Development and characterization of the readout system for POLARBEAR-2

D. Barron; P. A.R. Ade; Y. Akiba; C. Aleman; K. Arnold; M. Atlas; A. Bender; J. Borrill; S. Chapman; Y. Chinone; A. Cukierman; M. Dobbs; T. Elleflot; J. Errard; G. Fabbian; G. Feng; A. Gilbert; N. W. Halverson; M. Hasegawa; K. Hattori; M. Hazumi; W. L. Holzapfel; Y. Hori; Y. Inoue; G. C. Jaehnig; N. Katayama; B. Keating; Z. Kermish; R. Keskitalo; T. Kisner; M. Le Jeune; A. T. Lee; F. Matsuda; T. Matsumura; H. Morii; M. J. Myers; M. Navroli; H. Nishino; T. Okamura; J. Peloton; G. Rebeiz; C. L. Reichardt; P. L. Richards; C. Ross; M. Sholl; P. Siritanasak; G. Smecher; N. Stebor; B. Steinbach; R. Stompor; A. Suzuki; J. Suzuki; S. Takada; T. Takakura; T. Tomaru; B. Wilson; H. Yamaguchi; O. Zahn

doi:10.1117/12.2055611

Development and characterization of the readout system for POLARBEAR-2

D. Barron, P. A.R. Ade, Y. Akiba, C. Aleman, K. Arnold, M. Atlas, A. Bender, J. Borrill, S. Chapman, Y. Chinone, A. Cukierman, M. Dobbs, T. Elleflot, J. Errard, G. Fabbian, G. Feng, A. Gilbert, N. W. Halverson, M. Hasegawa, K. HattoriM. Hazumi, W. L. Holzapfel, Y. Hori, Y. Inoue, G. C. Jaehnig, N. Katayama, B. Keating, Z. Kermish, R. Keskitalo, T. Kisner, M. Le Jeune, A. T. Lee, F. Matsuda, T. Matsumura, H. Morii, M. J. Myers, M. Navroli, H. Nishino, T. Okamura, J. Peloton, G. Rebeiz, C. L. Reichardt, P. L. Richards, C. Ross, M. Sholl, P. Siritanasak, G. Smecher, N. Stebor, B. Steinbach, R. Stompor, A. Suzuki, J. Suzuki, S. Takada, T. Takakura, T. Tomaru, B. Wilson, H. Yamaguchi, O. Zahn

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

3 Scopus citations

Abstract

Polarbear-2 is a next-generation receiver for precision measurements of the polarization of the cosmic mi-crowave background (Cosmic Microwave Background (CMB)). Scheduled to deploy in early 2015, it will observealongside the existing Polarbear-1 receiver, on a new telescope in the Simons Arrayon Cerro Toco in theAtacama desert of Chile. For increased sensitivity, it will feature a larger area focal plane, with a total of 7,588 polarization sensitive antenna-coupled Transition Edge Sensor (TES) bolometers, with a design sensitivity of 4.1 μKs. The focal plane will be cooled to 250 milliKelvin, and the bolometers will be read-out with 40 × frequency domain multiplexing, with 36 optical bolometers on a single SQUID amplier, along with 2 dark bolometers and 2 calibration resistors. To increase the multiplexing factor from 8 × for Polarbear-1 to 40 × for Polarbear-2 requires additional bandwidth for SQUID readout and well-dened frequency channel spacing. Extending to these higher frequencies requires new components and design for the LC lters which dene channel spacing. The LC lters are cold resonant circuits with an inductor and capacitor in series with each bolometer, and stray inductance in the wiring and equivalent series resistance from the capacitors can aect bolometer operation. We present results from characterizing these new readout components. Integration of the readout system is being done rst on a small scale, to ensure that the readout system does not aect bolometer sensitivity or stability, and to validate the overall system before expansion into the full receiver. We present the status of readout integration, and the initial results and status of components for the full array.

