HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey

We present followup imaging of two bright (L > L*) galaxy candidates at z > 8 from the Brightest of Reionizing Galaxies (BoRG) survey with the F098M filter on HST/WFC3. The F098M filter provides an additional constraint on the flux blueward of the spectral break, and the observations are desig...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2018-07
Hauptverfasser: Livermore, R C, Trenti, M, Bradley, L D, Bernard, S R, Holwerda, B W, Mason, C A, Treu, T
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Livermore, R C
Trenti, M
Bradley, L D
Bernard, S R
Holwerda, B W
Mason, C A
Treu, T
description We present followup imaging of two bright (L > L*) galaxy candidates at z > 8 from the Brightest of Reionizing Galaxies (BoRG) survey with the F098M filter on HST/WFC3. The F098M filter provides an additional constraint on the flux blueward of the spectral break, and the observations are designed to discriminate between low- and high-z photometric redshift solutions for these galaxies. Our results confirm one galaxy, BoRG 0116+1425 747, as a highly probable z ~ 8 source, but reveal that BoRG 0116+1425 630 - previously the brightest known z > 8 candidate (mAB = 24.5) - is likely to be a z ~ 2 interloper. As this source was substantially brighter than any other z > 8 candidate, removing it from the sample has a significant impact on the derived UV luminosity function in this epoch. We show that while previous BoRG results favored a shallow power-law decline in the bright end of the luminosity function prior to reionization, there is now no evidence for departure from a Schechter function form and therefore no evidence for a difference in galaxy formation processes before and after reionization.
doi_str_mv 10.48550/arxiv.1805.05038
format Article
fullrecord <record><control><sourceid>proquest_arxiv</sourceid><recordid>TN_cdi_arxiv_primary_1805_05038</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2073881924</sourcerecordid><originalsourceid>FETCH-LOGICAL-a524-711cb1ff1dc78122057bef6d501b22b8518fd5c7e7827c275a9d7d4e94d91b9d3</originalsourceid><addsrcrecordid>eNotkMtKAzEYRoMgWGofwJU_uJ6ay6TJLLVoKxQEnf2QTJJ2StqMyUwvLnx2a-vq2xw-DgehO4LHueQcP6p4aHZjIjEfY46ZvEIDyhjJZE7pDRqltMYY04mgnLMBquefJbjgfdj3LQSdbNyprgnbBMFBtw-gY7NcdfANPyChVlvTGNVZWCqvDo1N4GLYQLey8Bw-ZtD20Watisp76yH1cWePt-jaKZ_s6H-HqHx9KafzbPE-e5s-LTLFaZ4JQmpNnCOmFpJQirnQ1k0Mx0RTqiUn0hleCyskFTUVXBVGmNwWuSmILgwbovvL7blA1cZmo-Kx-itRnUuciIcL0cbw1dvUVevQx-3JqaJYMClJQXP2CxulYSk</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2073881924</pqid></control><display><type>article</type><title>HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey</title><source>arXiv.org</source><source>Free E- Journals</source><creator>Livermore, R C ; Trenti, M ; Bradley, L D ; Bernard, S R ; Holwerda, B W ; Mason, C A ; Treu, T</creator><creatorcontrib>Livermore, R C ; Trenti, M ; Bradley, L D ; Bernard, S R ; Holwerda, B W ; Mason, C A ; Treu, T</creatorcontrib><description>We present followup imaging of two bright (L &gt; L*) galaxy candidates at z &gt; 8 from the Brightest of Reionizing Galaxies (BoRG) survey with the F098M filter on HST/WFC3. The F098M filter provides an additional constraint on the flux blueward of the spectral break, and the observations are designed to discriminate between low- and high-z photometric redshift solutions for these galaxies. Our results confirm one galaxy, BoRG 0116+1425 747, as a highly probable z ~ 8 source, but reveal that BoRG 0116+1425 630 - previously the brightest known z &gt; 8 candidate (mAB = 24.5) - is likely to be a z ~ 2 interloper. As this source was substantially brighter than any other z &gt; 8 candidate, removing it from the sample has a significant impact on the derived UV luminosity function in this epoch. We show that while previous BoRG results favored a shallow power-law decline in the bright end of the luminosity function prior to reionization, there is now no evidence for departure from a Schechter function form and therefore no evidence for a difference in galaxy formation processes before and after reionization.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1805.05038</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Galactic evolution ; Galaxies ; Ionization ; Luminosity ; Photometry ; Physics - Astrophysics of Galaxies ; Physics - Cosmology and Nongalactic Astrophysics ; Red shift ; Star &amp; galaxy formation ; Stars &amp; galaxies</subject><ispartof>arXiv.org, 2018-07</ispartof><rights>2018. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,780,881,27904</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1805.05038$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.3847/2041-8213/aacd16$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>Livermore, R C</creatorcontrib><creatorcontrib>Trenti, M</creatorcontrib><creatorcontrib>Bradley, L D</creatorcontrib><creatorcontrib>Bernard, S R</creatorcontrib><creatorcontrib>Holwerda, B W</creatorcontrib><creatorcontrib>Mason, C A</creatorcontrib><creatorcontrib>Treu, T</creatorcontrib><title>HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey</title><title>arXiv.org</title><description>We present followup imaging of two bright (L &gt; L*) galaxy candidates at z &gt; 8 from the Brightest of Reionizing Galaxies (BoRG) survey with the F098M filter on HST/WFC3. The F098M filter provides an additional constraint on the flux blueward of the spectral break, and the observations are designed to discriminate between low- and high-z photometric redshift solutions for these galaxies. Our results confirm one galaxy, BoRG 0116+1425 747, as a highly probable z ~ 8 source, but reveal that BoRG 0116+1425 630 - previously the brightest known z &gt; 8 candidate (mAB = 24.5) - is likely to be a z ~ 2 interloper. As this source was substantially brighter than any other z &gt; 8 candidate, removing it from the sample has a significant impact on the derived UV luminosity function in this epoch. We show that while previous BoRG results favored a shallow power-law decline in the bright end of the luminosity function prior to reionization, there is now no evidence for departure from a Schechter function form and therefore no evidence for a difference in galaxy formation processes before and after reionization.