ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy

ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of har...

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Veröffentlicht in:Monthly notices of the Royal Astronomical Society Jg. 493; H. 3; S. 4294 - 4307
Hauptverfasser: Bakx, Tom J L C, Tamura, Yoichi, Hashimoto, Takuya, Inoue, Akio K, Lee, Minju M, Mawatari, Ken, Ota, Kazuaki, Umehata, Hideki, Zackrisson, Erik, Hatsukade, Bunyo, Kohno, Kotaro, Matsuda, Yuichi, Matsuo, Hiroshi, Okamoto, Takashi, Shibuya, Takatoshi, Shimizu, Ikkoh, Taniguchi, Yoshiaki, Yoshida, Naoki
Format: Journal Article
Sprache:Englisch
Veröffentlicht: London Oxford University Press 01.04.2020
Schlagworte:
Confidence limits
Continuum radiation
Cosmic dust
Dust
Galaxies
galaxies: formation
galaxies: high-redshift
galaxies: ISM
Interstellar matter
Interstellar radiation
Ionization
Luminosity
Photodissociation
Physical properties
Radio telescopes
galaxies: formation
galaxies: ISM
galaxies: high-redshift
ISSN:0035-8711, 1365-2966, 1365-2966
Online-Zugang:Volltext
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Abstract ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of hard interstellar radiation fields and/or a low covering fraction of photodissociation regions. The emission of [C ii] is cospatial to the 850 μm dust emission (90 μm rest frame, from previous campaigns), however the peak [C ii] emission does not agree with the peak [O iii] emission, suggesting that the lines originate from different conditions in the interstellar medium. We fail to detect continuum emission at 1.5 mm (160 μm rest frame) down to 18 μJy (3σ). This non-detection places a strong limits on the dust spectrum, considering the 137 ± 26 μJy continuum emission at 850 μm. This suggests an unusually warm dust component (T > 80 K, 90 per cent confidence limit), and/or a steep dust-emissivity index (βdust > 2), compared to galaxy-wide dust emission found at lower redshifts (typically T ∼ 30–50 K, βdust ∼ 1–2). If such temperatures are common, this would reduce the required dust mass and relax the dust production problem at the highest redshifts. We therefore warn against the use of only single-wavelength information to derive physical properties, recommend a more thorough examination of dust temperatures in the early Universe, and stress the need for instrumentation that probes the peak of warm dust in the Epoch of Reionization.
AbstractList ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of hard interstellar radiation fields and/or a low covering fraction of photodissociation regions. The emission of [C ii] is cospatial to the 850 μm dust emission (90 μm rest frame, from previous campaigns), however the peak [C ii] emission does not agree with the peak [O iii] emission, suggesting that the lines originate from different conditions in the interstellar medium. We fail to detect continuum emission at 1.5 mm (160 μm rest frame) down to 18 μJy (3σ). This non-detection places a strong limits on the dust spectrum, considering the 137 ± 26 μJy continuum emission at 850 μm. This suggests an unusually warm dust component (T > 80 K, 90 per cent confidence limit), and/or a steep dust-emissivity index (βdust > 2), compared to galaxy-wide dust emission found at lower redshifts (typically T ∼ 30–50 K, βdust ∼ 1–2). If such temperatures are common, this would reduce the required dust mass and relax the dust production problem at the highest redshifts. We therefore warn against the use of only single-wavelength information to derive physical properties, recommend a more thorough examination of dust temperatures in the early Universe, and stress the need for instrumentation that probes the peak of warm dust in the Epoch of Reionization.
ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of hard interstellar radiation fields and/or a low covering fraction of photodissociation regions. The emission of [C ii] is cospatial to the 850 μm dust emission (90 μm rest frame, from previous campaigns), however the peak [C ii] emission does not agree with the peak [O iii] emission, suggesting that the lines originate from different conditions in the interstellar medium. We fail to detect continuum emission at 1.5 mm (160 μm rest frame) down to 18 μJy (3σ). This non-detection places a strong limits on the dust spectrum, considering the 137 ± 26 μJy continuum emission at 850 μm. This suggests an unusually warm dust component (T > 80 K, 90 per cent confidence limit), and/or a steep dust-emissivity index (βdust > 2), compared to galaxy-wide dust emission found at lower redshifts (typically T ∼ 30–50 K, βdust ∼ 1–2). If such temperatures are common, this would reduce the required dust mass and relax the dust production problem at the highest redshifts. We therefore warn against the use of only single-wavelength information to derive physical properties, recommend a more thorough examination of dust temperatures in the early Universe, and stress the need for instrumentation that probes the peak of warm dust in the Epoch of Reionization.
We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O iii] 88 μm (from previous campaigns) to [C ii] is 9.3 ± 2.6, indicative of hard interstellar radiation fields and/or a low covering fraction of photodissociation regions. The emission of [C ii] is cospatial to the 850 μm dust emission (90 μm rest frame, from previous campaigns), however the peak [C ii] emission does not agree with the peak [O iii] emission, suggesting that the lines originate from different conditions in the interstellar medium. We fail to detect continuum emission at 1.5 mm (160 μm rest frame) down to 18 μJy (3σ). This non-detection places a strong limits on the dust spectrum, considering the 137 ± 26 μJy continuum emission at 850 μm. This suggests an unusually warm dust component (T > 80 K, 90 per cent confidence limit), and/or a steep dust-emissivity index (βdust > 2), compared to galaxy-wide dust emission found at lower redshifts (typically T ∼ 30–50 K, βdust ∼ 1–2). If such temperatures are common, this would reduce the required dust mass and relax the dust production problem at the highest redshifts. We therefore warn against the use of only single-wavelength information to derive physical properties, recommend a more thorough examination of dust temperatures in the early Universe, and stress the need for instrumentation that probes the peak of warm dust in the Epoch of Reionization.