Original language	English
Title of host publication	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Editors	Jonas Zmuidzinas, Wayne S. Holland
Publisher	SPIE
ISBN (Electronic)	9780819496218
DOIs	https://doi.org/10.1117/12.2055611
State	Published - 2014
Event	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII - Montreal, Canada Duration: 24 Jun 2014 → 27 Jun 2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9153
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Country/Territory	Canada
City	Montreal
Period	24/06/14 → 27/06/14

Keywords

CMB
CMB polarization
antenna
bolometer
ination
millimeter-wave
neutrinos

Access to Document

10.1117/12.2055611

Cite this

Barron, D., Ade, P. A. R., Akiba, Y., Aleman, C., Arnold, K., Atlas, M., Bender, A., Borrill, J., Chapman, S., Chinone, Y., Cukierman, A., Dobbs, M., Elleflot, T., Errard, J., Fabbian, G., Feng, G., Gilbert, A., Halverson, N. W., Hasegawa, M., ... Zahn, O. (2014). Development and characterization of the readout system for POLARBEAR-2. In J. Zmuidzinas, & W. S. Holland (Eds.), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII Article 915335 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9153). SPIE. https://doi.org/10.1117/12.2055611

@inproceedings{b2c3926836994edeb3f357e4d2852c39,

title = "Development and characterization of the readout system for POLARBEAR-2",

abstract = "Polarbear-2 is a next-generation receiver for precision measurements of the polarization of the cosmic mi-crowave background (Cosmic Microwave Background (CMB)). Scheduled to deploy in early 2015, it will observealongside the existing Polarbear-1 receiver, on a new telescope in the Simons Arrayon Cerro Toco in theAtacama desert of Chile. For increased sensitivity, it will feature a larger area focal plane, with a total of 7,588 polarization sensitive antenna-coupled Transition Edge Sensor (TES) bolometers, with a design sensitivity of 4.1 μKs. The focal plane will be cooled to 250 milliKelvin, and the bolometers will be read-out with 40 × frequency domain multiplexing, with 36 optical bolometers on a single SQUID amplier, along with 2 dark bolometers and 2 calibration resistors. To increase the multiplexing factor from 8 × for Polarbear-1 to 40 × for Polarbear-2 requires additional bandwidth for SQUID readout and well-dened frequency channel spacing. Extending to these higher frequencies requires new components and design for the LC lters which dene channel spacing. The LC lters are cold resonant circuits with an inductor and capacitor in series with each bolometer, and stray inductance in the wiring and equivalent series resistance from the capacitors can aect bolometer operation. We present results from characterizing these new readout components. Integration of the readout system is being done rst on a small scale, to ensure that the readout system does not aect bolometer sensitivity or stability, and to validate the overall system before expansion into the full receiver. We present the status of readout integration, and the initial results and status of components for the full array.",

keywords = "CMB, CMB polarization, antenna, bolometer, ination, millimeter-wave, neutrinos",

author = "D. Barron and Ade, {P. A.R.} and Y. Akiba and C. Aleman and K. Arnold and M. Atlas and A. Bender and J. Borrill and S. Chapman and Y. Chinone and A. Cukierman and M. Dobbs and T. Elleflot and J. Errard and G. Fabbian and G. Feng and A. Gilbert and Halverson, {N. W.} and M. Hasegawa and K. Hattori and M. Hazumi and Holzapfel, {W. L.} and Y. Hori and Y. Inoue and Jaehnig, {G. C.} and N. Katayama and B. Keating and Z. Kermish and R. Keskitalo and T. Kisner and {Le Jeune}, M. and Lee, {A. T.} and F. Matsuda and T. Matsumura and H. Morii and Myers, {M. J.} and M. Navroli and H. Nishino and T. Okamura and J. Peloton and G. Rebeiz and Reichardt, {C. L.} and Richards, {P. L.} and C. Ross and M. Sholl and P. Siritanasak and G. Smecher and N. Stebor and B. Steinbach and R. Stompor and A. Suzuki and J. Suzuki and S. Takada and T. Takakura and T. Tomaru and B. Wilson and H. Yamaguchi and O. Zahn",

