The Cℓover experiment

L. Piccirillo; P. Ade; M. D. Audley; C. Baines; R. Battye; M. Brown; P. Calisse; A. Challinor; W. D. Duncan; P. Ferreira; W. Gear; D. M. Glowacka; D. Goldie; P. K. Grimes; M. Halpern; V. Haynes; G. C. Hilton; K. D. Irwin; B. Johnson; M. Jones; A. Lasenby; P. Leahy; J. Leech; S. Lewis; B. Maffei; L. Martinis; P. D. Mauskopf; S. J. Melhuish; C. E. North; D. O'Dea; S. Parsley; G. Pisano; C. D. Reintsema; G. Savini; R. V. Sudiwala; D. Sutton; A. Taylor; G. Teleberg; D. Titterington; V. N. Tsaneva; C. Tucker; R. Watson; S. Withington; G. Yassin; J. Zhang

doi:10.1117/12.788927

The C_ℓover experiment

L. Piccirillo, P. Ade, M. D. Audley, C. Baines, R. Battye, M. Brown, P. Calisse, A. Challinor, W. D. Duncan, P. Ferreira, W. Gear, D. M. Glowacka, D. Goldie, P. K. Grimes, M. Halpern, V. Haynes, G. C. Hilton, K. D. Irwin, B. Johnson, M. JonesA. Lasenby, P. Leahy, J. Leech, S. Lewis, B. Maffei, L. Martinis, P. D. Mauskopf, S. J. Melhuish, C. E. North, D. O'Dea, S. Parsley, G. Pisano, C. D. Reintsema, G. Savini, R. V. Sudiwala, D. Sutton, A. Taylor, G. Teleberg, D. Titterington, V. N. Tsaneva, C. Tucker, R. Watson, S. Withington, G. Yassin, J. Zhang

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

8 Scopus citations

Abstract

C_ℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. C_ℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of C_ℓOVER is to be sensitive to gravitational waves down to r ∼ 0.03 (at 3σ) in two years of operations.

Original language	English (US)
Title of host publication	Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV
DOIs	https://doi.org/10.1117/12.788927
State	Published - 2008
Externally published	Yes
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

ASJC Scopus subject areas

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

Access to Document

10.1117/12.788927

Cite this

Piccirillo, L., Ade, P., Audley, M. D., Baines, C., Battye, R., Brown, M., Calisse, P., Challinor, A., Duncan, W. D., Ferreira, P., Gear, W., Glowacka, D. M., Goldie, D., Grimes, P. K., Halpern, M., Haynes, V., Hilton, G. C., Irwin, K. D., Johnson, B., ... Zhang, J. (2008). The C_ℓover experiment. In Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV Article 70201E (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 7020). https://doi.org/10.1117/12.788927

Piccirillo, L, Ade, P, Audley, MD, Baines, C, Battye, R, Brown, M, Calisse, P, Challinor, A, Duncan, WD, Ferreira, P, Gear, W, Glowacka, DM, Goldie, D, Grimes, PK, Halpern, M, Haynes, V, Hilton, GC, Irwin, KD, Johnson, B, Jones, M, Lasenby, A, Leahy, P, Leech, J, Lewis, S, Maffei, B, Martinis, L, Mauskopf, PD, Melhuish, SJ, North, CE, O'Dea, D, Parsley, S, Pisano, G, Reintsema, CD, Savini, G, Sudiwala, RV, Sutton, D, Taylor, A, Teleberg, G, Titterington, D, Tsaneva, VN, Tucker, C, Watson, R, Withington, S, Yassin, G & Zhang, J 2008, The C_ℓover experiment. in Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV., 70201E, 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/10.1117/12.788927

@inproceedings{1029d40a994c4b639d05d5b59e2fabea,

title = "The Cℓover experiment",

abstract = "CℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. CℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of CℓOVER is to be sensitive to gravitational waves down to r ∼ 0.03 (at 3σ) in two years of operations.",

author = "L. Piccirillo and P. Ade and Audley, {M. D.} and C. Baines and R. Battye and M. Brown and P. Calisse and A. Challinor and Duncan, {W. D.} and P. Ferreira and W. Gear and Glowacka, {D. M.} and D. Goldie and Grimes, {P. K.} and M. Halpern and V. Haynes and Hilton, {G. C.} and Irwin, {K. D.} and B. Johnson and M. Jones and A. Lasenby and P. Leahy and J. Leech and S. Lewis and B. Maffei and L. Martinis and Mauskopf, {P. D.} and Melhuish, {S. J.} and North, {C. E.} and D. O'Dea and S. Parsley and G. Pisano and Reintsema, {C. D.} and G. Savini and Sudiwala, {R. V.} and D. Sutton and A. Taylor and G. Teleberg and D. Titterington and Tsaneva, {V. N.} and C. Tucker and R. Watson and S. Withington and G. Yassin and J. Zhang",

year = "2008",

doi = "10.1117/12.788927",

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",

}

TY - GEN

T1 - The Cℓover experiment

AU - Piccirillo, L.

AU - Ade, P.

AU - Audley, M. D.

AU - Baines, C.

AU - Battye, R.

AU - Brown, M.

AU - Calisse, P.

AU - Challinor, A.

AU - Duncan, W. D.

AU - Ferreira, P.

AU - Gear, W.

AU - Glowacka, D. M.

AU - Goldie, D.

AU - Grimes, P. K.

AU - Halpern, M.

AU - Haynes, V.

AU - Hilton, G. C.

AU - Irwin, K. D.

AU - Johnson, B.

AU - Jones, M.

AU - Lasenby, A.

AU - Leahy, P.

AU - Leech, J.

AU - Lewis, S.

AU - Maffei, B.

AU - Martinis, L.

AU - Mauskopf, P. D.

AU - Melhuish, S. J.

AU - North, C. E.

AU - O'Dea, D.

AU - Parsley, S.

AU - Pisano, G.

AU - Reintsema, C. D.

AU - Savini, G.

AU - Sudiwala, R. V.

AU - Sutton, D.

AU - Taylor, A.

AU - Teleberg, G.

AU - Titterington, D.

AU - Tsaneva, V. N.

AU - Tucker, C.

AU - Watson, R.

AU - Withington, S.

AU - Yassin, G.

AU - Zhang, J.

PY - 2008

Y1 - 2008

N2 - CℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. CℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of CℓOVER is to be sensitive to gravitational waves down to r ∼ 0.03 (at 3σ) in two years of operations.

AB - CℓOVER is a multi-frequency experiment optimised to measure the Cosmic Microwave Background (CMB) polarization, in particular the B-mode component. CℓOVER comprises two instruments observing respectively at 97 GHz and 150/225 GHz. The focal plane of both instruments consists of an array of corrugated feed-horns coupled to TES detectors cooled at 100 mK. The primary science goal of CℓOVER is to be sensitive to gravitational waves down to r ∼ 0.03 (at 3σ) in two years of operations.

UR - http://www.scopus.com/inward/record.url?scp=52249099666&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=52249099666&partnerID=8YFLogxK

U2 - 10.1117/12.788927

DO - 10.1117/12.788927

M3 - Conference contribution

AN - SCOPUS:52249099666

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 -