[SKO2012] SXDF-NB1006-2 , the SIMBAD biblio

[SKO2012] SXDF-NB1006-2 , the SIMBAD biblio (33 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST18:07:54


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Title First 3 Authors
2012ApJ...752..114S 1746     A D     X C       45 13 132 The first systematic survey for Lyα emitters at z = 7.3 with red-sensitive Subaru/Suprime-Cam. SHIBUYA T., KASHIKAWA N., OTA K., et al.
2012RAA....12..865F 77             C       1 33 14 Observations of the first light and the epoch of reionization. FAN X.
2013Natur.502..524F 12 9 226 A galaxy rapidly forming stars 700 million years after the Big Bang at redshift 7.51. FINKELSTEIN S.L., PAPOVICH C., DICKINSON M., et al.
2015A&A...584A..78C 45           X         1 6 69 ALMA constraints on the faint millimetre source number counts and their contribution to the cosmic infrared background. CARNIANI S., MAIOLINO R., DE ZOTTI G., et al.
2016Sci...352.1559I 24 7 172 Detection of an oxygen emission line from a high-redshift galaxy in the reionization epoch. INOUE A.K., TAMURA Y., MATSUO H., et al.
2017MNRAS.464..469S 41       D               1 11 281 Lyα and C III] emission in z = 7-9 Galaxies: accelerated reionization around luminous star-forming systems? STARK D.P., ELLIS R.S., CHARLOT S., et al.
2017MNRAS.467.1300V 254           X C F     4 3 31 Molecular cloud photoevaporation and far-infrared line emission. VALLINI L., FERRARA A., PALLOTTINI A., et al.
2017ApJ...846..105O viz 18       D               2 36 76 SIGAME simulations of the [C II], [O I] and [O III] line emission from star-forming galaxies at z ~= 6. OLSEN K., GREVE T.R., NARAYANAN D., et al.
2018ApJ...859...84H 17       D               1 87 105 SILVERRUSH. V. Census of Lyα, [O III] λ5007, Hα, and [C II] 158 µm line emission with ∼1000 LAEs at z = 4.9-7.0 revealed with Subaru/HSC. HARIKANE Y., OUCHI M., SHIBUYA T., et al.
2018MNRAS.478.1170C 101       D       C       3 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2019ApJ...874...27T 346           X C       7 12 154 Detection of the far-infrared [O III] and dust emission in a galaxy at redshift 8.312: early metal enrichment in the heart of the reionization era. TAMURA Y., MAWATARI K., HASHIMOTO T., et al.
2019A&A...624L..13L 45           X         1 14 54 Dust production scenarios in galaxies at z ∼6-8.3. LESNIEWSKA A. and MICHALOWSKI M.J.
2019A&A...626A..85O 184       D     X         5 22 ~ Starburst and post-starburst high-redshift protogalaxies. The feedback impact of high energy cosmic rays. OWEN E.R., WU K., JIN X., et al.
2019ApJ...881..124M 19       D               3 34 73 Resolved UV and [C II] structures of luminous galaxies within the epoch of reionization. MATTHEE J., SOBRAL D., BOOGAARD L.A., et al.
2019A&A...631A.167D viz 128           X C       2 10 32 A dense, solar metallicity ISM in the z = 4.2 dusty star-forming galaxy SPT 0418-47. DE BREUCK C., WEISS A., BETHERMIN M., et al.
2019PASJ...71...71H 23       D               2 31 193 Big Three Dragons: A z = 7.15 Lyman-break galaxy detected in [O III] 88 μm, [C II] 158 μm, and dust continuum with ALMA. HASHIMOTO T., INOUE A.K., MAWATARI K., et al.
2019PASJ...71..109H 85             C       3 25 33 Detections of [O III] 88 μm in two quasars in the reionization epoch. HASHIMOTO T., INOUE A.K., TAMURA Y., et al.
2020MNRAS.493.4294B 91           X         2 14 97 ALMA uncovers the [C II] emission and warm dust continuum in a z = 8.31 Lyman break galaxy. BAKX T.J.L.C., TAMURA Y., HASHIMOTO T., et al.
2020ApJ...896...93H 62       D     X         2 50 106 Large population of ALMA galaxies at z > 6 with very high [O III] 88 µm to [C II] 158 µm flux ratios: evidence of extremely high ionization parameter or PDR deficit? HARIKANE Y., OUCHI M., INOUE A.K., et al.
2020ApJ...903..150J 273       D     X C       6 32 41 The mass-metallicity relation at z ≃ 8: direct-method metallicity constraints and near-future prospects. JONES T., SANDERS R., ROBERTS-BORSANI G., et al.
2020MNRAS.499.3417Y 272       D     X   F     6 9 ~ An analytic model for [O III] fine structure emission from high redshift galaxies. YANG S. and LIDZ A.
2020MNRAS.499.5136C 489       D S   X C F     9 14 65 Missing [C II] emission from early galaxies. CARNIANI S., FERRARA A., MAIOLINO R., et al.
2021A&A...646A..26B 740           X C F     15 16 ~ A puzzling non-detection of [O III] and [C II] from a z ≃ 7.7 galaxy observed with ALMA. BINGGELI C., INOUE A.K., HASHIMOTO T., et al.
2021MNRAS.504..723Y 696     A D     X C F     15 10 ~ The prospects for observing [O III] 52 micron emission from galaxies during the Epoch of Reionization. YANG S., LIDZ A. and POPPING G.
2021MNRAS.505.5543V 454       D     X   F     10 15 29 High [O III]/[C II] surface brightness ratios trace early starburst galaxies. VALLINI L., FERRARA A., PALLOTTINI A., et al.
2022MNRAS.510.5603K 111       D         F     2 9 29 The nature of high [O III]_88 µ m_/[C II]_158 µm_ galaxies in the epoch of reionization: Low carbon abundance and a top-heavy IMF? KATZ H., ROSDAHL J., KIMM T., et al.
2022MNRAS.513.3122S 91             C       1 30 49 The ALMA REBELS Survey: cosmic dust temperature evolution out to z ∼ 7. SOMMOVIGO L., FERRARA A., PALLOTTINI A., et al.
2022ApJ...931..160B 109       D       C       2 50 96 Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe. BOUWENS R.J., SMIT R., SCHOUWS S., et al.
2022MNRAS.515.3126I viz 108       D         F     3 46 45 The ALMA REBELS Survey: dust continuum detections at z > 6.5. INAMI H., ALGERA H.S.B., SCHOUWS S., et al.
2022ApJ...935..119S 136           X         3 4 9 Bridging Optical and Far-infrared Emission-line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 μm/SFR at z > 6. SUGAHARA Y., INOUE A.K., FUDAMOTO Y., et al.
2022ApJ...941...74O 90           X         2 11 ~ ALMA Observations of CO Emission from Luminous Lyman-break Galaxies at z = 6.0293-6.2037. ONO Y., FUJIMOTO S., HARIKANE Y., et al.
2023ApJ...945...69R 48           X         1 3 3 Updated Measurements of [O III] 88 μm, [C II] 158 μm, and Dust Continuum Emission from a z = 7.2 Galaxy. REN Y.W., FUDAMOTO Y., INOUE A.K., et al.
2023ApJ...948....3U 187           X C       3 9 ~ Detections of [C II] 158 μm and [O III] 88 μm in a Local Lyman Continuum Emitter, Mrk 54, and Its Implications to High-redshift ALMA Studies. URA R., HASHIMOTO T., INOUE A.K., et al.

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