Academic Journal
أعرض في EDS

The ALPINE-ALMA [C II] survey: Investigation of 10 galaxies at z 4.5 with [O II] and [C II] line emission - ISM properties and [O II]-SFR relation

التفاصيل البيبلوغرافية
العنوان: The ALPINE-ALMA [C II] survey: Investigation of 10 galaxies at z 4.5 with [O II] and [C II] line emission - ISM properties and [O II]-SFR relation
المؤلفون: Brittany N Vanderhoof, A L Faisst, L Shen, B C Lemaux, M B??thermin, P L Capak, P Cassata, O Le??F??vre, D Schaerer, J Silverman, L Yan, M Boquien, R Gal, J Kartaltepe, L M Lubin, M Dessauges-Zavadsky, Y Fudamoto, M Ginolfi, N P Hathi, G C Jones, A M Koekemoer, D Narayanan, M Romano, M Talia, D Vergani, G Zamorani
المساهمون: Brittany N Vanderhoof, A L Faisst, L Shen, B C Lemaux, M B??thermin, P L Capak, P Cassata, O Le??F??vre, D Schaerer, J Silverman, L Yan, M Boquien, R Gal, J Kartaltepe, L M Lubin, M Dessauges-Zavadsky, Y Fudamoto, M Ginolfi, N P Hathi, G C Jone, A M Koekemoer, D Narayanan, M Romano, M Talia, D Vergani, G Zamorani
سنة النشر: 2022
المجموعة: IRIS Università degli Studi di Bologna (CRIS - Current Research Information System)
مصطلحات موضوعية: galaxies: evolution, galaxies: high-redshift, galaxies: ISM
الوصف: We present 10 main-sequence ALPINE galaxies (log (M/M-circle dot) = 9.2-11.1 and SFR = 23 - 190 M-circle dot yr(-1)) at z similar to 4.5 with optical [O II] measurements from Keck/MOSFIRE spectroscopy and Subaru/MOIRCS narrow-band imaging. This is the largest such multiwavelength sample at these redshifts, combining various measurements in the ultraviolet, optical, and far-infrared including [C II]158 mu m line emission and dust continuum from ALMA and H alpha emission from Spitzer photometry.For the first time, this unique sample allows us to analyse the relation between [O II] and total star-formation rate (SFR) and the interstellar medium (ISM) properties via [O II]/[C II] and [O II]/H alpha luminosity ratios at z similar to 4.5. The [O II]-SFR relation at z similar to 4.5 cannot be described using standard local descriptions, but is consistent with a metal-dependent relation assuming metallicities around 50 per cent solar. To explain the measured dust-corrected luminosity ratios of log(L-[OII]/L-[CII]) similar to 0.98(-0.22)(+0.21) and log(L-[OII]/L-H alpha) similar to -0.22(-0.15)(+0.13) for our sample, ionization parameters log (U) < -2 and electron densities log(ne/[cm(-3)])similar to 2.5 - 3 are required. The former is consistent with galaxies at z similar to 2-3, however lower than at z > 6. The latter may be slightly higher than expected given the galaxies' specific SFR. The analysis of this pilot sample suggests that typical log (M/M-circle dot) > 9 galaxies at z similar to 4.5 to have broadly similar ISM properties as their descendants at z similar to 2 and suggest a strong evolution of ISM properties since the epoch of reionization at z > 6.
