Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation

Planck Collaboration; P A R Ade; N Aghanim; C Armitage-Caplan; M Arnaud; M Ashdown; F Atrio-Barandela; J Aumont; C Baccigalupi; A J Banday; R B Barreiro; J G Bartlett; S Basak; E Battaner; K Benabed; A BenoÓt; A Benoit-LÈvy; J-P Bernard; M Bersanelli; M Bethermin; P Bielewicz; J Bobin; J J Bock; A Bonaldi; J R Bond; J Borrill; F R Bouchet; F Boulanger; M Bridges; M Bucher; C Burigana; R C Butler; J-F Cardoso; A Catalano; A Challinor; A Chamballu; H C Chiang; L-Y Chiang; P R Christensen; S Church; D L Clements; S Colombi; L P L Colombo; F Couchot; A Coulais; B P Crill; A Curto; F Cuttaia; L Danese; R D Davies; P de Bernardis; A de Rosa; G de Zotti; J Delabrouille; J-M Delouis; F-X DÈsert; J M Diego; H Dole; S Donzelli; O DorÈ; M Douspis; X Dupac; G Efstathiou; T A Enﬂlin; H K Eriksen; F Finelli; O Forni; M Frailis; E Franceschi; S Galeotta; K Ganga; M Giard; G Giardino; Y Giraud-HÈraud; J Gonz·lez-Nuevo; K M GÛrski; S Gratton; A Gregorio; A Gruppuso; J E Gudmundsson; F K Hansen; D Hanson; D Harrison; S Henrot-VersillÈ; C Hern·ndez-Monteagudo; D Herranz; S R Hildebrandt; E Hivon; M Hobson; W A Holmes; A Hornstrup; W Hovest; K M Huffenberger; A H Jaffe; T R Jaffe; W C Jones; M Juvela; E Keih‰nen; R Keskitalo; T S Kisner; R Kneissl; J Knoche; L Knox; M Kunz; H Kurki-Suonio; F Lacasa; G Lagache; A L‰hteenm‰ki; J-M Lamarre; A Lasenby; R J Laureijs; C R Lawrence; R Leonardi; J LeÛn-Tavares; J Lesgourgues; M Liguori; P B Lilje; M Linden-V¯rnle; M LÛpez-Caniego; P M Lubin; J F MacÌas-PÈrez; B Maffei; D Maino; N Mandolesi; M Maris; D J Marshall; P G Martin; E MartÌnez-Gonz·lez; S Masi; M Massardi; S Matarrese; F Matthai; P Mazzotta; A Melchiorri; L Mendes; A Mennella; M Migliaccio; S Mitra; M-A Miville-DeschÍnes; A Moneti; L Montier; G Morgante; D Mortlock; D Munshi; P Naselsky; F Nati; P Natoli; C B Netterfield; H U N¯rgaard-Nielsen; F Noviello; D Novikov; I Novikov; S Osborne; C A Oxborrow; F Paci; L Pagano; F Pajot; D Paoletti; F Pasian; G Patanchon; O Perdereau; L Perotto; F Perrotta; F Piacentini; M Piat; E Pierpaoli; D Pietrobon; S Plaszczynski; E Pointecouteau; G Polenta; N Ponthieu; L Popa; T Poutanen; G W Pratt; G PrÈzeau; S Prunet; J-L Puget; J P Rachen; R Rebolo; M Reinecke; M Remazeilles; C Renault; S Ricciardi; T Riller; I Ristorcelli; G Rocha; C Rosset; G Roudier; M Rowan-Robinson; B Rusholme; M Sandri; D Santos; G Savini; D Scott; M D Seiffert; P Serra; E P S Shellard; L D Spencer; J-L Starck; V Stolyarov; R Stompor; R Sudiwala; R Sunyaev; F Sureau; D Sutton; A-S Suur-Uski; J-F Sygnet; J A Tauber; D Tavagnacco; L Terenzi; L Toffolatti; M Tomasi; M Tristram; M Tucci; J Tuovinen; L Valenziano; J Valiviita; B Van Tent; P Vielva; F Villa; N Vittorio; L A Wade; B D Wandelt; S D M White; D Yvon; A Zacchei; A Zonca

Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation

Planck Collaboration, P A R Ade, N Aghanim, C Armitage-Caplan, M Arnaud, M Ashdown, F Atrio-Barandela, J Aumont, C Baccigalupi, A J Banday, R B Barreiro, J G Bartlett, S Basak, E Battaner, K Benabed, A BenoÓt, A Benoit-LÈvy, J-P Bernard, M Bersanelli, M BetherminP Bielewicz, J Bobin, J J Bock, A Bonaldi, J R Bond, J Borrill, F R Bouchet, F Boulanger, M Bridges, M Bucher, C Burigana, R C Butler, J-F Cardoso, A Catalano, A Challinor, A Chamballu, H C Chiang, L-Y Chiang, P R Christensen, S Church, D L Clements, S Colombi, L P L Colombo, F Couchot, A Coulais, B P Crill, A Curto, F Cuttaia, L Danese, R D Davies, P de Bernardis, A de Rosa, G de Zotti, J Delabrouille, J-M Delouis, F-X DÈsert, J M Diego, H Dole, S Donzelli, O DorÈ, M Douspis, X Dupac, G Efstathiou, T A Enﬂlin, H K Eriksen, F Finelli, O Forni, M Frailis, E Franceschi, S Galeotta, K Ganga, M Giard, G Giardino, Y Giraud-HÈraud, J Gonz·lez-Nuevo, K M GÛrski, S Gratton, A Gregorio, A Gruppuso, J E Gudmundsson, F K Hansen, D Hanson, D Harrison, S Henrot-VersillÈ, C Hern·ndez-Monteagudo, D Herranz, S R Hildebrandt, E Hivon, M Hobson, W A Holmes, A Hornstrup, W Hovest, K M Huffenberger, A H Jaffe, T R Jaffe, W C Jones, M Juvela, E Keih‰nen, R Keskitalo, T S Kisner, R Kneissl, J Knoche, L Knox, M Kunz, H Kurki-Suonio, F Lacasa, G Lagache, A L‰hteenm‰ki, J-M Lamarre, A Lasenby, R J Laureijs, C R Lawrence, R Leonardi, J LeÛn-Tavares, J Lesgourgues, M Liguori, P B Lilje, M Linden-V¯rnle, M LÛpez-Caniego, P M Lubin, J F MacÌas-PÈrez, B Maffei, D Maino, N Mandolesi, M Maris, D J Marshall, P G Martin, E MartÌnez-Gonz·lez, S Masi, M Massardi, S Matarrese, F Matthai, P Mazzotta, A Melchiorri, L Mendes, A Mennella, M Migliaccio, S Mitra, M-A Miville-DeschÍnes, A Moneti, L Montier, G Morgante, D Mortlock, D Munshi, P Naselsky, F Nati, P Natoli, C B Netterfield, H U N¯rgaard-Nielsen, F Noviello, D Novikov, I Novikov, S Osborne, C A Oxborrow, F Paci, L Pagano, F Pajot, D Paoletti, F Pasian, G Patanchon, O Perdereau, L Perotto, F Perrotta, F Piacentini, M Piat, E Pierpaoli, D Pietrobon, S Plaszczynski, E Pointecouteau, G Polenta, N Ponthieu, L Popa, T Poutanen, G W Pratt, G PrÈzeau, S Prunet, J-L Puget, J P Rachen, R Rebolo, M Reinecke, M Remazeilles, C Renault, S Ricciardi, T Riller, I Ristorcelli, G Rocha, C Rosset, G Roudier, M Rowan-Robinson, B Rusholme, M Sandri, D Santos, G Savini, D Scott, M D Seiffert, P Serra, E P S Shellard, L D Spencer, J-L Starck, V Stolyarov, R Stompor, R Sudiwala, R Sunyaev, F Sureau, D Sutton, A-S Suur-Uski, J-F Sygnet, J A Tauber, D Tavagnacco, L Terenzi, L Toffolatti, M Tomasi, M Tristram, M Tucci, J Tuovinen, L Valenziano, J Valiviita, B Van Tent, P Vielva, F Villa, N Vittorio, L A Wade, B D Wandelt, S D M White, D Yvon, A Zacchei, A Zonca

