Blueberry Galaxies: The Lowest Mass Young Starbursts
Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be se...
Saved in:
Published in | The Astrophysical journal Vol. 847; no. 1; pp. 38 - 46 |
---|---|
Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Philadelphia
The American Astronomical Society
20.09.2017
IOP Publishing |
Subjects | |
Online Access | Get full text |
Cover
Loading…
Abstract | Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10-60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly emitting galaxies. |
---|---|
AbstractList | Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts (z≲0.05) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at z≲0.05 (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10–60). They also have some of the lowest stellar masses (log(M/M{sub ⊙})∼6.5--7.5) and lowest metallicities (7.1<12+log(O/H)<7.8) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Lyα emitting galaxies. Abstract Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly α emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii ]/[O ii ] ∼ 10–60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly α emitting galaxies. Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts ( ) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10-60). They also have some of the lowest stellar masses ( ) and lowest metallicities ( ) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Ly emitting galaxies. Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These low-mass extreme emission line galaxies are also potential Lyman-continuum leakers. Finding them at very low redshifts (\(z\lesssim 0.05\)) allows us to be sensitive to even lower stellar masses and metallicities. We report on a sample of extreme emission line galaxies at \(z\lesssim 0.05\) (blueberry galaxies). We selected them from SDSS broadband images on the basis of their broadband colors and studied their properties with MMT spectroscopy. From the entire SDSS DR12 photometric catalog, we found 51 photometric candidates. We spectroscopically confirm 40 as blueberry galaxies. (An additional seven candidates are contaminants, and four remain without spectra.) These blueberries are dwarf starburst galaxies with very small sizes (<1 kpc) and very high ionization ([O iii]/[O ii] ∼ 10–60). They also have some of the lowest stellar masses (\(\mathrm{log}(M/{M}_{\odot })\sim 6.5\mbox{--}7.5\)) and lowest metallicities (\(7.1\lt 12+\mathrm{log}({\rm{O}}/{\rm{H}})\lt 7.8\)) of starburst galaxies. Thus, they are small counterparts to green pea galaxies and high redshift Lyα emitting galaxies. |
Author | Wang, Junxian Rhoads, James E. Yang, Huan Malhotra, Sangeeta |
