Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation
We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a stacking analysis towards Planck-confirmed galaxy clusters. We detect infrared e...
Published in: | Astronomy & Astrophysics |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Other Authors: | |
Format: | Article in Journal/Newspaper |
Language: | English |
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EDP SCIENCES S A
2016
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Subjects: | |
Online Access: | http://hdl.handle.net/10044/1/59905 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000385832200034&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202 https://doi.org/10.1051/0004-6361/201527418 |
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ftimperialcol:oai:spiral.imperial.ac.uk:10044/1/59905 |
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record_format |
openpolar |
institution |
Open Polar |
collection |
Imperial College London: Spiral |
op_collection_id |
ftimperialcol |
language |
English |
topic |
Science & Technology Physical Sciences Astronomy & Astrophysics galaxies: clusters: general infrared: galaxies large-scale structure of Universe methods: data analysis SOUTH-POLE TELESCOPE ANGULAR POWER SPECTRUM DARK-MATTER HALOES GALAXY CLUSTERS STAR-FORMATION COSMOLOGICAL PARAMETERS SUBMILLIMETER GALAXIES SCALING RELATIONS COMPACT SOURCES DUST EMISSION astro-ph.CO PRIMORDIAL NON-GAUSSIANITY 0201 Astronomical And Space Sciences |
spellingShingle |
Science & Technology Physical Sciences Astronomy & Astrophysics galaxies: clusters: general infrared: galaxies large-scale structure of Universe methods: data analysis SOUTH-POLE TELESCOPE ANGULAR POWER SPECTRUM DARK-MATTER HALOES GALAXY CLUSTERS STAR-FORMATION COSMOLOGICAL PARAMETERS SUBMILLIMETER GALAXIES SCALING RELATIONS COMPACT SOURCES DUST EMISSION astro-ph.CO PRIMORDIAL NON-GAUSSIANITY 0201 Astronomical And Space Sciences Ade, PAR Aghanim, N Arnaud, M Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Benabed, K Sygnet, J-F Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Borrill, J Lasenby, A Valiviita, J Van Tent, B Vielva, P Villa, F Wade, LA Wandelt, BD Wehus, IK Welikala, N Yvon, D Zacchei, A Lattanzi, M Bouchet, FR Zonca, A Burigana, C Butler, RC Calabrese, E Catalano, A Chamballu, A Chiang, HC Christensen, PR Churazov, E Lawrence, CR Clements, DL Colombo, LPL Combet, C Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Leonardi, R Davies, RD Davis, RJ De Bernardis, P De Rosa, A De Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Levrier, F Dore, O Douspis, M Ducout, A Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Lilje, PB Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Galli, S Ganga, K Genova-Santos, RT Giard, M Giraud-Heraud, Y Linden-Vornle, M Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Harrison, DL Helou, G Hernandez-Monteagudo, C Lopez-Caniego, M Herranz, D Hildebrandt, SR Hivon, E Hobson, M Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Lubin, PM Jones, WC Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lamarre, J-M Macias-Perez, JF Langer, M Benoit-Levy, A Maffei, B Maggio, G Maino, D Mak, DSY Mandolesi, N Mangilli, A Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Bernard, J-P Matarrese, S Melchiorri, A Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, M-A Moneti, A Montier, L Morgante, G Mortlock, D Bersanelli, M Munshi, D Murphy, JA Nati, F Natoli, P Noviello, F Novikov, D Novikov, I Oxborrow, CA Paci, F Pagano, L Bielewicz, P Pajot, F Paoletti, D Partridge, B Pasian, F Pearson, TJ Perdereau, O Perotto, L Pettorino, V Piacentini, F Piat, M Bock, JJ Pierpaoli, E Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Pratt, GW Prunet, S Puget, J-L Rachen, JP Reinecke, M Bonaldi, A Remazeilles, M Renault, C Renzi, A Ristorcelli, I Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Bonavera, L Sandri, M Santos, D Savelainen, M Savini, G Scott, D Spencer, LD Stolyarov, V Stompor, R Sunyaev, R Sutton, D Bond, JR Suur-Uski, A-S Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
topic_facet |
