Deployment of Polarbear-2A

Daisuke Kaneko; S. Adachi; P. A.R. Ade; M. Aguilar Faúndez; Y. Akiba; K. Arnold; C. Baccigalupi; D. Barron; D. Beck; S. Beckman; F. Bianchini; D. Boettger; J. Borrill; J. Carron; S. Chapman; K. Cheung; Y. Chinone; K. Crowley; A. Cukierman; M. Dobbs; R. Dűnner; H. El-Bouhargani; T. Elleflot; J. Errard; G. Fabbian; S. M. Feeney; C. Feng; T. Fujino; N. Galitzki; A. Gilbert; N. Goeckner-Wald; J. Groh; G. Hall; N. W. Halverson; T. Hamada; M. Hasegawa; M. Hazumi; C. A. Hill; L. Howe; Y. Inoue; G. Jaehnig; O. Jeong; N. Katayama; B. Keating; R. Keskitalo; S. Kikuchi; T. Kisner; N. Krachmalnicoff; A. Kusaka; A. T. Lee; D. Leon; E. Linder; L. N. Lowry; A. Mangu; F. Matsuda; Y. Minami; M. Navaroli; H. Nishino; J. Peloton; A. T.P. Pham; D. Poletti; G. Puglisi; C. L. Reichardt; C. Ross; Y. Segawa; M. Silva-Feaver; P. Siritanasak; N. Stebor; R. Stompor; A. Suzuki; O. Tajima; S. Takakura; S. Takatori; D. Tanabe; G. P. Teply; T. Tomaru; C. Tsai; C. Verges; B. Westbrook; Y. Zhou

doi:10.1007/s10909-020-02366-w

Deployment of Polarbear-2A

Daisuke Kaneko, S. Adachi, P. A.R. Ade, M. Aguilar Faúndez, Y. Akiba, K. Arnold, C. Baccigalupi, D. Barron, D. Beck, S. Beckman, F. Bianchini, D. Boettger, J. Borrill, J. Carron, S. Chapman, K. Cheung, Y. Chinone, K. Crowley, A. Cukierman, M. DobbsR. Dűnner, H. El-Bouhargani, T. Elleflot, J. Errard, G. Fabbian, S. M. Feeney, C. Feng, T. Fujino, N. Galitzki, A. Gilbert, N. Goeckner-Wald, J. Groh, G. Hall, N. W. Halverson, T. Hamada, M. Hasegawa, M. Hazumi, C. A. Hill, L. Howe, Y. Inoue, G. Jaehnig, O. Jeong, N. Katayama, B. Keating, R. Keskitalo, S. Kikuchi, T. Kisner, N. Krachmalnicoff, A. Kusaka, A. T. Lee, D. Leon, E. Linder, L. N. Lowry, A. Mangu, F. Matsuda, Y. Minami, M. Navaroli, H. Nishino, J. Peloton, A. T.P. Pham, D. Poletti, G. Puglisi, C. L. Reichardt, C. Ross, Y. Segawa, M. Silva-Feaver, P. Siritanasak, N. Stebor, R. Stompor, A. Suzuki, O. Tajima, S. Takakura, S. Takatori, D. Tanabe, G. P. Teply, T. Tomaru, C. Tsai, C. Verges, B. Westbrook, Y. Zhou

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

10 Citations (Scopus)

Abstract

Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.

Original language	English
Pages (from-to)	1137-1147
Number of pages	11
Journal	Journal of Low Temperature Physics
Volume	199
Issue number	3-4
DOIs	https://doi.org/10.1007/s10909-020-02366-w
Publication status	Published - May 1 2020
Externally published	Yes

Keywords

B-mode polarization
CMB
Millimeter wave
TES bolometer

ASJC Scopus subject areas

Atomic and Molecular Physics, and Optics
Materials Science(all)
Condensed Matter Physics

