Issue |
A&A
Volume 571, November 2014
Planck 2013 results
|
|
---|---|---|
Article Number | A10 | |
Number of page(s) | 23 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201321577 | |
Published online | 29 October 2014 |
Planck 2013 results. X. HFI energetic particle effects: characterization, removal, and simulation
1
APC, AstroParticule et Cosmologie, Université Paris Diderot,
CNRS/IN2P3, CEA/lrfu, Observatoire de Paris, Sorbonne Paris Cité, 10 rue Alice Domon et Léonie
Duquet, 75205
Paris Cedex 13,
France
2
Aalto University Metsähovi Radio Observatory,
Metsähovintie 114, 02540
Kylmälä,
Finland
3
African Institute for Mathematical Sciences,
6-8 Melrose Road, Muizenberg,
7945
Cape Town, South
Africa
4
Agenzia Spaziale Italiana Science Data Center, via del Politecnico
snc, 00133
Roma,
Italy
5
Agenzia Spaziale Italiana, Viale Liegi 26,
Roma,
Italy
6
Astrophysics Group, Cavendish Laboratory, University of
Cambridge, J J Thomson
Avenue, Cambridge
CB3 0HE,
UK
7
Astrophysics & Cosmology Research Unit, School of
Mathematics, Statistics & Computer Science, University of
KwaZulu-Natal, Westville Campus,
Private Bag X54001, 4000
Durban, South
Africa
8
Atacama Large Millimeter/submillimeter Array, ALMA Santiago Central
Offices, Alonso de Cordova 3107, Vitacura, Casilla 763 0355, Santiago, Chile
9
CITA, University of Toronto, 60 St. George St., Toronto, ON
M5S 3H8,
Canada
10
CNR, SIRAP, 9 Av.
Colonel Roche, BP
44346, 31028
Toulouse Cedex 4,
France
11
California Institute of Technology, Pasadena, California, USA
12
Centre for Theoretical Cosmology, DAMTP, University of
Cambridge, Wilberforce
Road, Cambridge
CB3 0WA,
UK
13
Centro de Estudios de Física del Cosmos de Aragón (CEFCA), Plaza San
Juan, 1, planta 2, 44001
Teruel,
Spain
14
Computational Cosmology Center, Lawrence Berkeley National
Laboratory, Berkeley,
California,
USA
15
DSM/Irfu/SPP, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
16
DTU Space, National Space Institute, Technical University of
Denmark, Elektrovej
327, 2800
Kgs. Lyngby,
Denmark
17
Département de Physique Théorique, Université de
Genève, 24 quai E.
Ansermet, 1211
Genève 4,
Switzerland
18
Departamento de Física Fundamental, Facultad de Ciencias,
Universidad de Salamanca, 37008
Salamanca,
Spain
19
Departamento de Física, Universidad de Oviedo,
Avda. Calvo Sotelo s/n,
33007
Oviedo,
Spain
20
Department of Astronomy and Astrophysics, University of
Toronto, 50 Saint George Street,
Toronto, Ontario,
Canada
21
Department of Astrophysics/IMAPP, Radboud University
Nijmegen, PO Box
9010, 6500 GL
Nijmegen, The
Netherlands
22
Department of Electrical Engineering and Computer Sciences,
University of California, Berkeley, California, USA
23
Department of Physics & Astronomy, University of British
Columbia, 6224 Agricultural Road,
Vancouver, British
Columbia, Canada
24
Department of Physics and Astronomy, Dana and David Dornsife College
of Letter, Arts and Sciences, University of Southern California,
Los Angeles, CA
90089,
USA
25
Department of Physics and Astronomy, University College
London, London
WC1E 6BT,
UK
26
Department of Physics, Florida State University,
Keen Physics Building, 77 Chieftan
Way, Tallahassee,
Florida,
USA
27
Department of Physics, Gustaf Hällströmin katu 2a, University of
Helsinki, 00014
Helsinki,
Finland
28
Department of Physics, Princeton University,
Princeton, New Jersey, USA
29
Department of Physics, University of California,
One Shields Avenue, Davis, California, USA
30
Department of Physics, University of California,
Santa Barbara, California, USA
31
Department of Physics, University of Illinois at
Urbana-Champaign, 1110 West Green
Street, Urbana,
Illinois,
USA
32
Dipartimento di Fisica e Astronomia G. Galilei, Università degli
Studi di Padova, via Marzolo
8, 35131
Padova,
Italy
33
Dipartimento di Fisica e Scienze della Terra, Università di