Author_xml | – sequence: 1 givenname: Huan orcidid: 0000-0003-2260-7420 surname: Yang fullname: Yang, Huan email: huan.y@asu.edu organization: Arizona State University , School of Earth and Space Exploration, USA – sequence: 2 givenname: Sangeeta orcidid: 0000-0002-9226-5350 surname: Malhotra fullname: Malhotra, Sangeeta organization: Arizona State University , School of Earth and Space Exploration, USA – sequence: 3 givenname: James E. surname: Rhoads fullname: Rhoads, James E. organization: Arizona State University , School of Earth and Space Exploration, USA – sequence: 4 givenname: Junxian orcidid: 0000-0002-4419-6434 surname: Wang fullname: Wang, Junxian organization: University of Science and Technology of China CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, China |
BackLink | https://www.osti.gov/biblio/22875776$$D View this record in Osti.gov |
BookMark | eNp1kE1Lw0AQhhdRsK3ePQa8Gruf2Y03LVqFigcr6GnZbCY2pWbr7gbtvzchol48DTM878vwjNF-4xpA6ITgc6a4nBLBVMqZkFNjlML5Hhr9nPbRCGPM04zJ50M0DmHdrzTPR4hfbVoowPtdMjcb81lDuEiWK0gW7gNCTO5NCMmLa5vX5DEaX7Q-xHCEDiqzCXD8PSfo6eZ6ObtNFw_zu9nlIrWc85hKShTJMVhakQKszQxXqhQgS8tKTkuZ58waW1KFKy6BEE5wgQvIBHAiRcYm6HTodSHWOtg6gl1Z1zRgo6ZUSSHlH2rr3XvbPa3XrvVN95imLBNSYUZIR-GBst6F4KHSW1-_Gb_TBOveoO516V6XHgx2kbMhUrvtb-e_-BeXTnEA |
CitedBy_id | crossref_primary_10_1051_0004_6361_202245167 crossref_primary_10_1093_mnras_staa1937 crossref_primary_10_3847_1538_3881_ace893 crossref_primary_10_1051_0004_6361_202346981 crossref_primary_10_3847_1538_4357_ac33a5 crossref_primary_10_3847_1538_4357_ab91af crossref_primary_10_1051_0004_6361_202346107 crossref_primary_10_3847_1538_4357_ac469f crossref_primary_10_3847_2041_8213_acab63 crossref_primary_10_3847_1538_4357_acf715 crossref_primary_10_3847_1538_4357_ad1409 crossref_primary_10_1093_mnras_stz940 crossref_primary_10_1093_mnras_sty378 crossref_primary_10_3847_1538_4365_ac7710 crossref_primary_10_1093_mnras_stad3018 crossref_primary_10_1051_0004_6361_202243931 crossref_primary_10_3847_1538_4357_ac5117 crossref_primary_10_3847_2041_8213_ab3c63 crossref_primary_10_1051_0004_6361_202141900 crossref_primary_10_3847_1538_4357_ab7447 crossref_primary_10_1093_mnras_stab3554 crossref_primary_10_3847_1538_4357_aba047 crossref_primary_10_3847_1538_4357_aca89b crossref_primary_10_1051_0004_6361_202245532 crossref_primary_10_3847_1538_4357_ab08ec crossref_primary_10_1093_mnras_staa2757 crossref_primary_10_1093_mnras_stab705 crossref_primary_10_1038_s41550_024_02218_7 crossref_primary_10_1093_mnras_staa851 crossref_primary_10_1093_mnras_staa2836 crossref_primary_10_3847_1538_4357_aad18a crossref_primary_10_3847_1538_4357_aabfd9 crossref_primary_10_3847_2041_8213_abf7cc crossref_primary_10_1093_mnras_stz058 crossref_primary_10_1093_mnras_stab2589 crossref_primary_10_1093_mnras_stab2789 crossref_primary_10_3847_1538_4357_acd181 crossref_primary_10_1093_mnras_stac2657 crossref_primary_10_3847_1538_4357_abec40 crossref_primary_10_1051_0004_6361_202347133 crossref_primary_10_1017_S1743921319003181 crossref_primary_10_1051_0004_6361_202347016 crossref_primary_10_1093_mnras_stab612 crossref_primary_10_3847_1538_4357_ab9ec0 crossref_primary_10_1051_0004_6361_202039772 crossref_primary_10_15407_kfnt2023_02_034 crossref_primary_10_1051_0004_6361_202348819 crossref_primary_10_3847_1538_4357_ac4bd9 crossref_primary_10_1093_mnras_stab3226 crossref_primary_10_1093_mnras_stad1618 crossref_primary_10_3847_1538_4357_acdbc1 