Research output: Contribution to journal › Article › peer-review

Abstract

The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). The conjunction of these two unique probes allows us to measure directly the connection between dark and luminous matter in the high redshift (1 10(M/M_&sun;) = 10.5 ± 0.6. Leveraging the frequency dependence of our signal, we isolate the high redshift contribution to the CIB, and constrain the star formation rate (SFR) density at z >= 1. We measure directly the SFR density with around 2sigma significance for three redshift bins between z = 1 and 7, thus opening a new window into the study of the formation of stars at early times.

Original language	English
Journal	Astronomy and Astrophysics
Volume	571
Publication status	Published - 2014

Keywords

gravitational lensing: weak
cosmic background radiation
large-scale
structure of Universe
dark matter
galaxies: star formation

Access to Document

http://adsabs.harvard.edu/abs/2014A%26A...571A..18P

Cite this

Collaboration, P., Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., Barreiro, R. B., Bartlett, J. G., Basak, S., Battaner, E., Benabed, K., BenoÓt, A., Benoit-LÈvy, A., Bernard, J.-P., Bersanelli, M., ... Zonca, A. (2014). Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation. Astronomy and Astrophysics, 571. http://adsabs.harvard.edu/abs/2014A%26A...571A..18P

@article{81ecce0349fc4d4fa837aeeed339c413,

title = "Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation",

abstract = "The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). The conjunction of these two unique probes allows us to measure directly the connection between dark and luminous matter in the high redshift (1 10(M/M\&sun;) = 10.5 ± 0.6. Leveraging the frequency dependence of our signal, we isolate the high redshift contribution to the CIB, and constrain the star formation rate (SFR) density at z >= 1. We measure directly the SFR density with around 2sigma significance for three redshift bins between z = 1 and 7, thus opening a new window into the study of the formation of stars at early times.",

keywords = "gravitational lensing: weak, cosmic background radiation, large-scale, structure of Universe, dark matter, galaxies: star formation",