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10.1007/s10909-020-02366-w

Cite this

Kaneko, D., Adachi, S., Ade, P. A. R., Aguilar Faúndez, M., Akiba, Y., Arnold, K., Baccigalupi, C., Barron, D., Beck, D., Beckman, S., Bianchini, F., Boettger, D., Borrill, J., Carron, J., Chapman, S., Cheung, K., Chinone, Y., Crowley, K., Cukierman, A., ... Zhou, Y. (2020). Deployment of Polarbear-2A. Journal of Low Temperature Physics, 199(3-4), 1137-1147. https://doi.org/10.1007/s10909-020-02366-w

Kaneko, D, Adachi, S, Ade, PAR, Aguilar Faúndez, M, Akiba, Y, Arnold, K, Baccigalupi, C, Barron, D, Beck, D, Beckman, S, Bianchini, F, Boettger, D, Borrill, J, Carron, J, Chapman, S, Cheung, K, Chinone, Y, Crowley, K, Cukierman, A, Dobbs, M, Dűnner, R, El-Bouhargani, H, Elleflot, T, Errard, J, Fabbian, G, Feeney, SM, Feng, C, Fujino, T, Galitzki, N, Gilbert, A, Goeckner-Wald, N, Groh, J, Hall, G, Halverson, NW, Hamada, T, Hasegawa, M, Hazumi, M, Hill, CA, Howe, L, Inoue, Y, Jaehnig, G, Jeong, O, Katayama, N, Keating, B, Keskitalo, R, Kikuchi, S, Kisner, T, Krachmalnicoff, N, Kusaka, A, Lee, AT, Leon, D, Linder, E, Lowry, LN, Mangu, A, Matsuda, F, Minami, Y, Navaroli, M, Nishino, H, Peloton, J, Pham, ATP, Poletti, D, Puglisi, G, Reichardt, CL, Ross, C, Segawa, Y, Silva-Feaver, M, Siritanasak, P, Stebor, N, Stompor, R, Suzuki, A, Tajima, O, Takakura, S, Takatori, S, Tanabe, D, Teply, GP, Tomaru, T, Tsai, C, Verges, C, Westbrook, B & Zhou, Y 2020, 'Deployment of Polarbear-2A', Journal of Low Temperature Physics, vol. 199, no. 3-4, pp. 1137-1147. https://doi.org/10.1007/s10909-020-02366-w

@article{73da8ab85cec47b5865fbb97be7213ee,

title = "Deployment of Polarbear-2A",

abstract = "Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.",

keywords = "B-mode polarization, CMB, Millimeter wave, TES bolometer",

author = "Daisuke Kaneko and S. Adachi and Ade, {P. A.R.} and {Aguilar Fa{\'u}ndez}, M. and Y. Akiba and K. Arnold and C. Baccigalupi and D. Barron and D. Beck and S. Beckman and F. Bianchini and D. Boettger and J. Borrill and J. Carron and S. Chapman and K. Cheung and Y. Chinone and K. Crowley and A. Cukierman and M. Dobbs and R. D{\H u}nner and H. El-Bouhargani and T. Elleflot and J. Errard and G. Fabbian and Feeney, {S. M.} and C. Feng and T. Fujino and N. Galitzki and A. Gilbert and N. Goeckner-Wald and J. Groh and G. Hall and Halverson, {N. W.} and T. Hamada and M. Hasegawa and M. Hazumi and Hill, {C. A.} and L. Howe and Y. Inoue and G. Jaehnig and O. Jeong and N. Katayama and B. Keating and R. Keskitalo and S. Kikuchi and T. Kisner and N. Krachmalnicoff and A. Kusaka and Lee, {A. T.} and D. Leon and E. Linder and Lowry, {L. N.} and A. Mangu and F. Matsuda and Y. Minami and M. Navaroli and H. Nishino and J. Peloton and Pham, {A. T.P.} and D. Poletti and G. Puglisi and Reichardt, {C. L.} and C. Ross and Y. Segawa and M. Silva-Feaver and P. Siritanasak and N. Stebor and R. Stompor and A. Suzuki and O. Tajima and S. Takakura and S. Takatori and D. Tanabe and Teply, {G. P.} and T. Tomaru and C. Tsai and C. Verges and B. Westbrook and Y. Zhou",

