{"_buckets": {"deposit": "f2182b60-458b-4431-8b59-c26e1ab2316d"}, "_deposit": {"created_by": 21, "id": "3506", "owners": [21], "pid": {"revision_id": 0, "type": "depid", "value": "3506"}, "status": "published"}, "_oai": {"id": "oai:ir.soken.ac.jp:00003506", "sets": ["274"]}, "author_link": ["1290", "734", "1293", "1287", "1291", "1292", "738"], "item_10001_biblio_info_7": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "1995-11", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "2", "bibliographicPageEnd": "544", "bibliographicPageStart": "541", "bibliographicVolumeNumber": "453", "bibliographic_titles": [{"bibliographic_title": "Astrophysical Journal "}, {"bibliographic_title": "Astrophysical Journal ", "bibliographic_titleLang": "en"}]}]}, "item_10001_creator_3": {"attribute_name": "著者別名", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "池内, 了"}], "nameIdentifiers": [{"nameIdentifier": "738", "nameIdentifierScheme": "WEKO"}, {"nameIdentifier": "1000090025461", "nameIdentifierScheme": "NRID", "nameIdentifierURI": " "}, {"nameIdentifier": "90025461", "nameIdentifierScheme": "e-Rad", "nameIdentifierURI": "https://kaken.nii.ac.jp/ja/search/?qm=90025461"}]}]}, "item_10001_description_19": {"attribute_name": "フォーマット", "attribute_value_mlt": [{"subitem_description": "application/pdf", "subitem_description_type": "Other"}]}, "item_10001_description_5": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We investigate the distance-redshift relation in a simple void model. As discussed by Moffat and Tatarski, if an observer stays at the center of the void, the observed Hubble parameter is not so different from the background Hubble parameter. However, if the position of the observer is not at the center of the void, we must consider the correction to the redshift due to the peculiar velocity, which is determined by the observed dipole anisotropy of the cosmic microwave background. This correction of the redshift is crucial to determine the Hubble parameter, and we shall consider this effect. Further, the results of the N-body simulation of Turner et al. will be also discussed.", "subitem_description_type": "Abstract"}]}, "item_10001_publisher_8": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "The American Astronomical Society"}]}, "item_10001_relation_14": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_name": [{"subitem_relation_name_text": "10.1086/176416"}], "subitem_relation_type": "isIdenticalTo", "subitem_relation_type_id": {"subitem_relation_type_id_text": "http://doi.org/10.1086/176416", "subitem_relation_type_select": "DOI"}}]}, "item_10001_relation_17": {"attribute_name": "関連サイト", "attribute_value_mlt": [{"subitem_relation_name": [{"subitem_relation_name_text": "Copyright"}], "subitem_relation_type_id": {"subitem_relation_type_id_text": "http://aas.org/publications/aas-copyright-policy", "subitem_relation_type_select": "URI"}}]}, "item_10001_rights_15": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "© 1995. The American Astronomical Society"}]}, "item_10001_source_id_9": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "subitem_source_identifier_type": "ISSN"}]}, "item_10001_version_type_20": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "NAKAO, Ken-ichi"}], "nameIdentifiers": [{"nameIdentifier": "1290", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "GOUDA, Naoteru"}], "nameIdentifiers": [{"nameIdentifier": "1291", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "CHIBA, Takeshi"}], "nameIdentifiers": [{"nameIdentifier": "1292", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "IKEUCHI, Satoru"}], "nameIdentifiers": [{"nameIdentifier": "734", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "NAKAMURA, Takashi"}], "nameIdentifiers": [{"nameIdentifier": "1287", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "SHIBATA, Masaru"}], "nameIdentifiers": [{"nameIdentifier": "1293", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "ファイル情報", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2014-02-19"}], "displaytype": "simple", "download_preview_message": "", "file_order": 0, "filename": "nph-iarticle_query10.pdf", "filesize": [{"value": "116.3 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_11", "mimetype": "application/pdf", "size": 116300.0, "url": {"label": "nph-iarticle_query10", "url": "https://ir.soken.ac.jp/record/3506/files/nph-iarticle_query10.pdf"}, "version_id": "4ed98ed8-b10f-46fd-8f3b-59596e225d2f"}]}, "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 hubble parameter in a void universe: Effect of the peculiar velocity", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "The hubble parameter in a void universe: Effect of the peculiar velocity"}, {"subitem_title": "The hubble parameter in a void universe: Effect of the peculiar velocity", "subitem_title_language": "en"}]}, "item_type_id": "10001", "owner": "21", "path": ["274"], "permalink_uri": "https://ir.soken.ac.jp/records/3506", "pubdate": {"attribute_name": "公開日", "attribute_value": "2013-04-24"}, "publish_date": "2013-04-24", "publish_status": "0", "recid": "3506", "relation": {}, "relation_version_is_last": true, "title": ["The hubble parameter in a void universe: Effect of the peculiar velocity"], "weko_shared_id": 21}