{"_buckets": {"deposit": "c5d566a9-ee30-4940-8dba-1f141da4d05b"}, "_deposit": {"created_by": 3, "id": "7869", "owners": [3], "pid": {"revision_id": 0, "type": "depid", "value": "7869"}, "status": "published"}, "_oai": {"id": "oai:kyutech.repo.nii.ac.jp:00007869", "sets": ["9"]}, "author_link": ["34636", "31407", "34653", "34662", "34665", "34643", "34659", "34642", "34644", "34664", "34658", "34635", "34634", "34667", "34638", "34650", "34666", "34645", "34640", "34637", "34654", "34651", "34655", "34639", "34649", "34647", "34656", "34641", "34652", "34657", "34648", "34660", "34661"], "item_21_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2022-02-08", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageEnd": "6-16", "bibliographicPageStart": "6-1", "bibliographicVolumeNumber": "926", "bibliographic_titles": [{"bibliographic_title": "Astrophysical Journal"}]}]}, "item_21_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We report the first measurement of the zodiacal light (ZL) polarization spectrum in the near-infrared between 0.8 and 1.8 μm. Using the low-resolution spectrometer on board the Cosmic Infrared Background Experiment, calibrated for absolute spectrophotometry and spectropolarimetry, we acquire long-slit polarization spectral images of the total diffuse sky brightness toward five fields. To extract the ZL spectrum, we subtract the contribution of other diffuse radiation, such as the diffuse galactic light, the integrated starlight, and the extragalactic background light. The measured ZL polarization spectrum shows little wavelength dependence in the near-infrared, and the degree of polarization clearly varies as a function of the ecliptic coordinates and solar elongation. Among the observed fields, the North Ecliptic Pole shows the maximum degree of polarization of ∼20%, which is consistent with an earlier observation from the Diffuse Infrared Background Experiment on board on the Cosmic Background Explorer. The measured degree of polarization and its solar elongation dependence are reproduced by an empirical scattering model in the visible band and also by a Mie scattering model for large absorptive particles, while a Rayleigh scattering model is ruled out. All of our results suggest that the interplanetary dust is dominated by large particles.", "subitem_description_type": "Abstract"}]}, "item_21_description_60": {"attribute_name": "資源タイプ", "attribute_value_mlt": [{"subitem_description": "Journal Article", "subitem_description_type": "Other"}]}, "item_21_full_name_3": {"attribute_name": "著者別名", "attribute_value_mlt": [{"nameIdentifiers": [{"nameIdentifier": "34651", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Takimoto,  K."}]}, {"nameIdentifiers": [{"nameIdentifier": "34652", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Arai,  T."}]}, {"nameIdentifiers": [{"nameIdentifier": "34653", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Matsuura,  S."}]}, {"nameIdentifiers": [{"nameIdentifier": "34654", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Bock,  J."}]}, {"nameIdentifiers": [{"nameIdentifier": "34655", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Cooray,  A."}]}, {"nameIdentifiers": [{"nameIdentifier": "34656", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Feder,  R."}]}, {"nameIdentifiers": [{"nameIdentifier": "34657", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Korngut,  P.M."}]}, {"nameIdentifiers": [{"nameIdentifier": "34658", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Lanz,  A."}]}, {"nameIdentifiers": [{"nameIdentifier": "34659", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Lee,  D.H."}]}, {"nameIdentifiers": [{"nameIdentifier": "34660", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Matsumoto,  T."}]}, {"nameIdentifiers": [{"nameIdentifier": "34661", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Nguyen,  C."}]}, {"nameIdentifiers": [{"nameIdentifier": "34662", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Onishi,  Y."}]}, {"nameIdentifiers": [{"nameIdentifier": "31407", "nameIdentifierScheme": "WEKO"}, {"nameIdentifier": "70802908", "nameIdentifierScheme": "e-Rad", "nameIdentifierURI": "https://nrid.nii.ac.jp/ja/nrid/1000070802908/"}, {"nameIdentifier": "56708069700", "nameIdentifierScheme": "Scopus著者ID", "nameIdentifierURI": "https://www.scopus.com/authid/detail.uri?authorId=56708069700"}, {"nameIdentifier": "0000-0002-6468-8532", "nameIdentifierScheme": "ORCiD", "nameIdentifierURI": "https://orcid.org/0000-0002-6468-8532"}, {"nameIdentifier": "100001400", "nameIdentifierScheme": "九工大研究者情報", "nameIdentifierURI": "https://hyokadb02.jimu.kyutech.ac.jp/html/100001400_ja.html"}], "names": [{"name": "Sano, K."}]}, {"nameIdentifiers": [{"nameIdentifier": "34664", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Shirahata,  M."}]}, {"nameIdentifiers": [{"nameIdentifier": "34665", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Takahashi,  A."}]}, {"nameIdentifiers": [{"nameIdentifier": "34666", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Tsumura,  K."}]}, {"nameIdentifiers": [{"nameIdentifier": "34667", "nameIdentifierScheme": "WEKO"}], "names": [{"name": "Zemcov,  M."}]}]}, "item_21_publisher_7": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "IOP Publishing"}]}, "item_21_relation_12": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.3847/1538-4357/ac416f", "subitem_relation_type_select": "DOI"}}]}, "item_21_rights_13": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "Copyright (c) 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence (http://creativecommons.org/licenses/by/4.0/). Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI."}]}, "item_21_select_59": {"attribute_name": "査読の有無", "attribute_value_mlt": [{"subitem_select_item": "yes"}]}, "item_21_source_id_8": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "subitem_source_identifier_type": "ISSN"}, {"subitem_source_identifier": "1538-4357", "subitem_source_identifier_type": "ISSN"}]}, "item_21_subject_16": {"attribute_name": "日本十進分類法", "attribute_value_mlt": [{"subitem_subject": "440", "subitem_subject_scheme": "NDC"}]}, "item_21_text_36": {"attribute_name": "著者所属", "attribute_value_mlt": [{"subitem_text_value": "Kwansei Gakuin University"}, {"subitem_text_value": "Japan Aerospace Exploration Agency (JAXA)"}, {"subitem_text_value": "Kwansei Gakuin University"}, {"subitem_text_value": "California Institute of Technology, National Aeronautics and Space Administration (NASA)"}, {"subitem_text_value": "University of California"}, {"subitem_text_value": "California Institute of Technology"}, {"subitem_text_value": "California Institute of Technology"}, {"subitem_text_value": "The Observatories of the Carnegie Institution for Science"}, {"subitem_text_value": "Korea Astronomy and Space Science Institute (KASI)"}, {"subitem_text_value": "Japan Aerospace Exploration Agency (JAXA)"}, {"subitem_text_value": "California Institute of Technology"}, {"subitem_text_value": "Japan Aerospace Exploration Agency (JAXA)"}, {"subitem_text_value": "Kyushu Institute of Technology"}, {"subitem_text_value": "Japan Aerospace Exploration Agency (JAXA)"}, {"subitem_text_value": "National Institutes of Natural Sciences"}, {"subitem_text_value": "Faculty of Science and Engineering"}, {"subitem_text_value": "Rochester Institute of Technology"}]}, "item_21_text_63": {"attribute_name": "連携ID", "attribute_value_mlt": [{"subitem_text_value": "10865"}]}, "item_21_version_type_58": 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