note = "Funding Information: The Simons Array is supported by the Simons Foundation, the National Science Foundation grant (AST-0618398, AST-1212230, AST-1440338), NASA grant NNG06GJ08G, the Moore Foundation (GBMF4633), the Heising-Simons Foundation, Templeton Foundation grant number 58724, the Ax Center for Experimental Cosmology at UC San Diego, the U.S. Department of Energy, Office of Science, Office of High Energy Physics, JSPS KAKENHI Grant Number (JP26220709, JP15H03670, JP15H05891, JP18H01240), and JSPS Core-to-core Program, A. Advanced Research Networks. Kavli IPMU authors are supported by World Premier International Research Center Initiative (WPI), MEXT, Japan. The McGill authors acknowledge the Natural Sciences and Engineering Research Council and Canadian Institute for Advanced Research, National Commission for Scientific and Technological Research. The SISSA authors acknowledge support from the ASI-COSMOS network (cosmosnet.it) and the INDARK INFN Initiative. The James Ax Observatory operates in the Parque Astronomico Atacama in Northern Chile under the auspices of the Comision Nacional de Investigacion Cientifica y Tecnologica de Chile (CONICYT). Funding Information: The McGill authors acknowledge the Natural Sciences and Engineering Research Council and Canadian Institute for Advanced Research, National Commission for Scientific and Technological Research. The SISSA authors acknowledge support from the ASI-COSMOS network (cosmosnet.it) and the INDARK INFN Initiative. Funding Information: The Simons Array is supported by the Simons Foundation, the National Science Foundation grant (AST-0618398, AST-1212230, AST-1440338), NASA grant NNG06GJ08G, the Moore Foundation (GBMF4633), the Heising-Simons Foundation, Templeton Foundation grant number 58724, the Ax Center for Experimental Cosmology at UC San Diego, the U.S. Department of Energy, Office of Science, Office of High Energy Physics, JSPS KAKENHI Grant Number (JP26220709, JP15H03670, JP15H05891, JP18H01240), and JSPS Core-to-core Program, A. Advanced Research Networks. Funding Information: Kavli IPMU authors are supported by World Premier International Research Center Initiative (WPI), MEXT, Japan. Publisher Copyright: {\textcopyright} 2020, Springer Science+Business Media, LLC, part of Springer Nature.",

year = "2020",

month = may,

day = "1",

doi = "10.1007/s10909-020-02366-w",

language = "English",

volume = "199",

pages = "1137--1147",

journal = "Journal of Low Temperature Physics",

issn = "0022-2291",

publisher = "Springer New York",

number = "3-4",

}

TY - JOUR

T1 - Deployment of Polarbear-2A

AU - Kaneko, Daisuke

AU - Adachi, S.

AU - Ade, P. A.R.

AU - Aguilar Faúndez, M.

AU - Akiba, Y.

AU - Arnold, K.

AU - Baccigalupi, C.

AU - Barron, D.

AU - Beck, D.

AU - Beckman, S.

AU - Bianchini, F.

AU - Boettger, D.

AU - Borrill, J.

AU - Carron, J.

AU - Chapman, S.

AU - Cheung, K.

AU - Chinone, Y.

AU - Crowley, K.

AU - Cukierman, A.

AU - Dobbs, M.

AU - Dűnner, R.

AU - El-Bouhargani, H.

AU - Elleflot, T.

AU - Errard, J.

AU - Fabbian, G.

AU - Feeney, S. M.

AU - Feng, C.

AU - Fujino, T.

AU - Galitzki, N.

AU - Gilbert, A.

AU - Goeckner-Wald, N.

AU - Groh, J.

AU - Hall, G.

AU - Halverson, N. W.

AU - Hamada, T.

AU - Hasegawa, M.

AU - Hazumi, M.

AU - Hill, C. A.

AU - Howe, L.

AU - Inoue, Y.

AU - Jaehnig, G.

AU - Jeong, O.

AU - Katayama, N.

AU - Keating, B.

AU - Keskitalo, R.

AU - Kikuchi, S.

AU - Kisner, T.

AU - Krachmalnicoff, N.

AU - Kusaka, A.

AU - Lee, A. T.

AU - Leon, D.

AU - Linder, E.

