Physical Properties of Hyperluminous, Dust-obscured Quasars at z ∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by ALMA

We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompos...

Celý popis

Uložené v:
Podrobná bibliografia
Vydané v:The Astrophysical journal Ročník 964; číslo 1; s. 95 - 110
Hlavní autori: Sun, Weibin, Fan, Lulu, Han, Yunkun, Knudsen, Kirsten K., Chen, Guangwen, Zhang, Hong-Xin
Médium: Journal Article
Jazyk:English
Vydavateľské údaje: Philadelphia The American Astronomical Society 01.03.2024
IOP Publishing
Predmet:
Active galactic nuclei
Active galaxies
Black holes
Cold gas
Cosmic dust
Depletion
Dust
Galaxies
High-redshift galaxies
Infrared astronomy
Median (statistics)
Molecular gases
Physical properties
Quasars
Radio telescopes
Samples (statistical)
Spectral energy distribution
Star & galaxy formation
Star formation
Starburst galaxies
Stellar mass
ISSN:0004-637X, 1538-4357, 1538-4357
On-line prístup:Získať plný text
Tagy: Pridať tag
Žiadne tagy, Buďte prvý, kto otaguje tento záznam!
Abstract We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompose the SEDs into three components: stellar, cold dust, and active galactic nucleus (AGN). By doing so, we are able to derive and analyze the relevant properties of each component. We determine the molecular gas mass from CO line emission based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. By including ALMA observations in the multiwavelength SED analysis, we derive the molecular gas fractions, gas depletion timescales, and star formation efficiencies (SFEs). Their sample median and 16th–84th quartile ranges are f gas ∼ 0.33 − 0.17 + 0.33 , t depl ∼ 39 − 28 + 85 Myr, and SFE ∼ 297 − 195 + 659 K km s −1 pc −2 , respectively. Compared to main-sequence galaxies, they have lower molecular gas content and higher SFEs, similar to quasars in the literature. This suggests that the gas in these quasars is rapidly depleted, likely as the result of intense starburst activity and AGN feedback. The observed correlations between these properties and the AGN luminosities further support this scenario. Additionally, we infer the black hole to stellar mass ratio and black hole mass growth rate, which indicate significant central black hole mass assembly over short timescales. Our results are consistent with the scenario that our sample represents a short transition phase toward unobscured quasars.
AbstractList We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompose the SEDs into three components: stellar, cold dust, and active galactic nucleus (AGN). By doing so, we are able to derive and analyze the relevant properties of each component. We determine the molecular gas mass from CO line emission based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. By including ALMA observations in the multiwavelength SED analysis, we derive the molecular gas fractions, gas depletion timescales, and star formation efficiencies (SFEs). Their sample median and 16th–84th quartile ranges are f gas ∼ 0.33 − 0.17 + 0.33 , t depl ∼ 39 − 28 + 85 Myr, and SFE ∼ 297 − 195 + 659 K km s −1 pc −2 , respectively. Compared to main-sequence galaxies, they have lower molecular gas content and higher SFEs, similar to quasars in the literature. This suggests that the gas in these quasars is rapidly depleted, likely as the result of intense starburst activity and AGN feedback. The observed correlations between these properties and the AGN luminosities further support this scenario. Additionally, we infer the black hole to stellar mass ratio and black hole mass growth rate, which indicate significant central black hole mass assembly over short timescales. Our results are consistent with the scenario that our sample represents a short transition phase toward unobscured quasars.
We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompose the SEDs into three components: stellar, cold dust, and active galactic nucleus (AGN). By doing so, we are able to derive and analyze the relevant properties of each component. We determine the molecular gas mass from CO line emission based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. By including ALMA observations in the multiwavelength SED analysis, we derive the molecular gas fractions, gas depletion timescales, and star formation efficiencies (SFEs). Their sample median and 16th–84th quartile ranges are ${f}_{\mathrm{gas}}\,\sim \,{0.33}_{-0.17}^{+0.33}$ , t _depl ∼ ${39}_{-28}^{+85}$ Myr, and SFE ∼ ${297}_{-195}^{+659}$ K km s ^−1 pc ^−2 , respectively. Compared to main-sequence galaxies, they have lower molecular gas content and higher SFEs, similar to quasars in the literature. This suggests that the gas in these quasars is rapidly depleted, likely as the result of intense starburst activity and AGN feedback. The observed correlations between these properties and the AGN luminosities further support this scenario. Additionally, we infer the black hole to stellar mass ratio and black hole mass growth rate, which indicate significant central black hole mass assembly over short timescales. Our results are consistent with the scenario that our sample represents a short transition phase toward unobscured quasars.
We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompose the SEDs into three components: stellar, cold dust, and active galactic nucleus (AGN). By doing so, we are able to derive and analyze the relevant properties of each component. We determine the molecular gas mass from CO line emission based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. By including ALMA observations in the multiwavelength SED analysis, we derive the molecular gas fractions, gas depletion timescales, and star formation efficiencies (SFEs). Their sample median and 16th-84th quartile ranges are f gas ∼ 0.33 − 0.17 + 0.33 , t depl ∼ 39 − 28 + 85 Myr, and SFE ∼ 297 − 195 + 659 K km s−1 pc−2, respectively. Compared to main-sequence galaxies, they have lower molecular gas content and higher SFEs, similar to quasars in the literature. This suggests that the gas in these quasars is rapidly depleted, likely as the result of intense starburst activity and AGN feedback. The observed correlations between these properties and the AGN luminosities further support this scenario. Additionally, we infer the black hole to stellar mass ratio and black hole mass growth rate, which indicate significant central black hole mass assembly over short timescales. Our results are consistent with the scenario that our sample represents a short transition phase toward unobscured quasars.
We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field Infrared Survey Explorer. We aim to investigate the physical properties of these quasars, with a focus on their molecular gas content. We decompose the SEDs into three components: stellar, cold dust, and active galactic nucleus (AGN). By doing so, we are able to derive and analyze the relevant properties of each component. We determine the molecular gas mass from CO line emission based on Atacama Large Millimeter/submillimeter Array (ALMA) observations. By including ALMA observations in the multiwavelength SED analysis, we derive the molecular gas fractions, gas depletion timescales, and star formation efficiencies (SFEs). Their sample median and 16th–84th quartile ranges are fgas∼0.33−0.17+0.33, tdepl ∼ 39−28+85 Myr, and SFE ∼ 297−195+659 K km s−1 pc−2, respectively. Compared to main-sequence galaxies, they have lower molecular gas content and higher SFEs, similar to quasars in the literature. This suggests that the gas in these quasars is rapidly depleted, likely as the result of intense starburst activity and AGN feedback. The observed correlations between these properties and the AGN luminosities further support this scenario. Additionally, we infer the black hole to stellar mass ratio and black hole mass growth rate, which indicate significant central black hole mass assembly over short timescales. Our results are consistent with the scenario that our sample represents a short transition phase toward unobscured quasars.
Author Sun, Weibin
Fan, Lulu
Knudsen, Kirsten K.
