ログイン
言語:

WEKO3

  • トップ
  • ランキング
To
lat lon distance
To

Field does not validate



インデックスリンク

インデックスツリー

メールアドレスを入力してください。

WEKO

One fine body…

WEKO

One fine body…

アイテム

{"_buckets": {"deposit": "e25f7725-fbeb-4920-87ce-3a746cb360b5"}, "_deposit": {"id": "5523", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "5523"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00005523", "sets": ["696"]}, "author_link": ["14305", "14306"], "item_10_biblio_info_6": {"attribute_name": "書誌情報", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2003-01", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "2", "bibliographicPageEnd": "021302", "bibliographicPageStart": "021302", "bibliographicVolumeNumber": "90", "bibliographic_titles": [{"bibliographic_title": "Physical Review Letters", "bibliographic_titleLang": "en"}]}]}, "item_10_description_4": {"attribute_name": "抄録", "attribute_value_mlt": [{"subitem_description": "We show that the apparent redshift-space clustering of galaxies in the redshift range of 0.2–0.4 provides surprisingly useful constraints on dark-energy components in the Universe, because of the right balance between the density of objects and the survey depth.We apply Fisher matrix analysis to the luminous red galaxies in the Sloan Digital Sky Survey, as a concrete example. Possible degeneracies in the evolution of the equation of state and the other cosmological parameters are clarified.", "subitem_description_language": "en", "subitem_description_type": "Abstract"}]}, "item_10_description_5": {"attribute_name": "内容記述", "attribute_value_mlt": [{"subitem_description": "4pages", "subitem_description_language": "en", "subitem_description_type": "Other"}]}, "item_10_identifier_60": {"attribute_name": "URI", "attribute_value_mlt": [{"subitem_identifier_type": "HDL", "subitem_identifier_uri": "http://hdl.handle.net/2237/7129"}]}, "item_10_publisher_32": {"attribute_name": "出版者", "attribute_value_mlt": [{"subitem_publisher": "The American Physical Society", "subitem_publisher_language": "en"}]}, "item_10_relation_11": {"attribute_name": "DOI", "attribute_value_mlt": [{"subitem_relation_type": "isVersionOf", "subitem_relation_type_id": {"subitem_relation_type_id_text": "https://doi.org/10.1103/PhysRevLett.90.021302", "subitem_relation_type_select": "DOI"}}]}, "item_10_rights_12": {"attribute_name": "権利", "attribute_value_mlt": [{"subitem_rights": "Copyright: American Physical Society, All rights reserved.", "subitem_rights_language": "en"}]}, "item_10_select_15": {"attribute_name": "著者版フラグ", "attribute_value_mlt": [{"subitem_select_item": "publisher"}]}, "item_10_source_id_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0031-9007", "subitem_source_identifier_type": "PISSN"}]}, "item_10_text_14": {"attribute_name": "フォーマット", "attribute_value_mlt": [{"subitem_text_value": "application/pdf"}]}, "item_1615787544753": {"attribute_name": "出版タイプ", "attribute_value_mlt": [{"subitem_version_resource": "http://purl.org/coar/version/c_970fb48d4fbd8a85", "subitem_version_type": "VoR"}]}, "item_access_right": {"attribute_name": "アクセス権", "attribute_value_mlt": [{"subitem_access_right": "open access", "subitem_access_right_uri": "http://purl.org/coar/access_right/c_abf2"}]}, "item_creator": {"attribute_name": "著者", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Matsubara, Takahiko", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "14305", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Szalay, Alexander S.", "creatorNameLang": "en"}], "nameIdentifiers": [{"nameIdentifier": "14306", "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": "2018-02-19"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "PhysRevLett_90_021302.pdf", "filesize": [{"value": "181.9 kB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_note", "mimetype": "application/pdf", "size": 181900.0, "url": {"label": "PhysRevLett_90_021302.pdf", "objectType": "fulltext", "url": "https://nagoya.repo.nii.ac.jp/record/5523/files/PhysRevLett_90_021302.pdf"}, "version_id": "dcd725bd-af43-4b45-929b-6fbf768e41e7"}]}, "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": "Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy", "item_titles": {"attribute_name": "タイトル", "attribute_value_mlt": [{"subitem_title": "Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy", "subitem_title_language": "en"}]}, "item_type_id": "10", "owner": "1", "path": ["696"], "permalink_uri": "http://hdl.handle.net/2237/7129", "pubdate": {"attribute_name": "PubDate", "attribute_value": "2006-11-29"}, "publish_date": "2006-11-29", "publish_status": "0", "recid": "5523", "relation": {}, "relation_version_is_last": true, "title": ["Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy"], "weko_shared_id": -1}
  1. B100 理学部/理学研究科
  2. B100a 雑誌掲載論文
  3. 学術雑誌

Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy

http://hdl.handle.net/2237/7129
http://hdl.handle.net/2237/7129
ca1aaa53-b4d4-4807-9dc7-f5635344c684
名前 / ファイル ライセンス アクション
PhysRevLett_90_021302.pdf PhysRevLett_90_021302.pdf (181.9 kB)
Item type 学術雑誌論文 / Journal Article(1)
公開日 2006-11-29
タイトル
タイトル Apparent Clustering of Intermediate-Redshift Galaxies as a Probe of Dark Energy
言語 en
著者 Matsubara, Takahiko

× Matsubara, Takahiko

WEKO 14305

en Matsubara, Takahiko

Search repository
Szalay, Alexander S.

× Szalay, Alexander S.

WEKO 14306

en Szalay, Alexander S.

Search repository
アクセス権
アクセス権 open access
アクセス権URI http://purl.org/coar/access_right/c_abf2
権利
言語 en
権利情報 Copyright: American Physical Society, All rights reserved.
抄録
内容記述 We show that the apparent redshift-space clustering of galaxies in the redshift range of 0.2–0.4 provides surprisingly useful constraints on dark-energy components in the Universe, because of the right balance between the density of objects and the survey depth.We apply Fisher matrix analysis to the luminous red galaxies in the Sloan Digital Sky Survey, as a concrete example. Possible degeneracies in the evolution of the equation of state and the other cosmological parameters are clarified.
言語 en
内容記述タイプ Abstract
内容記述
内容記述 4pages
言語 en
内容記述タイプ Other
出版者
言語 en
出版者 The American Physical Society
言語
言語 eng
資源タイプ
資源タイプresource http://purl.org/coar/resource_type/c_6501
タイプ journal article
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
DOI
関連タイプ isVersionOf
識別子タイプ DOI
関連識別子 https://doi.org/10.1103/PhysRevLett.90.021302
ISSN
収録物識別子タイプ PISSN
収録物識別子 0031-9007
書誌情報 en : Physical Review Letters

巻 90, 号 2, p. 021302-021302, 発行日 2003-01
フォーマット
application/pdf
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/7129
識別子タイプ HDL
戻る
0
views
See details
Views

Versions

Ver.1 2021-03-01 13:09:12.374207
Show All versions

Share

Mendeley Twitter Facebook Print Addthis

Cite as

エクスポート

OAI-PMH
  • OAI-PMH JPCOAR
  • OAI-PMH DublinCore
  • OAI-PMH DDI
Other Formats
  • JSON
  • BIBTEX

Confirm


Powered by WEKO3


Powered by WEKO3