نوع الوثيقة: article in journal/newspaper
وصف الملف: STAMPA
اللغة: English
Relation: info:eu-repo/semantics/altIdentifier/wos/WOS:000770034000006; volume:511; issue:1; firstpage:1303; lastpage:1316; numberofpages:14; journal:MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; https://hdl.handle.net/11585/905570; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85128269434; https://academic.oup.com/mnras/article/511/1/1303/6507585?login=false
DOI: 10.1093/mnras/stac071
الاتاحة: https://hdl.handle.net/11585/905570
https://doi.org/10.1093/mnras/stac071
https://academic.oup.com/mnras/article/511/1/1303/6507585?login=false
Rights: info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.E45C597A
قاعدة البيانات: BASE
ResultId 1
Header edsbas
BASE
edsbas.E45C597A
938
3
Academic Journal
academicJournal
937.599182128906
PLink https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsbas&AN=edsbas.E45C597A&custid=s6537998&authtype=sso
FullText Array ( [Availability] => 0 )
Array ( [0] => Array ( [Url] => https://hdl.handle.net/11585/905570# [Name] => EDS - BASE [Category] => fullText [Text] => View record in BASE [MouseOverText] => View record in BASE ) )
Items Array ( [Name] => Title [Label] => Title [Group] => Ti [Data] => The ALPINE-ALMA [C II] survey: Investigation of 10 galaxies at z 4.5 with [O II] and [C II] line emission - ISM properties and [O II]-SFR relation )
Array ( [Name] => Author [Label] => Authors [Group] => Au [Data] => &lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22Brittany+N+Vanderhoof%22&quot;&gt;Brittany N Vanderhoof&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22A+L+Faisst%22&quot;&gt;A L Faisst&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22L+Shen%22&quot;&gt;L Shen&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22B+C+Lemaux%22&quot;&gt;B C Lemaux&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+B%3F%3Fthermin%22&quot;&gt;M B??thermin&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22P+L+Capak%22&quot;&gt;P L Capak&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22P+Cassata%22&quot;&gt;P Cassata&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22O+Le%3F%3FF%3F%3Fvre%22&quot;&gt;O Le??F??vre&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22D+Schaerer%22&quot;&gt;D Schaerer&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22J+Silverman%22&quot;&gt;J Silverman&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22L+Yan%22&quot;&gt;L Yan&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+Boquien%22&quot;&gt;M Boquien&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22R+Gal%22&quot;&gt;R Gal&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22J+Kartaltepe%22&quot;&gt;J Kartaltepe&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22L+M+Lubin%22&quot;&gt;L M Lubin&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+Dessauges-Zavadsky%22&quot;&gt;M Dessauges-Zavadsky&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22Y+Fudamoto%22&quot;&gt;Y Fudamoto&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+Ginolfi%22&quot;&gt;M Ginolfi&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22N+P+Hathi%22&quot;&gt;N P Hathi&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22G+C+Jones%22&quot;&gt;G C Jones&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22A+M+Koekemoer%22&quot;&gt;A M Koekemoer&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22D+Narayanan%22&quot;&gt;D Narayanan&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+Romano%22&quot;&gt;M Romano&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22M+Talia%22&quot;&gt;M Talia&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22D+Vergani%22&quot;&gt;D Vergani&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;AR&quot; term=&quot;%22G+Zamorani%22&quot;&gt;G Zamorani&lt;/searchLink&gt; )
Array ( [Name] => Author [Label] => Contributors [Group] => Au [Data] => Brittany N Vanderhoof&lt;br /&gt;A L Faisst&lt;br /&gt;L Shen&lt;br /&gt;B C Lemaux&lt;br /&gt;M B??thermin&lt;br /&gt;P L Capak&lt;br /&gt;P Cassata&lt;br /&gt;O Le??F??vre&lt;br /&gt;D Schaerer&lt;br /&gt;J Silverman&lt;br /&gt;L Yan&lt;br /&gt;M Boquien&lt;br /&gt;R Gal&lt;br /&gt;J Kartaltepe&lt;br /&gt;L M Lubin&lt;br /&gt;M Dessauges-Zavadsky&lt;br /&gt;Y Fudamoto&lt;br /&gt;M Ginolfi&lt;br /&gt;N P Hathi&lt;br /&gt;G C Jone&lt;br /&gt;A M Koekemoer&lt;br /&gt;D Narayanan&lt;br /&gt;M Romano&lt;br /&gt;M Talia&lt;br /&gt;D Vergani&lt;br /&gt;G Zamorani )
