Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

Y. Akrami; M. Ashdown; J. Aumont; C. Baccigalupi; M. Ballardini; A. J. Banday; R. B. Barreiro; N. Bartolo; S. Basak; K. Benabed; J. P. Bernard; M. Bersanelli; P. Bielewicz; J. R. Bond; J. Borrill; F. R. Bouchet; C. Burigana; E. Calabrese; J. F. Cardoso; B. Casaponsa; H. C. Chiang; C. Combet; D. Contreras; B. P. Crill; F. Cuttaia; P. De Bernardis; A. De Rosa; G. De Zotti; J. Delabrouille; E. Di Valentino; J. M. Diego; O. Doré; M. Douspis; X. Dupac; T. A. Enßlin; H. K. Eriksen; R. Fernandez-Cobos; F. Finelli; M. Frailis; E. Franceschi; A. Frolov; S. Galeotta; S. Galli; K. Ganga; R. T. Génova-Santos; M. Gerbino; J. González-Nuevo; K. M. Górski; A. Gruppuso; J. E. Gudmundsson; W. Handley; D. Herranz; E. Hivon; Z. Huang; A. H. Jaffe; W. C. Jones; E. Keihänen; R. Keskitalo; K. Kiiveri; J. Kim; T. S. Kisner; N. Krachmalnicoff; M. Kunz; H. Kurki-Suonio; J. M. Lamarre; M. Lattanzi; C. R. Lawrence; M. Le Jeune; F. Levrier; M. Liguori; P. B. Lilje; V. Lindholm; M. López-Caniego; J. F. Maciás-Pérez; D. Maino; N. Mandolesi; A. Marcos-Caballero; M. Maris; P. G. Martin; E. Martínez-González; S. Matarrese; N. Mauri; J. D. McEwen; A. Mennella; M. Migliaccio; D. Molinari; A. Moneti; L. Montier; G. Morgante; A. Moss; P. Natoli; L. Pagano; D. Paoletti; F. Perrotta; V. Pettorino; F. Piacentini; G. Polenta; J. P. Rachen; M. Reinecke; M. Remazeilles; A. Renzi; G. Roha; C. Roset; J. A. Rubiño-Martín; B. Ruiz-Granados; L. Salvati; M. Savelainen; D. Scott; C. Sirignano; G. Sirri; L. D. Spencer; R. M. Sullivan; R. Sunyaev; A. S. Suur-Uski; J. A. Tauber; D. Tavagnacco; M. Tenti; L. Toffolatti; M. Tomasi; T. Trombetti; J. Valiviita; B. Van Tent; P. Vielva; F. Villa; N. Vittorio; I. K. Wehus; A. Zacchei; A. Zonca

doi:10.1051/0004-6361/202038053

Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

Y. Akrami
, M. Ashdown
, J. Aumont
, C. Baccigalupi
, M. Ballardini
, A. J. Banday
, R. B. Barreiro
, N. Bartolo
, S. Basak
, K. Benabed
, J. P. Bernard
, M. Bersanelli
, P. Bielewicz
, J. R. Bond
, J. Borrill
, F. R. Bouchet
, C. Burigana
, E. Calabrese
, J. F. Cardoso
, B. Casaponsa

H. C. Chiang, C. Combet, D. Contreras, B. P. Crill, F. Cuttaia, P. De Bernardis, A. De Rosa, G. De Zotti, J. Delabrouille, E. Di Valentino, J. M. Diego, O. Doré, M. Douspis, X. Dupac, T. A. Enßlin, H. K. Eriksen, R. Fernandez-Cobos, F. Finelli, M. Frailis, E. Franceschi, A. Frolov, S. Galeotta, S. Galli, K. Ganga, R. T. Génova-Santos, M. Gerbino, J. González-Nuevo, K. M. Górski, A. Gruppuso, J. E. Gudmundsson, W. Handley, D. Herranz, E. Hivon, Z. Huang, A. H. Jaffe, W. C. Jones, E. Keihänen, R. Keskitalo, K. Kiiveri, J. Kim, T. S. Kisner, N. Krachmalnicoff, M. Kunz, H. Kurki-Suonio, J. M. Lamarre, M. Lattanzi, C. R. Lawrence, M. Le Jeune, F. Levrier, M. Liguori, P. B. Lilje, V. Lindholm, M. López-Caniego, J. F. Maciás-Pérez, D. Maino, N. Mandolesi, A. Marcos-Caballero, M. Maris, P. G. Martin, E. Martínez-González, S. Matarrese, N. Mauri, J. D. McEwen, A. Mennella, M. Migliaccio, D. Molinari, A. Moneti, L. Montier, G. Morgante, A. Moss, P. Natoli, L. Pagano, D. Paoletti, F. Perrotta, V. Pettorino, F. Piacentini, G. Polenta, J. P. Rachen, M. Reinecke, M. Remazeilles, A. Renzi, G. Roha, C. Roset, J. A. Rubiño-Martín, B. Ruiz-Granados, L. Salvati, M. Savelainen, D. Scott, C. Sirignano, G. Sirri, L. D. Spencer, R. M. Sullivan, R. Sunyaev, A. S. Suur-Uski, J. A. Tauber, D. Tavagnacco, M. Tenti, L. Toffolatti, M. Tomasi, T. Trombetti, J. Valiviita, B. Van Tent, P. Vielva, F. Villa, N. Vittorio, I. K. Wehus, A. Zacchei, A. Zonca