AU - Lowry, L. N.

AU - Mangu, A.

AU - Matsuda, F.

AU - Minami, Y.

AU - Navaroli, M.

AU - Nishino, H.

AU - Peloton, J.

AU - Pham, A. T.P.

AU - Poletti, D.

AU - Puglisi, G.

AU - Reichardt, C. L.

AU - Ross, C.

AU - Segawa, Y.

AU - Silva-Feaver, M.

AU - Siritanasak, P.

AU - Stebor, N.

AU - Stompor, R.

AU - Suzuki, A.

AU - Tajima, O.

AU - Takakura, S.

AU - Takatori, S.

AU - Tanabe, D.

AU - Teply, G. P.

AU - Tomaru, T.

AU - Tsai, C.

AU - Verges, C.

AU - Westbrook, B.

AU - Zhou, Y.

N1 - Funding Information: The Simons Array is supported by the Simons Foundation, the National Science Foundation grant (AST-0618398, AST-1212230, AST-1440338), NASA grant NNG06GJ08G, the Moore Foundation (GBMF4633), the Heising-Simons Foundation, Templeton Foundation grant number 58724, the Ax Center for Experimental Cosmology at UC San Diego, the U.S. Department of Energy, Office of Science, Office of High Energy Physics, JSPS KAKENHI Grant Number (JP26220709, JP15H03670, JP15H05891, JP18H01240), and JSPS Core-to-core Program, A. Advanced Research Networks. Kavli IPMU authors are supported by World Premier International Research Center Initiative (WPI), MEXT, Japan. The McGill authors acknowledge the Natural Sciences and Engineering Research Council and Canadian Institute for Advanced Research, National Commission for Scientific and Technological Research. The SISSA authors acknowledge support from the ASI-COSMOS network (cosmosnet.it) and the INDARK INFN Initiative. The James Ax Observatory operates in the Parque Astronomico Atacama in Northern Chile under the auspices of the Comision Nacional de Investigacion Cientifica y Tecnologica de Chile (CONICYT). Funding Information: The McGill authors acknowledge the Natural Sciences and Engineering Research Council and Canadian Institute for Advanced Research, National Commission for Scientific and Technological Research. The SISSA authors acknowledge support from the ASI-COSMOS network (cosmosnet.it) and the INDARK INFN Initiative. Funding Information: The Simons Array is supported by the Simons Foundation, the National Science Foundation grant (AST-0618398, AST-1212230, AST-1440338), NASA grant NNG06GJ08G, the Moore Foundation (GBMF4633), the Heising-Simons Foundation, Templeton Foundation grant number 58724, the Ax Center for Experimental Cosmology at UC San Diego, the U.S. Department of Energy, Office of Science, Office of High Energy Physics, JSPS KAKENHI Grant Number (JP26220709, JP15H03670, JP15H05891, JP18H01240), and JSPS Core-to-core Program, A. Advanced Research Networks. Funding Information: Kavli IPMU authors are supported by World Premier International Research Center Initiative (WPI), MEXT, Japan. Publisher Copyright: © 2020, Springer Science+Business Media, LLC, part of Springer Nature.

PY - 2020/5/1

Y1 - 2020/5/1

N2 - Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.

AB - Polarbear-2A is the first of three receivers in the Simons array, a cosmic microwave background experiment located on the Atacama Plateau in Chile. Polarbear-2A was deployed and achieved the first light in January 2019 by mapping the microwave emission from planet observations. Commissioning work is underway to prepare the receiver for science observations.

KW - B-mode polarization

KW - CMB

KW - Millimeter wave

KW - TES bolometer

UR - http://www.scopus.com/inward/record.url?scp=85081900688&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85081900688&partnerID=8YFLogxK

U2 - 10.1007/s10909-020-02366-w

DO - 10.1007/s10909-020-02366-w

M3 - Article

AN - SCOPUS:85081900688

SN - 0022-2291

VL - 199

SP - 1137

EP - 1147

JO - Journal of Low Temperature Physics

JF - Journal of Low Temperature Physics

IS - 3-4

ER -

Deployment of Polarbear-2A

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