Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope

R. J. Thornton; P. A.R. Ade; C. Allen; M. Amiri; J. W. Appel; E. S. Battistelli; B. Burger; J. A. Chervenak; M. J. Devlin; S. R. Dicker; W. B. Doriese; T. Essinger-Hileman; R. P. Fishery; J. W. Fowler; M. Halpern; P. C. Hargrave; M. Hasselfield; G. C. Hilton; A. D. Hincks; K. D. Irwin; N. Jarosik; M. Kaul; J. Klein; J. M. Lau; M. Limon; T. A. Marriage; K. L. Martocci; P. Mauskopf; S. H. Moseley; M. D. Niemack; L. Page; L. P. Parker; J. Reidel; C. D. Reintsema; S. T. Staggs; O. R. Stryzak; D. S. Swetz; E. R. Switzer; C. Tucker; E. J. Wollack; Y. Zhao

doi:10.1117/12.790078

Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope

R. J. Thornton
, P. A.R. Ade
, C. Allen
, M. Amiri
, J. W. Appel
, E. S. Battistelli
, B. Burger
, J. A. Chervenak
, M. J. Devlin
, S. R. Dicker
, W. B. Doriese
, T. Essinger-Hileman
, R. P. Fishery
, J. W. Fowler
, M. Halpern
, P. C. Hargrave
, M. Hasselfield
, G. C. Hilton
, A. D. Hincks
, K. D. Irwin

N. Jarosik, M. Kaul, J. Klein, J. M. Lau, M. Limon, T. A. Marriage, K. L. Martocci, P. Mauskopf, S. H. Moseley, M. D. Niemack, L. Page, L. P. Parker, J. Reidel, C. D. Reintsema, S. T. Staggs, O. R. Stryzak, D. S. Swetz, E. R. Switzer, C. Tucker, E. J. Wollack, Y. Zhao

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

10 Scopus citations

Abstract

The 6-meter Atacama Cosmology Telescope will map the cosmic microwave background at millimeter wave-lengths. The commissioning instrument for the telescope, the Millimeter Bolometer Array Camera, is based on a refractive optical system which simultaneously images three separate fields of view at three different frequencies: 145, 220, and 280 GHz. Each frequency band contains around twelve individual optical elements at five different temperature stages ranging from 300 K to 300 mK and a 32 × 32 array of Transition Edge Sensor bolometers at 300 mK. We discuss the design of the close-packed on-axis optical design of the three frequencies. The thermal design and performance of the system are presented in the context of the scientific requirements and observing schedule. A major part of the design was the incorporation of multiple layers of magnetic shielding. We discuss the performance of the 145 GHz optical system in 2007 and the implementation of the additional two frequency channels in 2008.

Original language	English (US)
Title of host publication	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
DOIs	https://doi.org/10.1117/12.790078
State	Published - 2008
Event	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV - Marseille, France Duration: Jun 26 2008 → Jun 28 2008

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	7020
ISSN (Print)	0277-786X

Other

Other	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
Country/Territory	France
City	Marseille
Period	6/26/08 → 6/28/08

All Science Journal Classification (ASJC) codes

Electronic, Optical and Magnetic Materials
Instrumentation
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Keywords

CMB telescope
Cryogenic
Mechanical design
Millimeter camera

Access to Document

10.1117/12.790078

Cite this

Thornton, R. J., Ade, P. A. R., Allen, C., Amiri, M., Appel, J. W., Battistelli, E. S., Burger, B., Chervenak, J. A., Devlin, M. J., Dicker, S. R., Doriese, W. B., Essinger-Hileman, T., Fishery, R. P., Fowler, J. W., Halpern, M., Hargrave, P. C., Hasselfield, M., Hilton, G. C., Hincks, A. D., ... Zhao, Y. (2008). Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Article 70201R (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7020). https://doi.org/10.1117/12.790078

@inproceedings{644b08aafe8d4185b3b269470ad71d6e,

title = "Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope",

abstract = "The 6-meter Atacama Cosmology Telescope will map the cosmic microwave background at millimeter wave-lengths. The commissioning instrument for the telescope, the Millimeter Bolometer Array Camera, is based on a refractive optical system which simultaneously images three separate fields of view at three different frequencies: 145, 220, and 280 GHz. Each frequency band contains around twelve individual optical elements at five different temperature stages ranging from 300 K to 300 mK and a 32 × 32 array of Transition Edge Sensor bolometers at 300 mK. We discuss the design of the close-packed on-axis optical design of the three frequencies. The thermal design and performance of the system are presented in the context of the scientific requirements and observing schedule. A major part of the design was the incorporation of multiple layers of magnetic shielding. We discuss the performance of the 145 GHz optical system in 2007 and the implementation of the additional two frequency channels in 2008.",

keywords = "CMB telescope, Cryogenic, Mechanical design, Millimeter camera",

author = "Thornton, \{R. J.\} and Ade, \{P. A.R.\} and C. Allen and M. Amiri and Appel, \{J. W.\} and Battistelli, \{E. S.\} and B. Burger and Chervenak, \{J. A.\} and Devlin, \{M. J.\} and Dicker, \{S. R.\} and Doriese, \{W. B.\} and T. Essinger-Hileman and Fishery, \{R. P.\} and Fowler, \{J. W.\} and M. Halpern and Hargrave, \{P. C.\} and M. Hasselfield and Hilton, \{G. C.\} and Hincks, \{A. D.\} and Irwin, \{K. D.\} and N. Jarosik and M. Kaul and J. Klein and Lau, \{J. M.\} and M. Limon and Marriage, \{T. A.\} and Martocci, \{K. L.\} and P. Mauskopf and Moseley, \{S. H.\} and Niemack, \{M. D.\} and L. Page and Parker, \{L. P.\} and J. Reidel and Reintsema, \{C. D.\} and Staggs, \{S. T.\} and Stryzak, \{O. R.\} and Swetz, \{D. S.\} and Switzer, \{E. R.\} and C. Tucker and Wollack, \{E. J.\} and Y. Zhao",

year = "2008",

doi = "10.1117/12.790078",

language = "English (US)",

isbn = "9780819472304",

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

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

note = "Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV ; Conference date: 26-06-2008 Through 28-06-2008",