Science & Technology Physical Sciences Astronomy & Astrophysics galaxies: clusters: general infrared: galaxies large-scale structure of Universe methods: data analysis SOUTH-POLE TELESCOPE ANGULAR POWER SPECTRUM DARK-MATTER HALOES GALAXY CLUSTERS STAR-FORMATION COSMOLOGICAL PARAMETERS SUBMILLIMETER GALAXIES SCALING RELATIONS COMPACT SOURCES DUST EMISSION astro-ph.CO PRIMORDIAL NON-GAUSSIANITY 0201 Astronomical And Space Sciences |
description |
We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a stacking analysis towards Planck-confirmed galaxy clusters. We detect infrared emission produced by dusty galaxies inside these clusters and demonstrate that the infrared emission is about 50% more extended than the tSZ effect. Modelling the emission with a Navarro-Frenk-White profile, we find that the radial profile concentration parameter is c500 = 1.00+0.18-0.15 . This indicates that infrared galaxies in the outskirts of clusters have higher infrared flux than cluster-core galaxies. We also study the cross-correlation between tSZ and CIB anisotropies, following three alternative approaches based on power spectrum analyses: (i) using a catalogue of confirmed clusters detected in Planck data; (ii) using an all-sky tSZ map built from Planck frequency maps; and (iii) using cross-spectra between Planck frequency maps. With the three different methods, we detect the tSZ-CIB cross-power spectrum at significance levels of (i) 6σ; (ii) 3σ; and (iii) 4σ. We model the tSZ-CIB cross-correlation signature and compare predictions with the measurements. The amplitude of the cross-correlation relative to the fiducial model is AtSZ−CIB = 1.2 ± 0.3. This result is consistent with predictions for the tSZ-CIB cross-correlation assuming the best-fit cosmological model from Planck 2015 results along with the tSZ and CIB scaling relations. |
author2 |
Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) |
format |
Article in Journal/Newspaper |
author |
Ade, PAR Aghanim, N Arnaud, M Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Benabed, K Sygnet, J-F Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Borrill, J Lasenby, A Valiviita, J Van Tent, B Vielva, P Villa, F Wade, LA Wandelt, BD Wehus, IK Welikala, N Yvon, D Zacchei, A Lattanzi, M Bouchet, FR Zonca, A Burigana, C Butler, RC Calabrese, E Catalano, A Chamballu, A Chiang, HC Christensen, PR Churazov, E Lawrence, CR Clements, DL Colombo, LPL Combet, C Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Leonardi, R Davies, RD Davis, RJ De Bernardis, P De Rosa, A De Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Levrier, F Dore, O Douspis, M Ducout, A Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Lilje, PB Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Galli, S Ganga, K Genova-Santos, RT Giard, M Giraud-Heraud, Y Linden-Vornle, M Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Harrison, DL Helou, G Hernandez-Monteagudo, C Lopez-Caniego, M Herranz, D Hildebrandt, SR Hivon, E Hobson, M Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Lubin, PM Jones, WC Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lamarre, J-M Macias-Perez, JF Langer, M Benoit-Levy, A Maffei, B Maggio, G Maino, D Mak, DSY Mandolesi, N Mangilli, A Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Bernard, J-P Matarrese, S Melchiorri, A Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, M-A Moneti, A Montier, L Morgante, G Mortlock, D Bersanelli, M Munshi, D Murphy, JA Nati, F Natoli, P Noviello, F Novikov, D Novikov, I Oxborrow, CA Paci, F Pagano, L Bielewicz, P Pajot, F Paoletti, D Partridge, B Pasian, F Pearson, TJ Perdereau, O Perotto, L Pettorino, V Piacentini, F Piat, M Bock, JJ Pierpaoli, E Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Pratt, GW Prunet, S Puget, J-L Rachen, JP Reinecke, M Bonaldi, A Remazeilles, M Renault, C Renzi, A Ristorcelli, I Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Bonavera, L Sandri, M Santos, D Savelainen, M Savini, G Scott, D Spencer, LD Stolyarov, V Stompor, R Sunyaev, R Sutton, D Bond, JR Suur-Uski, A-S |
author_facet |