Chen, Guangwen
Han, Yunkun
Zhang, Hong-Xin
Author_xml – sequence: 1
  givenname: Weibin
  orcidid: 0009-0004-7885-5882
  surname: Sun
  fullname: Sun, Weibin
  organization: University of Science and Technology of China School of Astronomy and Space Science, Hefei 230026, People's Republic of China
– sequence: 2
  givenname: Lulu
  orcidid: 0000-0003-4200-4432
  surname: Fan
  fullname: Fan, Lulu
  organization: Deep Space Exploration Laboratory , Hefei 230088, People's Republic of China
– sequence: 3
  givenname: Yunkun
  orcidid: 0000-0002-2547-0434
  surname: Han
  fullname: Han, Yunkun
  organization: Chinese Academy of Sciences Key Laboratory for the Structure and Evolution of Celestial Objects, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China
– sequence: 4
  givenname: Kirsten K.
  orcidid: 0000-0002-7821-8873
  surname: Knudsen
  fullname: Knudsen, Kirsten K.
  organization: Chalmers University of Technology Department of Space, Earth and Environment, Onsala Space Observatory, SE-439 92 Onsala, Sweden
– sequence: 5
  givenname: Guangwen
  orcidid: 0000-0002-4742-8800
  surname: Chen
  fullname: Chen, Guangwen
  organization: University of Science and Technology of China School of Astronomy and Space Science, Hefei 230026, People's Republic of China
– sequence: 6
  givenname: Hong-Xin
  orcidid: 0000-0003-1632-2541
  surname: Zhang
  fullname: Zhang, Hong-Xin
  organization: University of Science and Technology of China School of Astronomy and Space Science, Hefei 230026, People's Republic of China
BackLink https://research.chalmers.se/publication/542227$$DView record from Swedish Publication Index (Chalmers tekniska högskola)
BookMark eNp9ks9u1DAQxiNUJLaFO0dLXBvqxI6dcFu1pa20FYWCxM1y7MmuV9442E6r5Ql4D16Dp-FJcAh_BBL4Yo8185vx5-8wO-hdD1n2tMDPSU35SVGROqek4idSlyWQB9ni19VBtsAY05wR_v5RdhjCdgrLpllkn282-2CUtOjGuwF8NBCQ69DlPgV23JnejeEYnY0h5q4NavSg0etRBukDkhF9RF8_fUHkBboebTT38g4s9Ou4QbcDqOgT97wHv96jMxOiN-0YjevRspc2tU2EXqNTZzW6kCEd-gh9RG_gDqRNfdo9Wq6ul4-zh520AZ782I-ydy_P355e5qtXF1eny1WuaFPGvKIdaaQuVFcVte5aqnSpcQGF5pSxruYtI53iGCdZtGq55pWqAIqOMM1wQ8hRdjVztZNbMXizk34vnDTi-4XzayGTQMqCYHUhodGctITQhlQNYYDLGhihkrZcJdbtzAr3MIztHzQPAaRXG6E20u7ABxEmIpMdV4WoqpoJmmYU6S1cNLLAQNsOK5ioz2bq4N2HEUIUWzf6JGYQZcNLTtOqUhabs5R3IXjohDJRTsKnDzFWFFhMlhGTP8TkDzFbJhXivwp_jv2fkuO5xLjh9zD_TP8GqvvWaQ
CitedBy_id crossref_primary_10_3847_1538_4357_adabe3
crossref_primary_10_3847_1538_4357_ad65da
crossref_primary_10_3847_1538_4357_addecf
crossref_primary_10_3847_1538_4357_ad968b
crossref_primary_10_3847_1538_4357_addbdd
crossref_primary_10_3847_1538_4357_ad5317
crossref_primary_10_1051_0004_6361_202453214
crossref_primary_10_3847_1538_4357_ad9aa3
crossref_primary_10_1093_mnras_staf769
crossref_primary_10_3847_1538_4357_adc9b5
Cites_doi 10.1088/0004-637X/794/2/102
10.3847/1538-4357/ac77fc
10.1093/mnras/stu1248
10.3847/1538-4357/ab9814
10.1051/0004-6361/201731641
10.1086/524362
10.1088/0067-0049/214/2/15
10.1088/0004-637X/793/1/19
10.1086/511055
10.1038/nature01792
10.3847/1538-4365/acfc3a
10.1051/0004-6361/202141075
10.1088/0004-6256/147/5/108
10.1086/173427
10.1051/0004-6361/201731387
10.1093/mnras/stad1464
10.1146/annurev-astro-081913-035722
10.1111/j.1365-2966.2011.19827.x
10.1051/0004-6361/201425491
10.1051/0004-6361/201322081
10.1088/0067-0049/192/2/18
10.1093/mnras/stx726
10.1111/j.1365-2966.2011.20286.x
10.1146/annurev-astro-081811-125521
10.1146/annurev-astro-081817-051803
10.1088/0004-637X/756/1/96
10.1093/mnras/stad589
10.1093/mnras/stw3019
10.1088/0067-0049/215/1/2
10.1051/0004-6361/202141219
10.3847/1538-4357/835/1/105
10.1146/annurev.astro.43.051804.102221
10.1146/annurev-astro-082812-140944
10.1088/0004-637X/793/1/8
10.1051/0004-6361/202040258
10.1051/0004-6361/201526034
10.1126/science.aap7605
10.1146/annurev.astro.41.011802.094840
10.3847/1538-4357/ac4971
10.1086/170020
10.1146/annurev-astro-081710-102542
10.3847/1538-4365/aae9f0
10.1146/annurev-astro-082214-122302
10.1093/mnras/stz2134
10.1051/0004-6361/201526105
10.1093/mnras/stv214
10.1088/0004-637X/803/2/57
10.1086/590483
10.1146/annurev-astro-082812-140953
10.1111/j.1365-2966.2006.09866.x
10.1051/0004-6361/201323310
10.1126/science.aaa4506
10.3847/2041-8213/acc58d
10.1086/518306
10.1146/annurev.astro.36.1.189
10.1086/300353
10.3847/1538-4357/ab01fb
10.3847/1538-3881/aa894e
10.1086/376392
10.1093/mnras/sty3449
10.1038/s41467-022-32297-x
10.1093/mnras/219.2.305
10.3847/0004-637X/820/1/46
10.1088/0004-6256/140/6/1868
10.1086/165983
10.3847/1538-4357/abc3bf
10.1146/annurev-astro-082708-101811
10.1086/590482
10.1051/0004-6361/201014519
10.1051/0004-6361/201730762
10.3847/1538-4357/ace25b
10.1051/0004-6361/201629478
10.1051/0004-6361/202346695
10.1051/0004-6361/202039057
10.1146/annurev-astro-082812-141017
10.1046/j.1365-8711.2002.05660.x
10.1111/j.1365-2966.2006.10228.x
10.1093/mnras/stx1141
10.1051/0004-6361/201833943
10.1086/177353
10.1007/s11214-005-3947-6
10.3847/2041-8213/aa6838
10.1051/0004-6361/200912676
10.1051/0004-6361/201935524
10.1051/0004-6361/201731052
10.3847/1538-4357/aa9ff3
10.1051/0004-6361/201220859
10.1088/0004-637X/804/1/27
10.1093/mnras/sts562
10.1051/0004-6361/201833040
10.1093/mnras/stx3120
10.3847/1538-4357/aaaaae
10.1051/0004-6361/201425324
10.1046/j.1365-8711.2003.06897.x
10.1088/0004-637X/755/2/173
10.1088/0004-637X/749/2/123
10.1051/0004-6361/201014759
10.3847/0004-637X/819/2/111
10.1088/0004-637X/805/2/90
10.1111/j.1365-2966.2008.13535.x
10.1051/0004-6361/201321716
10.1088/1538-3873/aa8e91
10.1111/j.1365-2966.2010.16969.x
10.3847/1538-4357/ab3e4f
10.3847/2041-8205/822/2/L32
10.1051/0004-6361/201732557
10.3847/1538-4365/aaeffa
10.1051/0004-6361/201834918
10.3847/1538-4357/aba8a1
10.3847/2041-8213/aab496
10.1051/0004-6361:200810628
10.3847/1538-4357/ab5e7b
10.3847/2041-8205/816/1/L6
10.1093/mnras/stu1157
10.1146/annurev-astro-082812-140951
10.3847/1538-4357/ab5059
10.1051/0004-6361/202038889
10.1088/0004-637X/708/1/137
10.3847/1538-4357/aae698
10.3847/1538-4357/aae075
10.1051/0004-6361/201014535
10.1051/0004-6361/201834156
10.1088/2041-8205/806/2/L25
10.1086/308692
10.1093/mnras/stw444
10.3847/1538-3881/ab089d
10.1051/0004-6361/201322803
10.1051/0004-6361/201118312
10.1051/0004-6361/202245168
10.3847/1538-4357/836/1/66
10.3847/0004-637X/823/2/107
10.1051/0004-6361/202140455
10.1093/mnras/stw289
10.1093/mnras/sty3128
10.1093/mnras/staa1959
10.1038/s41550-017-0232-z
10.1093/mnras/staa1582
10.1051/0004-6361/201936817
10.1111/j.1365-2966.2012.21512.x
10.3847/1538-4357/ac8162
10.3847/1538-4365/ab48e8
ContentType Journal Article
Copyright 2024. The Author(s). Published by the American Astronomical Society.