}

Thornton, RJ, Ade, PAR, Allen, C, Amiri, M, Appel, JW, Battistelli, ES, Burger, B, Chervenak, JA, Devlin, MJ, Dicker, SR, Doriese, WB, Essinger-Hileman, T, Fishery, RP, Fowler, JW, Halpern, M, Hargrave, PC, Hasselfield, M, Hilton, GC, Hincks, AD, Irwin, KD, Jarosik, N, Kaul, M, Klein, J, Lau, JM, Limon, M, Marriage, TA, Martocci, KL, Mauskopf, P, Moseley, SH, Niemack, MD, Page, L, Parker, LP, Reidel, J, Reintsema, CD, Staggs, ST, Stryzak, OR, Swetz, DS, Switzer, ER, Tucker, C, Wollack, EJ & Zhao, Y 2008, Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV., 70201R, Proceedings of SPIE - The International Society for Optical Engineering, vol. 7020, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, Marseille, France, 6/26/08. https://doi.org/10.1117/12.790078

Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope. / Thornton, R. J.; Ade, P. A.R.; Allen, C. et al.
Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. 2008. 70201R (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7020).

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

TY - GEN

T1 - Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope

AU - Thornton, R. J.

AU - Ade, P. A.R.

AU - Allen, C.

AU - Amiri, M.

AU - Appel, J. W.

AU - Battistelli, E. S.

AU - Burger, B.

AU - Chervenak, J. A.

AU - Devlin, M. J.

AU - Dicker, S. R.

AU - Doriese, W. B.

AU - Essinger-Hileman, T.

AU - Fishery, R. P.

AU - Fowler, J. W.

AU - Halpern, M.

AU - Hargrave, P. C.

AU - Hasselfield, M.

AU - Hilton, G. C.

AU - Hincks, A. D.

AU - Irwin, K. D.

AU - Jarosik, N.

AU - Kaul, M.

AU - Klein, J.

AU - Lau, J. M.

AU - Limon, M.

AU - Marriage, T. A.

AU - Martocci, K. L.

AU - Mauskopf, P.

AU - Moseley, S. H.

AU - Niemack, M. D.

AU - Page, L.

AU - Parker, L. P.

AU - Reidel, J.

AU - Reintsema, C. D.

AU - Staggs, S. T.

AU - Stryzak, O. R.

AU - Swetz, D. S.

AU - Switzer, E. R.

AU - Tucker, C.

AU - Wollack, E. J.

AU - Zhao, Y.

PY - 2008

Y1 - 2008

N2 - The 6-meter Atacama Cosmology Telescope will map the cosmic microwave background at millimeter wave-lengths. The commissioning instrument for the telescope, the Millimeter Bolometer Array Camera, is based on a refractive optical system which simultaneously images three separate fields of view at three different frequencies: 145, 220, and 280 GHz. Each frequency band contains around twelve individual optical elements at five different temperature stages ranging from 300 K to 300 mK and a 32 × 32 array of Transition Edge Sensor bolometers at 300 mK. We discuss the design of the close-packed on-axis optical design of the three frequencies. The thermal design and performance of the system are presented in the context of the scientific requirements and observing schedule. A major part of the design was the incorporation of multiple layers of magnetic shielding. We discuss the performance of the 145 GHz optical system in 2007 and the implementation of the additional two frequency channels in 2008.

AB - The 6-meter Atacama Cosmology Telescope will map the cosmic microwave background at millimeter wave-lengths. The commissioning instrument for the telescope, the Millimeter Bolometer Array Camera, is based on a refractive optical system which simultaneously images three separate fields of view at three different frequencies: 145, 220, and 280 GHz. Each frequency band contains around twelve individual optical elements at five different temperature stages ranging from 300 K to 300 mK and a 32 × 32 array of Transition Edge Sensor bolometers at 300 mK. We discuss the design of the close-packed on-axis optical design of the three frequencies. The thermal design and performance of the system are presented in the context of the scientific requirements and observing schedule. A major part of the design was the incorporation of multiple layers of magnetic shielding. We discuss the performance of the 145 GHz optical system in 2007 and the implementation of the additional two frequency channels in 2008.

KW - CMB telescope

KW - Cryogenic

KW - Mechanical design

KW - Millimeter camera

UR - https://www.scopus.com/pages/publications/52249099882

UR - https://www.scopus.com/pages/publications/52249099882#tab=citedBy

U2 - 10.1117/12.790078

DO - 10.1117/12.790078

M3 - Conference contribution

AN - SCOPUS:52249099882

SN - 9780819472304

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

BT - Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV

T2 - Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV

Y2 - 26 June 2008 through 28 June 2008

ER -

Thornton RJ, Ade PAR, Allen C, Amiri M, Appel JW, Battistelli ES et al. Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. 2008. 70201R. (Proceedings of SPIE - The International Society for Optical Engineering). doi: 10.1117/12.790078

Opto-mechanical design and performance of a compact three-frequency camera for the Millimeter Bolometer Array Camera on the Atacama Cosmology Telescope

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All Science Journal Classification (ASJC) codes

Keywords

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