{"created":"2023-05-15T12:00:28.125161+00:00","id":7277,"links":{},"metadata":{"_buckets":{"deposit":"09156f8d-1772-402e-a00d-0fc0e456151a"},"_deposit":{"created_by":3,"id":"7277","owners":[3],"pid":{"revision_id":0,"type":"depid","value":"7277"},"status":"published"},"_oai":{"id":"oai:kyutech.repo.nii.ac.jp:00007277","sets":["8:9"]},"author_link":["31409","31407","31410","31408"],"item_21_biblio_info_6":{"attribute_name":"書誌情報","attribute_value_mlt":[{"bibliographicIssueDates":{"bibliographicIssueDate":"2020-09-28","bibliographicIssueDateType":"Issued"},"bibliographicIssueNumber":"2","bibliographicPageEnd":"112-26","bibliographicPageStart":"112-1","bibliographicVolumeNumber":"901","bibliographic_titles":[{"bibliographic_title":"Astrophysical Journal"}]}]},"item_21_description_4":{"attribute_name":"抄録","attribute_value_mlt":[{"subitem_description":"We report observation of isotropic interplanetary dust (IPD) by analyzing the infrared (IR) maps of the Diffuse Infrared Background Experiment (DIRBE) on board the Cosmic Background Explorer (COBE) spacecraft. To search for the isotropic IPD, we perform new analysis in terms of the solar elongation angle (∊), because we expect the zodiacal light (ZL) intensity from the isotropic IPD to decrease as a function of ∊. We use the DIRBE weekly averaged maps covering 64° ≲ ∊ ≲ 124° and inspect the ò dependence of residual intensity after subtracting conventional ZL components. We find the ò dependence of the residuals, indicating the presence of the isotropic IPD. However, the mid-IR ò dependence is different from that of the isotropic IPD model at ∊ ≳ 90°, where the residual intensity increases as a function of ∊. To explain the observed ∊ dependence, we assume a spheroidal IPD cloud showing higher density farther away from the Sun. We estimate the intensity of the near-IR extragalactic background light (EBL) by subtracting the spheroidal component, assuming the spectral energy distribution from the residual brightness at 12 μm. The EBL intensity is derived as 45 +11 -8, 21 +3 -4, and 15 ± 3 nWm -2 sr -1 at 1.25, 2.2, and 3.5 μm, respectively. The EBL is still a few times larger than the integrated light of normal galaxies, suggesting the existence of unaccounted-for extragalactic sources.","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_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":"isVersionOf","subitem_relation_type_id":{"subitem_relation_type_id_text":"https://doi.org/10.3847/1538-4357/abad3d","subitem_relation_type_select":"DOI"}}]},"item_21_rights_13":{"attribute_name":"権利","attribute_value_mlt":[{"subitem_rights":"Copyright (c) 2020. The American Astronomical Society. All rights reserved."}]},"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":"Kanazawa University, Kwansei Gakuin University"},{"subitem_text_value":"Kwansei Gakuin University"},{"subitem_text_value":"Kwansei Gakuin University, Tohoku University"},{"subitem_text_value":"Astrobiology Center"}]},"item_21_text_63":{"attribute_name":"連携ID","attribute_value_mlt":[{"subitem_text_value":"8989"}]},"item_21_version_type_58":{"attribute_name":"著者版フラグ","attribute_value_mlt":[{"subitem_version_resource":"http://purl.org/coar/version/c_ab4af688f83e57aa","subitem_version_type":"AM"}]},"item_creator":{"attribute_name":"著者","attribute_type":"creator","attribute_value_mlt":[{"creatorAffiliations":[{"affiliationNameIdentifiers":[],"affiliationNames":[{"affiliationName":""}]}],"creatorNames":[{"creatorName":"Sano, Kei","creatorNameLang":"en"},{"creatorName":"佐野, 圭","creatorNameLang":"ja"},{"creatorName":"サノ, ケイ","creatorNameLang":"ja-Kana"}],"familyNames":[{},{},{}],"givenNames":[{},{},{}],"nameIdentifiers":[{},{},{},{},{}]},{"creatorNames":[{"creatorName":"Matsuura,  S."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Yomo,  K."}],"nameIdentifiers":[{}]},{"creatorNames":[{"creatorName":"Takahashi,  A."}],"nameIdentifiers":[{}]}]},"item_files":{"attribute_name":"ファイル情報","attribute_type":"file","attribute_value_mlt":[{"accessrole":"open_date","date":[{"dateType":"Available","dateValue":"2021-09-28"}],"displaytype":"detail","filename":"LaSEINE-2020_09.pdf","filesize":[{"value":"4.3 MB"}],"format":"application/pdf","licensetype":"license_note","mimetype":"application/pdf","url":{"label":"LaSEINE-2020_09.pdf","url":"https://kyutech.repo.nii.ac.jp/record/7277/files/LaSEINE-2020_09.pdf"},"version_id":"b2a6b5e4-3127-4c5e-9301-d83f9ed5d594"}]},"item_keyword":{"attribute_name":"キーワード","attribute_value_mlt":[{"subitem_subject":"Infrared astronomy","subitem_subject_scheme":"Other"},{"subitem_subject":"Zodiacal cloud","subitem_subject_scheme":"Other"},{"subitem_subject":"Cosmic background radiation","subitem_subject_scheme":"Other"},{"subitem_subject":"Interplanetary dust","subitem_subject_scheme":"Other"},{"subitem_subject":"Observational cosmology","subitem_subject_scheme":"Other"},{"subitem_subject":"Infrared Astronomical Satellite","subitem_subject_scheme":"Other"},{"subitem_subject":"Galaxy evolution","subitem_subject_scheme":"Other"},{"subitem_subject":"Diffuse radiation","subitem_subject_scheme":"Other"},{"subitem_subject":"Early universe","subitem_subject_scheme":"Other"},{"subitem_subject":"Intergalactic medium","subitem_subject_scheme":"Other"},{"subitem_subject":"Population III stars","subitem_subject_scheme":"Other"},{"subitem_subject":"Primordial black holes","subitem_subject_scheme":"Other"}]},"item_language":{"attribute_name":"言語","attribute_value_mlt":[{"subitem_language":"eng"}]},"item_resource_type":{"attribute_name":"資源タイプ","attribute_value_mlt":[{"resourcetype":"journal article","resourceuri":"http://purl.org/coar/resource_type/c_6501"}]},"item_title":"The Isotropic Interplanetary Dust Cloud and Near-infrared Extragalactic Background Light Observed with COBE/DIRBE","item_titles":{"attribute_name":"タイトル","attribute_value_mlt":[{"subitem_title":"The Isotropic Interplanetary Dust Cloud and Near-infrared Extragalactic Background Light Observed with COBE/DIRBE"}]},"item_type_id":"21","owner":"3","path":["9"],"pubdate":{"attribute_name":"公開日","attribute_value":"2021-09-28"},"publish_date":"2021-09-28","publish_status":"0","recid":"7277","relation_version_is_last":true,"title":["The Isotropic Interplanetary Dust Cloud and Near-infrared Extragalactic Background Light Observed with COBE/DIRBE"],"weko_creator_id":"3","weko_shared_id":3},"updated":"2024-04-02T08:38:20.696690+00:00"}