2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
Copyright_xml – notice: 2024. The Author(s). Published by the American Astronomical Society.
– notice: 2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
DBID O3W
TSCCA
AAYXX
CITATION
7TG
8FD
H8D
KL.
L7M
ABBSD
ADTPV
AOWAS
D8T
F1S
ZZAVC
DOA
DOI 10.3847/1538-4357/ad22e3
DatabaseName Institute of Physics Open Access Journal Titles
IOPscience (Open Access)
CrossRef
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Aerospace Database
Meteorological & Geoastrophysical Abstracts - Academic
Advanced Technologies Database with Aerospace
SWEPUB Chalmers tekniska högskola full text
SwePub
SwePub Articles
SWEPUB Freely available online
SWEPUB Chalmers tekniska högskola
SwePub Articles full text
Directory of Open Access Journals
DatabaseTitle CrossRef
Aerospace Database
Meteorological & Geoastrophysical Abstracts
Technology Research Database
Advanced Technologies Database with Aerospace
Meteorological & Geoastrophysical Abstracts - Academic
DatabaseTitleList CrossRef


Aerospace Database
Database_xml – sequence: 1
  dbid: DOA
  name: Directory of Open Access Journals
  url: https://www.doaj.org/
  sourceTypes: Open Website
– sequence: 2
  dbid: O3W
  name: Institute of Physics Journals Open Access
  url: http://iopscience.iop.org/
  sourceTypes: Publisher
DeliveryMethod fulltext_linktorsrc
Discipline Astronomy & Astrophysics
Physics
EISSN 1538-4357
ExternalDocumentID oai_doaj_org_article_681ae9d73b334935936e028e634a4b7c
oai_research_chalmers_se_686af7c1_5586_4538_ad17_9a10e4bf0cec
10_3847_1538_4357_ad22e3
apjad22e3
GrantInformation_xml – fundername: MOE ∣ Fundamental Research Funds for the Central Universities (Fundamental Research Fund for the Central Universities)
  grantid: WK3440000006
  funderid: https://doi.org/10.13039/501100012226
– fundername: MOST ∣ National Natural Science Foundation of China (NSFC)
  grantid: 12173037
  funderid: https://doi.org/10.13039/501100001809
– fundername: MOST ∣ National Natural Science Foundation of China (NSFC)
  grantid: 12233008
  funderid: https://doi.org/10.13039/501100001809
– fundername: MOST ∣ National Natural Science Foundation of China (NSFC)
  grantid: 11773063
  funderid: https://doi.org/10.13039/501100001809
– fundername: MOST | National Key Research and Development Program of China
  grantid: 2023YFA1608100
GroupedDBID -DZ
-~X
123
1JI
23N
2FS
4.4
6J9
85S
AAFWJ
AAGCD
AAJIO
ABHWH
ACBEA
ACGFS
ACHIP
ACNCT
ADACN
AEFHF
AENEX
AFPKN
AKPSB
ALMA_UNASSIGNED_HOLDINGS
ASPBG
ATQHT
AVWKF
AZFZN
CJUJL
CRLBU
CS3
EBS
F5P
FRP
GROUPED_DOAJ
IJHAN
IOP
KOT
M~E
N5L
O3W
O43
OK1
PJBAE
RIN
RNS
ROL
SJN
SY9
T37
TN5
TR2
TSCCA
WH7
XSW
AAYXX
AEINN
CITATION
7TG
8FD
H8D
KL.
L7M
2WC
41~
6TJ
6TS
9M8
AALHV
ABBSD
ABDPE
ADIYS
ADTPV
ADXHL
AETEA
AI.
AOWAS
D8T
EJD
F1S
FA8
MVM
OHT
VH1
WHG
YYP
ZCG
ZKB
ZY4
ZZAVC
ID FETCH-LOGICAL-c492t-54f39ad1cf518dfb4cd2d01e1d7466f87b63fc700538dcb7d75c5ee1f36d60933
IEDL.DBID O3W
ISICitedReferencesCount 10
ISICitedReferencesURI http://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=Summon&SrcAuth=ProQuest&DestLinkType=CitingArticles&DestApp=WOS_CPL&KeyUT=001188035200001&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
ISSN 0004-637X
1538-4357
IngestDate Fri Oct 03 12:44:21 EDT 2025
Wed Nov 05 04:10:10 EST 2025
Wed Aug 13 11:20:01 EDT 2025
Sat Nov 29 05:44:10 EST 2025
Tue Nov 18 22:34:20 EST 2025
Sun Aug 18 16:10:26 EDT 2024
IsDoiOpenAccess true
IsOpenAccess true
IsPeerReviewed true
IsScholarly true
Issue 1
Language English
License Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
LinkModel DirectLink
MergedId FETCHMERGED-LOGICAL-c492t-54f39ad1cf518dfb4cd2d01e1d7466f87b63fc700538dcb7d75c5ee1f36d60933
Notes Galaxies and Cosmology
AAS50306
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 14
ORCID 0009-0004-7885-5882
0000-0002-4742-8800
0000-0003-1632-2541
0000-0002-7821-8873
0000-0003-4200-4432
0000-0002-2547-0434
OpenAccessLink https://iopscience.iop.org/article/10.3847/1538-4357/ad22e3
PQID 2972744445
PQPubID 4562441
PageCount 16
ParticipantIDs iop_journals_10_3847_1538_4357_ad22e3
swepub_primary_oai_research_chalmers_se_686af7c1_5586_4538_ad17_9a10e4bf0cec
crossref_citationtrail_10_3847_1538_4357_ad22e3
crossref_primary_10_3847_1538_4357_ad22e3
proquest_journals_2972744445
doaj_primary_oai_doaj_org_article_681ae9d73b334935936e028e634a4b7c
PublicationCentury 2000
PublicationDate 2024-03-01
PublicationDateYYYYMMDD 2024-03-01
PublicationDate_xml – month: 03
  year: 2024
  text: 2024-03-01
  day: 01
PublicationDecade 2020
PublicationPlace Philadelphia
PublicationPlace_xml – name: Philadelphia
PublicationTitle The Astrophysical journal
PublicationTitleAbbrev APJ
PublicationTitleAlternate Astrophys. J
PublicationYear 2024
Publisher The American Astronomical Society
IOP Publishing
Publisher_xml – name: The American Astronomical Society
– name: IOP Publishing
References Targett (apjad22e3bib131) 2012; 420
Wright (apjad22e3bib140) 2010; 140
Genzel (apjad22e3bib54) 2010; 407
Jones (apjad22e3bib71) 2004
Kakkad (apjad22e3bib76) 2017; 468
Draine (apjad22e3bib31) 2007; 663
Assef (apjad22e3bib4) 2022; 934
Ichikawa (apjad22e3bib68) 2015; 803
Díaz-Santos (apjad22e3bib29) 2021; 654
Buat (apjad22e3bib19) 2014; 561
Sargent (apjad22e3bib115) 2014; 793
Lang (apjad22e3bib81) 2014; 147
Fan (apjad22e3bib41) 2016a; 822
Fritz (apjad22e3bib52) 2006; 366
Bongiorno (apjad22e3bib13) 2014; 443
Jones (apjad22e3bib74) 2014; 443
Han (apjad22e3bib61) 2019; 240
Luo (apjad22e3bib85) 2022; 935
Magorrian (apjad22e3bib88) 1998; 115
Conroy (apjad22e3bib23) 2013; 51
Weymann (apjad22e3bib139) 1991; 373
Penney (apjad22e3bib103) 2019; 483
Berta (apjad22e3bib9) 2013; 551
Fan (apjad22e3bib40) 2018; 854
Bruzual (apjad22e3bib18) 2003; 344
Hopkins (apjad22e3bib66) 2008; 175
