Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array

Adam L. Woodcraft; Matthew I. Hollister; Dan Bintley; Maureen A. Ellis; Xiaofeng Gao; Wayne S. Holland; Michael J. MacIntosh; Peter A. R. Ade; Julian S. House; Cynthia L. Hunt; Rashmi V. Sudiwala; William D. Duncan; Gene C. Hilton; Kent D. Irwin; Carl D. Reintsema; Camelia C. Dunare; William Parkes; Anthony J. Walton; Jan B. Kycia; Mandana Amiri; Bryce Burger; Mark Halpern

doi:10.1117/12.671310

Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array

Adam L. Woodcraft, Matthew I. Hollister, Dan Bintley, Maureen A. Ellis, Xiaofeng Gao, Wayne S. Holland, Michael J. MacIntosh, Peter A. R. Ade, Julian S. House, Cynthia L. Hunt, Rashmi V. Sudiwala, William D. Duncan, Gene C. Hilton, Kent D. Irwin, Carl D. Reintsema, Camelia C. Dunare, William Parkes, Anthony J. Walton, Jan B. Kycia, Mandana AmiriBryce Burger, Mark Halpern

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

Abstract

We present the results of characterization measurements on a 1280 pixel superconducting bolometer array designed for operation at wavelengths around 450 pm. The array is a prototype for the sub-arrays which will form the focal plane for the SCUBA-2 sub-mm camera, being built for the James Clerk Maxwell Telescope (JCMT) in Hawaii. With over 10 000 pixels in total, it will provide a huge improvement in both sensitivity and mapping speed over existing instruments. The array consists of molybdenum-copper bi-layer TES (transition edge sensor) pixels, bonded to a multiplexer. The detectors operate at a temperature of approximately 175 mK, and require a heat sink at a temperature of approximately 60 mK. In contrast to previous TES arrays, the multiplexing elements are located beneath each pixel (an "in-focal plane" configuration). We present the results of electrical and optical measurements, and show that the optical NEP (noise equivalent power) is less than 1.4 x 10(-16) W Hz(-0.5), and thus within the requirement of 2.9 x 10(-16) W Hz(-0.5).

Original language	English
Title of host publication	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
Editors	J Zmuidzinas, WS Holland, S Withington, WD Duncan
Place of Publication	BELLINGHAM
Publisher	SPIE
Pages	F2751-F2751
Number of pages	11
ISBN (Print)	0-8194-6340-X
DOIs	https://doi.org/10.1117/12.671310
Publication status	Published - 2006
Event	Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III - Orlando Duration: 29 May 2006 → 31 May 2006

Conference

Conference	Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III
City	Orlando
Period	29/05/06 → 31/05/06

Keywords / Materials (for Non-textual outputs)

TES
superconducting detectors
submillimetre astronomy
large format
imaging
array
SCUBA-2
detectors
characterization
JCMT
ASTRONOMY
MULTIPLEXER
DESIGN
CAMERA

Access to Document

10.1117/12.671310

SCUBA-2
Walton, A. (Principal Investigator), Gundlach, A. (Co-investigator), Stevenson, T. (Co-investigator) & Terry, J. (Researcher)
STFC
1/02/01 → 31/01/08
Project: Research

Cite this

Woodcraft, A. L., Hollister, M. I., Bintley, D., Ellis, M. A., Gao, X., Holland, W. S., MacIntosh, M. J., Ade, P. A. R., House, J. S., Hunt, C. L., Sudiwala, R. V., Duncan, W. D., Hilton, G. C., Irwin, K. D., Reintsema, C. D., Dunare, C. C., Parkes, W., Walton, A. J., Kycia, J. B., ... Halpern, M. (2006). Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array. In J. Zmuidzinas, WS. Holland, S. Withington, & WD. Duncan (Eds.), Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III (pp. F2751-F2751). SPIE. https://doi.org/10.1117/12.671310

@inproceedings{b50a7556dfc6458c9c3f79ed1eeae82c,

title = "Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array",

abstract = "We present the results of characterization measurements on a 1280 pixel superconducting bolometer array designed for operation at wavelengths around 450 pm. The array is a prototype for the sub-arrays which will form the focal plane for the SCUBA-2 sub-mm camera, being built for the James Clerk Maxwell Telescope (JCMT) in Hawaii. With over 10 000 pixels in total, it will provide a huge improvement in both sensitivity and mapping speed over existing instruments. The array consists of molybdenum-copper bi-layer TES (transition edge sensor) pixels, bonded to a multiplexer. The detectors operate at a temperature of approximately 175 mK, and require a heat sink at a temperature of approximately 60 mK. In contrast to previous TES arrays, the multiplexing elements are located beneath each pixel (an {"}in-focal plane{"} configuration). We present the results of electrical and optical measurements, and show that the optical NEP (noise equivalent power) is less than 1.4 x 10(-16) W Hz(-0.5), and thus within the requirement of 2.9 x 10(-16) W Hz(-0.5).",

keywords = "TES, superconducting detectors, submillimetre astronomy, large format, imaging, array, SCUBA-2, detectors, characterization, JCMT, ASTRONOMY, MULTIPLEXER, DESIGN, CAMERA",

author = "Woodcraft, \{Adam L.\} and Hollister, \{Matthew I.\} and Dan Bintley and Ellis, \{Maureen A.\} and Xiaofeng Gao and Holland, \{Wayne S.\} and MacIntosh, \{Michael J.\} and Ade, \{Peter A. R.\} and House, \{Julian S.\} and Hunt, \{Cynthia L.\} and Sudiwala, \{Rashmi V.\} and Duncan, \{William D.\} and Hilton, \{Gene C.\} and Irwin, \{Kent D.\} and Reintsema, \{Carl D.\} and Dunare, \{Camelia C.\} and William Parkes and Walton, \{Anthony J.\} and Kycia, \{Jan B.\} and Mandana Amiri and Bryce Burger and Mark Halpern",

year = "2006",

doi = "10.1117/12.671310",

language = "English",

isbn = "0-8194-6340-X",

pages = "F2751--F2751",

editor = "J Zmuidzinas and WS Holland and S Withington and WD Duncan",

booktitle = "Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III",

publisher = "SPIE",

address = "United States",

note = "Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III ; Conference date: 29-05-2006 Through 31-05-2006",