Ferrara, via Saragat
1, 44122
Ferrara,
Italy
34
Dipartimento di Fisica, Università La Sapienza,
P.le A. Moro 2, 00185
Roma,
Italy
35
Dipartimento di Fisica, Università degli Studi di
Milano, via Celoria,
16, 20133
Milano,
Italy
36
Dipartimento di Fisica, Università degli Studi di
Trieste, via A. Valerio
2, 34127
Trieste,
Italy
37
Dipartimento di Fisica, Università di Roma Tor
Vergata, via della Ricerca Scientifica
1, 00133
Roma,
Italy
38
Discovery Center, Niels Bohr Institute, Blegdamsvej 17, 2100
Copenhagen,
Denmark
39
European Southern Observatory, ESO Vitacura, Alonso de Cordova 3107, Vitacura, Casilla
19001
Santiago,
Chile
40
European Space Agency, ESAC, Planck Science Office, Camino bajo del
Castillo, s/n, Urbanización Villafranca del Castillo, Villanueva de la
Cañada, 28691
Madrid,
Spain
41
European Space Agency, ESTEC, Keplerlaan 1,
2201 AZ
Noordwijk, The
Netherlands
42
Helsinki Institute of Physics, Gustaf Hällströmin katu 2, University
of Helsinki, 00014
Helsinki,
Finland
43
INAF – Osservatorio Astrofisico di Catania, via S. Sofia
78, 95123
Catania,
Italy
44
INAF – Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio
5, 35122
Padova,
Italy
45
INAF – Osservatorio Astronomico di Roma, via di Frascati
33, 00040
Monte Porzio Catone,
Italy
46
INAF – Osservatorio Astronomico di Trieste, via G.B. Tiepolo
11, 34131
Trieste,
Italy
47
INAF Istituto di Radioastronomia, via P. Gobetti 101,
40129
Bologna,
Italy
48
INAF/IASF Bologna, via Gobetti 101, 40129
Bologna,
Italy
49
INAF/IASF Milano, via E. Bassini 15, 20133
Milano,
Italy
50
INFN, Sezione di Bologna, via Irnerio 46,
40126
Bologna,
Italy
51
INFN, Sezione di Roma 1, Università di Roma Sapienza,
Piazzale Aldo Moro 2,
00185
Roma,
Italy
52
IPAG: Institut de Planétologie et d’Astrophysique de Grenoble,
Université Joseph Fourier, Grenoble 1/CNRS-INSU, UMR 5274, 38041 Grenoble, France
53
IUCAA, Post Bag 4, Ganeshkhind, Pune University
Campus, Pune
411 007,
India
54
Imperial College London, Astrophysics group, Blackett
Laboratory, Prince Consort
Road, London,
SW7 2AZ,
UK
55
Infrared Processing and Analysis Center, California Institute of
Technology, Pasadena,
CA
91125,
USA
56
Institut Néel, CNRS, Université Joseph Fourier Grenoble
I, 25 rue des
Martyrs, 38042
Grenoble,
France
57
Institut Universitaire de France, 103, bd Saint-Michel, 75005
Paris,
France
58
Institut d’Astrophysique Spatiale, CNRS (UMR 8617) Université
Paris-Sud 11, Bâtiment
121, 91405
Orsay,
France
59
Institut d’Astrophysique de Paris, CNRS (UMR 7095),
98bis boulevard Arago,
75014
Paris,
France
60
Institute for Space Sciences, 077125
Bucharest-Magurale,
Romania
61
Institute of Astronomy and Astrophysics, Academia
Sinica, 10617
Taipei,
Taiwan
62
Institute of Astronomy, University of Cambridge,
Madingley Road, Cambridge
CB3 0HA,
UK
63
Institute of Theoretical Astrophysics, University of
Oslo, Blindern,
0315
Oslo,
Norway
64
Instituto de Física de Cantabria (CSIC-Universidad de
Cantabria), Avda. de los Castros
s/n, 39005
Santander,
Spain
65
Jet Propulsion Laboratory, California Institute of
Technology, 4800 Oak Grove
Drive, Pasadena,
California,
USA
66
Jodrell Bank Centre for Astrophysics, Alan Turing Building, School
of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester, M13
9PL, UK
67
Kavli Institute for Cosmology Cambridge,
Madingley Road, Cambridge, CB3 0HA, UK
68
LAL, Université Paris-Sud, CNRS/IN2P3, Orsay, France
69
LERMA, CNRS, Observatoire de Paris, 61 avenue de
l’Observatoire, 75014
Paris,
France
70
Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS –
Université Paris Diderot, Bât. 709, CEA-Saclay, 91191
Gif-sur-Yvette Cedex,
France
71
Laboratoire Traitement et Communication de l’Information, CNRS (UMR
5141) and Télécom ParisTech, 46 rue
Barrault, 75634
Paris Cedex 13,
France
72
Laboratoire de Physique Subatomique et de Cosmologie, Université
