Imperial College London
Alternate

Professor Andrew H Jaffe

Faculty of Natural Sciences, Department of Physics

Professor of Astrophysics and Cosmology
 
 
 
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Contact

 

+44 (0)20 7594 7526a.jaffe Website

 
 
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Assistant

 

Miss Louise Hayward +44 (0)20 7594 7679

 
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Location

 

1018BBlackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@unpublished{Collaboration:2020,
author = {Collaboration, P and Akrami, Y and Ashdown, M and Aumont, J and Baccigalupi, C and Ballardini, M and Banday, AJ and Barreiro, RB and Bartolo, N and Basak, S and Benabed, K and Bernard, J-P and Bersanelli, M and Bielewicz, P and Bond, JR and Borrill, J and Bouchet, FR and Burigana, C and Calabrese, E and Cardoso, J-F and Casaponsa, B and Chiang, HC and Combet, C and Contreras, D and Crill, BP and Cuttaia, F and Bernardis, PD and Rosa, AD and Zotti, GD and Delabrouille, J and Valentino, ED and Diego, JM and Doré, O and Douspis, M and Dupac, X and Enßlin, TA and Eriksen, HK and Fernandez-Cobos, R and Finelli, F and Frailis, M and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ganga, K and Génova-Santos, RT and Gerbino, M and González-Nuevo, J and Górski, KM and Gruppuso, A and Gudmundsson, JE and Handley, W and Herranz, D and Hivon, E and Huang, Z and Jaffe, AH and Jones, WC and Keihänen, E and Keskitalo, R and Kiiveri, K and Kim, J and Kisner, TS and Krachmalnicoff, N and K},
publisher = {arXiv},
title = {Planck intermediate results. LVI. Detection of the CMB dipole through  modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II},
url = {http://arxiv.org/abs/2003.12646v2},
year = {2020}
}
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RIS format (EndNote, RefMan)

TY  - UNPB
AB  - The largest temperature anisotropy in the cosmic microwave background (CMB)is the dipole, which has been measured with increasing accuracy for more thanthree decades, particularly with the Planck satellite. The simplestinterpretation of the dipole is that it is due to our motion with respect tothe rest frame of the CMB. Since current CMB experiments infer temperatureanisotropies from angular intensity variations, the dipole modulates thetemperature anisotropies with the same frequency dependence as the thermalSunyaev-Zeldovich (tSZ) effect. We present the first, and significant,detection of this signal in the tSZ maps and find that it is consistent withdirect measurements of the CMB dipole, as expected. The signal contributespower in the tSZ maps, which is modulated in a quadrupolar pattern, and weestimate its contribution to the tSZ bispectrum, noting that it contributesnegligible noise to the bispectrum at relevant scales.
AU  - Collaboration,P
AU  - Akrami,Y
AU  - Ashdown,M
AU  - Aumont,J
AU  - Baccigalupi,C
AU  - Ballardini,M
AU  - Banday,AJ
AU  - Barreiro,RB
AU  - Bartolo,N
AU  - Basak,S
AU  - Benabed,K
AU  - Bernard,J-P
AU  - Bersanelli,M
AU  - Bielewicz,P
AU  - Bond,JR
AU  - Borrill,J
AU  - Bouchet,FR
AU  - Burigana,C
AU  - Calabrese,E
AU  - Cardoso,J-F
AU  - Casaponsa,B
AU  - Chiang,HC
AU  - Combet,C
AU  - Contreras,D
AU  - Crill,BP
AU  - Cuttaia,F
AU  - Bernardis,PD
AU  - Rosa,AD
AU  - Zotti,GD
AU  - Delabrouille,J
AU  - Valentino,ED
AU  - Diego,JM
AU  - Doré,O
AU  - Douspis,M
AU  - Dupac,X
AU  - Enßlin,TA
AU  - Eriksen,HK
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,RT
AU  - Gerbino,M
AU  - González-Nuevo,J
AU  - Górski,KM
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Handley,W
AU  - Herranz,D
AU  - Hivon,E
AU  - Huang,Z
AU  - Jaffe,AH
AU  - Jones,WC
AU  - Keihänen,E
AU  - Keskitalo,R
AU  - Kiiveri,K
AU  - Kim,J
AU  - Kisner,TS
AU  - Krachmalnicoff,N
AU  - Kunz,M
AU  - Kurki-Suonio,H
AU  - Lamarre,J-M
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Jeune,ML
AU  - Levrier,F
AU  - Liguori,M
AU  - Lilje,PB
AU  - Lindholm,V
AU  - López-Caniego,M
AU  - Macías-Pérez,JF
AU  - Maino,D
AU  - Mandolesi,N
AU  - Marcos-Caballero,A
AU  - Maris,M
AU  - Martin,PG
AU  - Martínez-González,E
AU  - Matarrese,S
AU  - Mauri,N
AU  - McEwen,JD
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,JP
AU  - Reinecke,M
AU  - Remazeilles,M
AU  - Renzi,A
AU  - Rocha,G
AU  - Rosset,C
AU  - Rubiño-Martín,JA
AU  - Ruiz-Granados,B
AU  - Salvati,L
AU  - Savelainen,M
AU  - Scott,D
AU  - Sirignano,C
AU  - Sirri,G
AU  - Spencer,LD
AU  - Sullivan,RM
AU  - Sunyaev,R
AU  - Suur-Uski,A-S
AU  - Tauber,JA
AU  - Tavagnacco,D
AU  - Tenti,M
AU  - Toffolatti,L
AU  - Tomasi,M
AU  - Trombetti,T
AU  - Valiviita,J
AU  - Tent,BV
AU  - Vielva,P
AU  - Villa,F
AU  - Vittorio,N
AU  - Wehus,IK
AU  - Zacchei,A
AU  - Zonca,A
PB  - arXiv
PY  - 2020///
TI  - Planck intermediate results. LVI. Detection of the CMB dipole through  modulation of the thermal Sunyaev-Zeldovich effect: Eppur si muove II
UR  - http://arxiv.org/abs/2003.12646v2
UR  - http://hdl.handle.net/10044/1/82829
ER  -
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