We report on the detection of the [C II] 157.7 mu m emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large Millimeter/submillimeter Array (ALMA). The luminosity ratio of [O III] 88 mu m (from previous campaigns) to [CII] is 9.3 +/- 2.6, indicative of hard interstellar radiation fields and/or a low covering fraction of photodissociation regions. The emission of [C II] is cospatial to the 850 mu m dust emission (90 mu m rest frame, from previous campaigns), however the peak [C II] emission does not agree with the peak [O III] emission, suggesting that the lines originate from different conditions in the interstellar medium. We fail to detect continuum emission at 1.5 mm (160 mu m rest frame) down to 18 mu Jy (3 sigma). This non-detection places a strong limits on the dust spectrum, considering the 137 +/- 26 mu Jy continuum emission at 850 mu m. This suggests an unusually warm dust component (T > 80 K, 90 per cent confidence limit), and/or a steep dust-emissivity index (beta(dust) > 2), compared to galaxy-wide dust emission found at lower redshifts (typically T similar to 30-50 K, beta(dust) similar to 1-2). If such temperatures are common, thiswould reduce the required dust mass and relax the dust production problem at the highest redshifts. We therefore warn against the use of only single-wavelength information to derive physical properties, recommend a more thorough examination of dust temperatures in the early Universe, and stress the need for instrumentation that probes the peak of warm dust in the Epoch of Reionization.
Author Mawatari, Ken
Hashimoto, Takuya
Shibuya, Takatoshi
Ota, Kazuaki
Zackrisson, Erik
Shimizu, Ikkoh
Lee, Minju M
Okamoto, Takashi
Inoue, Akio K
Hatsukade, Bunyo
Kohno, Kotaro
Tamura, Yoichi
Umehata, Hideki
Matsuo, Hiroshi
Bakx, Tom J L C
Yoshida, Naoki
Taniguchi, Yoshiaki
Matsuda, Yuichi
Author_xml – sequence: 1
  givenname: Tom J L C
  orcidid: 0000-0002-5268-2221
  surname: Bakx
  fullname: Bakx, Tom J L C
  email: bakx@a.phys.nagoya-u.ac.jp
  organization: Division of Particle and Astrophysical Science, Graduate School of Science, Nagoya University, Aichi 464-8602, Japan
– sequence: 2
  givenname: Yoichi
  surname: Tamura
  fullname: Tamura, Yoichi
  organization: Division of Particle and Astrophysical Science, Graduate School of Science, Nagoya University, Aichi 464-8602, Japan
– sequence: 3
  givenname: Takuya
  orcidid: 0000-0002-0898-4038
  surname: Hashimoto
  fullname: Hashimoto, Takuya
  organization: National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
– sequence: 4
  givenname: Akio K
  orcidid: 0000-0002-7779-8677
  surname: Inoue
  fullname: Inoue, Akio K
  organization: Department of Physics, School of Advanced Science and Engineering, Faculty of Science and Engineering, Waseda University, 3-4-1 Okubo, Shinjuku, Tokyo 169-8555, Japan
– sequence: 5
  givenname: Minju M
  surname: Lee
  fullname: Lee, Minju M
  organization: Max-Planck-Institut für Extraterrestrische Physik (MPE), Giessenbachstr., D-85748 Garching, Germany
– sequence: 6
  givenname: Ken
  orcidid: 0000-0003-4985-0201
  surname: Mawatari
  fullname: Mawatari, Ken
  organization: Department of Environmental Science and Technology, Faculty of Design Technology, Osaka Sangyo University, 3-1-1, Nakagaito, Daito, Osaka 574-8530, Japan
– sequence: 7
  givenname: Kazuaki
  surname: Ota
  fullname: Ota, Kazuaki
  organization: Kyoto University Research Administration Office, Yoshida-Honmachi, Sakyo-ku, Kyoto 606-8501, Japan
– sequence: 8
  givenname: Hideki
  surname: Umehata
  fullname: Umehata, Hideki
  organization: The Open University of Japan, 2-11 Wakaba, Mihama-ku, Chiba 261-8586, Japan
– sequence: 9
  givenname: Erik
  orcidid: 0000-0003-1096-2636
  surname: Zackrisson
  fullname: Zackrisson, Erik
  organization: Observational Astrophysics, Department of Physics and Astronomy, Uppsala University, Box 516, SE-751 20 Uppsala, Sweden
– sequence: 10
  givenname: Bunyo
  surname: Hatsukade
  fullname: Hatsukade, Bunyo
  organization: Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo 181-0015, Japan
– sequence: 11
  givenname: Kotaro
  orcidid: 0000-0002-4052-2394
  surname: Kohno
  fullname: Kohno, Kotaro
  organization: Institute of Astronomy, Graduate School of Science, The University of Tokyo, 2-21-1, Osawa, Mitaka, Tokyo 181-0015, Japan