</description><subject>Galactic evolution</subject><subject>Galaxies</subject><subject>Ionization</subject><subject>Luminosity</subject><subject>Photometry</subject><subject>Physics - Astrophysics of Galaxies</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Red shift</subject><subject>Star &amp; galaxy formation</subject><subject>Stars &amp; galaxies</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkMtKAzEYRoMgWGofwJU_uJ6ay6TJLLVoKxQEnf2QTJJ2StqMyUwvLnx2a-vq2xw-DgehO4LHueQcP6p4aHZjIjEfY46ZvEIDyhjJZE7pDRqltMYY04mgnLMBquefJbjgfdj3LQSdbNyprgnbBMFBtw-gY7NcdfANPyChVlvTGNVZWCqvDo1N4GLYQLey8Bw-ZtD20Watisp76yH1cWePt-jaKZ_s6H-HqHx9KafzbPE-e5s-LTLFaZ4JQmpNnCOmFpJQirnQ1k0Mx0RTqiUn0hleCyskFTUVXBVGmNwWuSmILgwbovvL7blA1cZmo-Kx-itRnUuciIcL0cbw1dvUVevQx-3JqaJYMClJQXP2CxulYSk</recordid><startdate>20180704</startdate><enddate>20180704</enddate><creator>Livermore, R C</creator><creator>Trenti, M</creator><creator>Bradley, L D</creator><creator>Bernard, S R</creator><creator>Holwerda, B W</creator><creator>Mason, C A</creator><creator>Treu, T</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20180704</creationdate><title>HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey</title><author>Livermore, R C ; Trenti, M ; Bradley, L D ; Bernard, S R ; Holwerda, B W ; Mason, C A ; Treu, T</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a524-711cb1ff1dc78122057bef6d501b22b8518fd5c7e7827c275a9d7d4e94d91b9d3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Galactic evolution</topic><topic>Galaxies</topic><topic>Ionization</topic><topic>Luminosity</topic><topic>Photometry</topic><topic>Physics - Astrophysics of Galaxies</topic><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><topic>Red shift</topic><topic>Star &amp; galaxy formation</topic><topic>Stars &amp; galaxies</topic><toplevel>online_resources</toplevel><creatorcontrib>Livermore, R C</creatorcontrib><creatorcontrib>Trenti, M</creatorcontrib><creatorcontrib>Bradley, L D</creatorcontrib><creatorcontrib>Bernard, S R</creatorcontrib><creatorcontrib>Holwerda, B W</creatorcontrib><creatorcontrib>Mason, C A</creatorcontrib><creatorcontrib>Treu, T</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Livermore, R C</au><au>Trenti, M</au><au>Bradley, L D</au><au>Bernard, S R</au><au>Holwerda, B W</au><au>Mason, C A</au><au>Treu, T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey</atitle><jtitle>arXiv.org</jtitle><date>2018-07-04</date><risdate>2018</risdate><eissn>2331-8422</eissn><abstract>We present followup imaging of two bright (L &gt; L*) galaxy candidates at z &gt; 8 from the Brightest of Reionizing Galaxies (BoRG) survey with the F098M filter on HST/WFC3. The F098M filter provides an additional constraint on the flux blueward of the spectral break, and the observations are designed to discriminate between low- and high-z photometric redshift solutions for these galaxies. Our results confirm one galaxy, BoRG 0116+1425 747, as a highly probable z ~ 8 source, but reveal that BoRG 0116+1425 630 - previously the brightest known z &gt; 8 candidate (mAB = 24.5) - is likely to be a z ~ 2 interloper. As this source was substantially brighter than any other z &gt; 8 candidate, removing it from the sample has a significant impact on the derived UV luminosity function in this epoch. We show that while previous BoRG results favored a shallow power-law decline in the bright end of the luminosity function prior to reionization, there is now no evidence for departure from a Schechter function form and therefore no evidence for a difference in galaxy formation processes before and after reionization.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1805.05038</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2018-07
issn 2331-8422
language eng
recordid cdi_arxiv_primary_1805_05038
source arXiv.org; Free E- Journals
subjects Galactic evolution
Galaxies
Ionization
Luminosity
Photometry
Physics - Astrophysics of Galaxies
Physics - Cosmology and Nongalactic Astrophysics
Red shift
Star & galaxy formation
Stars & galaxies
title HST followup observations of two bright z ~ 8 candidate galaxies from the BoRG pure-parallel survey
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-26T20%3A03%3A02IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_arxiv&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=HST%20followup%20observations%20of%20two%20bright%20z%20~%208%20candidate%20galaxies%20from%20the%20BoRG%20pure-parallel%20survey&rft.jtitle=arXiv.org&rft.au=Livermore,%20R%20C&rft.date=2018-07-04&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.1805.05038&rft_dat=%3Cproquest_arxiv%3E2073881924%3C/proquest_arxiv%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2073881924&rft_id=info:pmid/&rfr_iscdi=true