A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses
We present a thorough study of the specific star formation rates (sSFRs) for MIPS 24 Delta *mm selected galaxies in the Coma cluster. We build galaxy spectral energy distributions using optical (u', g', r', i', z'), near-infrared (J, H, Ks ), and mid- to far-infrared (Infrar...
Gespeichert in:
Veröffentlicht in: | The Astronomical journal 2011-11, Vol.142 (5), p.148-jQuery1323896794567='48' |
---|---|
Hauptverfasser: | , |
Format: | Artikel |
Sprache: | eng |
Schlagworte: | |
Online-Zugang: | Volltext bestellen |
Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
container_end_page | jQuery1323896794567='48' |
---|---|
container_issue | 5 |
container_start_page | 148 |
container_title | The Astronomical journal |
container_volume | 142 |
creator | Edwards, Louise O. V Fadda, Dario |
description | We present a thorough study of the specific star formation rates (sSFRs) for MIPS 24 Delta *mm selected galaxies in the Coma cluster. We build galaxy spectral energy distributions using optical (u', g', r', i', z'), near-infrared (J, H, Ks ), and mid- to far-infrared (Infrared Array Camera and MIPS) photometry. New and archival spectra confirm 210 cluster members. Subsequently, the total infrared luminosity, galaxy stellar mass, and sSFR for the members are determined by measuring best-fit templates. Using an array of complementary diagnostics, we search for any contaminating active galactic nuclei, but find few. We compare obscured SFRs to unobscured rates derived from extinction-corrected H Delta *a emission line measurements. The agreement between these two values leads us to conclude that there is no evidence for an additionally obscured component. In our spectroscopic sample, complete to 80% for r' < 19.5, we find that all starbursts are blue and are dwarfs, having masses |
doi_str_mv | 10.1088/0004-6256/142/5/148 |
format | Article |
fullrecord | <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_miscellaneous_920796809</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>920796809</sourcerecordid><originalsourceid>FETCH-LOGICAL-c383t-73fdab66f1c89ea595381f6ce6decbefcdb4c18ca26b597355aac78453a537753</originalsourceid><addsrcrecordid>eNp9kU1r3DAQhk1JoPnoL-hF0EOg4KxkWbLc27LkCxIC2eQsZuVRo-K1XI82afrro2UDyaH0MhKj532ZeVUUXwU_FdyYGee8LnWl9EzU1Uzlaj4VB0JJU0pjxN6H--fikOgX50IYXh8Ufs5uNn0K5TM8YY_Dz_TI5gP0LxSIRc-WY0h_cWLL_OgSdmwR18AW_YZS7l5AD38C0g-2TDCx8zitIYU4sDtISAyGjt0AEdJxse-hJ_zydh4VD-dn94vL8vr24moxvy6dNDKVjfQdrLT2wpkWQbV5auG1Q92hW6F33ap2wjio9Eq1jVQKwDWmVhKUbBolj4pvO99IKVhyIaF7dHEY8vC2EspUhutMneyocYq_N0jJrgM57HsYMG7IthVvWm14m0m5I90UiSb0dpzCGqYXK7jdRm-30dtt9DZHb1WuJqu-71Qhju-CvIvd_sA7aMfOZ_j0H_B_3F8BtfaRwQ</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>920796809</pqid></control><display><type>article</type><title>A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses</title><source>Institute of Physics Open Access Journal Titles</source><creator>Edwards, Louise O. V ; Fadda, Dario</creator><creatorcontrib>Edwards, Louise O. V ; Fadda, Dario</creatorcontrib><description>We present a thorough study of the specific star formation rates (sSFRs) for MIPS 24 Delta *mm selected galaxies in the Coma cluster. We build galaxy spectral energy distributions using optical (u', g', r', i', z'), near-infrared (J, H, Ks ), and mid- to far-infrared (Infrared Array Camera and MIPS) photometry. New and archival spectra confirm 210 cluster members. Subsequently, the total infrared luminosity, galaxy stellar mass, and sSFR for the members are determined by measuring best-fit templates. Using an array of complementary diagnostics, we search for any contaminating active galactic nuclei, but find few. We compare obscured SFRs to unobscured rates derived from extinction-corrected H Delta *a emission line measurements. The agreement between these two values leads us to conclude that there is no evidence for an additionally obscured component. In our spectroscopic sample, complete to 80% for r' < 19.5, we find that all starbursts are blue and are dwarfs, having masses <109 M . Examining the location of these starbursts within the cluster, we confirm that there is a lower fraction in the cluster core.