note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII ; Conference date: 24-06-2014 Through 27-06-2014",

year = "2014",

doi = "10.1117/12.2055611",

language = "???core.languages.en_GB???",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

publisher = "SPIE",

editor = "Jonas Zmuidzinas and Holland, {Wayne S.}",

booktitle = "Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII",

}

Barron, D, Ade, PAR, Akiba, Y, Aleman, C, Arnold, K, Atlas, M, Bender, A, Borrill, J, Chapman, S, Chinone, Y, Cukierman, A, Dobbs, M, Elleflot, T, Errard, J, Fabbian, G, Feng, G, Gilbert, A, Halverson, NW, Hasegawa, M, Hattori, K, Hazumi, M, Holzapfel, WL, Hori, Y, Inoue, Y, Jaehnig, GC, Katayama, N, Keating, B, Kermish, Z, Keskitalo, R, Kisner, T, Le Jeune, M, Lee, AT, Matsuda, F, Matsumura, T, Morii, H, Myers, MJ, Navroli, M, Nishino, H, Okamura, T, Peloton, J, Rebeiz, G, Reichardt, CL, Richards, PL, Ross, C, Sholl, M, Siritanasak, P, Smecher, G, Stebor, N, Steinbach, B, Stompor, R, Suzuki, A, Suzuki, J, Takada, S, Takakura, T, Tomaru, T, Wilson, B, Yamaguchi, H & Zahn, O 2014, Development and characterization of the readout system for POLARBEAR-2. in J Zmuidzinas & WS Holland (eds), Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII., 915335, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9153, SPIE, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, Montreal, Canada, 24/06/14. https://doi.org/10.1117/12.2055611

Development and characterization of the readout system for POLARBEAR-2. / Barron, D.; Ade, P. A.R.; Akiba, Y. et al.
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. ed. / Jonas Zmuidzinas; Wayne S. Holland. SPIE, 2014. 915335 (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9153).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Development and characterization of the readout system for POLARBEAR-2

AU - Barron, D.

AU - Ade, P. A.R.

AU - Akiba, Y.

AU - Aleman, C.

AU - Arnold, K.

AU - Atlas, M.

AU - Bender, A.

AU - Borrill, J.

AU - Chapman, S.

AU - Chinone, Y.

AU - Cukierman, A.

AU - Dobbs, M.

AU - Elleflot, T.

AU - Errard, J.

AU - Fabbian, G.

AU - Feng, G.

AU - Gilbert, A.

AU - Halverson, N. W.

AU - Hasegawa, M.

AU - Hattori, K.

AU - Hazumi, M.

AU - Holzapfel, W. L.

AU - Hori, Y.

AU - Inoue, Y.

AU - Jaehnig, G. C.

AU - Katayama, N.

AU - Keating, B.

AU - Kermish, Z.

AU - Keskitalo, R.

AU - Kisner, T.

AU - Le Jeune, M.

AU - Lee, A. T.

AU - Matsuda, F.

AU - Matsumura, T.

AU - Morii, H.

AU - Myers, M. J.

AU - Navroli, M.

AU - Nishino, H.

AU - Okamura, T.

AU - Peloton, J.

AU - Rebeiz, G.

AU - Reichardt, C. L.

AU - Richards, P. L.

AU - Ross, C.

AU - Sholl, M.

AU - Siritanasak, P.

AU - Smecher, G.

AU - Stebor, N.

AU - Steinbach, B.

AU - Stompor, R.

AU - Suzuki, A.

AU - Suzuki, J.

AU - Takada, S.

AU - Takakura, T.

AU - Tomaru, T.

AU - Wilson, B.

AU - Yamaguchi, H.

AU - Zahn, O.

