{"_buckets": {"deposit": "138e1361-9560-4d8e-bf82-9362be0ba835"}, "_deposit": {"id": "8179", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "8179"}, "status": "published"}, "_oai": {"id": "oai:kitami-it.repo.nii.ac.jp:00008179", "sets": ["1"]}, "item_3_biblio_info_186": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2005-09", "bibliographicIssueDateType": "Issued"}, "bibliographicPageEnd": "1285", "bibliographicPageStart": "1278", "bibliographicVolumeNumber": "130", "bibliographic_titles": [{"bibliographic_title": "The Astronomical Journal"}]}]}, "item_3_description_184": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "We present a novel method of detecting faint moving objects in the solar system. The method is based on the\nevaluation of relative likelihood, which is newly introduced in this paper. Features of this method are that no thresholding\noperation is required and that both spatial and temporal statistical processing is implemented. These features\nare advantageous for detecting faint objects. In addition, relative likelihood can be used to quantitatively assess the\ncertainty of detected objects. We applied our method to data taken at two different observatories in Japan. Experimental\nresults indicate that this method is capable of detecting faint moving objects with signals comparable to the\nnoise level.", "subitem_description_type": "Abstract"}]}, "item_3_full_name_183": {"attribute_name": "\u8457\u8005\u5225\u540d", "attribute_value_mlt": [{"nameIdentifiers": [{"nameIdentifier": "44861", "nameIdentifierScheme": "WEKO"}, {"nameIdentifier": "1000030209720 ", "nameIdentifierScheme": "NRID", "nameIdentifierURI": "http://rns.nii.ac.jp/d/nr/1000030209720 "}], "names": [{"name": "\u4e09\u6d66, \u5247\u660e"}]}]}, "item_3_link_221": {"attribute_name": "\u95a2\u9023\u30b5\u30a4\u30c8", "attribute_value_mlt": [{"subitem_link_url": "http://iopscience.iop.org/article/10.1086/431955"}]}, "item_3_publisher_212": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "The American Astronomical Society"}]}, "item_3_rights_192": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "c 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A."}]}, "item_3_select_195": {"attribute_name": "\u8457\u8005\u7248\u30d5\u30e9\u30b0", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_3_subject_196": {"attribute_name": "\u65e5\u672c\u5341\u9032\u5206\u985e\u6cd5", "attribute_value_mlt": [{"subitem_subject": "540", "subitem_subject_scheme": "NDC"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Miura, Noriaki"}], "nameIdentifiers": [{"nameIdentifier": "42859", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Itagaki, Kazuyuki"}], "nameIdentifiers": [{"nameIdentifier": "42860", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Baba, Naoshi"}], "nameIdentifiers": [{"nameIdentifier": "42861", "nameIdentifierScheme": "WEKO"}]}]}, "item_files": {"attribute_name": "\u30d5\u30a1\u30a4\u30eb\u60c5\u5831", "attribute_type": "file", "attribute_value_mlt": [{"accessrole": "open_date", "date": [{"dateType": "Available", "dateValue": "2016-11-22"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "2005_Likelihood-vased method for detecting faint moving objects.pdf", "filesize": [{"value": "399.4 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 399400.0, "url": {"label": "2005_Likelihood-vased method for detecting faint moving objects.pdf", "url": "https://kitami-it.repo.nii.ac.jp/record/8179/files/2005_Likelihood-vased method for detecting faint moving objects.pdf"}, "version_id": "695b331d-4e69-45c1-9431-e2120545fe3a"}]}, "item_keyword": {"attribute_name": "\u30ad\u30fc\u30ef\u30fc\u30c9", "attribute_value_mlt": [{"subitem_subject": "data analysis", "subitem_subject_scheme": "Other"}, {"subitem_subject": "minor planets", "subitem_subject_scheme": "Other"}, {"subitem_subject": "asteroids", "subitem_subject_scheme": "Other"}, {"subitem_subject": "image processing", "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": "Likelihood-vased method for detecting faint moving objects", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "Likelihood-vased method for detecting faint moving objects"}]}, "item_type_id": "3", "owner": "1", "path": ["1"], "permalink_uri": "https://kitami-it.repo.nii.ac.jp/records/8179", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2016-06-17"}, "publish_date": "2016-06-17", "publish_status": "0", "recid": "8179", "relation": {}, "relation_version_is_last": true, "title": ["Likelihood-vased method for detecting faint moving objects"], "weko_shared_id": 3}