinen, J.

AU - Lockman, F.J.

AU - Murphy, A.

AU - Christensen, P.R.

AU - Naselsky, P.

AU - Novikov, I.

AU - Crill, B.P.

AU - Savini, G.

AU - Baccigalupi, C.

AU - Bonavera, L.

AU - Danese, L.

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 - Banday, A.J.

AU - Bernard, J.-P.

AU - Forni, O.

AU - Giard, M.

AU - Leroy, C.

AU - Montier, L.

AU - Pointecouteau, E.

AU - Ristorcelli, I.

AU - Reach, W.T.

AU - Battaner, E.

AU - Huffenberger, K.M.

AU - Górski, K.M.

PY - 2011

Y1 - 2011

N2 - Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg2, we determine the angular power spectra of cosmic infrared background (CIB) anisotropies from multipole = 200 to = 2000 at 217, 353, 545 and 857 GHz. We use 21-cm observations of Hi as a tracer of thermal dust emission to reduce the already low level of Galactic dust emission and use the 143 GHz Planck maps in these fields to clean out cosmic microwave background anisotropies. Both of these cleaning processes are necessary to avoid significant contamination of the CIB signal. We measure correlated CIB structure across frequencies. As expected, the correlation decreases with increasing frequency separation, because the contribution of high-redshift galaxies to CIB anisotropies increases with wavelengths. We find no significant difference between the frequency spectrum of the CIB anisotropies and the CIB mean, with ΔI / I = 15% from 217 to 857 GHz. In terms of clustering properties, the Planck data alone rule out the linear scale- and redshift-independent bias model. Non-linear corrections are significant. Consequently, we develop an alternative model that couples a dusty galaxy, parametric evolution model with a simple halo-model approach. It provides an excellent fit to the measured anisotropy angular power spectra and suggests that a different halo occupation distribution is required at each frequency, which is consistent with our expectation that each frequency is dominated by contributions from different redshifts. In our best-fit model, half of the anisotropy power at = 2000 comes from redshifts z <0.8 at 857 GHz and z <1.5 at 545 GHz, while about 90% come from redshifts z > 2 at 353 and 217 GHz, respectively. © ESO, 2011.

AB - Using Planck maps of six regions of low Galactic dust emission with a total area of about 140 deg2, we determine the angular power spectra of cosmic infrared background (CIB) anisotropies from multipole = 200 to = 2000 at 217, 353, 545 and 857 GHz. We use 21-cm observations of Hi as a tracer of thermal dust emission to reduce the already low level of Galactic dust emission and use the 143 GHz Planck maps in these fields to clean out cosmic microwave background anisotropies. Both of these cleaning processes are necessary to avoid significant contamination of the CIB signal. We measure correlated CIB structure across frequencies. As expected, the correlation decreases with increasing frequency separation, because the contribution of high-redshift galaxies to CIB anisotropies increases with wavelengths. We find no significant difference between the frequency spectrum of the CIB anisotropies and the CIB mean, with ΔI / I = 15% from 217 to 857 GHz. In terms of clustering properties, the Planck data alone rule out the linear scale- and redshift-independent bias model. Non-linear corrections are significant. Consequently, we develop an alternative model that couples a dusty galaxy, parametric evolution model with a simple halo-model approach. It provides an excellent fit to the measured anisotropy angular power spectra and suggests that a different halo occupation distribution is required at each frequency, which is consistent with our expectation that each frequency is dominated by contributions from different redshifts. In our best-fit model, half of the anisotropy power at = 2000 comes from redshifts z <0.8 at 857 GHz and z <1.5 at 545 GHz, while about 90% come from redshifts z > 2 at 353 and 217 GHz, respectively. © ESO, 2011.

U2 - 10.1051/0004-6361/201116461

DO - 10.1051/0004-6361/201116461

M3 - Journal article

VL - 536

SP - A18

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

SN - 0004-6361

ER -