author = "Planck Collaboration and Ade, \{P A R\} and N Aghanim and C Armitage-Caplan and M Arnaud and M Ashdown and F Atrio-Barandela and J Aumont and C Baccigalupi and Banday, \{A J\} and Barreiro, \{R B\} and Bartlett, \{J G\} and S Basak and E Battaner and K Benabed and A Beno{\'O}t and A Benoit-L{\`E}vy and J-P Bernard and M Bersanelli and M Bethermin and P Bielewicz and J Bobin and Bock, \{J J\} and A Bonaldi and Bond, \{J R\} and J Borrill and Bouchet, \{F R\} and F Boulanger and M Bridges and M Bucher and C Burigana and Butler, \{R C\} and J-F Cardoso and A Catalano and A Challinor and A Chamballu and Chiang, \{H C\} and L-Y Chiang and Christensen, \{P R\} and S Church and Clements, \{D L\} and S Colombi and Colombo, \{L P L\} and F Couchot and A Coulais and Crill, \{B P\} and A Curto and F Cuttaia and L Danese and Davies, \{R D\} and \{de Bernardis\}, P and \{de Rosa\}, A and \{de Zotti\}, G and J Delabrouille and J-M Delouis and F-X D{\`E}sert and Diego, \{J M\} and H Dole and S Donzelli and O Dor{\`E} and M Douspis and X Dupac and G Efstathiou and Enﬂlin, \{T A\} and Eriksen, \{H K\} and F Finelli and O Forni and M Frailis and E Franceschi and S Galeotta and K Ganga and M Giard and G Giardino and Y Giraud-H{\`E}raud and J Gonz·lez-Nuevo and G{\^U}rski, \{K M\} and S Gratton and A Gregorio and A Gruppuso and Gudmundsson, \{J E\} and Hansen, \{F K\} and D Hanson and D Harrison and S Henrot-Versill{\`E} and C Hern·ndez-Monteagudo and D Herranz and Hildebrandt, \{S R\} and E Hivon and M Hobson and Holmes, \{W A\} and A Hornstrup and W Hovest and Huffenberger, \{K M\} and Jaffe, \{A H\} and Jaffe, \{T R\} and Jones, \{W C\} and M Juvela and E Keih‰nen and R Keskitalo and Kisner, \{T S\} and R Kneissl and J Knoche and L Knox and M Kunz and H Kurki-Suonio and F Lacasa and G Lagache and A L‰hteenm‰ki and J-M Lamarre and A Lasenby and Laureijs, \{R J\} and Lawrence, \{C R\} and R Leonardi and J Le{\^U}n-Tavares and J Lesgourgues and M Liguori and Lilje, \{P B\} and M Linden-V¯rnle and M L{\^U}pez-Caniego and Lubin, \{P M\} and Mac{\`I}as-P{\`E}rez, \{J F\} and B Maffei and D Maino and N Mandolesi and M Maris and Marshall, \{D J\} and Martin, \{P G\} and E Mart{\`I}nez-Gonz·lez and S Masi and M Massardi and S Matarrese and F Matthai and P Mazzotta and A Melchiorri and L Mendes and A Mennella and M Migliaccio and S Mitra and M-A Miville-Desch{\'I}nes and A Moneti and L Montier and G Morgante and D Mortlock and D Munshi and P Naselsky and F Nati and P Natoli and Netterfield, \{C B\} and N¯rgaard-Nielsen, \{H U\} and F Noviello and D Novikov and I Novikov and S Osborne and Oxborrow, \{C A\} and F Paci and L Pagano and F Pajot and D Paoletti and F Pasian and G Patanchon and O Perdereau and L Perotto and F Perrotta and F Piacentini and M Piat and E Pierpaoli and D Pietrobon and S Plaszczynski and E Pointecouteau and G Polenta and N Ponthieu and L Popa and T Poutanen and Pratt, \{G W\} and G Pr{\`E}zeau and S Prunet and J-L Puget and Rachen, \{J P\} and R Rebolo and M Reinecke and M Remazeilles and C Renault and S Ricciardi and T Riller and I Ristorcelli and G Rocha and C Rosset and G Roudier and M Rowan-Robinson and B Rusholme and M Sandri and D Santos and G Savini and D Scott and Seiffert, \{M D\} and P Serra and Shellard, \{E P S\} and Spencer, \{L D\} and J-L Starck and V Stolyarov and R Stompor and R Sudiwala and R Sunyaev and F Sureau and D Sutton and A-S Suur-Uski and J-F Sygnet and Tauber, \{J A\} and D Tavagnacco and L Terenzi and L Toffolatti and M Tomasi and M Tristram and M Tucci and J Tuovinen and L Valenziano and J Valiviita and \{Van Tent\}, B and P Vielva and F Villa and N Vittorio and Wade, \{L A\} and Wandelt, \{B D\} and White, \{S D M\} and D Yvon and A Zacchei and A Zonca",