Alonso-Herrero (apjad22e3bib2) 2021; 652
Assef (apjad22e3bib5) 2020; 897
Fabian (apjad22e3bib39) 2012; 50
Meisner (apjad22e3bib93) 2017; 154
Díaz-Santos (apjad22e3bib27) 2016; 816
Siebenmorgen (apjad22e3bib120) 2015; 583
Kennicutt (apjad22e3bib77) 1998; 36
Hönig (apjad22e3bib65) 2017; 838
Fan (apjad22e3bib45) 2019; 887
Hickox (apjad22e3bib63) 2018; 56
Roseboom (apjad22e3bib113) 2012; 419
Sokol (apjad22e3bib123) 2023; 521
Solomon (apjad22e3bib124) 2005; 43
Marasco (apjad22e3bib89) 2020; 644
Han (apjad22e3bib59) 2012; 749
Han (apjad22e3bib58) 2023; 269
Dey (apjad22e3bib26) 2019; 157
Díaz-Santos (apjad22e3bib28) 2018; 362
Brusa (apjad22e3bib16) 2018; 612
Fan (apjad22e3bib44) 2018; 856
Calzetti (apjad22e3bib20) 2000; 533
Trakhtenbrot (apjad22e3bib133) 2015; 349
Han (apjad22e3bib60) 2014; 215
Brusa (apjad22e3bib17) 2015; 578
Sanders (apjad22e3bib114) 1988; 325
Zou (apjad22e3bib147) 2019; 245
Stalevski (apjad22e3bib128) 2016; 458
Zewdie (apjad22e3bib146) 2023; 677
Shangguan (apjad22e3bib118) 2020; 899
Stern (apjad22e3bib129) 2014; 794
Fluetsch (apjad22e3bib51) 2019; 483
Wu (apjad22e3bib142) 2018; 852
Bischetti (apjad22e3bib11) 2019; 628
Toba (apjad22e3bib132) 2016; 820
McLure (apjad22e3bib91) 2006; 368
Boquien (apjad22e3bib14) 2019; 622
Jenkins (apjad22e3bib70) 2004
Lyu (apjad22e3bib86) 2018; 866
Duras (apjad22e3bib36) 2020; 636
McMullin (apjad22e3bib92) 2007; 376
Ricci (apjad22e3bib112) 2017; 835
Rémy-Ruyer (apjad22e3bib111) 2014; 563
Schneider (apjad22e3bib116) 2015; 579
Eisenhardt (apjad22e3bib38) 2012; 755
Fan (apjad22e3bib43) 2017; 129
García-Burillo (apjad22e3bib53) 2021; 652
Bolatto (apjad22e3bib12) 2013; 51
Fiore (apjad22e3bib50) 2017; 601
Perna (apjad22e3bib104) 2018; 619
Chabrier (apjad22e3bib22) 2003; 115
Matsuoka (apjad22e3bib90) 2018; 620
Banerji (apjad22e3bib8) 2017; 465
Sommovigo (apjad22e3bib126) 2020; 497
Jun (apjad22e3bib75) 2020; 888
Piconcelli (apjad22e3bib105) 2015; 574
Penney (apjad22e3bib102) 2020; 496
Ossenkopf (apjad22e3bib101) 1992; 261
Feruglio (apjad22e3bib48) 2017; 608
Shapley (apjad22e3bib119) 2011; 49
Nenkova (apjad22e3bib97) 2008a; 685
Finnerty (apjad22e3bib49) 2020; 905
Pilbratt (apjad22e3bib107) 2010; 518
Draine (apjad22e3bib30) 2003; 41
Netzer (apjad22e3bib99) 2015; 53
Draine (apjad22e3bib32) 2007; 657
Speagle (apjad22e3bib127) 2014; 214
Somerville (apjad22e3bib125) 2015; 53
Pozzi (apjad22e3bib109) 2021; 653
Ferrarese (apjad22e3bib47) 2005; 116
Assef (apjad22e3bib6) 2015; 804
da Cunha (apjad22e3bib25) 2008; 388
Hopkins (apjad22e3bib67) 2016; 458
Nenkova (apjad22e3bib98) 2008b; 685
Scoville (apjad22e3bib117) 2017; 836
Assef (apjad22e3bib7) 2016; 819
Liang (apjad22e3bib83) 2019; 489
Tsai (apjad22e3bib136) 2015; 805
Aravena (apjad22e3bib3) 2008; 491
Ginolfi (apjad22e3bib55) 2022; 13
Griffin (apjad22e3bib57) 2010; 518
González-Martín (apjad22e3bib56) 2019; 884
Ramos Almeida (apjad22e3bib110) 2017; 1
Poglitsch (apjad22e3bib108) 2010; 518
Dunne (apjad22e3bib34) 2003; 424
Kormendy (apjad22e3bib79) 2013; 51
Siebenmorgen (apjad22e3bib121) 2014; 561
Merloni (apjad22e3bib94) 2010; 708
Duras (apjad22e3bib35) 2017; 604
James (apjad22e3bib69) 2002; 335
Tsukui (apjad22e3bib137) 2023; 523
Drouart (apjad22e3bib33) 2014; 566
Noguchi (apjad22e3bib100) 1986; 219
Heckman (apjad22e3bib62) 2014; 52
Hönig (apjad22e3bib64) 2010; 523
Jones (apjad22e3bib72) 2017; 469
Bischetti (apjad22e3bib10) 2021; 645
Wu (apjad22e3bib141) 2014; 793
Yang (apjad22e3bib144) 2022; 927
Mihos (apjad22e3bib96) 1996; 464
Suh (apjad22e3bib130) 2019; 872
Zappacosta (apjad22e3bib145) 2018; 618
Magnelli (apjad22e3bib87) 2012; 539
Edge (apjad22e3bib37) 2013; 154
Tsai (apjad22e3bib135) 2018; 868
Carilli (apjad22e3bib21) 2013; 51
Cutri (apjad22e3bib24) 2013; II/328
Vito (apjad22e3bib138) 2018; 474
Miettinen (apjad22e3bib95) 2017; 606
Komatsu (apjad22e3bib78) 2011; 192
Abbott (apjad22e3bib1) 2018; 239
Wu (apjad22e3bib143) 2012; 756
López (apjad22e3bib84) 2023; 672
Fan (apjad22e3bib42) 2016b; 823
Faucher-Giguère (apjad22e3bib46) 2012; 425
Silva (apjad22e3bib122) 2015; 806
Pier (apjad22e3bib106) 1993; 418
Bothwell (apjad22e3bib15) 2013; 429
Kuijken (apjad22e3bib80) 2019; 625
Jones (apjad22e3bib73) 2015; 448
Li (apjad22e3bib82) 2023; 958
Tripodi (apjad22e3bib134) 2023; 946
References_xml – volume: 794
  start-page: 102
  year: 2014
  ident: apjad22e3bib129
  publication-title: ApJ
  doi: 10.1088/0004-637X/794/2/102
– volume: 934
  start-page: 101
  year: 2022
  ident: apjad22e3bib4
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac77fc
– volume: 443
  start-page: 2077
  year: 2014
  ident: apjad22e3bib13
  publication-title: MNRAS
  doi: 10.1093/mnras/stu1248
– volume: 897
  start-page: 112
  year: 2020
  ident: apjad22e3bib5
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab9814
– volume: 612
  start-page: A29
  year: 2018
  ident: apjad22e3bib16
  publication-title: A&A
  doi: 10.1051/0004-6361/201731641
– volume: 175
  start-page: 356
  year: 2008
  ident: apjad22e3bib66
  publication-title: ApJS
  doi: 10.1086/524362
– volume: 214
  start-page: 15
  year: 2014
  ident: apjad22e3bib127
  publication-title: ApJS
  doi: 10.1088/0067-0049/214/2/15
– volume: 793
  start-page: 19
  year: 2014
  ident: apjad22e3bib115
  publication-title: ApJ
  doi: 10.1088/0004-637X/793/1/19
– volume: 657
  start-page: 810
  year: 2007
  ident: apjad22e3bib32
  publication-title: ApJ
  doi: 10.1086/511055
– volume: 424
  start-page: 285
  year: 2003
  ident: apjad22e3bib34
  publication-title: Natur
  doi: 10.1038/nature01792
– volume: 269
  start-page: 39
  year: 2023
  ident: apjad22e3bib58
  publication-title: ApJS
  doi: 10.3847/1538-4365/acfc3a
– volume: 652
  start-page: A98
  year: 2021
  ident: apjad22e3bib53
  publication-title: A&A
  doi: 10.1051/0004-6361/202141075
– volume: 147
  start-page: 108