Faculty of Physical Sciences

University of Iceland

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

Abstract

The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole is that it is due to our motion with respect to the rest frame of the CMB. Since current CMB experiments infer temperature anisotropies from angular intensity variations, the dipole modulates the temperature anisotropies with the same frequency dependence as the thermal Sunyaev-Zeldovich (tSZ) effect. We present the first, and significant, detection of this signal in the tSZ maps and find that it is consistent with direct measurements of the CMB dipole, as expected. The signal contributes power in the tSZ maps, which is modulated in a quadrupolar pattern, and we estimate its contribution to the tSZ bispectrum, noting that it contributes negligible noise to the bispectrum at relevant scales.

Original language	English
Article number	A100
Journal	Astronomy and Astrophysics
Volume	644
DOIs	https://doi.org/10.1051/0004-6361/202038053
Publication status	Published - 1 Dec 2020

Bibliographical note

Funding Information: Acknowledgements. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/ planck-collaboration. Some of the results in this paper have been derived using the HEALPix package and the NaMaster package and some plots were generated using the pygtc package. Funding Information: ★ Corresponding author: R. M. Sullivan, e-mail: [email protected] 1 Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA) with instruments provided by two scientific consortia funded by ESA member states and led by Principal Investigators from France and Italy, telescope reflectors provided through a collaboration between ESA and a scientific consortium led and funded by Denmark, and additional contributions from NASA (USA). Publisher Copyright: © ESO 2020.

Other keywords

Cosmic background radiation
Cosmology: observations
Reference systems
Relativistic processes

Access to Document

10.1051/0004-6361/202038053

Cite this

Akrami, Y., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A. J., Barreiro, R. B., Bartolo, N., Basak, S., Benabed, K., Bernard, J. P., Bersanelli, M., Bielewicz, P., Bond, J. R., Borrill, J., Bouchet, F. R., Burigana, C., Calabrese, E., Cardoso, J. F., ... Zonca, A. (2020). Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II. Astronomy and Astrophysics, 644, Article A100. https://doi.org/10.1051/0004-6361/202038053

@article{b7d179e328824f2aac7e77d762a874d9,

title = "Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II",

abstract = "The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole is that it is due to our motion with respect to the rest frame of the CMB. Since current CMB experiments infer temperature anisotropies from angular intensity variations, the dipole modulates the temperature anisotropies with the same frequency dependence as the thermal Sunyaev-Zeldovich (tSZ) effect. We present the first, and significant, detection of this signal in the tSZ maps and find that it is consistent with direct measurements of the CMB dipole, as expected. The signal contributes power in the tSZ maps, which is modulated in a quadrupolar pattern, and we estimate its contribution to the tSZ bispectrum, noting that it contributes negligible noise to the bispectrum at relevant scales.",

keywords = "Cosmic background radiation, Cosmology: observations, Reference systems, Relativistic processes",

