{"_buckets": {"deposit": "45525d6a-eec2-4acb-810c-222ab8b6c6f3"}, "_deposit": {"id": "28347", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "28347"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00028347"}, "item_10_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2019-03", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "1", "bibliographicPageStart": "27", "bibliographicVolumeNumber": "874", "bibliographic_titles": [{"bibliographic_title": "The Astrophysical Journal"}]}]}, "item_10_description_4": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "We present the Atacama Large Millimeter/submillimeter Array detection of the [O iii] 88 \u03bcm line and rest-frame 90 \u03bcm dust continuum emission in a Y-dropout Lyman break galaxy (LBG), MACS0416_Y1 lying behind the Frontier Field cluster MACS J0416.1\u22122403. This [O iii] detection confirms the LBG with a spectroscopic redshift of z = 8.3118 \u00b1 0.0003, making this object one of the farthest galaxies ever identified spectroscopically. The observed 850 \u03bcm flux density of 137 \u00b1 26 \u03bcJy corresponds to a de-lensed total infrared (IR) luminosity of LIR=(1.7\u00b10.3)\u00d710^11L\u2299 if assuming a dust temperature of T dust = 50 K and an emissivity index of \u03b2 = 1.5, yielding a large dust mass of 4\u00d710^6M\u2299. The ultraviolet-to-far-IR spectral energy distribution modeling where the [O iii] emissivity model is incorporated suggests the presence of a young (\u03c4 age \u2248 4 Myr), star-forming (SFR \u2248 60M\u2299 yr^\u22121), moderately metal-polluted (Z \u2248 0.2Z \u2299) stellar component with a mass of M star = 3 \u00d7 10^8 M \u2299. An analytic dust mass evolution model with a single episode of star formation does not reproduce the metallicity and dust mass in \u03c4 age \u2248 4 Myr, suggesting a pre-existing evolved stellar component with M star ~ 3 \u00d7 10^9 M\u2609 and \u03c4age ~ 0.3 Gyr as the origin of the dust mass.", "subitem_description_type": "Abstract"}]}, "item_10_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "IOP publishing"}]}, "item_10_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.3847/1538-4357/ab0374", "subitem_relation_type_select": "DOI"}}]}, "item_10_rights_12": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "\u00a9 2019. The American Astronomical Society"}]}, "item_10_select_15": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_10_source_id_61": {"attribute_name": "ISSN\uff08print\uff09", "attribute_value_mlt": [{"subitem_source_identifier": "1538-4357", "subitem_source_identifier_type": "ISSN"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Tamura, Yoichi"}], "nameIdentifiers": [{"nameIdentifier": "92579", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Mawatari, Ken"}], "nameIdentifiers": [{"nameIdentifier": "92580", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Hashimoto, Takuya"}], "nameIdentifiers": [{"nameIdentifier": "92581", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Inoue, Akio K."}], "nameIdentifiers": [{"nameIdentifier": "92582", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Zackrisson, Erik"}], "nameIdentifiers": [{"nameIdentifier": "92583", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Christensen, Lise"}], "nameIdentifiers": [{"nameIdentifier": "92584", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Binggeli, Christian"}], "nameIdentifiers": [{"nameIdentifier": "92585", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Matsuda, Yuichi"}], "nameIdentifiers": [{"nameIdentifier": "92586", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Matsuo, Hiroshi"}], "nameIdentifiers": [{"nameIdentifier": "92587", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Takeuchi, Tsutomu T."}], "nameIdentifiers": [{"nameIdentifier": "92588", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Asano, Ryosuke S."}], "nameIdentifiers": [{"nameIdentifier": "92589", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Sunaga, Kaho"}], "nameIdentifiers": [{"nameIdentifier": "92590", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Shimizu, Ikkoh"}], "nameIdentifiers": [{"nameIdentifier": "92591", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Okamoto, Takashi"}], "nameIdentifiers": [{"nameIdentifier": "92592", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Yoshida, Naoki"}], "nameIdentifiers": [{"nameIdentifier": "92593", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Lee, Minju M."}], "nameIdentifiers": [{"nameIdentifier": "92594", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Shibuya, Takatoshi"}], "nameIdentifiers": [{"nameIdentifier": "92595", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Taniguchi, Yoshiaki"}], "nameIdentifiers": [{"nameIdentifier": "92596", "nameIdentifierScheme": 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false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 1900000.0, "url": {"label": "Tamura_2019_ApJ_874_27", "url": "https://nagoya.repo.nii.ac.jp/record/28347/files/Tamura_2019_ApJ_874_27.pdf"}, "version_id": "5b38b1c1-d821-46a0-8496-39070ec020c6"}]}, "item_keyword": {"attribute_name": "\u30ad\u30fc\u30ef\u30fc\u30c9", "attribute_value_mlt": [{"subitem_subject": "dust, extinction", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: formation", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: high-redshift", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: ISM", "subitem_subject_scheme": "Other"}]}, "item_language": {"attribute_name": "\u8a00\u8a9e", "attribute_value_mlt": [{"subitem_language": "eng"}]}, "item_resource_type": {"attribute_name": "\u8cc7\u6e90\u30bf\u30a4\u30d7", "attribute_value_mlt": [{"resourcetype": "journal article", "resourceuri": "http://purl.org/coar/resource_type/c_6501"}]}, "item_title": "Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era"}]}, "item_type_id": "10", "owner": "1", "path": ["336/695/696"], "permalink_uri": "http://hdl.handle.net/2237/00030542", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2019-07-11"}, "publish_date": "2019-07-11", "publish_status": "0", "recid": "28347", "relation": {}, "relation_version_is_last": true, "title": ["Detection of the Far-infrared [O iii] and Dust Emission in a Galaxy at Redshift 8.312: Early Metal Enrichment in the Heart of the Reionization Era"], "weko_shared_id": null}