– sequence: 12
  givenname: Yuichi
  surname: Matsuda
  fullname: Matsuda, Yuichi
  organization: National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
– sequence: 13
  givenname: Hiroshi
  surname: Matsuo
  fullname: Matsuo, Hiroshi
  organization: National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
– sequence: 14
  givenname: Takashi
  surname: Okamoto
  fullname: Okamoto, Takashi
  organization: Faculty of Science, Hokkaido University, N10 W8 Kita-ku, Sapporo 060-0810 Japan
– sequence: 15
  givenname: Takatoshi
  surname: Shibuya
  fullname: Shibuya, Takatoshi
  organization: Kitami Institute of Technology, 165 Koen-cho, Kitami, Hokkaido 090-8507, Japan
– sequence: 16
  givenname: Ikkoh
  surname: Shimizu
  fullname: Shimizu, Ikkoh
  organization: National Astronomical Observatory of Japan, 2-21-1, Osawa, Mitaka, Tokyo 181-8588, Japan
– sequence: 17
  givenname: Yoshiaki
  surname: Taniguchi
  fullname: Taniguchi, Yoshiaki
  organization: Kyoto University Research Administration Office, Yoshida-Honmachi, Sakyo-ku, Kyoto 606-8501, Japan
– sequence: 18
  givenname: Naoki
  surname: Yoshida
  fullname: Yoshida, Naoki
  organization: Department of Physics, Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan
BackLink https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-411003$$DView record from Swedish Publication Index (Uppsala universitet)
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Cites_doi 10.1051/0004-6361/201834673
10.1051/0004-6361/201732019
10.1126/science.aaf0714
10.1093/mnras/stv372
10.1046/j.1365-8711.2001.04789.x
10.1051/0004-6361/201525830
10.1051/0004-6361/201630366
10.1093/mnrasl/slw165
10.3847/1538-4357/ab3e0b
10.1093/mnras/stx1792
10.1051/0004-6361/201424649
10.1093/mnrasl/slz094
10.1086/379118
10.1038/nature24629
10.1093/mnras/stx1898
10.1086/668636
10.3847/1538-4357/aaebf8
10.1088/0004-637X/808/2/139
10.1088/2041-8205/771/2/L20
10.1093/mnrasl/slw114
10.3847/0004-637X/820/2/83
10.1051/0004-6361/201628806
10.1051/0004-6361:20066130
10.1086/170062
10.3847/1538-4357/aa81d7
10.1146/annurev-astro-082812-140953
10.1038/nature14164
10.1088/0004-637X/706/2/1364
10.3847/2041-8213/aa62aa
10.3847/1538-4357/aa9931
10.1038/nature14500
10.1038/nature13558
10.1093/mnras/stz2031
10.1051/0004-6361/201425040
10.1093/mnras/stw3088
10.1051/0004-6361/201323195
10.1093/mnras/stz1486
10.1086/376392
10.1051/0004-6361/201425207
10.1088/0004-637X/766/1/13
10.3847/2041-8213/836/1/L2
10.3847/1538-4357/aa886c
10.1093/mnras/sty1088
10.1088/0004-637X/756/1/40
10.1093/mnras/stz1672
10.1093/mnras/sty2779
10.1086/671138
10.3847/1538-4357/ab6596
10.1093/mnras/stz1383
10.1088/0004-637X/724/2/957
10.1088/0004-637X/774/1/68
10.1086/304247
10.1093/mnras/sty313
10.1109/TTHZ.2011.2159649
10.1093/pasj/psw041
10.1088/2041-8205/787/2/L17
10.3847/1538-4357/aa7eda
10.1088/0004-637X/815/1/18
10.1146/annurev-astro-081811-125615
10.1088/0004-637X/777/1/66
10.1093/mnras/stz1887
10.1086/311044
10.1093/mnras/stv780
10.3847/1538-4357/837/1/97
10.3847/1538-4357/833/1/72
10.1088/2041-8205/740/1/L15
10.1093/mnras/stx180
10.1093/pasj/psx107
10.1088/0004-637X/803/1/34
10.1086/303434
10.3847/0004-637X/819/2/129
10.1051/0004-6361/201527514
10.3847/1538-4357/aa7d0d
10.1093/mnras/stx3227
10.1086/154870
10.1051/0004-6361/201525644
10.1093/mnras/stx839
10.1093/mnras/stw2847
10.1093/pasj/psy087
10.1051/0004-6361/201322489
10.1088/0004-637X/810/1/71
10.1051/0004-6361/201834457
10.1086/505341
10.1051/0004-6361/201935149
10.1146/annurev.astro.43.051804.102221
10.5047/eps.2012.04.014
10.1093/mnras/sty552
10.1051/0004-6361/201015465
10.1038/nature24631
10.1016/j.physrep.2018.10.002
10.1515/9781400828722
10.3847/1538-4357/aab03f
10.1007/s00159-018-0112-2
10.3847/2041-8213/aaf4fa
10.1088/0004-637X/807/2/180
10.1051/0004-6361/201731883
10.3847/0004-637X/819/2/114
10.1088/0004-637X/792/1/34
10.1086/600092
10.1038/s41586-018-0117-z
10.3847/1538-4357/ab0374
10.3847/0004-637X/820/2/98
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Issue 3
Keywords galaxies: formation
galaxies: ISM
galaxies: high-redshift
Language English
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References González-López (2021030920103477500_bib49) 2017; 597
Michałowski (2021030920103477500_bib85) 2015; 577
Bowler (2021030920103477500_bib13) 2017; 469
Gnerucci (2021030920103477500_bib48) 2011; 528