Ade, PAR Aghanim, N Arnaud, M Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Benabed, K Sygnet, J-F Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Borrill, J Lasenby, A Valiviita, J Van Tent, B Vielva, P Villa, F Wade, LA Wandelt, BD Wehus, IK Welikala, N Yvon, D Zacchei, A Lattanzi, M Bouchet, FR Zonca, A Burigana, C Butler, RC Calabrese, E Catalano, A Chamballu, A Chiang, HC Christensen, PR Churazov, E Lawrence, CR Clements, DL Colombo, LPL Combet, C Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Leonardi, R Davies, RD Davis, RJ De Bernardis, P De Rosa, A De Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Levrier, F Dore, O Douspis, M Ducout, A Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Lilje, PB Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Galli, S Ganga, K Genova-Santos, RT Giard, M Giraud-Heraud, Y Linden-Vornle, M Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Harrison, DL Helou, G Hernandez-Monteagudo, C Lopez-Caniego, M Herranz, D Hildebrandt, SR Hivon, E Hobson, M Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Lubin, PM Jones, WC Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lamarre, J-M Macias-Perez, JF Langer, M Benoit-Levy, A Maffei, B Maggio, G Maino, D Mak, DSY Mandolesi, N Mangilli, A Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Bernard, J-P Matarrese, S Melchiorri, A Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, M-A Moneti, A Montier, L Morgante, G Mortlock, D Bersanelli, M Munshi, D Murphy, JA Nati, F Natoli, P Noviello, F Novikov, D Novikov, I Oxborrow, CA Paci, F Pagano, L Bielewicz, P Pajot, F Paoletti, D Partridge, B Pasian, F Pearson, TJ Perdereau, O Perotto, L Pettorino, V Piacentini, F Piat, M Bock, JJ Pierpaoli, E Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Pratt, GW Prunet, S Puget, J-L Rachen, JP Reinecke, M Bonaldi, A Remazeilles, M Renault, C Renzi, A Ristorcelli, I Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Bonavera, L Sandri, M Santos, D Savelainen, M Savini, G Scott, D Spencer, LD Stolyarov, V Stompor, R Sunyaev, R Sutton, D Bond, JR Suur-Uski, A-S |
author_sort |
Ade, PAR |
title |
Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
title_short |
Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
title_full |
Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
title_fullStr |
Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
title_full_unstemmed |
Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation |
title_sort |
planck 2015 results xxiii. the thermal sunyaev-zeldovich effect-cosmic infrared background correlation |
publisher |
EDP SCIENCES S A |
publishDate |
2016 |
url |
http://hdl.handle.net/10044/1/59905 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000385832200034&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202 https://doi.org/10.1051/0004-6361/201527418 |
long_lat |
ENVELOPE(-62.167,-62.167,-64.650,-64.650) |
geographic |
Navarro South Pole |
geographic_facet |
Navarro South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
ASTRONOMY & ASTROPHYSICS |
op_rights |
© 2016 ESO |
op_doi |
https://doi.org/10.1051/0004-6361/201527418 |
container_title |
Astronomy & Astrophysics |
container_volume |
594 |
container_start_page |
A23 |
_version_ |
1766202554752958464 |
spelling |
ftimperialcol:oai:spiral.imperial.ac.uk:10044/1/59905 2023-05-15T18:23:07+02:00 Planck 2015 results XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation Ade, PAR Aghanim, N Arnaud, M Aumont, J Baccigalupi, C Banday, AJ Barreiro, RB Bartlett, JG Bartolo, N Battaner, E Benabed, K Sygnet, J-F Tauber, JA Terenzi, L Toffolatti, L Tomasi, M Tristram, M Tucci, M Umana, G Valenziano, L Borrill, J Lasenby, A Valiviita, J Van Tent, B Vielva, P Villa, F Wade, LA Wandelt, BD Wehus, IK Welikala, N Yvon, D Zacchei, A Lattanzi, M Bouchet, FR Zonca, A Burigana, C Butler, RC Calabrese, E Catalano, A Chamballu, A Chiang, HC Christensen, PR Churazov, E Lawrence, CR Clements, DL Colombo, LPL Combet, C Comis, B Couchot, F Coulais, A Crill, BP Curto, A Cuttaia, F Danese, L Leonardi, R Davies, RD Davis, RJ De Bernardis, P De Rosa, A De Zotti, G Delabrouille, J Dickinson, C Diego, JM Dole, H Donzelli, S Levrier, F Dore, O Douspis, M Ducout, A Dupac, X Efstathiou, G Elsner, F Ensslin, TA Eriksen, HK Finelli, F