Array ( [Name] => DatePubCY [Label] => Publication Year [Group] => Date [Data] => 2022 )
Array ( [Name] => Subset [Label] => Collection [Group] => HoldingsInfo [Data] => IRIS Universit&#224; degli Studi di Bologna (CRIS - Current Research Information System) )
Array ( [Name] => Subject [Label] => Subject Terms [Group] => Su [Data] => &lt;searchLink fieldCode=&quot;DE&quot; term=&quot;%22galaxies%3A+evolution%22&quot;&gt;galaxies: evolution&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;DE&quot; term=&quot;%22galaxies%3A+high-redshift%22&quot;&gt;galaxies: high-redshift&lt;/searchLink&gt;&lt;br /&gt;&lt;searchLink fieldCode=&quot;DE&quot; term=&quot;%22galaxies%3A+ISM%22&quot;&gt;galaxies: ISM&lt;/searchLink&gt; )
Array ( [Name] => Abstract [Label] => Description [Group] => Ab [Data] => We present 10 main-sequence ALPINE galaxies (log (M/M-circle dot) = 9.2-11.1 and SFR = 23 - 190 M-circle dot yr(-1)) at z similar to 4.5 with optical [O II] measurements from Keck/MOSFIRE spectroscopy and Subaru/MOIRCS narrow-band imaging. This is the largest such multiwavelength sample at these redshifts, combining various measurements in the ultraviolet, optical, and far-infrared including [C II]158 mu m line emission and dust continuum from ALMA and H alpha emission from Spitzer photometry.For the first time, this unique sample allows us to analyse the relation between [O II] and total star-formation rate (SFR) and the interstellar medium (ISM) properties via [O II]/[C II] and [O II]/H alpha luminosity ratios at z similar to 4.5. The [O II]-SFR relation at z similar to 4.5 cannot be described using standard local descriptions, but is consistent with a metal-dependent relation assuming metallicities around 50 per cent solar. To explain the measured dust-corrected luminosity ratios of log(L-[OII]/L-[CII]) similar to 0.98(-0.22)(+0.21) and log(L-[OII]/L-H alpha) similar to -0.22(-0.15)(+0.13) for our sample, ionization parameters log (U) &lt; -2 and electron densities log(ne/[cm(-3)])similar to 2.5 - 3 are required. The former is consistent with galaxies at z similar to 2-3, however lower than at z &gt; 6. The latter may be slightly higher than expected given the galaxies&#39; specific SFR. The analysis of this pilot sample suggests that typical log (M/M-circle dot) &gt; 9 galaxies at z similar to 4.5 to have broadly similar ISM properties as their descendants at z similar to 2 and suggest a strong evolution of ISM properties since the epoch of reionization at z &gt; 6. )
Array ( [Name] => TypeDocument [Label] => Document Type [Group] => TypDoc [Data] => article in journal/newspaper )
Array ( [Name] => Format [Label] => File Description [Group] => SrcInfo [Data] => STAMPA )
Array ( [Name] => Language [Label] => Language [Group] => Lang [Data] => English )
Array ( [Name] => NoteTitleSource [Label] => Relation [Group] => SrcInfo [Data] => info:eu-repo/semantics/altIdentifier/wos/WOS:000770034000006; volume:511; issue:1; firstpage:1303; lastpage:1316; numberofpages:14; journal:MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; https://hdl.handle.net/11585/905570; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85128269434; https://academic.oup.com/mnras/article/511/1/1303/6507585?login=false )
Array ( [Name] => DOI [Label] => DOI [Group] => ID [Data] => 10.1093/mnras/stac071 )
Array ( [Name] => URL [Label] => Availability [Group] => URL [Data] => https://hdl.handle.net/11585/905570&lt;br /&gt;https://doi.org/10.1093/mnras/stac071&lt;br /&gt;https://academic.oup.com/mnras/article/511/1/1303/6507585?login=false )
Array ( [Name] => Copyright [Label] => Rights [Group] => Cpyrght [Data] => info:eu-repo/semantics/openAccess )
Array ( [Name] => AN [Label] => Accession Number [Group] => ID [Data] => edsbas.E45C597A )