}

Woodcraft, AL, Hollister, MI, Bintley, D, Ellis, MA, Gao, X, Holland, WS, MacIntosh, MJ, Ade, PAR, House, JS, Hunt, CL, Sudiwala, RV, Duncan, WD, Hilton, GC, Irwin, KD, Reintsema, CD, Dunare, CC, Parkes, W, Walton, AJ, Kycia, JB, Amiri, M, Burger, B & Halpern, M 2006, Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array. in J Zmuidzinas, WS Holland, S Withington & WD Duncan (eds), Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. SPIE, BELLINGHAM, pp. F2751-F2751, Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III, Orlando, 29/05/06. https://doi.org/10.1117/12.671310

Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array. / Woodcraft, Adam L.; Hollister, Matthew I.; Bintley, Dan et al.
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. ed. / J Zmuidzinas; WS Holland; S Withington; WD Duncan. BELLINGHAM: SPIE, 2006. p. F2751-F2751.

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

TY - GEN

T1 - Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array

AU - Woodcraft, Adam L.

AU - Hollister, Matthew I.

AU - Bintley, Dan

AU - Ellis, Maureen A.

AU - Gao, Xiaofeng

AU - Holland, Wayne S.

AU - MacIntosh, Michael J.

AU - Ade, Peter A. R.

AU - House, Julian S.

AU - Hunt, Cynthia L.

AU - Sudiwala, Rashmi V.

AU - Duncan, William D.

AU - Hilton, Gene C.

AU - Irwin, Kent D.

AU - Reintsema, Carl D.

AU - Dunare, Camelia C.

AU - Parkes, William

AU - Walton, Anthony J.

AU - Kycia, Jan B.

AU - Amiri, Mandana

AU - Burger, Bryce

AU - Halpern, Mark

PY - 2006

Y1 - 2006

N2 - We present the results of characterization measurements on a 1280 pixel superconducting bolometer array designed for operation at wavelengths around 450 pm. The array is a prototype for the sub-arrays which will form the focal plane for the SCUBA-2 sub-mm camera, being built for the James Clerk Maxwell Telescope (JCMT) in Hawaii. With over 10 000 pixels in total, it will provide a huge improvement in both sensitivity and mapping speed over existing instruments. The array consists of molybdenum-copper bi-layer TES (transition edge sensor) pixels, bonded to a multiplexer. The detectors operate at a temperature of approximately 175 mK, and require a heat sink at a temperature of approximately 60 mK. In contrast to previous TES arrays, the multiplexing elements are located beneath each pixel (an "in-focal plane" configuration). We present the results of electrical and optical measurements, and show that the optical NEP (noise equivalent power) is less than 1.4 x 10(-16) W Hz(-0.5), and thus within the requirement of 2.9 x 10(-16) W Hz(-0.5).

AB - We present the results of characterization measurements on a 1280 pixel superconducting bolometer array designed for operation at wavelengths around 450 pm. The array is a prototype for the sub-arrays which will form the focal plane for the SCUBA-2 sub-mm camera, being built for the James Clerk Maxwell Telescope (JCMT) in Hawaii. With over 10 000 pixels in total, it will provide a huge improvement in both sensitivity and mapping speed over existing instruments. The array consists of molybdenum-copper bi-layer TES (transition edge sensor) pixels, bonded to a multiplexer. The detectors operate at a temperature of approximately 175 mK, and require a heat sink at a temperature of approximately 60 mK. In contrast to previous TES arrays, the multiplexing elements are located beneath each pixel (an "in-focal plane" configuration). We present the results of electrical and optical measurements, and show that the optical NEP (noise equivalent power) is less than 1.4 x 10(-16) W Hz(-0.5), and thus within the requirement of 2.9 x 10(-16) W Hz(-0.5).

KW - TES

KW - superconducting detectors

KW - submillimetre astronomy

KW - large format

KW - imaging

KW - array

KW - SCUBA-2

KW - detectors

KW - characterization

KW - JCMT

KW - ASTRONOMY

KW - MULTIPLEXER

KW - DESIGN

KW - CAMERA

U2 - 10.1117/12.671310

DO - 10.1117/12.671310

M3 - Conference contribution

SN - 0-8194-6340-X

SP - F2751-F2751

BT - Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III

A2 - Zmuidzinas, J

A2 - Holland, WS

A2 - Withington, S

A2 - Duncan, WD

PB - SPIE

CY - BELLINGHAM

T2 - Conference on Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III

Y2 - 29 May 2006 through 31 May 2006

ER -

Woodcraft AL, Hollister MI, Bintley D, Ellis MA, Gao X, Holland WS et al. Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array. In Zmuidzinas J, Holland WS, Withington S, Duncan WD, editors, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy III. BELLINGHAM: SPIE. 2006. p. F2751-F2751 doi: 10.1117/12.671310

Characterization of a prototype SCUBA-2 1280 pixel submillimetre superconducting bolometer array

Abstract

Conference

Keywords / Materials (for Non-textual outputs)

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Projects

SCUBA-2

Cite this