</description><identifier>ISSN: 1538-3881</identifier><identifier>ISSN: 0004-6256</identifier><identifier>EISSN: 1538-3881</identifier><identifier>DOI: 10.1088/0004-6256/142/5/148</identifier><language>eng</language><publisher>United States: IOP Publishing</publisher><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; CAMERAS ; EMISSION ; ENERGY SPECTRA ; GALAXIES ; GALAXY CLUSTERS ; GALAXY NUCLEI ; LUMINOSITY ; MASS ; OPTICAL PROPERTIES ; PHOTOMETRY ; PHYSICAL PROPERTIES ; SPECTRA ; STARS</subject><ispartof>The Astronomical journal, 2011-11, Vol.142 (5), p.148-jQuery1323896794567='48'</ispartof><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c383t-73fdab66f1c89ea595381f6ce6decbefcdb4c18ca26b597355aac78453a537753</citedby><cites>FETCH-LOGICAL-c383t-73fdab66f1c89ea595381f6ce6decbefcdb4c18ca26b597355aac78453a537753</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.1088/0004-6256/142/5/148/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,780,784,885,1553,27628,27924,27925,53904,53931</link.rule.ids><linktorsrc>$$Uhttp://iopscience.iop.org/1538-3881/142/5/148$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/21582806$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Edwards, Louise O. V</creatorcontrib><creatorcontrib>Fadda, Dario</creatorcontrib><title>A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses</title><title>The Astronomical journal</title><description>We present a thorough study of the specific star formation rates (sSFRs) for MIPS 24 Delta *mm selected galaxies in the Coma cluster. We build galaxy spectral energy distributions using optical (u', g', r', i', z'), near-infrared (J, H, Ks ), and mid- to far-infrared (Infrared Array Camera and MIPS) photometry. New and archival spectra confirm 210 cluster members. Subsequently, the total infrared luminosity, galaxy stellar mass, and sSFR for the members are determined by measuring best-fit templates. Using an array of complementary diagnostics, we search for any contaminating active galactic nuclei, but find few. We compare obscured SFRs to unobscured rates derived from extinction-corrected H Delta *a emission line measurements. The agreement between these two values leads us to conclude that there is no evidence for an additionally obscured component. In our spectroscopic sample, complete to 80% for r' < 19.5, we find that all starbursts are blue and are dwarfs, having masses <109 M . Examining the location of these starbursts within the cluster, we confirm that there is a lower fraction in the cluster core.</description><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>CAMERAS</subject><subject>EMISSION</subject><subject>ENERGY SPECTRA</subject><subject>GALAXIES</subject><subject>GALAXY CLUSTERS</subject><subject>GALAXY NUCLEI</subject><subject>LUMINOSITY</subject><subject>MASS</subject><subject>OPTICAL PROPERTIES</subject><subject>PHOTOMETRY</subject><subject>PHYSICAL PROPERTIES</subject><subject>SPECTRA</subject><subject>STARS</subject><issn>1538-3881</issn><issn>0004-6256</issn><issn>1538-3881</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2011</creationdate><recordtype>article</recordtype><recordid>eNp9kU1r3DAQhk1JoPnoL-hF0EOg4KxkWbLc27LkCxIC2eQsZuVRo-K1XI82afrro2UDyaH0MhKj532ZeVUUXwU_FdyYGee8LnWl9EzU1Uzlaj4VB0JJU0pjxN6H--fikOgX50IYXh8Ufs5uNn0K5TM8YY_Dz_TI5gP0LxSIRc-WY0h_cWLL_OgSdmwR18AW_YZS7l5AD38C0g-2TDCx8zitIYU4sDtISAyGjt0AEdJxse-hJ_zydh4VD-dn94vL8vr24moxvy6dNDKVjfQdrLT2wpkWQbV5auG1Q92hW6F33ap2wjio9Eq1jVQKwDWmVhKUbBolj4pvO99IKVhyIaF7dHEY8vC2EspUhutMneyocYq_N0jJrgM57HsYMG7IthVvWm14m0m5I90UiSb0dpzCGqYXK7jdRm-30dtt9DZHb1WuJqu-71Qhju-CvIvd_sA7aMfOZ_j0H_B_3F8BtfaRwQ</recordid><startdate>20111101</startdate><enddate>20111101</enddate><creator>Edwards, Louise