crossref_primary_10_1093_mnras_stae252 crossref_primary_10_3390_galaxies8010006 crossref_primary_10_1093_mnras_stae1490 crossref_primary_10_3847_1538_4357_acdb4b crossref_primary_10_3847_1538_4357_ac5c4b crossref_primary_10_1093_mnras_stac1437 crossref_primary_10_3847_1538_4357_ab3df7 crossref_primary_10_3847_1538_4357_ac402a crossref_primary_10_3847_1538_4357_aae585 crossref_primary_10_3847_2041_8213_aaa0ce crossref_primary_10_1051_0004_6361_202142898 crossref_primary_10_3103_S0884591323020022 crossref_primary_10_1051_0004_6361_202346698 crossref_primary_10_1093_pasj_psab105 crossref_primary_10_1093_mnras_stab1239 crossref_primary_10_3847_2041_8213_acdbce crossref_primary_10_3847_1538_4357_ab2f87 crossref_primary_10_1038_s41550_021_01575_x crossref_primary_10_1093_mnras_stad1903 crossref_primary_10_1093_mnras_stad1704 crossref_primary_10_3847_1538_4357_accf14 crossref_primary_10_3847_1538_4357_ac01ed |
Cites_doi | 10.3847/0067-0049/227/1/2 10.1088/0004-637X/809/1/89 10.1088/0004-637X/809/1/19 10.3847/0004-637X/820/2/130 10.3847/2041-8213/aa794f 10.1086/507575 10.1088/2041-8205/714/2/L202 10.1088/0004-637X/794/1/5 10.1086/374737 10.1088/0004-637X/754/2/98 10.1088/0004-637X/765/2/140 10.1088/0004-637X/725/1/394 10.1086/525272 10.1051/0004-6361:20053763 10.1051/0004-6361/201629264 10.1093/mnras/195.4.839 10.1051/0004-6361:200810722 10.1093/mnras/stw2962 10.1088/0004-6256/143/6/133 10.1051/0004-6361/201629728 10.1088/2041-8205/750/2/L36 10.1051/0004-6361/201629181 10.1111/j.1365-2966.2010.18155.x 10.1088/0004-637X/706/1/599 10.1086/159094 10.1093/mnras/stw1205 10.1088/0004-637X/780/2/122 10.1088/2041-8205/715/2/L128 10.1111/j.1365-2966.2009.15383.x 10.1088/0004-637X/803/1/34 10.1046/j.1365-8711.2003.06291.x 10.1088/0004-637X/728/2/161 10.1086/427182 10.1088/0004-637X/737/2/103 10.1088/0004-637X/730/2/136 10.1088/2041-8205/728/1/L2 10.1086/505573 10.1093/mnras/sts116 10.1086/382245 10.1146/annurev-astro-081811-125610 10.3847/1538-4357/aa7d4d 10.1086/522955 10.1088/0004-637X/723/1/869 10.1086/316293 10.1088/0004-637X/806/1/19 10.1088/0004-6256/143/6/145 10.1088/0004-6256/139/1/279 10.3847/0004-637X/819/2/110 10.1086/313233 10.1088/2041-8205/791/2/L19 10.1086/519485 10.1093/mnras/stv947 |
ContentType | Journal Article |
Copyright | 2017. The American Astronomical Society. All rights reserved. Copyright IOP Publishing Sep 20, 2017 |
Copyright_xml | – notice: 2017. The American Astronomical Society. All rights reserved. – notice: Copyright IOP Publishing Sep 20, 2017 |
DBID | AAYXX CITATION 7TG 8FD H8D KL. L7M OTOTI |
DOI | 10.3847/1538-4357/aa8809 |
DatabaseName | CrossRef Meteorological & Geoastrophysical Abstracts Technology Research Database Aerospace Database Meteorological & Geoastrophysical Abstracts - Academic Advanced Technologies Database with Aerospace OSTI.GOV |
DatabaseTitle | CrossRef Aerospace Database Meteorological & Geoastrophysical Abstracts Technology Research Database Advanced Technologies Database with Aerospace Meteorological & Geoastrophysical Abstracts - Academic |
DatabaseTitleList | CrossRef Aerospace Database |