year = "2014",

language = "English",

volume = "571",

journal = "Astronomy and Astrophysics",

issn = "1432-0746",

publisher = "EDP Sciences",

}

Collaboration, P, Ade, PAR, Aghanim, N, Armitage-Caplan, C, Arnaud, M, Ashdown, M, Atrio-Barandela, F, Aumont, J, Baccigalupi, C, Banday, AJ, Barreiro, RB, Bartlett, JG, Basak, S, Battaner, E, Benabed, K, BenoÓt, A, Benoit-LÈvy, A, Bernard, J-P, Bersanelli, M, Bethermin, M, Bielewicz, P, Bobin, J, Bock, JJ, Bonaldi, A, Bond, JR, Borrill, J, Bouchet, FR, Boulanger, F, Bridges, M, Bucher, M, Burigana, C, Butler, RC, Cardoso, J-F, Catalano, A, Challinor, A, Chamballu, A, Chiang, HC, Chiang, L-Y, Christensen, PR, Church, S, Clements, DL, Colombi, S, Colombo, LPL, Couchot, F, Coulais, A, Crill, BP, Curto, A, Cuttaia, F, Danese, L, Davies, RD, de Bernardis, P, de Rosa, A, de Zotti, G, Delabrouille, J, Delouis, J-M, DÈsert, F-X, Diego, JM, Dole, H, Donzelli, S, DorÈ, O, Douspis, M, Dupac, X, Efstathiou, G, Enﬂlin, TA, Eriksen, HK, Finelli, F, Forni, O, Frailis, M, Franceschi, E, Galeotta, S, Ganga, K, Giard, M, Giardino, G, Giraud-HÈraud, Y, Gonz·lez-Nuevo, J, GÛrski, KM, Gratton, S, Gregorio, A, Gruppuso, A, Gudmundsson, JE, Hansen, FK, Hanson, D, Harrison, D, Henrot-VersillÈ, S, Hern·ndez-Monteagudo, C, Herranz, D, Hildebrandt, SR, Hivon, E, Hobson, M, Holmes, WA, Hornstrup, A, Hovest, W, Huffenberger, KM, Jaffe, AH, Jaffe, TR, Jones, WC, Juvela, M, Keih‰nen, E, Keskitalo, R, Kisner, TS, Kneissl, R, Knoche, J, Knox, L, Kunz, M, Kurki-Suonio, H, Lacasa, F, Lagache, G, L‰hteenm‰ki, A, Lamarre, J-M, Lasenby, A, Laureijs, RJ, Lawrence, CR, Leonardi, R, LeÛn-Tavares, J, Lesgourgues, J, Liguori, M, Lilje, PB, Linden-V¯rnle, M, LÛpez-Caniego, M, Lubin, PM, MacÌas-PÈrez, JF, Maffei, B, Maino, D, Mandolesi, N, Maris, M, Marshall, DJ, Martin, PG, MartÌnez-Gonz·lez, E, Masi, S, Massardi, M, Matarrese, S, Matthai, F, Mazzotta, P, Melchiorri, A, Mendes, L, Mennella, A, Migliaccio, M, Mitra, S, Miville-DeschÍnes, M-A, Moneti, A, Montier, L, Morgante, G, Mortlock, D, Munshi, D, Naselsky, P, Nati, F, Natoli, P, Netterfield, CB, N¯rgaard-Nielsen, HU, Noviello, F, Novikov, D, Novikov, I, Osborne, S, Oxborrow, CA, Paci, F, Pagano, L, Pajot, F, Paoletti, D, Pasian, F, Patanchon, G, Perdereau, O, Perotto, L, Perrotta, F, Piacentini, F, Piat, M, Pierpaoli, E, Pietrobon, D, Plaszczynski, S, Pointecouteau, E, Polenta, G, Ponthieu, N, Popa, L, Poutanen, T, Pratt, GW, PrÈzeau, G, Prunet, S, Puget, J-L, Rachen, JP, Rebolo, R, Reinecke, M, Remazeilles, M, Renault, C, Ricciardi, S, Riller, T, Ristorcelli, I, Rocha, G, Rosset, C, Roudier, G, Rowan-Robinson, M, Rusholme, B, Sandri, M, Santos, D, Savini, G, Scott, D, Seiffert, MD, Serra, P, Shellard, EPS, Spencer, LD, Starck, J-L, Stolyarov, V, Stompor, R, Sudiwala, R, Sunyaev, R, Sureau, F, Sutton, D, Suur-Uski, A-S, Sygnet, J-F, Tauber, JA, Tavagnacco, D, Terenzi, L, Toffolatti, L, Tomasi, M, Tristram, M, Tucci, M, Tuovinen, J, Valenziano, L, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Vittorio, N, Wade, LA, Wandelt, BD, White, SDM, Yvon, D, Zacchei, A & Zonca, A 2014, 'Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation', Astronomy and Astrophysics, vol. 571. <http://adsabs.harvard.edu/abs/2014A%26A...571A..18P>

