Status of the GroundBIRD Telescope
Our understanding of physics at very early Universe, as early as 10−35 s after the Big Bang, relies on the scenario known as the inflationary cosmology. Inflation predicts a particular polarization pattern in the cosmic microwave background, known as the B-mode yet the strength of such polarization...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Article |
Language: | English |
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EDP Sciences
2018-01-01
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Series: | EPJ Web of Conferences |
Online Access: | https://doi.org/10.1051/epjconf/201816801014 |
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author | Choi J. Génova-Santos R. Hattori M. Hazumi M. Ishitsuka H. Kanno F. Karatsu K. Kiuchi K. Koyano R. Kutsuma H. Lee K. Mima S. Minowa M. Nagai M. Nagasaki T. Naruse M. Oguri S. Okada T. Otani C. Rebolo R. Rubiño-Martín J. Sekimoto Y. Suzuki J. Taino T. Tajima O. Tomita N. Uchida T. Won E. Yoshida M. |
author_facet | Choi J. Génova-Santos R. Hattori M. Hazumi M. Ishitsuka H. Kanno F. Karatsu K. Kiuchi K. Koyano R. Kutsuma H. Lee K. Mima S. Minowa M. Nagai M. Nagasaki T. Naruse M. Oguri S. Okada T. Otani C. Rebolo R. Rubiño-Martín J. Sekimoto Y. Suzuki J. Taino T. Tajima O. Tomita N. Uchida T. Won E. Yoshida M. |
author_sort | Choi J. |
collection | DOAJ |
description | Our understanding of physics at very early Universe, as early as 10−35 s after the Big Bang, relies on the scenario known as the inflationary cosmology. Inflation predicts a particular polarization pattern in the cosmic microwave background, known as the B-mode yet the strength of such polarization pattern is extremely weak. To search for the B-mode of the polarization in the cosmic microwave background, we are constructing an off-axis rotating telescope to mitigate systematic effects as well as to maximize the sky coverage of the observation. We will discuss the present status of the GroundBIRD telescope. |
first_indexed | 2024-12-22T03:28:20Z |
format | Article |
id | doaj.art-ac10617e4d5c4ba792fdc78cfde4e35b |
institution | Directory Open Access Journal |
issn | 2100-014X |
language | English |
last_indexed | 2024-12-22T03:28:20Z |
publishDate | 2018-01-01 |
publisher | EDP Sciences |
record_format | Article |
series | EPJ Web of Conferences |
spelling | doaj.art-ac10617e4d5c4ba792fdc78cfde4e35b2022-12-21T18:40:33ZengEDP SciencesEPJ Web of Conferences2100-014X2018-01-011680101410.1051/epjconf/201816801014epjconf_icgaxiii-ik2018_01014Status of the GroundBIRD TelescopeChoi J.Génova-Santos R.Hattori M.Hazumi M.Ishitsuka H.Kanno F.Karatsu K.Kiuchi K.Koyano R.Kutsuma H.Lee K.Mima S.Minowa M.Nagai M.Nagasaki T.Naruse M.Oguri S.Okada T.Otani C.Rebolo R.Rubiño-Martín J.Sekimoto Y.Suzuki J.Taino T.Tajima O.Tomita N.Uchida T.Won E.Yoshida M.Our understanding of physics at very early Universe, as early as 10−35 s after the Big Bang, relies on the scenario known as the inflationary cosmology. Inflation predicts a particular polarization pattern in the cosmic microwave background, known as the B-mode yet the strength of such polarization pattern is extremely weak. To search for the B-mode of the polarization in the cosmic microwave background, we are constructing an off-axis rotating telescope to mitigate systematic effects as well as to maximize the sky coverage of the observation. We will discuss the present status of the GroundBIRD telescope.https://doi.org/10.1051/epjconf/201816801014 |
spellingShingle | Choi J. Génova-Santos R. Hattori M. Hazumi M. Ishitsuka H. Kanno F. Karatsu K. Kiuchi K. Koyano R. Kutsuma H. Lee K. Mima S. Minowa M. Nagai M. Nagasaki T. Naruse M. Oguri S. Okada T. Otani C. Rebolo R. Rubiño-Martín J. Sekimoto Y. Suzuki J. Taino T. Tajima O. Tomita N. Uchida T. Won E. Yoshida M. Status of the GroundBIRD Telescope EPJ Web of Conferences |
title | Status of the GroundBIRD Telescope |
title_full | Status of the GroundBIRD Telescope |
title_fullStr | Status of the GroundBIRD Telescope |
title_full_unstemmed | Status of the GroundBIRD Telescope |
title_short | Status of the GroundBIRD Telescope |
title_sort | status of the groundbird telescope |
url | https://doi.org/10.1051/epjconf/201816801014 |
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