  year: 2014
  ident: apjad22e3bib81
  publication-title: AJ
  doi: 10.1088/0004-6256/147/5/108
– volume: 418
  start-page: 673
  year: 1993
  ident: apjad22e3bib106
  publication-title: ApJ
  doi: 10.1086/173427
– volume: 608
  start-page: A30
  year: 2017
  ident: apjad22e3bib48
  publication-title: A&A
  doi: 10.1051/0004-6361/201731387
– volume: 523
  start-page: 4654
  year: 2023
  ident: apjad22e3bib137
  publication-title: MNRAS
  doi: 10.1093/mnras/stad1464
– volume: 52
  start-page: 589
  year: 2014
  ident: apjad22e3bib62
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081913-035722
– volume: 419
  start-page: 2758
  year: 2012
  ident: apjad22e3bib113
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2011.19827.x
– volume: 578
  start-page: A11
  year: 2015
  ident: apjad22e3bib17
  publication-title: A&A
  doi: 10.1051/0004-6361/201425491
– volume: 561
  start-page: A39
  year: 2014
  ident: apjad22e3bib19
  publication-title: A&A
  doi: 10.1051/0004-6361/201322081
– volume: 192
  start-page: 18
  year: 2011
  ident: apjad22e3bib78
  publication-title: ApJS
  doi: 10.1088/0067-0049/192/2/18
– volume: 468
  start-page: 4205
  year: 2017
  ident: apjad22e3bib76
  publication-title: MNRAS
  doi: 10.1093/mnras/stx726
– volume: 420
  start-page: 3621
  year: 2012
  ident: apjad22e3bib131
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2011.20286.x
– volume: 50
  start-page: 455
  year: 2012
  ident: apjad22e3bib39
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081811-125521
– volume: 56
  start-page: 625
  year: 2018
  ident: apjad22e3bib63
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081817-051803
– volume: II/328
  year: 2013
  ident: apjad22e3bib24
  publication-title: yCat
– volume: 756
  start-page: 96
  year: 2012
  ident: apjad22e3bib143
  publication-title: ApJ
  doi: 10.1088/0004-637X/756/1/96
– volume: 521
  start-page: 818
  year: 2023
  ident: apjad22e3bib123
  publication-title: MNRAS
  doi: 10.1093/mnras/stad589
– volume: 465
  start-page: 4390
  year: 2017
  ident: apjad22e3bib8
  publication-title: MNRAS
  doi: 10.1093/mnras/stw3019
– volume: 215
  start-page: 2
  year: 2014
  ident: apjad22e3bib60
  publication-title: ApJS
  doi: 10.1088/0067-0049/215/1/2
– volume: 652
  start-page: A99
  year: 2021
  ident: apjad22e3bib2
  publication-title: A&A
  doi: 10.1051/0004-6361/202141219
– volume: 835
  start-page: 105
  year: 2017
  ident: apjad22e3bib112
  publication-title: ApJ
  doi: 10.3847/1538-4357/835/1/105
– volume: 43
  start-page: 677
  year: 2005
  ident: apjad22e3bib124
  publication-title: ARA&A
  doi: 10.1146/annurev.astro.43.051804.102221
– volume: 51
  start-page: 207
  year: 2013
  ident: apjad22e3bib12
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082812-140944
– volume: 793
  start-page: 8
  year: 2014
  ident: apjad22e3bib141
  publication-title: ApJ
  doi: 10.1088/0004-637X/793/1/8
– volume: 653
  start-page: A84
  year: 2021
  ident: apjad22e3bib109
  publication-title: A&A
  doi: 10.1051/0004-6361/202040258
– volume: 583
  start-page: A120
  year: 2015
  ident: apjad22e3bib120
  publication-title: A&A
  doi: 10.1051/0004-6361/201526034
– volume: 362
  start-page: 1034
  year: 2018
  ident: apjad22e3bib28
  publication-title: Sci
  doi: 10.1126/science.aap7605
– volume: 41
  start-page: 241
  year: 2003
  ident: apjad22e3bib30
  publication-title: ARA&A
  doi: 10.1146/annurev.astro.41.011802.094840
– volume: 927
  start-page: 192
  year: 2022
  ident: apjad22e3bib144
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac4971
– volume: 373
  start-page: 23
  year: 1991
  ident: apjad22e3bib139
  publication-title: ApJ
  doi: 10.1086/170020
– volume: 49
  start-page: 525
  year: 2011
  ident: apjad22e3bib119
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081710-102542
– volume: 239
  start-page: 18
  year: 2018
  ident: apjad22e3bib1
  publication-title: ApJS
  doi: 10.3847/1538-4365/aae9f0
– volume: 53
  start-page: 365
  year: 2015
  ident: apjad22e3bib99
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082214-122302
– volume: 489
  start-page: 1397
  year: 2019
  ident: apjad22e3bib83
  publication-title: MNRAS
  doi: 10.1093/mnras/stz2134
– volume: 579
  start-page: A60
  year: 2015
  ident: apjad22e3bib116
  publication-title: A&A
  doi: 10.1051/0004-6361/201526105
– volume: 448
  start-page: 3325
  year: 2015
  ident: apjad22e3bib73
  publication-title: MNRAS
  doi: 10.1093/mnras/stv214
– volume: 803
  start-page: 57
  year: 2015
  ident: apjad22e3bib68
  publication-title: ApJ
  doi: 10.1088/0004-637X/803/2/57
– volume: 685
  start-page: 160
  year: 2008b
  ident: apjad22e3bib98
  publication-title: ApJ
  doi: 10.1086/590483
– volume: 51
  start-page: 105
  year: 2013
  ident: apjad22e3bib21
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082812-140953
– volume: 366
  start-page: 767
  year: 2006
  ident: apjad22e3bib52
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2006.09866.x
– volume: 566
  start-page: A53
  year: 2014
  ident: apjad22e3bib33
  publication-title: A&A
  doi: 10.1051/0004-6361/201323310
– volume: 349
  start-page: 168
  year: 2015
  ident: apjad22e3bib133
  publication-title: Sci
  doi: 10.1126/science.aaa4506
– volume: 946
  start-page: L45
  year: 2023
  ident: apjad22e3bib134
  publication-title: ApJL
  doi: 10.3847/2041-8213/acc58d
– volume: 663
  start-page: 866
  year: 2007
  ident: apjad22e3bib31
  publication-title: ApJ
  doi: 10.1086/518306
– volume: 36
  start-page: 189
  year: 1998
  ident: apjad22e3bib77
  publication-title: ARA&A
  doi: 10.1146/annurev.astro.36.1.189
– volume: 115
  start-page: 2285
  year: 1998
  ident: apjad22e3bib88
  publication-title: AJ
  doi: 10.1086/300353
– volume: 872
  start-page: 168
