- S. W. Henderson1,
- R. Allison2,
- J. Austermann3,
- T. Baildon4,
- N. Battaglia5,
- J. A. Beall3,
- D. Becker3,
- F. De Bernardis1,
- J. R. Bond6,
- E. Calabrese5,
- S. K. Choi7,
- K. P. Coughlin4,
- K. T. Crowley7,
- R. Datta4,
- M. J. Devlin8,
- S. M. Duff3,
- J. Dunkley2,
- R. Dünner9,
- A. van Engelen6,
- P. A. Gallardo1,
- E. Grace7,
- M. Hasselfield5,
- F. Hills4,
- G. C. Hilton3,
- A. D. Hincks10,
- R. Hloẑek5,
- S. P. Ho7,
- J. Hubmayr3,
- K. Huffenberger11,
- J. P. Hughes12,
- K. D. Irwin13,
- B. J. Koopman1,
- A. B. Kosowsky14,
- D. Li3,15,
- J. McMahon4,
- C. Munson4,
- F. Nati8,
- L. Newburgh16,
- M. D. Niemack1,
- P. Niraula7,
- L. A. Page7,
- C. G. Pappas7,
- M. Salatino7,
- A. Schillaci7,22,
- B. L. Schmitt8,
- N. Sehgal17,
- B. D. Sherwin18,
- J. L. Sievers19,
- S. M. Simon7,
- D. N. Spergel5,
- S. T. Staggs7,
- J. R. Stevens1,
- R. Thornton20,
- J. Van Lanen3,
- E. M. Vavagiakis1,
- J. T. Ward8 &
- …
- E. J. Wollack21
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317Citations
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Abstract
Advanced ACTPol is a polarization-sensitive upgrade for the 6 m aperture Atacama Cosmology Telescope, adding new frequencies and increasing sensitivity over the previous ACTPol receiver. In 2016, Advanced ACTPol will begin to map approximately half the sky in five frequency bands (28–230 GHz). Its maps of primary and secondary cosmic microwave background anisotropies—imaged in intensity and polarization at few arcminute-scale resolution—will enable precision cosmological constraints and also a wide array of cross-correlation science that probes the expansion history of the universe and the growth of structure via gravitational collapse. To accomplish these scientific goals, the Advanced ACTPol receiver will be a significant upgrade to the ACTPol receiver, including four new multichroic arrays of cryogenic, feedhorn-coupled AlMn transition edge sensor polarimeters (fabricated on 150 mm diameter wafers); a system of continuously rotating meta-material silicon half-wave plates; and a new multiplexing readout architecture which uses superconducting quantum interference devices and time division to achieve a 64-row multiplexing factor. Here we present the status and scientific goals of the Advanced ACTPol instrument, emphasizing the design and implementation of the Advanced ACTPol cryogenic detector arrays.
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Acknowledgments
This work was supported by the U.S. National Science Foundation through Awards 1312380 and 1440226. The NIST authors would like to acknowledge the support of the NIST Quantum Initiative. The development of multichroic detectors and lenses was supported by NASA Grants NNX13AE56G and NNX14AB58G. The work of KPC, KTC, EG, BJK, CM, BLS, JTW, and SMS was supported by NASA Space Technology Research Fellowship awards.
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Authors and Affiliations
Department of Physics, Cornell University, Ithaca, NY, 14853, USA
S. W. Henderson, F. De Bernardis, P. A. Gallardo, B. J. Koopman, M. D. Niemack, J. R. Stevens & E. M. Vavagiakis
Sub-Department of Astrophysics, University of Oxford, Keble Road, Oxford, OX1 3RH, UK
R. Allison & J. Dunkley
NIST Quantum Devices Group, 325 Broadway Mailcode 817.03, Boulder, CO, 80305, USA
J. Austermann, J. A. Beall, D. Becker, S. M. Duff, G. C. Hilton, J. Hubmayr, D. Li & J. Van Lanen
Department of Physics, University of Michigan, Ann Arbor, 48103, USA
T. Baildon, K. P. Coughlin, R. Datta, F. Hills, J. McMahon & C. Munson
Department of Astrophysical Sciences, Peyton Hall, Princeton University, Princeton, NJ, 08544, USA
N. Battaglia, E. Calabrese, M. Hasselfield, R. Hloẑek & D. N. Spergel
Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, ON, M5S 3H8, Canada
J. R. Bond & A. van Engelen
Joseph Henry Laboratories of Physics, Jadwin Hall, Princeton University, Princeton, NJ, 08544, USA
S. K. Choi, K. T. Crowley, E. Grace, S. P. Ho, P. Niraula, L. A. Page, C. G. Pappas, M. Salatino, A. Schillaci, S. M. Simon & S. T. Staggs
Department of Physics and Astronomy, University of Pennsylvania, 209 South 33rd Street, Philadelphia, PA, 19104, USA
M. J. Devlin, F. Nati, B. L. Schmitt & J. T. Ward
Departamento de Astronomía y Astrofísica, Ponticía Universidad Católica, Casilla 306, Santiago 22, Chile
R. Dünner
Department of Physics and Astronomy, University of British Columbia, Vancouver, BC, V6T 1Z4, Canada
A. D. Hincks
Department of Physics, Florida State University, Tallahassee, FL, 32306, USA
K. Huffenberger
Department of Physics and Astronomy, Rutgers, The State University of New Jersey, Piscataway, NJ, 08854-8019, USA
J. P. Hughes
Department of Physics, Stanford University, Stanford, CA, 94305-4085, USA
K. D. Irwin
Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, PA, 15260, USA
A. B. Kosowsky
SLAC National Accelerator Laboratory, 2575 Sandy Hill Road, Menlo Park, CA, 94025, USA
D. Li
Dunlap Institute, University of Toronto, 50 St. George St., Toronto, ON, M5S 3H4, Canada
L. Newburgh
Physics and Astronomy Department, Stony Brook University, Stony Brook, NY, 11794, USA
N. Sehgal
Berkeley Center for Cosmological Physics, University of California, Berkeley, CA, 94720, USA
B. D. Sherwin
Astrophysics and Cosmology Research Unit, School of Mathematics, Statistics and Computer Science, University of KwaZulu-Natal, Durban, 4041, South Africa
J. L. Sievers
Department of Physics, West Chester University of Pennsylvania, West Chester, PA, 19383, USA
R. Thornton
NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA
E. J. Wollack
Sociedad Radiosky Asesorías de Ingeniería Limitada Lincoyán 54, Depto 805, Concepción, Chile
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Correspondence toS. W. Henderson.
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Henderson, S.W., Allison, R., Austermann, J.et al. Advanced ACTPol Cryogenic Detector Arrays and Readout.J Low Temp Phys184, 772–779 (2016). https://doi.org/10.1007/s10909-016-1575-z
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