TY - JOUR

T1 - Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation

AU - Collaboration, Planck

AU - Ade, P A R

AU - Aghanim, N

AU - Armitage-Caplan, C

AU - Arnaud, M

AU - Ashdown, M

AU - Atrio-Barandela, F

AU - Aumont, J

AU - Baccigalupi, C

AU - Banday, A J

AU - Barreiro, R B

AU - Bartlett, J G

AU - Basak, S

AU - Battaner, E

AU - Benabed, K

AU - BenoÓt, A

AU - Benoit-LÈvy, A

AU - Bernard, J-P

AU - Bersanelli, M

AU - Bethermin, M

AU - Bielewicz, P

AU - Bobin, J

AU - Bock, J J

AU - Bonaldi, A

AU - Bond, J R

AU - Borrill, J

AU - Bouchet, F R

AU - Boulanger, F

AU - Bridges, M

AU - Bucher, M

AU - Burigana, C

AU - Butler, R C

AU - Cardoso, J-F

AU - Catalano, A

AU - Challinor, A

AU - Chamballu, A

AU - Chiang, H C

AU - Chiang, L-Y

AU - Christensen, P R

AU - Church, S

AU - Clements, D L

AU - Colombi, S

AU - Colombo, L P L

AU - Couchot, F

AU - Coulais, A

AU - Crill, B P

AU - Curto, A

AU - Cuttaia, F

AU - Danese, L

AU - Davies, R D

AU - de Bernardis, P

AU - de Rosa, A

AU - de Zotti, G

AU - Delabrouille, J

AU - Delouis, J-M

AU - DÈsert, F-X

AU - Diego, J M

AU - Dole, H

AU - Donzelli, S

AU - DorÈ, O

AU - Douspis, M

AU - Dupac, X

AU - Efstathiou, G

AU - Enﬂlin, T A

AU - Eriksen, H K

AU - Finelli, F

AU - Forni, O

AU - Frailis, M

AU - Franceschi, E

AU - Galeotta, S

AU - Ganga, K

AU - Giard, M

AU - Giardino, G

AU - Giraud-HÈraud, Y

AU - Gonz·lez-Nuevo, J

AU - GÛrski, K M

AU - Gratton, S

AU - Gregorio, A

AU - Gruppuso, A

AU - Gudmundsson, J E

AU - Hansen, F K

AU - Hanson, D

AU - Harrison, D

AU - Henrot-VersillÈ, S

AU - Hern·ndez-Monteagudo, C

AU - Herranz, D

AU - Hildebrandt, S R

AU - Hivon, E

AU - Hobson, M

AU - Holmes, W A

AU - Hornstrup, A

AU - Hovest, W

AU - Huffenberger, K M

AU - Jaffe, A H

AU - Jaffe, T R

AU - Jones, W C

AU - Juvela, M

AU - Keih‰nen, E

AU - Keskitalo, R

AU - Kisner, T S

AU - Kneissl, R

AU - Knoche, J

AU - Knox, L

AU - Kunz, M

AU - Kurki-Suonio, H

AU - Lacasa, F

AU - Lagache, G

AU - L‰hteenm‰ki, A

AU - Lamarre, J-M

AU - Lasenby, A

AU - Laureijs, R J

AU - Lawrence, C R

AU - Leonardi, R

AU - LeÛn-Tavares, J

AU - Lesgourgues, J

AU - Liguori, M

AU - Lilje, P B

AU - Linden-V¯rnle, M

AU - LÛpez-Caniego, M

AU - Lubin, P M

AU - MacÌas-PÈrez, J F

AU - Maffei, B

AU - Maino, D

AU - Mandolesi, N

AU - Maris, M

AU - Marshall, D J

AU - Martin, P G

AU - MartÌnez-Gonz·lez, E

AU - Masi, S

AU - Massardi, M

AU - Matarrese, S

AU - Matthai, F

AU - Mazzotta, P

AU - Melchiorri, A

AU - Mendes, L

AU - Mennella, A

AU - Migliaccio, M

AU - Mitra, S

AU - Miville-DeschÍnes, M-A

AU - Moneti, A

AU - Montier, L

AU - Morgante, G

AU - Mortlock, D

AU - Munshi, D

AU - Naselsky, P

AU - Nati, F

AU - Natoli, P

AU - Netterfield, C B

AU - N¯rgaard-Nielsen, H U

AU - Noviello, F

AU - Novikov, D

AU - Novikov, I

AU - Osborne, S

AU - Oxborrow, C A

AU - Paci, F

AU - Pagano, L

AU - Pajot, F

AU - Paoletti, D

AU - Pasian, F

AU - Patanchon, G

AU - Perdereau, O

AU - Perotto, L

AU - Perrotta, F