PY - 2014

Y1 - 2014

N2 - Polarbear-2 is a next-generation receiver for precision measurements of the polarization of the cosmic mi-crowave background (Cosmic Microwave Background (CMB)). Scheduled to deploy in early 2015, it will observealongside the existing Polarbear-1 receiver, on a new telescope in the Simons Arrayon Cerro Toco in theAtacama desert of Chile. For increased sensitivity, it will feature a larger area focal plane, with a total of 7,588 polarization sensitive antenna-coupled Transition Edge Sensor (TES) bolometers, with a design sensitivity of 4.1 μKs. The focal plane will be cooled to 250 milliKelvin, and the bolometers will be read-out with 40 × frequency domain multiplexing, with 36 optical bolometers on a single SQUID amplier, along with 2 dark bolometers and 2 calibration resistors. To increase the multiplexing factor from 8 × for Polarbear-1 to 40 × for Polarbear-2 requires additional bandwidth for SQUID readout and well-dened frequency channel spacing. Extending to these higher frequencies requires new components and design for the LC lters which dene channel spacing. The LC lters are cold resonant circuits with an inductor and capacitor in series with each bolometer, and stray inductance in the wiring and equivalent series resistance from the capacitors can aect bolometer operation. We present results from characterizing these new readout components. Integration of the readout system is being done rst on a small scale, to ensure that the readout system does not aect bolometer sensitivity or stability, and to validate the overall system before expansion into the full receiver. We present the status of readout integration, and the initial results and status of components for the full array.

AB - Polarbear-2 is a next-generation receiver for precision measurements of the polarization of the cosmic mi-crowave background (Cosmic Microwave Background (CMB)). Scheduled to deploy in early 2015, it will observealongside the existing Polarbear-1 receiver, on a new telescope in the Simons Arrayon Cerro Toco in theAtacama desert of Chile. For increased sensitivity, it will feature a larger area focal plane, with a total of 7,588 polarization sensitive antenna-coupled Transition Edge Sensor (TES) bolometers, with a design sensitivity of 4.1 μKs. The focal plane will be cooled to 250 milliKelvin, and the bolometers will be read-out with 40 × frequency domain multiplexing, with 36 optical bolometers on a single SQUID amplier, along with 2 dark bolometers and 2 calibration resistors. To increase the multiplexing factor from 8 × for Polarbear-1 to 40 × for Polarbear-2 requires additional bandwidth for SQUID readout and well-dened frequency channel spacing. Extending to these higher frequencies requires new components and design for the LC lters which dene channel spacing. The LC lters are cold resonant circuits with an inductor and capacitor in series with each bolometer, and stray inductance in the wiring and equivalent series resistance from the capacitors can aect bolometer operation. We present results from characterizing these new readout components. Integration of the readout system is being done rst on a small scale, to ensure that the readout system does not aect bolometer sensitivity or stability, and to validate the overall system before expansion into the full receiver. We present the status of readout integration, and the initial results and status of components for the full array.

KW - CMB

KW - CMB polarization

KW - antenna

KW - bolometer

KW - ination

KW - millimeter-wave

KW - neutrinos

UR - http://www.scopus.com/inward/record.url?scp=84922928146&partnerID=8YFLogxK

U2 - 10.1117/12.2055611

DO - 10.1117/12.2055611

M3 - 會議論文篇章

AN - SCOPUS:84922928146

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII

A2 - Zmuidzinas, Jonas

A2 - Holland, Wayne S.

PB - SPIE

T2 - Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII

Y2 - 24 June 2014 through 27 June 2014

ER -

Barron D, Ade PAR, Akiba Y, Aleman C, Arnold K, Atlas M et al. Development and characterization of the readout system for POLARBEAR-2. In Zmuidzinas J, Holland WS, editors, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII. SPIE. 2014. 915335. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.2055611

Development and characterization of the readout system for POLARBEAR-2

Abstract

Publication series

Conference

Keywords

Access to Document

Fingerprint

Cite this