RecordInfo Array ( [BibEntity] => Array ( [Identifiers] => Array ( [0] => Array ( [Type] => doi [Value] => 10.1093/mnras/stac071 ) ) [Languages] => Array ( [0] => Array ( [Text] => English ) ) [Subjects] => Array ( [0] => Array ( [SubjectFull] => galaxies: evolution [Type] => general ) [1] => Array ( [SubjectFull] => galaxies: high-redshift [Type] => general ) [2] => Array ( [SubjectFull] => galaxies: ISM [Type] => general ) ) [Titles] => Array ( [0] => Array ( [TitleFull] => The ALPINE-ALMA [C II] survey: Investigation of 10 galaxies at z 4.5 with [O II] and [C II] line emission - ISM properties and [O II]-SFR relation [Type] => main ) ) ) [BibRelationships] => Array ( [HasContributorRelationships] => Array ( [0] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => Brittany N Vanderhoof ) ) ) [1] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => A L Faisst ) ) ) [2] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L Shen ) ) ) [3] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => B C Lemaux ) ) ) [4] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M B??thermin ) ) ) [5] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => P L Capak ) ) ) [6] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => P Cassata ) ) ) [7] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => O Le??F??vre ) ) ) [8] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Schaerer ) ) ) [9] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => J Silverman ) ) ) [10] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L Yan ) ) ) [11] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Boquien ) ) ) [12] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => R Gal ) ) ) [13] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => J Kartaltepe ) ) ) [14] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L M Lubin ) ) ) [15] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Dessauges-Zavadsky ) ) ) [16] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => Y Fudamoto ) ) ) [17] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Ginolfi ) ) ) [18] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => N P Hathi ) ) ) [19] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => G C Jones ) ) ) [20] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => A M Koekemoer ) ) ) [21] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Narayanan ) ) ) [22] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Romano ) ) ) [23] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Talia ) ) ) [24] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Vergani ) ) ) [25] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => G Zamorani ) ) ) [26] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => Brittany N Vanderhoof ) ) ) [27] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => A L Faisst ) ) ) [28] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L Shen ) ) ) [29] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => B C Lemaux ) ) ) [30] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M B??thermin ) ) ) [31] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => P L Capak ) ) ) [32] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => P Cassata ) ) ) [33] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => O Le??F??vre ) ) ) [34] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Schaerer ) ) ) [35] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => J Silverman ) ) ) [36] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L Yan ) ) ) [37] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Boquien ) ) ) [38] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => R Gal ) ) ) [39] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => J Kartaltepe ) ) ) [40] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => L M Lubin ) ) ) [41] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Dessauges-Zavadsky ) ) ) [42] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => Y Fudamoto ) ) ) [43] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Ginolfi ) ) ) [44] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => N P Hathi ) ) ) [45] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => G C Jone ) ) ) [46] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => A M Koekemoer ) ) ) [47] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Narayanan ) ) ) [48] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Romano ) ) ) [49] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => M Talia ) ) ) [50] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => D Vergani ) ) ) [51] => Array ( [PersonEntity] => Array ( [Name] => Array ( [NameFull] => G Zamorani ) ) ) ) [IsPartOfRelationships] => Array ( [0] => Array ( [BibEntity] => Array ( [Dates] => Array ( [0] => Array ( [D] => 01 [M] => 01 [Type] => published [Y] => 2022 ) ) [Identifiers] => Array ( [0] => Array ( [Type] => issn-locals [Value] => edsbas ) [1] => Array ( [Type] => issn-locals [Value] => edsbas.oa ) ) ) ) ) ) )
IllustrationInfo