DeliveryMethod | fulltext_linktorsrc |
Discipline | Astronomy & Astrophysics Physics |
DocumentTitleAlternate | Blueberry Galaxies: The Lowest Mass Young Starbursts |
EISSN | 1538-4357 |
ExternalDocumentID | 22875776 10_3847_1538_4357_aa8809 apjaa8809 |
GroupedDBID | -DZ -~X 123 1JI 23N 2FS 2WC 4.4 6J9 85S AAFWJ AAGCD AAJIO AALHV ABHWH ACBEA ACGFS ACHIP ACNCT ADACN AEFHF AENEX AFPKN AKPSB ALMA_UNASSIGNED_HOLDINGS ASPBG ATQHT AVWKF AZFZN CJUJL CRLBU CS3 EBS EJD F5P FRP GROUPED_DOAJ IJHAN IOP KOT M~E N5L O3W O43 OK1 PJBAE RIN RNS ROL SJN SY9 T37 TN5 TR2 WH7 XSW AAYXX CITATION 7TG 8FD H8D KL. L7M ABPTK OTOTI |
ID | FETCH-LOGICAL-c444t-7218190ec2f1becc6a488d5e7dc3d42d7993cacd280f47e11410b0be65e417563 |
IEDL.DBID | O3W |
ISSN | 0004-637X |
IngestDate | Fri May 19 01:47:14 EDT 2023 Thu Oct 10 16:27:27 EDT 2024 Fri Aug 23 03:43:35 EDT 2024 Wed Aug 21 03:41:33 EDT 2024 |
IsDoiOpenAccess | false |
IsOpenAccess | true |
IsPeerReviewed | true |
IsScholarly | true |
Issue | 1 |
Language | English |
LinkModel | DirectLink |
MergedId | FETCHMERGED-LOGICAL-c444t-7218190ec2f1becc6a488d5e7dc3d42d7993cacd280f47e11410b0be65e417563 |
Notes | Galaxies and Cosmology AAS06012 |
ORCID | 0000-0002-4419-6434 0000-0002-9226-5350 0000-0003-2260-7420 |
OpenAccessLink | https://iopscience.iop.org/article/10.3847/1538-4357/aa8809/pdf |
PQID | 2365780311 |
PQPubID | 4562441 |
PageCount | 9 |
ParticipantIDs | osti_scitechconnect_22875776 proquest_journals_2365780311 crossref_primary_10_3847_1538_4357_aa8809 iop_journals_10_3847_1538_4357_aa8809 |
PublicationCentury | 2000 |
PublicationDate | 20170920 2017-09-20 |
PublicationDateYYYYMMDD | 2017-09-20 |
PublicationDate_xml | – month: 09 year: 2017 text: 20170920 day: 20 |
PublicationDecade | 2010 |
PublicationPlace | Philadelphia |
PublicationPlace_xml | – name: Philadelphia – name: United States |
PublicationTitle | The Astrophysical journal |
PublicationTitleAbbrev | APJ |
PublicationTitleAlternate | Astrophys. J |
PublicationYear | 2017 |
Publisher | The American Astronomical Society IOP Publishing |
Publisher_xml | – name: The American Astronomical Society – name: IOP Publishing |
References | Fitzpatrick (apjaa8809bib10) 1999; 111 Ly (apjaa8809bib29) 2014; 780 Huang (apjaa8809bib16) 2012; 143 Lupton (apjaa8809bib54) 2004; 116 Hu (apjaa8809bib15) 2010; 725 Pentericci (apjaa8809bib36) 2009; 494 Kellar (apjaa8809bib24) 2012; 143 Gil de Paz (apjaa8809bib12) 2003; 147 Amorín (apjaa8809bib1) 2010; 715 Izotov (apjaa8809bib17) 2011; 728 Ouchi (apjaa8809bib35) 2010; 723 Yang (apjaa8809bib51) 2017; 844 Tilvi (apjaa8809bib45) 2014; 794 Dressler (apjaa8809bib8) 2015; 806 Thuan (apjaa8809bib44) 1981; 247 Terlevich (apjaa8809bib43) 1981; 195 Guseva (apjaa8809bib13) 2017; 599 Lee (apjaa8809bib26) 2006; 647 Izotov (apjaa8809bib19) 2006; 448 Chambers (apjaa8809bib6) 2016 Pirzkal (apjaa8809bib37) 2007; 667 Melnick (apjaa8809bib34) 2017; 599 Salim (apjaa8809bib38) 2016; 227 Gawiser (apjaa8809bib11) 2007; 671 Malhotra (apjaa8809bib30) 2004; 617 Trainor (apjaa8809bib46) 2015; 809 