author = "Y. Akrami and M. Ashdown and J. Aumont and C. Baccigalupi and M. Ballardini and Banday, \{A. J.\} and Barreiro, \{R. B.\} and N. Bartolo and S. Basak and K. Benabed and Bernard, \{J. P.\} and M. Bersanelli and P. Bielewicz and Bond, \{J. R.\} and J. Borrill and Bouchet, \{F. R.\} and C. Burigana and E. Calabrese and Cardoso, \{J. F.\} and B. Casaponsa and Chiang, \{H. C.\} and C. Combet and D. Contreras and Crill, \{B. P.\} and F. Cuttaia and \{De Bernardis\}, P. and \{De Rosa\}, A. and \{De Zotti\}, G. and J. Delabrouille and \{Di Valentino\}, E. and Diego, \{J. M.\} and O. Dor{\'e} and M. Douspis and X. Dupac and En{\ss}lin, \{T. A.\} and Eriksen, \{H. K.\} and R. Fernandez-Cobos and F. Finelli and M. Frailis and E. Franceschi and A. Frolov and S. Galeotta and S. Galli and K. Ganga and G{\'e}nova-Santos, \{R. T.\} and M. Gerbino and J. Gonz{\'a}lez-Nuevo and G{\'o}rski, \{K. M.\} and A. Gruppuso and Gudmundsson, \{J. E.\} and W. Handley and D. Herranz and E. Hivon and Z. Huang and Jaffe, \{A. H.\} and Jones, \{W. C.\} and E. Keih{\"a}nen and R. Keskitalo and K. Kiiveri and J. Kim and Kisner, \{T. S.\} and N. Krachmalnicoff and M. Kunz and H. Kurki-Suonio and Lamarre, \{J. M.\} and M. Lattanzi and Lawrence, \{C. R.\} and \{Le Jeune\}, M. and F. Levrier and M. Liguori and Lilje, \{P. B.\} and V. Lindholm and M. L{\'o}pez-Caniego and Maci{\'a}s-P{\'e}rez, \{J. F.\} and D. Maino and N. Mandolesi and A. Marcos-Caballero and M. Maris and Martin, \{P. G.\} and E. Mart{\'i}nez-Gonz{\'a}lez and S. Matarrese and N. Mauri and McEwen, \{J. D.\} and A. Mennella and M. Migliaccio and D. Molinari and A. Moneti and L. Montier and G. Morgante and A. Moss and P. Natoli and L. Pagano and D. Paoletti and F. Perrotta and V. Pettorino and F. Piacentini and G. Polenta and Rachen, \{J. P.\} and M. Reinecke and M. Remazeilles and A. Renzi and G. Roha and C. Roset and Rubi{\~n}o-Mart{\'i}n, \{J. A.\} and B. Ruiz-Granados and L. Salvati and M. Savelainen and D. Scott and C. Sirignano and G. Sirri and Spencer, \{L. D.\} and Sullivan, \{R. M.\} and R. Sunyaev and Suur-Uski, \{A. S.\} and Tauber, \{J. A.\} and D. Tavagnacco and M. Tenti and L. Toffolatti and M. Tomasi and T. Trombetti and J. Valiviita and \{Van Tent\}, B. and P. Vielva and F. Villa and N. Vittorio and Wehus, \{I. K.\} and A. Zacchei and A. Zonca",

note = "Funding Information: Acknowledgements. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/ planck-collaboration. Some of the results in this paper have been derived using the HEALPix package and the NaMaster package and some plots were generated using the pygtc package. Funding Information: ★ Corresponding author: R. M. Sullivan, e-mail: [email protected] 1 Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA) with instruments provided by two scientific consortia funded by ESA member states and led by Principal Investigators from France and Italy, telescope reflectors provided through a collaboration between ESA and a scientific consortium led and funded by Denmark, and additional contributions from NASA (USA). Publisher Copyright: {\textcopyright} ESO 2020.",