Kawamata (2021030920103477500_bib61) 2016; 819
Carniani (2021030920103477500_bib17) 2017; 605
Ferrara (2021030920103477500_bib41) 2017; 471
Cormier (2021030920103477500_bib23) 2015; 578
Díaz-Santos (2021030920103477500_bib32) 2013; 774
Mawatari (2021030920103477500_bib80) 2020; 889
Scoville (2021030920103477500_bib98) 2016; 820
Harikane (2021030920103477500_bib52) 2019
Lotz (2021030920103477500_bib70) 2017; 837
Pallottini (2021030920103477500_bib92) 2019; 487
Laporte (2021030920103477500_bib68) 2019; 487
Demyk (2021030920103477500_bib31) 2013
Cousin (2021030920103477500_bib25) 2019; 627
Inoue (2021030920103477500_bib56) 2016; 352
Willott (2021030920103477500_bib113) 2015; 807
Carniani (2021030920103477500_bib18) 2018; 478
Marrone (2021030920103477500_bib77) 2018; 553
Oesch (2021030920103477500_bib88) 2018; 855
Smit (2021030920103477500_bib100) 2018; 553
Carilli (2021030920103477500_bib16) 2013; 51
Ferrara (2021030920103477500_bib40) 2016; 463
Maiolino (2021030920103477500_bib75) 2019; 27
Ota (2021030920103477500_bib89) 2014; 792
Oesch (2021030920103477500_bib87) 2016; 819
Ferland (2021030920103477500_bib39) 2017; 53
Pallottini (2021030920103477500_bib90) 2017; 465
Kohandel (2021030920103477500_bib63) 2019; 487
Stacey (2021030920103477500_bib105) 2011; 1
Sobral (2021030920103477500_bib103) 2019; 482
Arata (2021030920103477500_bib2) 2019; 488
Barisic (2021030920103477500_bib7) 2017; 845
Planck Collaboration XVI (2021030920103477500_bib94) 2016; 594
Vallini (2021030920103477500_bib110) 2017; 467
Meijerink (2021030920103477500_bib83) 2007; 461
Madden (2021030920103477500_bib72) 1997; 483
Mawatari (2021030920103477500_bib79) 2016; 68
Hashimoto (2021030920103477500_bib53) 2018; 557
Matthee (2021030920103477500_bib78) 2017; 851
Capak (2021030920103477500_bib15) 2015; 522
Magdis (2021030920103477500_bib74) 2011; 740
Laporte (2021030920103477500_bib67) 2017; 837
Behrens (2021030920103477500_bib8) 2018; 477
Madden (2021030920103477500_bib73) 2013; 125
Bouwens (2021030920103477500_bib11) 2015; 803
Planck Collaboration VI (2021030920103477500_bib95) 2018
Faisst (2021030920103477500_bib38) 2017; 847
Watson (2021030920103477500_bib112) 2015; 519
Pallottini (2021030920103477500_bib91) 2017; 471
Erb (2021030920103477500_bib37) 2006; 647
Dayal (2021030920103477500_bib27) 2018; 780
Lagache (2021030920103477500_bib64) 2018; 609
Gullberg (2021030920103477500_bib51) 2015; 449
Nozawa (2021030920103477500_bib86) 2014; 787
Cormier (2021030920103477500_bib24) 2019; 626
Hashimoto (2021030920103477500_bib54) 2019
Bradač (2021030920103477500_bib14) 2017; 836
Shibuya (2021030920103477500_bib99) 2018; 70
da Cunha (2021030920103477500_bib26) 2013; 766
Knudsen (2021030920103477500_bib62) 2016; 462
Bouwens (2021030920103477500_bib12) 2016; 833
Stacey (2021030920103477500_bib107) 2010; 724
Ferrara (2021030920103477500_bib42) 2019; 489
Avni (2021030920103477500_bib6) 1976; 210
Katz (2021030920103477500_bib60) 2019; 487
Armus (2021030920103477500_bib4) 2009; 121
Kanekar (2021030920103477500_bib58) 2013; 771
Walter (2021030920103477500_bib111) 2018; 869
Asano (2021030920103477500_bib5) 2013; 65
Gall (2021030920103477500_bib46) 2014; 511
Madau (2021030920103477500_bib71) 2014; 52
Schaerer (2021030920103477500_bib97) 2015; 574
Smith (2021030920103477500_bib101) 2012; 756
Dunlop (2021030920103477500_bib35) 2017; 466
Malhotra (2021030920103477500_bib76) 1997; 491
McLeod (2021030920103477500_bib81) 2015; 450
Stacey (2021030920103477500_bib106) 1991; 373
Castellano (2021030920103477500_bib19) 2016; 590
Solomon (2021030920103477500_bib104) 2005; 43
Appleton (2021030920103477500_bib1) 2013; 777
Planck Collaboration XI (2021030920103477500_bib93) 2014; 571
Díaz-Santos (2021030920103477500_bib33) 2017; 846
Kato (2021030920103477500_bib59) 2018; 70
McMullin (2021030920103477500_bib82) 2007
Meixner (2021030920103477500_bib84) 2019
Belitsky (2021030920103477500_bib9) 2018; 611
Clements (2021030920103477500_bib22) 2018; 475
Tegmark (2021030920103477500_bib109) 1997; 474
De Rossi (2021030920103477500_bib30) 2018; 869
Binney (2021030920103477500_bib10) 2008
De Rossi (2021030920103477500_bib29) 2019; 883
Fujimoto (2021030920103477500_bib45) 2019
Finkelstein (2021030920103477500_bib43) 2015; 810
Draine (2021030920103477500_bib34) 2003; 598
Sawicki (2021030920103477500_bib96) 2012; 124