Flores-Cacho, I Lilje, PB Forni, O Frailis, M Fraisse, AA Franceschi, E Galeotta, S Galli, S Ganga, K Genova-Santos, RT Giard, M Giraud-Heraud, Y Linden-Vornle, M Gjerlow, E Gonzalez-Nuevo, J Gorski, KM Gregorio, A Gruppuso, A Gudmundsson, JE Hansen, FK Harrison, DL Helou, G Hernandez-Monteagudo, C Lopez-Caniego, M Herranz, D Hildebrandt, SR Hivon, E Hobson, M Hornstrup, A Hovest, W Huffenberger, KM Hurier, G Jaffe, AH Jaffe, TR Lubin, PM Jones, WC Keihanen, E Keskitalo, R Kisner, TS Kneissl, R Knoche, J Kunz, M Kurki-Suonio, H Lagache, G Lamarre, J-M Macias-Perez, JF Langer, M Benoit-Levy, A Maffei, B Maggio, G Maino, D Mak, DSY Mandolesi, N Mangilli, A Maris, M Martin, PG Martinez-Gonzalez, E Masi, S Bernard, J-P Matarrese, S Melchiorri, A Mennella, A Migliaccio, M Mitra, S Miville-Deschenes, M-A Moneti, A Montier, L Morgante, G Mortlock, D Bersanelli, M Munshi, D Murphy, JA Nati, F Natoli, P Noviello, F Novikov, D Novikov, I Oxborrow, CA Paci, F Pagano, L Bielewicz, P Pajot, F Paoletti, D Partridge, B Pasian, F Pearson, TJ Perdereau, O Perotto, L Pettorino, V Piacentini, F Piat, M Bock, JJ Pierpaoli, E Plaszczynski, S Pointecouteau, E Polenta, G Ponthieu, N Pratt, GW Prunet, S Puget, J-L Rachen, JP Reinecke, M Bonaldi, A Remazeilles, M Renault, C Renzi, A Ristorcelli, I Rocha, G Rosset, C Rossetti, M Roudier, G Rubino-Martin, JA Rusholme, B Bonavera, L Sandri, M Santos, D Savelainen, M Savini, G Scott, D Spencer, LD Stolyarov, V Stompor, R Sunyaev, R Sutton, D Bond, JR Suur-Uski, A-S Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) Science and Technology Facilities Council (STFC) 2016-04-23 http://hdl.handle.net/10044/1/59905 http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000385832200034&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202 https://doi.org/10.1051/0004-6361/201527418 English eng EDP SCIENCES S A ASTRONOMY & ASTROPHYSICS © 2016 ESO Science & Technology Physical Sciences Astronomy & Astrophysics galaxies: clusters: general infrared: galaxies large-scale structure of Universe methods: data analysis SOUTH-POLE TELESCOPE ANGULAR POWER SPECTRUM DARK-MATTER HALOES GALAXY CLUSTERS STAR-FORMATION COSMOLOGICAL PARAMETERS SUBMILLIMETER GALAXIES SCALING RELATIONS COMPACT SOURCES DUST EMISSION astro-ph.CO PRIMORDIAL NON-GAUSSIANITY 0201 Astronomical And Space Sciences Journal Article 2016 ftimperialcol https://doi.org/10.1051/0004-6361/201527418 2018-09-16T06:02:42Z We use Planck data to detect the cross-correlation between the thermal Sunyaev-Zeldovich (tSZ) effect and the infrared emission from the galaxies that make up the the cosmic infrared background (CIB). We first perform a stacking analysis towards Planck-confirmed galaxy clusters. We detect infrared emission produced by dusty galaxies inside these clusters and demonstrate that the infrared emission is about 50% more extended than the tSZ effect. Modelling the emission with a Navarro-Frenk-White profile, we find that the radial profile concentration parameter is c500 = 1.00+0.18-0.15 . This indicates that infrared galaxies in the outskirts of clusters have higher infrared flux than cluster-core galaxies. We also study the cross-correlation between tSZ and CIB anisotropies, following three alternative approaches based on power spectrum analyses: (i) using a catalogue of confirmed clusters detected in Planck data; (ii) using an all-sky tSZ map built from Planck frequency maps; and (iii) using cross-spectra between Planck frequency maps. With the three different methods, we detect the tSZ-CIB cross-power spectrum at significance levels of (i) 6σ; (ii) 3σ; and (iii) 4σ. We model the tSZ-CIB cross-correlation signature and compare predictions with the measurements. The amplitude of the cross-correlation relative to the fiducial model is AtSZ−CIB = 1.2 ± 0.3. This result is consistent with predictions for the tSZ-CIB cross-correlation assuming the best-fit cosmological model from Planck 2015 results along with the tSZ and CIB scaling relations. Article in Journal/Newspaper South pole Imperial College London: Spiral Navarro ENVELOPE(-62.167,-62.167,-64.650,-64.650) South Pole Astronomy & Astrophysics 594 A23 |