O. V</creator><creator>Fadda, Dario</creator><general>IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>OTOTI</scope></search><sort><creationdate>20111101</creationdate><title>A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses</title><author>Edwards, Louise O. V ; Fadda, Dario</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c383t-73fdab66f1c89ea595381f6ce6decbefcdb4c18ca26b597355aac78453a537753</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2011</creationdate><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>CAMERAS</topic><topic>EMISSION</topic><topic>ENERGY SPECTRA</topic><topic>GALAXIES</topic><topic>GALAXY CLUSTERS</topic><topic>GALAXY NUCLEI</topic><topic>LUMINOSITY</topic><topic>MASS</topic><topic>OPTICAL PROPERTIES</topic><topic>PHOTOMETRY</topic><topic>PHYSICAL PROPERTIES</topic><topic>SPECTRA</topic><topic>STARS</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Edwards, Louise O. V</creatorcontrib><creatorcontrib>Fadda, Dario</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>OSTI.GOV</collection><jtitle>The Astronomical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Edwards, Louise O. V</au><au>Fadda, Dario</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses</atitle><jtitle>The Astronomical journal</jtitle><date>2011-11-01</date><risdate>2011</risdate><volume>142</volume><issue>5</issue><spage>148</spage><epage>jQuery1323896794567='48'</epage><pages>148-jQuery1323896794567='48'</pages><issn>1538-3881</issn><issn>0004-6256</issn><eissn>1538-3881</eissn><abstract>We present a thorough study of the specific star formation rates (sSFRs) for MIPS 24 Delta *mm selected galaxies in the Coma cluster. We build galaxy spectral energy distributions using optical (u', g', r', i', z'), near-infrared (J, H, Ks ), and mid- to far-infrared (Infrared Array Camera and MIPS) photometry. New and archival spectra confirm 210 cluster members. Subsequently, the total infrared luminosity, galaxy stellar mass, and sSFR for the members are determined by measuring best-fit templates. Using an array of complementary diagnostics, we search for any contaminating active galactic nuclei, but find few. We compare obscured SFRs to unobscured rates derived from extinction-corrected H Delta *a emission line measurements. The agreement between these two values leads us to conclude that there is no evidence for an additionally obscured component. In our spectroscopic sample, complete to 80% for r' < 19.5, we find that all starbursts are blue and are dwarfs, having masses <109 M . Examining the location of these starbursts within the cluster, we confirm that there is a lower fraction in the cluster core.</abstract><cop>United States</cop><pub>IOP Publishing</pub><doi>10.1088/0004-6256/142/5/148</doi></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 1538-3881 |
ispartof | The Astronomical journal, 2011-11, Vol.142 (5), p.148-jQuery1323896794567='48' |
issn | 1538-3881 0004-6256 1538-3881 |
language | eng |
recordid | cdi_proquest_miscellaneous_920796809 |
source | Institute of Physics Open Access Journal Titles |
subjects | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CAMERAS EMISSION ENERGY SPECTRA GALAXIES GALAXY CLUSTERS GALAXY NUCLEI LUMINOSITY MASS OPTICAL PROPERTIES PHOTOMETRY PHYSICAL PROPERTIES SPECTRA STARS |
title | A Multi-wavelength Analysis of Spitzer Selected Coma Cluster Galaxies: Star Formation Rates and Masses |
url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-22T06%3A15%3A24IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20Multi-wavelength%20Analysis%20of%20Spitzer%20Selected%20Coma%20Cluster%20Galaxies:%20Star%20Formation%20Rates%20and%20Masses&rft.jtitle=The%20Astronomical%20journal&rft.au=Edwards,%20Louise%20O.%20V&rft.date=2011-11-01&rft.volume=142&rft.issue=5&rft.spage=148&rft.epage=jQuery1323896794567='48'&rft.pages=148-jQuery1323896794567='48'&rft.issn=1538-3881&rft.eissn=1538-3881&rft_id=info:doi/10.1088/0004-6256/142/5/148&rft_dat=%3Cproquest_O3W%3E920796809%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=920796809&rft_id=info:pmid/&rfr_iscdi=true |