González-López (2021030920103477500_bib50) 2017; 597
Infante (2021030920103477500_bib55) 2015; 815
Tamura (2021030920103477500_bib108) 2019; 874
Arata (2021030920103477500_bib3) 2020
Jones (2021030920103477500_bib57) 2017; 845
Chabrier (2021030920103477500_bib21) 2003; 115
Dunne (2021030920103477500_bib36) 2001; 327
Laporte (2021030920103477500_bib65) 2015; 575
de Looze (2021030920103477500_bib28) 2014; 568
Förster Schreiber (2021030920103477500_bib44) 2009; 706
Sobral (2021030920103477500_bib102) 2015; 808
Laporte (2021030920103477500_bib66) 2016; 820
Leśniewska (2021030920103477500_bib69) 2019; 624
Ceccarelli (2021030920103477500_bib20) 2018; 476
Ginolfi (2021030920103477500_bib47) 2020
References_xml – volume: 627
  start-page: A131
  year: 2019
  ident: 2021030920103477500_bib25
  publication-title: A&A
  doi: 10.1051/0004-6361/201834673
– start-page: 107
  volume-title: ApJ
  year: 2019
  ident: 2021030920103477500_bib45
– volume: 609
  start-page: A130
  year: 2018
  ident: 2021030920103477500_bib64
  publication-title: A&A
  doi: 10.1051/0004-6361/201732019
– volume: 352
  start-page: 1559
  year: 2016
  ident: 2021030920103477500_bib56
  publication-title: Science
  doi: 10.1126/science.aaf0714
– volume: 449
  start-page: 2883
  year: 2015
  ident: 2021030920103477500_bib51
  publication-title: MNRAS
  doi: 10.1093/mnras/stv372
– volume: 327
  start-page: 697
  year: 2001
  ident: 2021030920103477500_bib36
  publication-title: MNRAS
  doi: 10.1046/j.1365-8711.2001.04789.x
– volume: 594
  start-page: A13
  year: 2016
  ident: 2021030920103477500_bib94
  publication-title: A&A
  doi: 10.1051/0004-6361/201525830
– volume: 605
  start-page: A42
  year: 2017
  ident: 2021030920103477500_bib17
  publication-title: A&A
  doi: 10.1051/0004-6361/201630366
– volume: 463
  start-page: L112
  year: 2016
  ident: 2021030920103477500_bib40
  publication-title: MNRAS
  doi: 10.1093/mnrasl/slw165
– volume: 883
  start-page: 113
  year: 2019
  ident: 2021030920103477500_bib29
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab3e0b
– volume: 471
  start-page: 4128
  year: 2017
  ident: 2021030920103477500_bib91
  publication-title: MNRAS
  doi: 10.1093/mnras/stx1792
– volume: 574
  start-page: A19
  year: 2015
  ident: 2021030920103477500_bib97
  publication-title: A&A
  doi: 10.1051/0004-6361/201424649
– volume: 487
  start-page: L81
  year: 2019
  ident: 2021030920103477500_bib68
  publication-title: MNRAS
  doi: 10.1093/mnrasl/slz094
– volume: 598
  start-page: 1017
  year: 2003
  ident: 2021030920103477500_bib34
  publication-title: ApJ
  doi: 10.1086/379118
– volume: 553
  start-page: 51
  year: 2018
  ident: 2021030920103477500_bib77
  publication-title: Nature
  doi: 10.1038/nature24629
– volume: 471
  start-page: 5018
  year: 2017
  ident: 2021030920103477500_bib41
  publication-title: MNRAS
  doi: 10.1093/mnras/stx1898
– volume: 124
  start-page: 1208
  year: 2012
  ident: 2021030920103477500_bib96
  publication-title: PASP
  doi: 10.1086/668636
– volume: 869
  start-page: 4
  year: 2018
  ident: 2021030920103477500_bib30
  publication-title: ApJ
  doi: 10.3847/1538-4357/aaebf8
– volume: 808
  start-page: 139
  year: 2015
  ident: 2021030920103477500_bib102
  publication-title: ApJ
  doi: 10.1088/0004-637X/808/2/139
– volume: 771
  start-page: L20
  year: 2013
  ident: 2021030920103477500_bib58
  publication-title: ApJ
  doi: 10.1088/2041-8205/771/2/L20
– volume: 462
  start-page: L6
  year: 2016
  ident: 2021030920103477500_bib62
  publication-title: MNRAS
  doi: 10.1093/mnrasl/slw114
– start-page: 127
  volume-title: ASP Conf. Ser. Vol. 376, Astronomical Data Analysis Software and Systems XVI
  year: 2007
  ident: 2021030920103477500_bib82
– volume: 820
  start-page: 83
  year: 2016
  ident: 2021030920103477500_bib98
  publication-title: ApJ
  doi: 10.3847/0004-637X/820/2/83
– volume: 597
  start-page: A41
  year: 2017
  ident: 2021030920103477500_bib50
  publication-title: A&A
  doi: 10.1051/0004-6361/201628806
– volume: 461
  start-page: 793
  year: 2007
  ident: 2021030920103477500_bib83
  publication-title: A&A
  doi: 10.1051/0004-6361:20066130
– volume: 373
  start-page: 423
  year: 1991
  ident: 2021030920103477500_bib106
  publication-title: ApJ
  doi: 10.1086/170062
– volume: 846
  start-page: 32
  year: 2017
