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@unpublished{Collaboration:2020,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 Andersen, KJ and Ashdown, M 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 Burigana, C and Butler, RC and Calabrese, E and Casaponsa, B and Chiang, HC and Colombo, LPL and Combet, C 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 Eriksen, HK and Fernandez-Cobos, R and Finelli, F and Frailis, M and Fraisse, AA and Franceschi, E and Frolov, A and Galeotta, S and Galli, S and Ganga, K and Gerbino, M and Ghosh, T and González-Nuevo, J and Górski, KM and Gruppuso, A and Gudmundsson, JE and Handley, W and Helou, G and Herranz, D and Hildebrandt, SR 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 Krachmalnicof},
publisher = {arXiv},
title = {Planck intermediate results. LVII. Joint Planck LFI and HFI data  processing},
url = {http://arxiv.org/abs/2007.04997v1},
year = {2020}
}
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RIS format (EndNote, RefMan)

TY  - UNPB
AB  - We present the NPIPE processing pipeline, which produces calibrated frequencymaps in temperature and polarization from data from the Planck Low FrequencyInstrument (LFI) and High Frequency Instrument (HFI) using high-performancecomputers. NPIPE represents a natural evolution of previous Planck analysisefforts, and combines some of the most powerful features of the separate LFIand HFI analysis pipelines. The net effect of the improvements is lower levelsof noise and systematics in both frequency and component maps at essentiallyall angular scales, as well as notably improved internal consistency betweenthe various frequency channels. Based on the NPIPE maps, we present the firstestimate of the Solar dipole determined through component separation across allnine Planck frequencies. The amplitude is ($3366.6 \pm 2.7$)$\mu$K, consistentwith, albeit slightly higher than, earlier estimates. From the large-scalepolarization data, we derive an updated estimate of the optical depth ofreionization of $\tau = 0.051 \pm 0.006$, which appears robust with respect todata and sky cuts. There are 600 complete signal, noise and systematicssimulations of the full-frequency and detector-set maps. As a Planck first,these simulations include full time-domain processing of the beam-convolved CMBanisotropies. The release of NPIPE maps and simulations is accompanied with acomplete suite of raw and processed time-ordered data and the software,scripts, auxiliary data, and parameter files needed to improve further on theanalysis and to run matching simulations.
AU  - Collaboration,P
AU  - Akrami,Y
AU  - Andersen,KJ
AU  - Ashdown,M
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  - Burigana,C
AU  - Butler,RC
AU  - Calabrese,E
AU  - Casaponsa,B
AU  - Chiang,HC
AU  - Colombo,LPL
AU  - Combet,C
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  - Eriksen,HK
AU  - Fernandez-Cobos,R
AU  - Finelli,F
AU  - Frailis,M
AU  - Fraisse,AA
AU  - Franceschi,E
AU  - Frolov,A
AU  - Galeotta,S
AU  - Galli,S
AU  - Ganga,K
AU  - Gerbino,M
AU  - Ghosh,T
AU  - González-Nuevo,J
AU  - Górski,KM
AU  - Gruppuso,A
AU  - Gudmundsson,JE
AU  - Handley,W
AU  - Helou,G
AU  - Herranz,D
AU  - Hildebrandt,SR
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  - Lasenby,A
AU  - Lattanzi,M
AU  - Lawrence,CR
AU  - Jeune,ML
AU  - Levrier,F
AU  - Liguori,M
AU  - Lilje,PB
AU  - Lilley,M
AU  - Lindholm,V
AU  - López-Caniego,M
AU  - Lubin,PM
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  - Meinhold,PR
AU  - Mennella,A
AU  - Migliaccio,M
AU  - Mitra,S
AU  - Molinari,D
AU  - Montier,L
AU  - Morgante,G
AU  - Moss,A
AU  - Natoli,P
AU  - Paoletti,D
AU  - Partridge,B
AU  - Patanchon,G
AU  - Pearson,D
AU  - Pearson,TJ
AU  - Perrotta,F
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  - Roudier,G
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  - Suur-Uski,A-S
AU  - Svalheim,TL
AU  - Tauber,JA
AU  - Tavagnacco,D
AU  - Tenti,M
AU  - Terenzi,L
AU  - Thommesen,H
AU  - Toffolatti,L
AU  - Tomasi,M
AU  - Tristram,M
AU  - Trombetti,T
AU  - Valiviita,J
AU  - Tent,BV
AU  - Vielva,P
AU  - Villa,F
AU  - Vittorio,N
AU  - Wandelt,BD
AU  - Wehus,IK
AU  - Zacchei,A
AU  - Zonca,A
PB  - arXiv
PY  - 2020///
TI  - Planck intermediate results. LVII. Joint Planck LFI and HFI data  processing
UR  - http://arxiv.org/abs/2007.04997v1
UR  - http://hdl.handle.net/10044/1/82462
ER  -
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