  year: 2019
  ident: apjad22e3bib130
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab01fb
– volume: 154
  start-page: 161
  year: 2017
  ident: apjad22e3bib93
  publication-title: AJ
  doi: 10.3847/1538-3881/aa894e
– volume: 115
  start-page: 763
  year: 2003
  ident: apjad22e3bib22
  publication-title: PASP
  doi: 10.1086/376392
– volume: 483
  start-page: 4586
  year: 2019
  ident: apjad22e3bib51
  publication-title: MNRAS
  doi: 10.1093/mnras/sty3449
– volume: 13
  start-page: 4574
  year: 2022
  ident: apjad22e3bib55
  publication-title: NatCo
  doi: 10.1038/s41467-022-32297-x
– volume: 219
  start-page: 305
  year: 1986
  ident: apjad22e3bib100
  publication-title: MNRAS
  doi: 10.1093/mnras/219.2.305
– volume: 820
  start-page: 46
  year: 2016
  ident: apjad22e3bib132
  publication-title: ApJ
  doi: 10.3847/0004-637X/820/1/46
– start-page: 347
  year: 2004
  ident: apjad22e3bib71
– volume: 140
  start-page: 1868
  year: 2010
  ident: apjad22e3bib140
  publication-title: AJ
  doi: 10.1088/0004-6256/140/6/1868
– volume: 325
  start-page: 74
  year: 1988
  ident: apjad22e3bib114
  publication-title: ApJ
  doi: 10.1086/165983
– volume: 905
  start-page: 16
  year: 2020
  ident: apjad22e3bib49
  publication-title: ApJ
  doi: 10.3847/1538-4357/abc3bf
– volume: 51
  start-page: 511
  year: 2013
  ident: apjad22e3bib79
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082708-101811
– volume: 685
  start-page: 147
  year: 2008a
  ident: apjad22e3bib97
  publication-title: ApJ
  doi: 10.1086/590482
– volume: 518
  start-page: L3
  year: 2010
  ident: apjad22e3bib57
  publication-title: A&A
  doi: 10.1051/0004-6361/201014519
– volume: 606
  start-page: A17
  year: 2017
  ident: apjad22e3bib95
  publication-title: A&A
  doi: 10.1051/0004-6361/201730762
– volume: 958
  start-page: 162
  year: 2023
  ident: apjad22e3bib82
  publication-title: APJ
  doi: 10.3847/1538-4357/ace25b
– volume: 601
  start-page: A143
  year: 2017
  ident: apjad22e3bib50
  publication-title: A&A
  doi: 10.1051/0004-6361/201629478
– volume: 677
  start-page: A54
  year: 2023
  ident: apjad22e3bib146
  publication-title: A&A
  doi: 10.1051/0004-6361/202346695
– volume: 645
  start-page: A33
  year: 2021
  ident: apjad22e3bib10
  publication-title: A&A
  doi: 10.1051/0004-6361/202039057
– volume: 51
  start-page: 393
  year: 2013
  ident: apjad22e3bib23
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082812-141017
– volume: 335
  start-page: 753
  year: 2002
  ident: apjad22e3bib69
  publication-title: MNRAS
  doi: 10.1046/j.1365-8711.2002.05660.x
– volume: 368
  start-page: 1395
  year: 2006
  ident: apjad22e3bib91
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2006.10228.x
– volume: 469
  start-page: 4565
  year: 2017
  ident: apjad22e3bib72
  publication-title: MNRAS
  doi: 10.1093/mnras/stx1141
– volume: 620
  start-page: L3
  year: 2018
  ident: apjad22e3bib90
  publication-title: A&A
  doi: 10.1051/0004-6361/201833943
– volume: 464
  start-page: 641
  year: 1996
  ident: apjad22e3bib96
  publication-title: ApJ
  doi: 10.1086/177353
– volume: 116
  start-page: 523
  year: 2005
  ident: apjad22e3bib47
  publication-title: SSRv
  doi: 10.1007/s11214-005-3947-6
– volume: 838
  start-page: L20
  year: 2017
  ident: apjad22e3bib65
  publication-title: ApJL
  doi: 10.3847/2041-8213/aa6838
– volume: 523
  start-page: A27
  year: 2010
  ident: apjad22e3bib64
  publication-title: A&A
  doi: 10.1051/0004-6361/200912676
– volume: 628
  start-page: A118
  year: 2019
  ident: apjad22e3bib11
  publication-title: A&A
  doi: 10.1051/0004-6361/201935524
– volume: 604
  start-page: A67
  year: 2017
  ident: apjad22e3bib35
  publication-title: A&A
  doi: 10.1051/0004-6361/201731052
– volume: 852
  start-page: 96
  year: 2018
  ident: apjad22e3bib142
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa9ff3
– volume: 551
  start-page: A100
  year: 2013
  ident: apjad22e3bib9
  publication-title: A&A
  doi: 10.1051/0004-6361/201220859
– volume: 804
  start-page: 27
  year: 2015
  ident: apjad22e3bib6
  publication-title: ApJ
  doi: 10.1088/0004-637X/804/1/27
– volume: 429
  start-page: 3047
  year: 2013
  ident: apjad22e3bib15
  publication-title: MNRAS
  doi: 10.1093/mnras/sts562
– volume: 619
  start-page: A90
  year: 2018
  ident: apjad22e3bib104
  publication-title: A&A
  doi: 10.1051/0004-6361/201833040
– volume: 474
  start-page: 4528
  year: 2018
  ident: apjad22e3bib138
  publication-title: MNRAS
  doi: 10.1093/mnras/stx3120
– volume: 854
  start-page: 157
  year: 2018
  ident: apjad22e3bib40
  publication-title: ApJ
  doi: 10.3847/1538-4357/aaaaae
– volume: 574
  start-page: L9
  year: 2015
  ident: apjad22e3bib105
  publication-title: A&A
  doi: 10.1051/0004-6361/201425324
– volume: 344
  start-page: 1000
  year: 2003
  ident: apjad22e3bib18
  publication-title: MNRAS
  doi: 10.1046/j.1365-8711.2003.06897.x
– volume: 755
  start-page: 173
  year: 2012
  ident: apjad22e3bib38
  publication-title: ApJ
  doi: 10.1088/0004-637X/755/2/173
– volume: 749
  start-page: 123
  year: 2012
  ident: apjad22e3bib59
  publication-title: ApJ
  doi: 10.1088/0004-637X/749/2/123
– volume: 518
  start-page: L1
  year: 2010
  ident: apjad22e3bib107
  publication-title: A&A
  doi: 10.1051/0004-6361/201014759
– volume: 819
  start-page: 111
  year: 2016
  ident: apjad22e3bib7
  publication-title: ApJ
  doi: 10.3847/0004-637X/819/2/111
– volume: 805
  start-page: 90
  year: 2015
  ident: apjad22e3bib136
  publication-title: ApJ
  doi: 10.1088/0004-637X/805/2/90
– volume: 388
  start-page: 1595
  year: 2008
  ident: apjad22e3bib25
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2008.13535.x
– volume: 561
  start-page: A82
  year: 2014
  ident: apjad22e3bib121
  publication-title: A&A