  ident: 2021030920103477500_bib33
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa81d7
– volume: 51
  start-page: 105
  year: 2013
  ident: 2021030920103477500_bib16
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-082812-140953
– volume: 519
  start-page: 327
  year: 2015
  ident: 2021030920103477500_bib112
  publication-title: Nature
  doi: 10.1038/nature14164
– volume: 706
  start-page: 1364
  year: 2009
  ident: 2021030920103477500_bib44
  publication-title: ApJ
  doi: 10.1088/0004-637X/706/2/1364
– volume: 597
  start-page: A41
  year: 2017
  ident: 2021030920103477500_bib49
  publication-title: A&A
  doi: 10.1051/0004-6361/201628806
– volume: 837
  start-page: L21
  year: 2017
  ident: 2021030920103477500_bib67
  publication-title: ApJ
  doi: 10.3847/2041-8213/aa62aa
– volume: 851
  start-page: 145
  year: 2017
  ident: 2021030920103477500_bib78
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa9931
– volume: 522
  start-page: 455
  year: 2015
  ident: 2021030920103477500_bib15
  publication-title: Nature
  doi: 10.1038/nature14500
– volume: 511
  start-page: 326
  year: 2014
  ident: 2021030920103477500_bib46
  publication-title: Nature
  doi: 10.1038/nature13558
– volume: 489
  start-page: 1
  year: 2019
  ident: 2021030920103477500_bib42
  publication-title: MNRAS
  doi: 10.1093/mnras/stz2031
– year: 2020
  ident: 2021030920103477500_bib3
– volume: 575
  start-page: A92
  year: 2015
  ident: 2021030920103477500_bib65
  publication-title: A&A
  doi: 10.1051/0004-6361/201425040
– volume: 466
  start-page: 861
  year: 2017
  ident: 2021030920103477500_bib35
  publication-title: MNRAS
  doi: 10.1093/mnras/stw3088
– volume: 571
  start-page: A11
  year: 2014
  ident: 2021030920103477500_bib93
  publication-title: A&A
  doi: 10.1051/0004-6361/201323195
– volume: 487
  start-page: 3007
  year: 2019
  ident: 2021030920103477500_bib63
  publication-title: MNRAS
  doi: 10.1093/mnras/stz1486
– volume: 115
  start-page: 763
  year: 2003
  ident: 2021030920103477500_bib21
  publication-title: PASP
  doi: 10.1086/376392
– volume: 578
  start-page: A53
  year: 2015
  ident: 2021030920103477500_bib23
  publication-title: A&A
  doi: 10.1051/0004-6361/201425207
– volume: 766
  start-page: 13
  year: 2013
  ident: 2021030920103477500_bib26
  publication-title: ApJ
  doi: 10.1088/0004-637X/766/1/13
– volume: 836
  start-page: L2
  year: 2017
  ident: 2021030920103477500_bib14
  publication-title: ApJ
  doi: 10.3847/2041-8213/836/1/L2
– volume: 847
  start-page: 21
  year: 2017
  ident: 2021030920103477500_bib38
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa886c
– volume: 478
  start-page: 1170
  year: 2018
  ident: 2021030920103477500_bib18
  publication-title: MNRAS
  doi: 10.1093/mnras/sty1088
– volume: 756
  start-page: 40
  year: 2012
  ident: 2021030920103477500_bib101
  publication-title: ApJ
  doi: 10.1088/0004-637X/756/1/40
– start-page: 71
  volume-title: PASJ
  year: 2019
  ident: 2021030920103477500_bib54
– volume: 487
  start-page: 5902
  year: 2019
  ident: 2021030920103477500_bib60
  publication-title: MNRAS
  doi: 10.1093/mnras/stz1672
– volume: 482
  start-page: 2422
  year: 2019
  ident: 2021030920103477500_bib103
  publication-title: MNRAS
  doi: 10.1093/mnras/sty2779
– volume: 125
  start-page: 600
  year: 2013
  ident: 2021030920103477500_bib73
  publication-title: PASP
  doi: 10.1086/671138
– volume: 889
  start-page: 137
  year: 2020
  ident: 2021030920103477500_bib80
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab6596
– volume: 487
  start-page: 1689
  year: 2019
  ident: 2021030920103477500_bib92
  publication-title: MNRAS
  doi: 10.1093/mnras/stz1383
– volume: 724
  start-page: 957
  year: 2010
  ident: 2021030920103477500_bib107
  publication-title: ApJ
  doi: 10.1088/0004-637X/724/2/957
– volume: 774
  start-page: 68
  year: 2013
  ident: 2021030920103477500_bib32
  publication-title: ApJ
  doi: 10.1088/0004-637X/774/1/68
– volume: 483
  start-page: 200
  year: 1997
  ident: 2021030920103477500_bib72
  publication-title: ApJ
  doi: 10.1086/304247
– volume: 476
  start-page: 1371
  year: 2018
  ident: 2021030920103477500_bib20
  publication-title: MNRAS
  doi: 10.1093/mnras/sty313
– volume: 1
  start-page: 241
  year: 2011
  ident: 2021030920103477500_bib105
  publication-title: IEEE Trans. Terahertz Sci. Technol.