AU - Piacentini, F

AU - Piat, M

AU - Pierpaoli, E

AU - Pietrobon, D

AU - Plaszczynski, S

AU - Pointecouteau, E

AU - Polenta, G

AU - Ponthieu, N

AU - Popa, L

AU - Poutanen, T

AU - Pratt, G W

AU - PrÈzeau, G

AU - Prunet, S

AU - Puget, J-L

AU - Rachen, J P

AU - Rebolo, R

AU - Reinecke, M

AU - Remazeilles, M

AU - Renault, C

AU - Ricciardi, S

AU - Riller, T

AU - Ristorcelli, I

AU - Rocha, G

AU - Rosset, C

AU - Roudier, G

AU - Rowan-Robinson, M

AU - Rusholme, B

AU - Sandri, M

AU - Santos, D

AU - Savini, G

AU - Scott, D

AU - Seiffert, M D

AU - Serra, P

AU - Shellard, E P S

AU - Spencer, L D

AU - Starck, J-L

AU - Stolyarov, V

AU - Stompor, R

AU - Sudiwala, R

AU - Sunyaev, R

AU - Sureau, F

AU - Sutton, D

AU - Suur-Uski, A-S

AU - Sygnet, J-F

AU - Tauber, J A

AU - Tavagnacco, D

AU - Terenzi, L

AU - Toffolatti, L

AU - Tomasi, M

AU - Tristram, M

AU - Tucci, M

AU - Tuovinen, J

AU - Valenziano, L

AU - Valiviita, J

AU - Van Tent, B

AU - Vielva, P

AU - Villa, F

AU - Vittorio, N

AU - Wade, L A

AU - Wandelt, B D

AU - White, S D M

AU - Yvon, D

AU - Zacchei, A

AU - Zonca, A

PY - 2014

Y1 - 2014

N2 - The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). The conjunction of these two unique probes allows us to measure directly the connection between dark and luminous matter in the high redshift (1 10(M/M&sun;) = 10.5 ± 0.6. Leveraging the frequency dependence of our signal, we isolate the high redshift contribution to the CIB, and constrain the star formation rate (SFR) density at z >= 1. We measure directly the SFR density with around 2sigma significance for three redshift bins between z = 1 and 7, thus opening a new window into the study of the formation of stars at early times.

AB - The multi-frequency capability of the Planck satellite provides information both on the integrated history of star formation (via the cosmic infrared background, or CIB) and on the distribution of dark matter (via the lensing effect on the cosmic microwave background, or CMB). The conjunction of these two unique probes allows us to measure directly the connection between dark and luminous matter in the high redshift (1 10(M/M&sun;) = 10.5 ± 0.6. Leveraging the frequency dependence of our signal, we isolate the high redshift contribution to the CIB, and constrain the star formation rate (SFR) density at z >= 1. We measure directly the SFR density with around 2sigma significance for three redshift bins between z = 1 and 7, thus opening a new window into the study of the formation of stars at early times.

KW - gravitational lensing: weak

KW - cosmic background radiation

KW - large-scale

KW - structure of Universe

KW - dark matter

KW - galaxies: star formation

UR - https://www.scopus.com/pages/publications/84908667800

M3 - Article

SN - 1432-0746

SN - 2329-1265

VL - 571

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

ER -

Planck 2013 results. XVIII. The gravitational lensing-infrared background correlation

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