{"_buckets": {"deposit": "37e16477-126a-40c7-95bf-24dd32a6a93a"}, "_deposit": {"id": "24807", "owners": [], "pid": {"revision_id": 0, "type": "depid", "value": "24807"}, "status": "published"}, "_oai": {"id": "oai:nagoya.repo.nii.ac.jp:00024807"}, "item_10_biblio_info_6": {"attribute_name": "\u66f8\u8a8c\u60c5\u5831", "attribute_value_mlt": [{"bibliographicIssueDates": {"bibliographicIssueDate": "2017-07-10", "bibliographicIssueDateType": "Issued"}, "bibliographicIssueNumber": "2", "bibliographicPageEnd": "138", "bibliographicPageStart": "138", "bibliographicVolumeNumber": "843", "bibliographic_titles": [{"bibliographic_title": "Astrophysical Journal"}]}]}, "item_10_description_4": {"attribute_name": "\u6284\u9332", "attribute_value_mlt": [{"subitem_description": "We study the properties of dark matter halos that contain star-forming galaxies at 1.43 \u2264 z \u2264 1.74, using the FMOS-COSMOS survey. The sample consists of 516 objects with a detection of the H\u03b1 emission line, which represent the star forming population at this epoch, having a stellar mass range of 10^9.57 \u2264 M */M \u2299 lesssim 10^11.4 and a star-formation rate range of 15 lesssim SFR/(M \u2299 yr^\u22121) lesssim ^600. We measure the projected two-point correlation function while carefully taking into account observational biases, and find a significant clustering amplitude at scales of 0.04\u201310 h ^\u22121 cMpc, with a correlation length r0 =5.26-0.62^+0.75h^-1cMpc and a bias b =2.44-0.32^+0.38. We interpret our clustering measurement using a halo occupation distribution model. The sample galaxies appear to reside in halos with mass Mh=4.71-1.62^+1.19\u00d710^12h^-1,M\u2299 on average, which will likely become present-day halos of mass M h (z = 0) ~ 2 \u00d7 10^13 h ^\u22121 M \u2299, equivalent to the typical halo mass scale of galaxy groups. We then confirm the decline of the stellar-to-halo mass ratio at M h \u003c 10^12 M \u2299, finding M */M h \u2248 5 \u00d7 10^\u22123 at M h = 7. 5 \u00d7 10^11 M \u2299, which is lower by a factor of 2\u20134 than those measured at higher masses (M h ~ 10^12\u201313 M \u2299). Finally, we use our results to illustrate the future capabilities of Subaru\u0027s Prime-Focus Spectrograph, a next-generation instrument that will provide strong constraints on the galaxy-formation scenario by obtaining precise measurements of galaxy clustering at z\u003e1.", "subitem_description_type": "Abstract"}]}, "item_10_identifier_60": {"attribute_name": "URI", "attribute_value_mlt": [{"subitem_identifier_type": "DOI", "subitem_identifier_uri": "http://doi.org/10.3847/1538-4357/aa789d"}, {"subitem_identifier_type": "HDL", "subitem_identifier_uri": "http://hdl.handle.net/2237/27029"}]}, "item_10_publisher_32": {"attribute_name": "\u51fa\u7248\u8005", "attribute_value_mlt": [{"subitem_publisher": "IOP publishing"}]}, "item_10_rights_12": {"attribute_name": "\u6a29\u5229", "attribute_value_mlt": [{"subitem_rights": "\u00a9 2017. 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_7": {"attribute_name": "ISSN", "attribute_value_mlt": [{"subitem_source_identifier": "0004-637X", "subitem_source_identifier_type": "ISSN"}]}, "item_creator": {"attribute_name": "\u8457\u8005", "attribute_type": "creator", "attribute_value_mlt": [{"creatorNames": [{"creatorName": "Kashino, Daichi"}], "nameIdentifiers": [{"nameIdentifier": "73771", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "More, Surhud"}], "nameIdentifiers": [{"nameIdentifier": "73772", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Silverman, John D."}], "nameIdentifiers": [{"nameIdentifier": "73773", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Daddi, Emanuele"}], "nameIdentifiers": [{"nameIdentifier": "73774", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Renzini, Alvio"}], "nameIdentifiers": [{"nameIdentifier": "73775", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Sanders, David B."}], "nameIdentifiers": [{"nameIdentifier": "73776", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Rodighiero, Giulia"}], "nameIdentifiers": [{"nameIdentifier": "73777", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Puglisi, Annagrazia"}], "nameIdentifiers": [{"nameIdentifier": "73778", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kajisawa, Masaru"}], "nameIdentifiers": [{"nameIdentifier": "73779", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Valentino, Francesco"}], "nameIdentifiers": [{"nameIdentifier": "73780", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Kartaltepe, Jeyhan S."}], "nameIdentifiers": [{"nameIdentifier": "73781", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "F\u00e8vre, Olivier Le"}], "nameIdentifiers": [{"nameIdentifier": "73782", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Nagao, Tohru"}], "nameIdentifiers": [{"nameIdentifier": "73783", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Arimoto, Nobuo"}], "nameIdentifiers": [{"nameIdentifier": "73784", "nameIdentifierScheme": "WEKO"}]}, {"creatorNames": [{"creatorName": "Sugiyama, Naoshi"}], "nameIdentifiers": [{"nameIdentifier": "73785", "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": "2018-02-22"}], "displaytype": "detail", "download_preview_message": "", "file_order": 0, "filename": "pdf.pdf", "filesize": [{"value": "2.7 MB"}], "format": "application/pdf", "future_date_message": "", "is_thumbnail": false, "licensetype": "license_free", "mimetype": "application/pdf", "size": 2700000.0, "url": {"label": "pdf.pdf", "url": "https://nagoya.repo.nii.ac.jp/record/24807/files/pdf.pdf"}, "version_id": "62b41ea5-d1da-4008-92ec-4b4c9cdae45b"}]}, "item_keyword": {"attribute_name": "\u30ad\u30fc\u30ef\u30fc\u30c9", "attribute_value_mlt": [{"subitem_subject": "galaxies: evolution", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: formation", "subitem_subject_scheme": "Other"}, {"subitem_subject": "galaxies: halos", "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": "The FMOS-COSMOS Survey of Star-forming Galaxies at Z ~ 1.6. V: Properties of Dark Matter Halos Containing H\u03b1 Emitting Galaxies", "item_titles": {"attribute_name": "\u30bf\u30a4\u30c8\u30eb", "attribute_value_mlt": [{"subitem_title": "The FMOS-COSMOS Survey of Star-forming Galaxies at Z ~ 1.6. V: Properties of Dark Matter Halos Containing H\u03b1 Emitting Galaxies"}]}, "item_type_id": "10", "owner": "1", "path": ["336/695/696"], "permalink_uri": "http://hdl.handle.net/2237/27029", "pubdate": {"attribute_name": "\u516c\u958b\u65e5", "attribute_value": "2017-10-11"}, "publish_date": "2017-10-11", "publish_status": "0", "recid": "24807", "relation": {}, "relation_version_is_last": true, "title": ["The FMOS-COSMOS Survey of Star-forming Galaxies at Z ~ 1.6. V: Properties of Dark Matter Halos Containing H\u03b1 Emitting Galaxies"], "weko_shared_id": null}