Imperial College London

Carlo R. Contaldi

Faculty of Natural SciencesDepartment of Physics

Professor of Theoretical Physics
 
 
 
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Contact

 

+44 (0)20 7594 1527c.contaldi

 
 
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Location

 

505Huxley BuildingSouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Gualtieri,
author = {Gualtieri, R and Filippini, JP and Ade, PAR and Amiri, M and Benton, SJ and Bergman, AS and Bihary, R and Bock, JJ and Bond, JR and Bryan, SA and Chiang, HC and Contaldi, CR and Doré, O and Duivenvoorden, AJ and Eriksen, HK and Farhang, M and Fissel, LM and Fraisse, AA and Freese, K and Galloway, M and Gambrel, AE and Gandilo, NN and Ganga, K and Gramillano, RV and Gudmundsson, JE and Halpern, M and Hartley, J and Hasselfield, M and Hilton, G and Holmes, W and Hristov, VV and Huang, Z and Irwin, KD and Jones, WC and Kuo, CL and Kermish, ZD and Li, S and Mason, PV and Megerian, K and Moncelsi, L and Morford, TA and Nagy, JM and Netterfield, CB and Nolta, M and Osherson, B and Padilla, IL and Racine, B and Rahlin, AS and Reintsema, C and Ruhl, JE and Runyan, MC and Ruud, TM and Shariff, JA and Soler, JD and Song, X and Trangsrud, A and Tucker, C and Tucker, RS and Turner, AD and List, JFVD and Weber, AC and Wehus, IK and Wiebe, DV and Young, EY},
journal = {Journal of Low Temperature Physics},
title = {SPIDER: CMB polarimetry from the edge of space},
url = {http://arxiv.org/abs/1711.10596v1},
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - SPIDER is a balloon-borne instrument designed to map the polarization of themillimeter-wave sky at large angular scales. SPIDER targets the B-modesignature of primordial gravitational waves in the cosmic microwave background(CMB), with a focus on mapping a large sky area with high fidelity at multiplefrequencies. SPIDER's first longduration balloon (LDB) flight in January 2015deployed a total of 2400 antenna-coupled Transition Edge Sensors (TESs) at 90GHz and 150 GHz. In this work we review the design and in-flight performance ofthe SPIDER instrument, with a particular focus on the measured performance ofthe detectors and instrument in a space-like loading and radiation environment.SPIDER's second flight in December 2018 will incorporate payload upgrades andnew receivers to map the sky at 285 GHz, providing valuable information forcleaning polarized dust emission from CMB maps.
AU - Gualtieri,R
AU - Filippini,JP
AU - Ade,PAR
AU - Amiri,M
AU - Benton,SJ
AU - Bergman,AS
AU - Bihary,R
AU - Bock,JJ
AU - Bond,JR
AU - Bryan,SA
AU - Chiang,HC
AU - Contaldi,CR
AU - Doré,O
AU - Duivenvoorden,AJ
AU - Eriksen,HK
AU - Farhang,M
AU - Fissel,LM
AU - Fraisse,AA
AU - Freese,K
AU - Galloway,M
AU - Gambrel,AE
AU - Gandilo,NN
AU - Ganga,K
AU - Gramillano,RV
AU - Gudmundsson,JE
AU - Halpern,M
AU - Hartley,J
AU - Hasselfield,M
AU - Hilton,G
AU - Holmes,W
AU - Hristov,VV
AU - Huang,Z
AU - Irwin,KD
AU - Jones,WC
AU - Kuo,CL
AU - Kermish,ZD
AU - Li,S
AU - Mason,PV
AU - Megerian,K
AU - Moncelsi,L
AU - Morford,TA
AU - Nagy,JM
AU - Netterfield,CB
AU - Nolta,M
AU - Osherson,B
AU - Padilla,IL
AU - Racine,B
AU - Rahlin,AS
AU - Reintsema,C
AU - Ruhl,JE
AU - Runyan,MC
AU - Ruud,TM
AU - Shariff,JA
AU - Soler,JD
AU - Song,X
AU - Trangsrud,A
AU - Tucker,C
AU - Tucker,RS
AU - Turner,AD
AU - List,JFVD
AU - Weber,AC
AU - Wehus,IK
AU - Wiebe,DV
AU - Young,EY
SN - 0022-2291
TI - SPIDER: CMB polarimetry from the edge of space
T2 - Journal of Low Temperature Physics
UR - http://arxiv.org/abs/1711.10596v1
UR - http://hdl.handle.net/10044/1/54989
ER -