  doi: 10.1109/TTHZ.2011.2159649
– volume: 68
  start-page: 46
  year: 2016
  ident: 2021030920103477500_bib79
  publication-title: PASJ
  doi: 10.1093/pasj/psw041
– volume: 787
  start-page: L17
  year: 2014
  ident: 2021030920103477500_bib86
  publication-title: ApJ
  doi: 10.1088/2041-8205/787/2/L17
– volume: 845
  start-page: 41
  year: 2017
  ident: 2021030920103477500_bib7
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa7eda
– volume: 815
  start-page: 18
  year: 2015
  ident: 2021030920103477500_bib55
  publication-title: ApJ
  doi: 10.1088/0004-637X/815/1/18
– volume: 52
  start-page: 415
  year: 2014
  ident: 2021030920103477500_bib71
  publication-title: ARA&A
  doi: 10.1146/annurev-astro-081811-125615
– volume: 777
  start-page: 66
  year: 2013
  ident: 2021030920103477500_bib1
  publication-title: ApJ
  doi: 10.1088/0004-637X/777/1/66
– volume: 488
  start-page: 2629
  year: 2019
  ident: 2021030920103477500_bib2
  publication-title: MNRAS
  doi: 10.1093/mnras/stz1887
– volume: 491
  start-page: L27
  year: 1997
  ident: 2021030920103477500_bib76
  publication-title: ApJ
  doi: 10.1086/311044
– volume: 450
  start-page: 3032
  year: 2015
  ident: 2021030920103477500_bib81
  publication-title: MNRAS
  doi: 10.1093/mnras/stv780
– volume: 837
  start-page: 97
  year: 2017
  ident: 2021030920103477500_bib70
  publication-title: ApJ
  doi: 10.3847/1538-4357/837/1/97
– volume: 833
  start-page: 72
  year: 2016
  ident: 2021030920103477500_bib12
  publication-title: ApJ
  doi: 10.3847/1538-4357/833/1/72
– volume: 740
  start-page: L15
  year: 2011
  ident: 2021030920103477500_bib74
  publication-title: ApJ
  doi: 10.1088/2041-8205/740/1/L15
– volume: 467
  start-page: 1300
  year: 2017
  ident: 2021030920103477500_bib110
  publication-title: MNRAS
  doi: 10.1093/mnras/stx180
– year: 2019
  ident: 2021030920103477500_bib84
– volume: 70
  start-page: S15
  year: 2018
  ident: 2021030920103477500_bib99
  publication-title: PASJ
  doi: 10.1093/pasj/psx107
– volume: 803
  start-page: 34
  year: 2015
  ident: 2021030920103477500_bib11
  publication-title: ApJ
  doi: 10.1088/0004-637X/803/1/34
– volume: 474
  start-page: 1
  year: 1997
  ident: 2021030920103477500_bib109
  publication-title: ApJ
  doi: 10.1086/303434
– volume: 819
  start-page: 129
  year: 2016
  ident: 2021030920103477500_bib87
  publication-title: ApJ
  doi: 10.3847/0004-637X/819/2/129
– year: 2018
  ident: 2021030920103477500_bib95
– volume: 590
  start-page: A31
  year: 2016
  ident: 2021030920103477500_bib19
  publication-title: A&A
  doi: 10.1051/0004-6361/201527514
– volume: 845
  start-page: 175
  year: 2017
  ident: 2021030920103477500_bib57
  publication-title: ApJ
  doi: 10.3847/1538-4357/aa7d0d
– volume: 475
  start-page: 2097
  year: 2018
  ident: 2021030920103477500_bib22
  publication-title: MNRAS
  doi: 10.1093/mnras/stx3227
– volume: 210
  start-page: 642
  year: 1976
  ident: 2021030920103477500_bib6
  publication-title: ApJ
  doi: 10.1086/154870
– volume: 577
  start-page: A80
  year: 2015
  ident: 2021030920103477500_bib85
  publication-title: A&A
  doi: 10.1051/0004-6361/201525644
– volume: 469
  start-page: 448
  year: 2017
  ident: 2021030920103477500_bib13
  publication-title: MNRAS
  doi: 10.1093/mnras/stx839
– volume: 465
  start-page: 2540
  year: 2017
  ident: 2021030920103477500_bib90
  publication-title: MNRAS
  doi: 10.1093/mnras/stw2847
– volume: 70
  start-page: L6
  year: 2018
  ident: 2021030920103477500_bib59
  publication-title: PASJ
  doi: 10.1093/pasj/psy087
– volume: 568
  start-page: A62
  year: 2014
  ident: 2021030920103477500_bib28
  publication-title: A&A
  doi: 10.1051/0004-6361/201322489
– volume: 810
  start-page: 71
  year: 2015
  ident: 2021030920103477500_bib43
  publication-title: ApJ
  doi: 10.1088/0004-637X/810/1/71
– volume: 626
  start-page: A23
  year: 2019
  ident: 2021030920103477500_bib24
  publication-title: A&A
  doi: 10.1051/0004-6361/201834457
– volume: 647
  start-page: 128
  year: 2006
  ident: 2021030920103477500_bib37
  publication-title: ApJ