Joseph Fourier Grenoble I, CNRS/IN2P3, Institut National Polytechnique de
Grenoble, 53 rue des
Martyrs, 38026
Grenoble Cedex,
France
73
Laboratoire de Physique Théorique, Université Paris-Sud 11 &
CNRS, Bâtiment 210,
91405
Orsay,
France
74
Lawrence Berkeley National Laboratory, Berkeley, California, USA
75
Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Str. 1, 85741
Garching,
Germany
76
McGill Physics, Ernest Rutherford Physics Building, McGill
University, 3600 rue University, Montréal, QC,
H3A 2T8,
Canada
77
National University of Ireland, Department of Experimental
Physics, Maynooth,
Co. Kildare,
Ireland
78
Niels Bohr Institute, Blegdamsvej 17, 2100
Copenhagen,
Denmark
79
Observational Cosmology, Mail Stop 367-17, California Institute of
Technology, Pasadena,
CA
91125,
USA
80
Optical Science Laboratory, University College London,
Gower Street, London, UK
81
SB-ITP-LPPC, EPFL, 1015, Lausanne, Switzerland
82
SISSA, Astrophysics Sector, via Bonomea 265,
34136
Trieste,
Italy
83
School of Physics and Astronomy, Cardiff University,
Queens Buildings, The Parade,
Cardiff, CF24 3AA, UK
84
Space Sciences Laboratory, University of California,
Berkeley, California, USA
85
Special Astrophysical Observatory, Russian Academy of
Sciences, Nizhnij Arkhyz,
Zelenchukskiy region, 369167
Karachai-Cherkessian Republic,
Russia
86
Stanford University, Dept of Physics, Varian Physics Bldg, 382 via Pueblo
Mall, Stanford,
California,
USA
87
Sub-Department of Astrophysics, University of Oxford,
Keble Road, Oxford
OX1 3RH,
UK
88
Theory Division, PH-TH, CERN, 1211
Geneva 23,
Switzerland
89
UPMC Univ Paris 06, UMR 7095, 98bis boulevard Arago, 75014, Paris, France
90
Université de Toulouse, UPS-OMP, IRAP, 31028
Toulouse Cedex 4,
France
91
University of Granada, Departamento de Física Teórica y del Cosmos,
Facultad de Ciencias, 1807
Granada,
Spain
92
Warsaw University Observatory, Aleje Ujazdowskie 4, 00-478
Warszawa,
Poland
Received:
26
March
2013
Accepted:
1
July
2014
We describe the detection, interpretation, and removal of the signal resulting from interactions of high energy particles with the Planck High Frequency Instrument (HFI). There are two types of interactions: heating of the 0.1 K bolometer plate; and glitches in each detector time stream. The transientresponses to detector glitch shapes are not simple single-pole exponential decays and fall into three families. The glitch shape for each family has been characterized empirically in flight data and these shapes have been used to remove glitches from the detector time streams. The spectrum of the count rate per unit energy is computed for each family and a correspondence is made to the location on the detector of the particle hit. Most of the detected glitches are from Galactic protons incident on the die frame supporting the micro-machined bolometric detectors. In the Planck orbit at L2, the particle flux is around 5 cm-2 s-1 and is dominated by protons incident on the spacecraft with energy >39 MeV, at a rate of typically one event per second per detector. Different categories of glitches have different signatures in the time stream. Two of the glitch types have a low amplitude component that decays over nearly 1 s. This component produces excess noise if not properly removed from the time-ordered data. We have used a glitch detection and subtraction method based on the joint fit of population templates. The application of this novel glitch subtraction method removes excess noise from the time streams. Using realistic simulations, we find that this method does not introduce signal bias into the Planck data.
Key words: cosmic background radiation / cosmology: observations / instrumentation: detectors / space vehicles: instruments / methods: data analysis
© ESO, 2014
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