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A Forecast of the Sensitivity on the Measurement of the Optical Depth to Reionization with the GroundBIRD Experiment

Authors
Lee, K.Genova-Santos, R. T.Hazumi, M.Honda, S.Kutsuma, H.Oguri, S.Otani, C.Peel, M. W.Sueno, Y.Suzuki, J.Tajima, O.Won, E.
Issue Date
7월-2021
Publisher
IOP PUBLISHING LTD
Citation
ASTROPHYSICAL JOURNAL, v.915, no.2
Indexed
SCIE
SCOPUS
Journal Title
ASTROPHYSICAL JOURNAL
Volume
915
Number
2
URI
https://scholar.korea.ac.kr/handle/2021.sw.korea/127739
DOI
10.3847/1538-4357/ac024b
ISSN
0004-637X
Abstract
We compute the expected sensitivity on measurements of optical depth to reionization for a ground-based experiment at Teide Observatory. We simulate polarized partial sky maps for the GroundBIRD experiment at the frequencies 145 and 220 GHz. We perform fits for the simulated maps with our pixel-based likelihood to extract the optical depth to reionization. The noise levels of polarization maps are estimated as 110 mu K arcmin and 780 mu K arcmin for 145 and 220 GHz, respectively, by assuming a three-year observing campaign and sky coverages of 0.537 for 145 GHz and 0.462 for 220 GHz. Our sensitivities for the optical depth to reionization are found to be sigma(tau) = 0.030 with the simulated GroundBIRD maps, and sigma(tau) = 0.012 by combining with the simulated QUIJOTE maps at 11, 13, 17, 19, 30, and 40 GHz.
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