  doi: 10.1086/505341
– volume: 624
  start-page: L13
  year: 2019
  ident: 2021030920103477500_bib69
  publication-title: A&A
  doi: 10.1051/0004-6361/201935149
– volume: 43
  start-page: 677
  year: 2005
  ident: 2021030920103477500_bib104
  publication-title: ARA&A
  doi: 10.1146/annurev.astro.43.051804.102221
– volume: 65
  start-page: 213
  year: 2013
  ident: 2021030920103477500_bib5
  publication-title: Earth Planets Space
  doi: 10.5047/eps.2012.04.014
– volume: 477
  start-page: 552
  year: 2018
  ident: 2021030920103477500_bib8
  publication-title: MNRAS
  doi: 10.1093/mnras/sty552
– start-page: A90
  volume-title: A&A
  year: 2020
  ident: 2021030920103477500_bib47
– volume: 528
  start-page: A88
  year: 2011
  ident: 2021030920103477500_bib48
  publication-title: A&A
  doi: 10.1051/0004-6361/201015465
– volume: 553
  start-page: 178
  year: 2018
  ident: 2021030920103477500_bib100
  publication-title: Nature
  doi: 10.1038/nature24631
– volume: 780
  start-page: 1
  year: 2018
  ident: 2021030920103477500_bib27
  publication-title: Phys. Rep.
  doi: 10.1016/j.physrep.2018.10.002
– volume-title: Galactic Dynamics
  year: 2008
  ident: 2021030920103477500_bib10
  doi: 10.1515/9781400828722
– volume: 855
  start-page: 105
  year: 2018
  ident: 2021030920103477500_bib88
  publication-title: ApJ
  doi: 10.3847/1538-4357/aab03f
– volume: 27
  start-page: 3
  year: 2019
  ident: 2021030920103477500_bib75
  publication-title: A&AR
  doi: 10.1007/s00159-018-0112-2
– volume: 869
  start-page: L22
  year: 2018
  ident: 2021030920103477500_bib111
  publication-title: ApJ
  doi: 10.3847/2041-8213/aaf4fa
– volume: 807
  start-page: 180
  year: 2015
  ident: 2021030920103477500_bib113
  publication-title: ApJ
  doi: 10.1088/0004-637X/807/2/180
– volume: 611
  start-page: A98
  year: 2018
  ident: 2021030920103477500_bib9
  publication-title: A&A
  doi: 10.1051/0004-6361/201731883
– volume: 819
  start-page: 114
  year: 2016
  ident: 2021030920103477500_bib61
  publication-title: ApJ
  doi: 10.3847/0004-637X/819/2/114
– volume: 792
  start-page: 34
  year: 2014
  ident: 2021030920103477500_bib89
  publication-title: ApJ
  doi: 10.1088/0004-637X/792/1/34
– volume: 53
  start-page: 385
  year: 2017
  ident: 2021030920103477500_bib39
  publication-title: RMxAA
– volume: 121
  start-page: 559
  year: 2009
  ident: 2021030920103477500_bib4
  publication-title: PASP
  doi: 10.1086/600092
– year: 2019
  ident: 2021030920103477500_bib52
– start-page: 44
  volume-title: Proc. Life Cycle of Dust in the Universe: Observations
  year: 2013
  ident: 2021030920103477500_bib31
– volume: 557
  start-page: 392
  year: 2018
  ident: 2021030920103477500_bib53
  publication-title: Nature
  doi: 10.1038/s41586-018-0117-z
– volume: 874
  start-page: 27
  year: 2019
  ident: 2021030920103477500_bib108
  publication-title: ApJ
  doi: 10.3847/1538-4357/ab0374
– volume: 820
  start-page: 98
  year: 2016
  ident: 2021030920103477500_bib66
  publication-title: ApJ
  doi: 10.3847/0004-637X/820/2/98
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Snippet ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large...
We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large...
ABSTRACT We report on the detection of the [C ii] 157.7 μm emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large...
We report on the detection of the [C II] 157.7 mu m emission from the Lyman break galaxy (LBG) MACS0416_Y1 at z = 8.3113, by using the Atacama Large...
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SubjectTerms Confidence limits
Continuum radiation
Cosmic dust
Dust
Galaxies
galaxies: formation
galaxies: high-redshift
galaxies: ISM
Interstellar matter
Interstellar radiation
Ionization
Luminosity
Photodissociation
Physical properties
Radio telescopes
Title ALMA uncovers the [C ii] emission and warm dust continuum in a z = 8.31 Lyman break galaxy
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https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-411003
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