Zwicky (apjaa8809bib53) 1971 Berg (apjaa8809bib3) 2012; 754 Leitherer (apjaa8809bib28) 1999; 123 Henry (apjaa8809bib14) 2015; 809 Sánchez Almeida (apjaa8809bib40) 2016; 819 Bouwens (apjaa8809bib4) 2015; 803 Trenti (apjaa8809bib47) 2010; 714 Jaskot (apjaa8809bib21) 2014; 791 Yang (apjaa8809bib50) 2016; 820 Kennicutt (apjaa8809bib25) 2012; 50 Jensen (apjaa8809bib22) 2013; 428 Stark (apjaa8809bib42) 2011; 728 Cardamone (apjaa8809bib5) 2009; 399 Zheng (apjaa8809bib52) 2017; 842 James (apjaa8809bib20) 2017; 465 Schlafly (apjaa8809bib41) 2011; 737 Salvaterra (apjaa8809bib39) 2011; 414 Verhamme (apjaa8809bib48) 2017; 597 Finkelstein (apjaa8809bib9) 2008; 678 Malhotra (apjaa8809bib31) 2012; 750 Corbin (apjaa8809bib7) 2006; 651 Werk (apjaa8809bib49) 2010; 139 Izotov (apjaa8809bib18) 2016; 461 McLinden (apjaa8809bib33) 2011; 730 Andrews (apjaa8809bib2) 2013; 765 Matthee (apjaa8809bib32) 2015; 451 Kauffmann (apjaa8809bib23) 2003; 341 Lee (apjaa8809bib27) 2009; 706 |
References_xml | – volume: 227 start-page: 2 year: 2016 ident: apjaa8809bib38 publication-title: ApJS doi: 10.3847/0067-0049/227/1/2 contributor: fullname: Salim – volume: 809 start-page: 89 year: 2015 ident: apjaa8809bib46 publication-title: ApJ doi: 10.1088/0004-637X/809/1/89 contributor: fullname: Trainor – volume: 809 start-page: 19 year: 2015 ident: apjaa8809bib14 publication-title: ApJ doi: 10.1088/0004-637X/809/1/19 contributor: fullname: Henry – volume: 820 start-page: 130 year: 2016 ident: apjaa8809bib50 publication-title: ApJ doi: 10.3847/0004-637X/820/2/130 contributor: fullname: Yang – volume: 842 start-page: L22 year: 2017 ident: apjaa8809bib52 doi: 10.3847/2041-8213/aa794f contributor: fullname: Zheng – volume: 651 start-page: 861 year: 2006 ident: apjaa8809bib7 publication-title: ApJ doi: 10.1086/507575 contributor: fullname: Corbin – volume: 714 start-page: L202 year: 2010 ident: apjaa8809bib47 publication-title: ApJL doi: 10.1088/2041-8205/714/2/L202 contributor: fullname: Trenti – volume: 794 start-page: 5 year: 2014 ident: apjaa8809bib45 publication-title: ApJ doi: 10.1088/0004-637X/794/1/5 contributor: fullname: Tilvi – volume: 147 start-page: 29 year: 2003 ident: apjaa8809bib12 publication-title: ApJS doi: 10.1086/374737 contributor: fullname: Gil de Paz – volume: 754 start-page: 98 year: 2012 ident: apjaa8809bib3 publication-title: ApJ doi: 10.1088/0004-637X/754/2/98 contributor: fullname: Berg – volume: 765 start-page: 140 year: 2013 ident: apjaa8809bib2 publication-title: ApJ doi: 10.1088/0004-637X/765/2/140 contributor: fullname: Andrews – volume: 725 start-page: 394 year: 2010 ident: apjaa8809bib15 publication-title: ApJ doi: 10.1088/0004-637X/725/1/394 contributor: fullname: Hu – volume: 678 start-page: 655 year: 2008 ident: apjaa8809bib9 publication-title: ApJ doi: 10.1086/525272 contributor: fullname: Finkelstein – volume: 448 start-page: 955 year: 2006 ident: apjaa8809bib19 publication-title: A&A doi: 10.1051/0004-6361:20053763 contributor: fullname: Izotov – year: 1971 ident: apjaa8809bib53 contributor: fullname: Zwicky – volume: 597 start-page: A13 year: 2017 ident: apjaa8809bib48 publication-title: A&A doi: 10.1051/0004-6361/201629264 contributor: fullname: Verhamme – volume: 195 start-page: 839 year: 1981 ident: apjaa8809bib43 publication-title: MNRAS doi: 10.1093/mnras/195.4.839 contributor: fullname: Terlevich – volume: 494 start-page: 553 year: 2009 ident: apjaa8809bib36 publication-title: A&A doi: 10.1051/0004-6361:200810722 contributor: fullname: Pentericci – volume: 465 start-page: 3977 year: 2017 ident: apjaa8809bib20 publication-title: MNRAS doi: 10.1093/mnras/stw2962 contributor: fullname: James – volume: 143 start-page: 133 year: 2012 ident: apjaa8809bib16 publication-title: AJ doi: 10.1088/0004-6256/143/6/133 contributor: fullname: Huang – volume: 599 start-page: A76 year: 2017 ident: apjaa8809bib34 publication-title: A&A doi: 10.1051/0004-6361/201629728 contributor: fullname: Melnick – volume: 750 start-page: L36 year: 2012 ident: apjaa8809bib31 publication-title: ApJL doi: 10.1088/2041-8205/750/2/L36 contributor: fullname: Malhotra – volume: 599 start-page: A65 year: 2017 ident: apjaa8809bib13 publication-title: A&A doi: 10.1051/0004-6361/201629181 contributor: fullname: Guseva – volume: 414 start-page: 847 year: 2011 ident: apjaa8809bib39 publication-title: MNRAS doi: 10.1111/j.1365-2966.2010.18155.x contributor: fullname: Salvaterra – volume: 706 start-page: 599 year: 2009 ident: apjaa8809bib27 publication-title: ApJ doi: 10.1088/0004-637X/706/1/599 contributor: fullname: Lee – volume: 247 start-page: 823 year: 1981 ident: apjaa8809bib44 publication-title: ApJ doi: 10.1086/159094 contributor: fullname: Thuan – volume: 461 start-page: 3683 year: 2016 ident: apjaa8809bib18 publication-title: MNRAS doi: 10.1093/mnras/stw1205 contributor: fullname: Izotov – volume: 780 start-page: 122 year: 2014 ident: apjaa8809bib29 publication-title: ApJ doi: 10.1088/0004-637X/780/2/122 contributor: fullname: Ly – volume: 715 start-page: L128 year: 2010 ident: apjaa8809bib1 publication-title: ApJL doi: 10.1088/2041-8205/715/2/L128 contributor: fullname: Amorín – volume: 399 start-page: 1191 year: 2009 ident: apjaa8809bib5 publication-title: MNRAS doi: 10.1111/j.1365-2966.2009.15383.x contributor: fullname: Cardamone – volume: 803 start-page: 34 year: 2015 ident: apjaa8809bib4 publication-title: ApJ doi: 10.1088/0004-637X/803/1/34 contributor: fullname: Bouwens – volume: 341 start-page: 33 year: 2003 ident: apjaa8809bib23 publication-title: MNRAS doi: 10.1046/j.1365-8711.2003.06291.x contributor: fullname: Kauffmann – volume: 728 start-page: 161 year: 2011 ident: apjaa8809bib17 publication-title: ApJ doi: 10.1088/0004-637X/728/2/161 contributor: fullname: Izotov – volume: 617 start-page: L5 year: 2004 ident: apjaa8809bib30 publication-title: ApJL doi: 10.1086/427182 contributor: fullname: Malhotra – volume: 737 start-page: 103 year: 2011 ident: apjaa8809bib41 publication-title: ApJ doi: 10.1088/0004-637X/737/2/103 contributor: fullname: Schlafly – volume: 730 start-page: 136 year: 2011 ident: apjaa8809bib33 publication-title: ApJ doi: 10.1088/0004-637X/730/2/136 contributor: fullname: McLinden – volume: 728 start-page: L2 year: 2011 ident: apjaa8809bib42 publication-title: ApJL doi: 10.1088/2041-8205/728/1/L2 contributor: fullname: Stark – volume: 647 start-page: 970 year: 2006 ident: apjaa8809bib26 publication-title: ApJ doi: 10.1086/505573 contributor: fullname: Lee – volume: 428 start-page: 1366 year: 2013 ident: apjaa8809bib22 publication-title: MNRAS doi: 10.1093/mnras/sts116 contributor: fullname: Jensen – volume: 116 start-page: 133 year: 2004 ident: apjaa8809bib54 publication-title: PASP doi: 10.1086/382245 contributor: fullname: Lupton – year: 2016 ident: apjaa8809bib6 contributor: fullname: Chambers – volume: 50 start-page: 531 year: 2012 ident: apjaa8809bib25 publication-title: ARA&A doi: 10.1146/annurev-astro-081811-125610 contributor: fullname: Kennicutt – volume: 844 start-page: 171 year: 2017 ident: apjaa8809bib51 doi: 10.3847/1538-4357/aa7d4d contributor: fullname: Yang – volume: 671 start-page: 278 year: 2007 ident: apjaa8809bib11 publication-title: ApJ doi: 10.1086/522955 contributor: fullname: Gawiser – volume: 723 start-page: 869 year: 2010 ident: apjaa8809bib35 publication-title: ApJ doi: 10.1088/0004-637X/723/1/869 contributor: fullname: Ouchi – volume: 111 start-page: 63 year: 1999 ident: apjaa8809bib10 publication-title: PASP doi: 10.1086/316293 contributor: fullname: Fitzpatrick – volume: 806 start-page: 19 year: 2015 ident: apjaa8809bib8 publication-title: ApJ doi: 10.1088/0004-637X/806/1/19 contributor: fullname: Dressler – volume: 143 start-page: 145 year: 2012 ident: apjaa8809bib24 publication-title: AJ doi: 10.1088/0004-6256/143/6/145 contributor: fullname: Kellar – volume: 139 start-page: 279 year: 2010 ident: apjaa8809bib49 publication-title: AJ doi: 10.1088/0004-6256/139/1/279 contributor: fullname: Werk – volume: 819 start-page: 110 year: 2016 ident: apjaa8809bib40 publication-title: ApJ doi: 10.3847/0004-637X/819/2/110 contributor: fullname: Sánchez Almeida – volume: 123 start-page: 3 year: 1999 ident: apjaa8809bib28 publication-title: ApJS doi: 10.1086/313233 contributor: fullname: Leitherer – volume: 791 start-page: L19 year: 2014 ident: apjaa8809bib21 publication-title: ApJL doi: 10.1088/2041-8205/791/2/L19 contributor: fullname: Jaskot – volume: 667 start-page: 49 year: 2007 ident: apjaa8809bib37 publication-title: ApJ doi: 10.1086/519485 contributor: fullname: Pirzkal – volume: 451 start-page: 400 year: 2015 ident: apjaa8809bib32 publication-title: MNRAS doi: 10.1093/mnras/stv947 contributor: fullname: Matthee |
SSID | ssj0004299 |
Score | 2.6234283 |
Snippet | Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly emitting galaxies. These... Abstract Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Ly α emitting... Searching for extreme emission line galaxies allows us to find low-mass metal-poor galaxies that are good analogs of high redshift Lyα emitting galaxies. These... |
SourceID | osti proquest crossref iop |
SourceType | Open Access Repository Aggregation Database Publisher |