year = "2020",

month = dec,

day = "1",

doi = "10.1051/0004-6361/202038053",

language = "English",

volume = "644",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Akrami, Y, Ashdown, M, Aumont, J, Baccigalupi, C, Ballardini, M, Banday, AJ, Barreiro, RB, Bartolo, N, Basak, S, Benabed, K, Bernard, JP, Bersanelli, M, Bielewicz, P, Bond, JR, Borrill, J, Bouchet, FR, Burigana, C, Calabrese, E, Cardoso, JF, Casaponsa, B, Chiang, HC, Combet, C, Contreras, D, Crill, BP, Cuttaia, F, De Bernardis, P, De Rosa, A, De Zotti, G, Delabrouille, J, Di Valentino, E, Diego, JM, Doré, O, Douspis, M, Dupac, X, Enßlin, TA, Eriksen, HK, Fernandez-Cobos, R, Finelli, F, Frailis, M, Franceschi, E, Frolov, A, Galeotta, S, Galli, S, Ganga, K, Génova-Santos, RT, Gerbino, M, González-Nuevo, J, Górski, KM, Gruppuso, A, Gudmundsson, JE, Handley, W, Herranz, D, Hivon, E, Huang, Z, Jaffe, AH, Jones, WC, Keihänen, E, Keskitalo, R, Kiiveri, K, Kim, J, Kisner, TS, Krachmalnicoff, N, Kunz, M, Kurki-Suonio, H, Lamarre, JM, Lattanzi, M, Lawrence, CR, Le Jeune, M, Levrier, F, Liguori, M, Lilje, PB, Lindholm, V, López-Caniego, M, Maciás-Pérez, JF, Maino, D, Mandolesi, N, Marcos-Caballero, A, Maris, M, Martin, PG, Martínez-González, E, Matarrese, S, Mauri, N, McEwen, JD, Mennella, A, Migliaccio, M, Molinari, D, Moneti, A, Montier, L, Morgante, G, Moss, A, Natoli, P, Pagano, L, Paoletti, D, Perrotta, F, Pettorino, V, Piacentini, F, Polenta, G, Rachen, JP, Reinecke, M, Remazeilles, M, Renzi, A, Roha, G, Roset, C, Rubiño-Martín, JA, Ruiz-Granados, B, Salvati, L, Savelainen, M, Scott, D, Sirignano, C, Sirri, G, Spencer, LD, Sullivan, RM, Sunyaev, R, Suur-Uski, AS, Tauber, JA, Tavagnacco, D, Tenti, M, Toffolatti, L, Tomasi, M, Trombetti, T, Valiviita, J, Van Tent, B, Vielva, P, Villa, F, Vittorio, N, Wehus, IK, Zacchei, A & Zonca, A 2020, 'Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II', Astronomy and Astrophysics, vol. 644, A100. https://doi.org/10.1051/0004-6361/202038053

TY - JOUR

T1 - Planck intermediate results

T2 - LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

AU - Akrami, Y.

AU - Ashdown, M.

AU - Aumont, J.

AU - Baccigalupi, C.

AU - Ballardini, M.

AU - Banday, A. J.

AU - Barreiro, R. B.

AU - Bartolo, N.

AU - Basak, S.

AU - Benabed, K.

AU - Bernard, J. P.

AU - Bersanelli, M.

AU - Bielewicz, P.

AU - Bond, J. R.

AU - Borrill, J.

AU - Bouchet, F. R.

AU - Burigana, C.

AU - Calabrese, E.

AU - Cardoso, J. F.

AU - Casaponsa, B.

AU - Chiang, H. C.

AU - Combet, C.

AU - Contreras, D.

AU - Crill, B. P.

AU - Cuttaia, F.

AU - De Bernardis, P.

AU - De Rosa, A.

AU - De Zotti, G.

AU - Delabrouille, J.

AU - Di Valentino, E.

AU - Diego, J. M.

AU - Doré, O.

AU - Douspis, M.

AU - Dupac, X.

AU - Enßlin, T. A.

AU - Eriksen, H. K.

AU - Fernandez-Cobos, R.

AU - Finelli, F.

AU - Frailis, M.

AU - Franceschi, E.

AU - Frolov, A.

AU - Galeotta, S.

AU - Galli, S.

AU - Ganga, K.

AU - Génova-Santos, R. T.

AU - Gerbino, M.

AU - González-Nuevo, J.

AU - Górski, K. M.

AU - Gruppuso, A.

AU - Gudmundsson, J. E.

AU - Handley, W.

AU - Herranz, D.

AU - Hivon, E.

AU - Huang, Z.

AU - Jaffe, A. H.

AU - Jones, W. C.

AU - Keihänen, E.

AU - Keskitalo, R.

AU - Kiiveri, K.

AU - Kim, J.

AU - Kisner, T. S.

AU - Krachmalnicoff, N.

AU - Kunz, M.

AU - Kurki-Suonio, H.

AU - Lamarre, J. M.

AU - Lattanzi, M.

AU - Lawrence, C. R.

AU - Le Jeune, M.

AU - Levrier, F.

AU - Liguori, M.

AU - Lilje, P. B.

AU - Lindholm, V.