  doi: 10.1051/0004-6361/201321716
– volume: 129
  start-page: 124101
  year: 2017
  ident: apjad22e3bib43
  publication-title: PASP
  doi: 10.1088/1538-3873/aa8e91
– start-page: 336 
  year: 2004
  ident: apjad22e3bib70
– volume: 407
  start-page: 2091
  year: 2010
  ident: apjad22e3bib54
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2010.16969.x
– volume: 884
  start-page: 11
  year: 2019
  ident: apjad22e3bib56
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab3e4f
– volume: 822
  start-page: L32
  year: 2016a
  ident: apjad22e3bib41
  publication-title: ApJL
  doi: 10.3847/2041-8205/822/2/L32
– volume: 618
  start-page: A28
  year: 2018
  ident: apjad22e3bib145
  publication-title: A&A
  doi: 10.1051/0004-6361/201732557
– volume: 240
  start-page: 3
  year: 2019
  ident: apjad22e3bib61
  publication-title: ApJS
  doi: 10.3847/1538-4365/aaeffa
– volume: 625
  start-page: A2
  year: 2019
  ident: apjad22e3bib80
  publication-title: A&A
  doi: 10.1051/0004-6361/201834918
– volume: 899
  start-page: 112
  year: 2020
  ident: apjad22e3bib118
  publication-title: ApJ
  doi: 10.3847/1538-4357/aba8a1
– volume: 856
  start-page: L5
  year: 2018
  ident: apjad22e3bib44
  publication-title: ApJL
  doi: 10.3847/2041-8213/aab496
– volume: 491
  start-page: 173
  year: 2008
  ident: apjad22e3bib3
  publication-title: A&A
  doi: 10.1051/0004-6361:200810628
– volume: 888
  start-page: 110
  year: 2020
  ident: apjad22e3bib75
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab5e7b
– volume: 154
  start-page: 32
  year: 2013
  ident: apjad22e3bib37
  publication-title: Msngr
– volume: 816
  start-page: L6
  year: 2016
  ident: apjad22e3bib27
  publication-title: ApJL
  doi: 10.3847/2041-8205/816/1/L6
– volume: 443
  start-page: 146
  year: 2014
  ident: apjad22e3bib74
  publication-title: MNRAS
  doi: 10.1093/mnras/stu1157
– volume: 53
  start-page: 51
  year: 2015
  ident: apjad22e3bib125
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082812-140951
– volume: 887
  start-page: 74
  year: 2019
  ident: apjad22e3bib45
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab5059
– volume: 644
  start-page: A15
  year: 2020
  ident: apjad22e3bib89
  publication-title: A&A
  doi: 10.1051/0004-6361/202038889
– volume: 261
  start-page: 567
  year: 1992
  ident: apjad22e3bib101
  publication-title: A&A
– volume: 708
  start-page: 137
  year: 2010
  ident: apjad22e3bib94
  publication-title: ApJ
  doi: 10.1088/0004-637X/708/1/137
– volume: 868
  start-page: 15
  year: 2018
  ident: apjad22e3bib135
  publication-title: ApJ
  doi: 10.3847/1538-4357/aae698
– volume: 866
  start-page: 92
  year: 2018
  ident: apjad22e3bib86
  publication-title: ApJ
  doi: 10.3847/1538-4357/aae075
– volume: 518
  start-page: L2
  year: 2010
  ident: apjad22e3bib108
  publication-title: A&A
  doi: 10.1051/0004-6361/201014535
– volume: 622
  start-page: A103
  year: 2019
  ident: apjad22e3bib14
  publication-title: A&A
  doi: 10.1051/0004-6361/201834156
– volume: 806
  start-page: L25
  year: 2015
  ident: apjad22e3bib122
  publication-title: ApJL
  doi: 10.1088/2041-8205/806/2/L25
– volume: 376
  start-page: 127
  year: 2007
  ident: apjad22e3bib92
  publication-title: adass XVI
– volume: 533
  start-page: 682
  year: 2000
  ident: apjad22e3bib20
  publication-title: ApJ
  doi: 10.1086/308692
– volume: 458
  start-page: 2288
  year: 2016
  ident: apjad22e3bib128
  publication-title: MNRAS
  doi: 10.1093/mnras/stw444
– volume: 157
  start-page: 168
  year: 2019
  ident: apjad22e3bib26
  publication-title: AJ
  doi: 10.3847/1538-3881/ab089d
– volume: 563
  start-page: A31
  year: 2014
  ident: apjad22e3bib111
  publication-title: A&A
  doi: 10.1051/0004-6361/201322803
– volume: 539
  start-page: A155
  year: 2012
  ident: apjad22e3bib87
  publication-title: A&A
  doi: 10.1051/0004-6361/201118312
– volume: 672
  start-page: A137
  year: 2023
  ident: apjad22e3bib84
  publication-title: A&A
  doi: 10.1051/0004-6361/202245168
– volume: 836
  start-page: 66
  year: 2017
  ident: apjad22e3bib117
  publication-title: ApJ
  doi: 10.3847/1538-4357/836/1/66
– volume: 823
  start-page: 107
  year: 2016b
  ident: apjad22e3bib42
  publication-title: ApJ
  doi: 10.3847/0004-637X/823/2/107
– volume: 654
  start-page: A37
  year: 2021
  ident: apjad22e3bib29
  publication-title: A&A
  doi: 10.1051/0004-6361/202140455
– volume: 458
  start-page: 816
  year: 2016
  ident: apjad22e3bib67
  publication-title: MNRAS
  doi: 10.1093/mnras/stw289
– volume: 483
  start-page: 514
  year: 2019
  ident: apjad22e3bib103
  publication-title: MNRAS
  doi: 10.1093/mnras/sty3128
– volume: 497
  start-page: 956
  year: 2020
  ident: apjad22e3bib126
  publication-title: MNRAS
  doi: 10.1093/mnras/staa1959
– volume: 1
  start-page: 679
  year: 2017
  ident: apjad22e3bib110
  publication-title: NatAs
  doi: 10.1038/s41550-017-0232-z
– volume: 496
  start-page: 1565
  year: 2020
  ident: apjad22e3bib102
  publication-title: MNRAS
  doi: 10.1093/mnras/staa1582
– volume: 636
  start-page: A73
  year: 2020
  ident: apjad22e3bib36
  publication-title: A&A
  doi: 10.1051/0004-6361/201936817
– volume: 425
  start-page: 605
  year: 2012
  ident: apjad22e3bib46
  publication-title: MNRAS
  doi: 10.1111/j.1365-2966.2012.21512.x
– volume: 935
  start-page: 80
  year: 2022
  ident: apjad22e3bib85
  publication-title: ApJ
  doi: 10.3847/1538-4357/ac8162
– volume: 245
  start-page: 4
  year: 2019
  ident: apjad22e3bib147
  publication-title: ApJS
  doi: 10.3847/1538-4365/ab48e8
SSID ssj0004299
Score 2.536105
Snippet We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field...
We present a UV to millimeter spectral energy distribution (SED) analysis of 16 hyperluminous, dust-obscured quasars at z ∼ 3, selected by the Wide-field...