StartPage | 38 |
SubjectTerms | Analogs Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Blueberries Broadband Contaminants Dwarf galaxies EMISSION Emission lines GALAXIES galaxies: dwarf galaxies: high-redshift galaxies: ISM galaxies: star formation galaxies: starburst IONIZATION LYMAN LINES MASS METALLICITY Photometry RED SHIFT regions SPECTRA Spectroscopy Spectrum analysis STAR EVOLUTION Starburst galaxies STARS Stars & galaxies |
Title | Blueberry Galaxies: The Lowest Mass Young Starbursts |
URI | https://iopscience.iop.org/article/10.3847/1538-4357/aa8809 https://www.proquest.com/docview/2365780311 https://www.osti.gov/biblio/22875776 |
Volume | 847 |
hasFullText | 1 |
inHoldings | 1 |
isFullTextHit | |
isPrint | |
link | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwjV3NS8MwFH9sE8GL6FTmJzmo4KGuTdJk05OKnzj1oLhbSZPspKusFfS_9722U0QRb4G0SfnlffzeS_IKsK20xfBG2gC7bZm6CVLvRcCNs0YLG3tNF4UHN-riQV4N42EDDj_vwmQvtenfx2ZVKLiCkPRboC3tljqKXl53jUHp6zdhRtBuGQrzrXj8uhTJ-zX3lYESeljtUf46wjef1MR50T5nqGE_7HPpdM4WYL5mi-yo-rZFaPhxGzpHOeWvs-d3tsvKdpWeyNswe1e1lkAeP70icpPJOzs3T-YNA-IDhjLBrjMqjsAGSJpZqeoM-SZBmxf5Mjycnd6fXAT1HxICK6UsAk0Ouh96y0cRLYYyqI8O8XVWOMmdRvZhjXW8F46k9hEd6kzD1KvYS-QNSqxAa5yNfQdYLCMMhuNUu9hJLSLDlXWhxbdGcWp6chX2phglL1UhjAQDCMIzITwTwjOp8FyFHQQxqbUh_-O5DYI5wRWnirWWjvbYIuGcquxrhd1T-L_G4kKhkUFTFK39c5Z1mOPki2krKdyAVjF59ZvIJIp0C5qXt3dbpdx8AIkHv74 |
link.rule.ids | 230,315,783,787,888,27936,27937,38877,38902,53854,53880 |
linkProvider | IOP Publishing |
linkToPdf | http://utb.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3NT9swFH8anZh22QYMFcaGDwNph7SJ49jtbuyjwPjqAaTejGO7l0FTNak09tfvvTgVAiaExM2KHTt5P7_n3_PHM8BnqSy6N8JGmG3rqZso9z6NuHHWqNRmXtFB4ZNTeXAhfo2yUXPPaX0Wppg2pr-DyRAoOIiQ9DtFW9qtdRRHedU1Bntfvzt14yV4iU8zCp5_eDa8PRjJ-w3_FZFM1SisU_63ljvj0hK2jTa6QC17YKPrgWfwFi4Xnxz2m_zuzKu8Y__ei-b4jH96B28aUsr2QvEVeOEnq9DeK2mavLi-YbusTodZkHIVlochtQbi29UcAZrNbti-uTJ_0O_-yrDrseOCYjCwE-TmrLYoDGktIVhW5Xu4GPw8_34QNRcxRFYIUUWKeEA_9paPE8JcGlR7hzA6mzrBnUKSY411vBePhfIJ7R3N49zLzAukJzJdh9akmPg2sEwk6HNnuXKZEypNDJfWxRbfGme56YkN-LKAQU9DvA2NfgoJSZOQNAlJByFtwA7KUzdKVz5SbouQ1AgCBca1tIPIVppzCuavJGYvEL6ti6cSbRlavGTzia1sw6vhj4E-Pjw9-gCvOY3-tHgVb0Grms39R-QuVf6p7p__ALrz4zU |
openUrl | ctx_ver=Z39.88-2004&ctx_enc=info%3Aofi%2Fenc%3AUTF-8&rfr_id=info%3Asid%2Fsummon.serialssolutions.com&rft_val_fmt=info%3Aofi%2Ffmt%3Akev%3Amtx%3Ajournal&rft.genre=article&rft.atitle=Blueberry+Galaxies%3A+The+Lowest+Mass+Young+Starbursts&rft.jtitle=The+Astrophysical+journal&rft.au=Yang%2C+Huan&rft.au=Wang%2C+Junxian&rft.au=Malhotra%2C+Sangeeta&rft.au=Rhoads%2C+James+E.&rft.date=2017-09-20&rft.issn=0004-637X&rft.eissn=1538-4357&rft.volume=847&rft.issue=1&rft_id=info:doi/10.3847%2F1538-4357%2Faa8809&rft.externalDocID=22875776 |
thumbnail_l | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/lc.gif&issn=0004-637X&client=summon |
thumbnail_m | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/mc.gif&issn=0004-637X&client=summon |
thumbnail_s | http://covers-cdn.summon.serialssolutions.com/index.aspx?isbn=/sc.gif&issn=0004-637X&client=summon |