AU - López-Caniego, M.

AU - Maciás-Pérez, J. F.

AU - Maino, D.

AU - Mandolesi, N.

AU - Marcos-Caballero, A.

AU - Maris, M.

AU - Martin, P. G.

AU - Martínez-González, E.

AU - Matarrese, S.

AU - Mauri, N.

AU - McEwen, J. D.

AU - Mennella, A.

AU - Migliaccio, M.

AU - Molinari, D.

AU - Moneti, A.

AU - Montier, L.

AU - Morgante, G.

AU - Moss, A.

AU - Natoli, P.

AU - Pagano, L.

AU - Paoletti, D.

AU - Perrotta, F.

AU - Pettorino, V.

AU - Piacentini, F.

AU - Polenta, G.

AU - Rachen, J. P.

AU - Reinecke, M.

AU - Remazeilles, M.

AU - Renzi, A.

AU - Roha, G.

AU - Roset, C.

AU - Rubiño-Martín, J. A.

AU - Ruiz-Granados, B.

AU - Salvati, L.

AU - Savelainen, M.

AU - Scott, D.

AU - Sirignano, C.

AU - Sirri, G.

AU - Spencer, L. D.

AU - Sullivan, R. M.

AU - Sunyaev, R.

AU - Suur-Uski, A. S.

AU - Tauber, J. A.

AU - Tavagnacco, D.

AU - Tenti, M.

AU - Toffolatti, L.

AU - Tomasi, M.

AU - Trombetti, T.

AU - Valiviita, J.

AU - Van Tent, B.

AU - Vielva, P.

AU - Villa, F.

AU - Vittorio, N.

AU - Wehus, I. K.

AU - Zacchei, A.

AU - Zonca, A.

N1 - Funding Information: Acknowledgements. The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, JA, and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/ planck-collaboration. Some of the results in this paper have been derived using the HEALPix package and the NaMaster package and some plots were generated using the pygtc package. Funding Information: ★ Corresponding author: R. M. Sullivan, e-mail: [email protected] 1 Planck (http://www.esa.int/Planck) is a project of the European Space Agency (ESA) with instruments provided by two scientific consortia funded by ESA member states and led by Principal Investigators from France and Italy, telescope reflectors provided through a collaboration between ESA and a scientific consortium led and funded by Denmark, and additional contributions from NASA (USA). Publisher Copyright: © ESO 2020.

PY - 2020/12/1

Y1 - 2020/12/1

N2 - The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole is that it is due to our motion with respect to the rest frame of the CMB. Since current CMB experiments infer temperature anisotropies from angular intensity variations, the dipole modulates the temperature anisotropies with the same frequency dependence as the thermal Sunyaev-Zeldovich (tSZ) effect. We present the first, and significant, detection of this signal in the tSZ maps and find that it is consistent with direct measurements of the CMB dipole, as expected. The signal contributes power in the tSZ maps, which is modulated in a quadrupolar pattern, and we estimate its contribution to the tSZ bispectrum, noting that it contributes negligible noise to the bispectrum at relevant scales.

AB - The largest temperature anisotropy in the cosmic microwave background (CMB) is the dipole, which has been measured with increasing accuracy for more than three decades, particularly with the Planck satellite. The simplest interpretation of the dipole is that it is due to our motion with respect to the rest frame of the CMB. Since current CMB experiments infer temperature anisotropies from angular intensity variations, the dipole modulates the temperature anisotropies with the same frequency dependence as the thermal Sunyaev-Zeldovich (tSZ) effect. We present the first, and significant, detection of this signal in the tSZ maps and find that it is consistent with direct measurements of the CMB dipole, as expected. The signal contributes power in the tSZ maps, which is modulated in a quadrupolar pattern, and we estimate its contribution to the tSZ bispectrum, noting that it contributes negligible noise to the bispectrum at relevant scales.

KW - Cosmic background radiation

KW - Cosmology: observations

KW - Reference systems

KW - Relativistic processes

UR - https://www.scopus.com/pages/publications/85097877481

U2 - 10.1051/0004-6361/202038053

DO - 10.1051/0004-6361/202038053

M3 - Article

SN - 0004-6361

VL - 644

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A100

ER -

Planck intermediate results: LVI. Detection of the CMB dipole through modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II

Abstract

Bibliographical note

Other keywords

Access to Document

Fingerprint

Cite this