Built on

W. L. K. Wu, L. M. Mocanu, P. A. R. Ade, A. J. Anderson, J. E. Austermann, J. S. Avva, J. A. Beall, A. N. Bender, B. A. Benson and F. Bianchini, et al
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D. N. Limber, Astrophys. J. 119
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1987
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M. Kamionkowski, A. Kosowsky and A. Stebbins, Phys. Rev. D 55
1997
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M. Zaldarriaga and U. Seljak, Phys. Rev. D 58
1998
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A. Lewis, A. Challinor and A. Lasenby, Astrophys. J. 538
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W. Hu and T. Okamoto, Astrophys. J. 574
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T. Okamoto and W. Hu, Phys. Rev. D 67
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M. H. Kesden, A. Cooray and M. Kamionkowski, Phys. Rev. D 67
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C. M. Hirata and U. Seljak, Phys. Rev. D 68
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C. M. Hirata, N. Padmanabhan, U. Seljak, D. Schlegel and J. Brinkmann, Phys. Rev. D 70
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O. Darwish, M. S. Madhavacheril, B. D. Sherwin, S. Aiola, N. Battaglia, J. A. Beall, D. T. Becker, J. R. Bond, E. Calabrese and S. Choi, et al
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K. M. Gorski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke and M. Bartelman, Astrophys. J. 622
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A. Lewis and A. Challinor, Phys. Rept. 429
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K. M. Smith, O. Zahn and O. Dore, Phys. Rev. D 76
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2007
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K. M. Smith, O. Zahn and O. Dore, Phys. Rev. D 76
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2007
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Then

P. A. R. Ade et al
Original
2014
Later among the works it cites.
D. Huterer, D. Kirkby, R. Bean, A. Connolly, K. Dawson, S. Dodelson, A. Evrard, B. Jain, M. Jarvis and E. Linder, et al
Original
2014
Later among the works it cites.
P. A. R. Ade et al
Original
2016
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P. A. R. Ade et al
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2016
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J. Carron and A. Lewis, Phys. Rev. D 96
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2017
Later among the works it cites.

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2022

Forecasts on CMB lensing observations with AliCPT-1

Liu, Jinyi, Sun, Zeyang, Han, Jiakang et al.

Understand

AliCPT-1 is the first Chinese CMB experiment aiming for high precision measurement of Cosmic Microwave Background B-mode polarization.

The telescope, currently under deployment in Tibet, will observe in two frequency bands centered at 90 and 150 GHz.
We forecast the CMB lensing reconstruction, lensing-galaxy as well as lensing-CIB (Cosmic Infrared Background) cross correlation signal-to-noise ratio (SNR) for AliCPT-1.
We consider two stages with different integrated observation time, namely "4 module*yr" (first stage) and "48 module*yr" (final stage).

Built on

W. L. K. Wu, L. M. Mocanu, P. A. R. Ade, A. J. Anderson, J. E. Austermann, J. S. Avva, J. A. Beall, A. N. Bender, B. A. Benson and F. Bianchini, et al
Original
1905
Earlier work this paper cites.
D. Lenz, O. Doré and G. Lagache, Astrophys. J. 883
Original
1905
Earlier work this paper cites.
J. T. Sayre et al
Original
1910
Earlier work this paper cites.
D. N. Limber, Astrophys. J. 119
1954
Earlier work this paper cites.
Blanchard, A. and Schneider, J. 1987, 184, 1
1987
Earlier work this paper cites.
M. Kamionkowski, A. Kosowsky and A. Stebbins, Phys. Rev. D 55
1997
Earlier work this paper cites.
M. Zaldarriaga and U. Seljak, Phys. Rev. D 58
1998
Earlier work this paper cites.
A. Lewis, A. Challinor and A. Lasenby, Astrophys. J. 538
2000
Earlier work this paper cites.
W. Hu and T. Okamoto, Astrophys. J. 574
2002
Earlier work this paper cites.
T. Okamoto and W. Hu, Phys. Rev. D 67
2003
Earlier work this paper cites.
M. H. Kesden, A. Cooray and M. Kamionkowski, Phys. Rev. D 67
2003
Earlier work this paper cites.
Y. S. Song, A. Cooray, L. Knox and M. Zaldarriaga, Astrophys. J. 590
2003
Earlier work this paper cites.
C. M. Hirata and U. Seljak, Phys. Rev. D 68
2003
Earlier work this paper cites.
C. M. Hirata, N. Padmanabhan, U. Seljak, D. Schlegel and J. Brinkmann, Phys. Rev. D 70
2004
Earlier work this paper cites.
O. Darwish, M. S. Madhavacheril, B. D. Sherwin, S. Aiola, N. Battaglia, J. A. Beall, D. T. Becker, J. R. Bond, E. Calabrese and S. Choi, et al
Original
2004
Earlier work this paper cites.
K. M. Gorski, E. Hivon, A. J. Banday, B. D. Wandelt, F. K. Hansen, M. Reinecke and M. Bartelman, Astrophys. J. 622
2005
Earlier work this paper cites.
A. Lewis and A. Challinor, Phys. Rept. 429
2006
Earlier work this paper cites.
K. M. Smith, O. Zahn and O. Dore, Phys. Rev. D 76
Original
2007
Earlier work this paper cites.
K. M. Smith, O. Zahn and O. Dore, Phys. Rev. D 76
Original
2007
Earlier work this paper cites.