SourceID doaj
swepub
proquest
crossref
iop
SourceType Open Website
Open Access Repository
Aggregation Database
Enrichment Source
Index Database
Publisher
StartPage 95
SubjectTerms Active galactic nuclei
Active galaxies
Black holes
Cold gas
Cosmic dust
Depletion
Dust
Galaxies
High-redshift galaxies
Infrared astronomy
Median (statistics)
Molecular gases
Physical properties
Quasars
Radio telescopes
Samples (statistical)
Spectral energy distribution
Star & galaxy formation
Star formation
Starburst galaxies
Stellar mass
SummonAdditionalLinks – databaseName: Directory of Open Access Journals
  dbid: DOA
  link: http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwrV3NbtQwELZQBRIXBAXUhYLmAEhIRLuJHTvhtvSHHpZqQYB6s_zLrlSSKskWlSfgPXgNnoYnweNkS_dSLtyiyJEdz__Y8w0hz7TLuAqOSJIKWyZ4dJaovKSJ1sxn2pY-i3nIzzNxfFycnJTzK62-8E5YDw_cb9yYF6lypRVUU8qwjJRyF2yi45QppoVB7TsR5TqYWldEBi3bH0rSoH7HUayDYyDGymaZoxtGKGL1B9OyrM823cyr0KHR3BzeJXcGPxGm_frukRuu2iY70xYz1_XXC3gB8blPTLTb5Na8f7pPfs6HrYc5JtobREyF2sNRiDiboIqWCMr6CvZXbZfUQWusGmfh_Uq1IcQF1cF3-P3jF9DXEGtzvynsTFF96RaAreoxLwIHsV4Q9hFzd2iXBWtwE1CVhb361MJb1ULEvqo6-ODO0SG1oC9gOns3fUA-HR583DtKhlYMiWFl1iU587RUNjU-TwvrNTM2s5PUpVYwzn0hNKfeCBTpwhotrMhN7lzqKbcckyYPyVZVV26HgM2DgVTBc9NOYUm1MsEpssaxchKUnRMjMl7TRpoBpxzbZZzKEK8gNSVSUyI1ZU_NEXl5-cVZj9Fxzdg3SO7LcYiuHV8EnpMDz8l_8dyIPA_MIgdpb6-ZbHfNTn8HZ6VAVEbG8hGZ9Sy2sZoB5GkhzSJ20GlliyviyguTyjwvuGQ4T6CGkKVKJ45pPzHOPPofv_aY3M6C29bfstslW12zck_ITXPeLdvmaRSyPysgKzg
  priority: 102
  providerName: Directory of Open Access Journals
Title Physical Properties of Hyperluminous, Dust-obscured Quasars at z ∼ 3: Multiwavelength Spectral Energy Distribution Analysis and Cold Gas Content Revealed by ALMA
URI https://iopscience.iop.org/article/10.3847/1538-4357/ad22e3
https://www.proquest.com/docview/2972744445
https://research.chalmers.se/publication/542227
https://doaj.org/article/681ae9d73b334935936e028e634a4b7c
Volume 964
WOSCitedRecordID wos001188035200001&url=https%3A%2F%2Fcvtisr.summon.serialssolutions.com%2F%23%21%2Fsearch%3Fho%3Df%26include.ft.matches%3Dt%26l%3Dnull%26q%3D
hasFullText 1
inHoldings 1
isFullTextHit
isPrint
journalDatabaseRights – providerCode: PRVAON
  databaseName: Directory of Open Access Journals
  customDbUrl:
  eissn: 1538-4357
  dateEnd: 99991231
  omitProxy: false
  ssIdentifier: ssj0004299
  issn: 0004-637X
  databaseCode: DOA
  dateStart: 20220101
  isFulltext: true
  titleUrlDefault: https://www.doaj.org/
  providerName: Directory of Open Access Journals
– providerCode: PRVIOP
  databaseName: Institute of Physics Journals Open Access
  customDbUrl:
  eissn: 1538-4357
  dateEnd: 99991231
  omitProxy: false
  ssIdentifier: ssj0004299
  issn: 0004-637X
  databaseCode: O3W
  dateStart: 19950701
  isFulltext: true
  titleUrlDefault: http://iopscience.iop.org/
  providerName: IOP Publishing
– providerCode: PRVHPJ
  databaseName: ROAD: Directory of Open Access Scholarly Resources
  customDbUrl:
  eissn: 1538-4357
  dateEnd: 99991231
  omitProxy: false
  ssIdentifier: ssj0004299
  issn: 0004-637X
  databaseCode: M~E
  dateStart: 18950101
  isFulltext: true
  titleUrlDefault: https://road.issn.org
  providerName: ISSN International Centre
link http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3NbhMxELZKAYkLPwXUQKnmAEhILMmuvfYunEKb0kNaAuInN8t_SyqVTZXdFJUDZ96D1-BpeBI83k1KJFQhcYmsyImtfOOZz7OZbwh5qF3ClSciUSxsHuGjs0ilOY20ZkWibV4kIQ_5YSgOD7PxOB-tkRfLWpjpSev6n_lhIxTc_IR4vqn3pd1wRn2UF11lk8TRS-QyzXwY98b8mn48L4pM8pb7sohTMW6eUf71G1ZiUpDu95HGL7_KOv9UEg3RZ-_Gf-37Jrnekk7oN1NvkTVXbpDNfoVp8OnnM3gMYdxkOaoNcnXUjG6TH6MWRxhh1n6G8qswLWDfX19n3q8docLrU9idV3U09S5oPnMW3sxV5e_LoGr4Cr--_wT6HEKh7xeFbS7KT_UEsO89JllgEIoPYRcFfNveW7BQSgFVWtiZHlt4pSoIQlplDW_dKbJbC_oM-sOD_h3yfm_wbmc_avs6RIblSR2lrKC5srEp0jizhWbGJrYXu9gKxnmRCc1pYQT6h8waLaxITepcXFBuOWZg7pL1clq6TQI29dFWeRqoncL6bGU8w7LGsbznPacTHdJdICtNK3qOvTeOpb_8ICoSUZGIimxQ6ZAny0-cNIIfF8x9icaynIdS3eEND79s4Zc8i5XLraCaUoZ10JQ7T-ocp0wxLUyHPPIWI1vXUV2w2NbCGM8nJ7lAiUfG0g4ZNga6sptWMWoizSS046lkhTviqhAmlmmacclwHY-GkLmKe47pomecufePu7pPriWe5jX_ytsi6_Vs7h6QK-a0Pqpm2yHD4V8Pvg22w-n8DRhROLk
linkProvider IOP Publishing
linkToPdf http://cvtisr.summon.serialssolutions.com/2.0.0/link/0/eLvHCXMwpV3bjtMwELVguYgXLgtoCwv4AZCQCG1ix054K9stiyil3Ptm-UpXWtIqSRctX8B_8Bt8DV-Cx0l3qYRWSLxZkZOMMuOZ43HmDEL3lU2Y9EAkirnJIzg6i2Sak0gp6hJlcpeEPOTHER-Ps-k0n7R9TkMtzHzRuv4nftgQBTefENY38b60G9aoj_K8K02SWNJdGHcWnQOeEjDr1-TTSWFkkrf4l0aM8GlzTvnXp6zFpUDf76ONF2Edef7JJhoi0PDKf8t-FV1uwSfuN9OvoTO22ERb_QrS4fMvR_ghDuMm21FtoguTZnQd_Zi0-sQTyN6XQMOK5w7v-W1s6f3bPjC9PsaDZVVHc--KlqU1-M1SVn7fjGWNv-Ff339i8hSHgt-vEtpdFJ_rGX4HlZ6lf-5uKELEAyDybXtw4RVjCpaFwTvzA4OfywoHQq2ixm_tIaBcg9UR7o9e9W-gD8Pd9zt7UdvfIdI0T-oopY7k0sTapXFmnKLaJKYX29hwypjLuGLEaQ5-IjNaccNTnVobO8IMg0zMTbRRzAu7hbBJfdSVHg4qK6FOW2qPtIy2NO95D2p5B3VX2hW6JT-HHhwHwm-CQDMCNCNAM6LRTAc9Or5j0RB_nDL3GRjM8Tyg7A4XvAmI1gQEy2Jpc8OJIoRCPTRh1oM7ywiVVHHdQQ-81YjWhVSnvGx7ZZAnk5OcA9UjpWkHjRojXZOmZY6aCT0LbXkqUYFETDquY5GmGRMU3uO1wUUu456lyvW01bf-Uap76OJkMBSjF-OXt9GlxCO_5ke9bbRRl0t7B53Xh_V-Vd4NC_Q3Dyw7-w
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=Physical+Properties+of+Hyperluminous%2C+Dust-obscured+Quasars+at+z+%E2%88%BC+3%3A+Multiwavelength+Spectral+Energy+Distribution+Analysis+and+Cold+Gas+Content+Revealed+by+ALMA&rft.jtitle=The+Astrophysical+journal&rft.au=Sun%2C+Weibin&rft.au=Fan%2C+Lulu&rft.au=Han%2C+Yunkun&rft.au=Knudsen%2C+Kirsten+K.&rft.date=2024-03-01&rft.pub=The+American+Astronomical+Society&rft.issn=0004-637X&rft.eissn=1538-4357&rft.volume=964&rft.issue=1&rft_id=info:doi/10.3847%2F1538-4357%2Fad22e3&rft.externalDocID=apjad22e3
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