[PNL2019] 191313 , the SIMBAD biblio

[PNL2019] 191313 , the SIMBAD biblio (33 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST09:57:49


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Title First 3 Authors
2013AJ....145....4W 15       D               1 45 51 An exponential decline at the bright end of the z = 6 galaxy luminosity function. WILLOTT C.J., McLURE R.J., HIBON P., et al.
2015ApJ...807..180W 1192       D S   X C       29 11 148 Star formation and the interstellar medium in z > 6 UV-luminous Lyman-break galaxies. WILLOTT C.J., CARILLI C.L., WAGG J., et al.
2016ApJ...829L..11P 46           X         1 9 133 Tracing the reionization epoch with ALMA: [C II] emission in z ∼ 7 galaxies. PENTERICCI L., CARNIANI S., CASTELLANO M., et al.
2017MNRAS.465.3475W 40           X         1 4 6 Dust evolution processes in normal galaxies at z > 6 detected by ALMA. WANG W.-C., HIRASHITA H. and HOU K.-C.
2017ApJ...845..175J 839     A D     X C       21 2 20 Galaxy formation through filamentary accretion at z = 6.1. JONES G.C., WILLOTT C.J., CARILLI C.L., et al.
2017ApJ...846..105O viz 17       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.
2017ApJ...847...21F 95       D     X         3 47 93 Are high-redshift galaxies hot? Temperature of z > 5 galaxies and implications for their dust properties. FAISST A.L., CAPAK P.L., YAN L., et al.
2017ApJ...850..108W 43           X         1 9 71 A wide dispersion in star formation rate and dynamical mass of 108 solar mass black hole host galaxies at redshift 6. WILLOTT C.J., BERGERON J. and OMONT A.
2017ApJ...850..180J 41           X         1 19 47 Dynamical characterization of galaxies at z ∼ 4-6 via tilted ring fitting to ALMA [C II] observations. JONES G.C., CARILLI C.L., SHAO Y., et al.
2017MNRAS.471.2143L 16       D               1 21 ~ [C I], [C II] and CO emission lines as a probe for α variations at low and high redshifts. LEVSHAKOV S.A., NG K.-W., HENKEL C., et al.
2018MNRAS.473.5363W 202           X   F     4 11 16 Dust-obscured star-forming galaxies in the early universe. WILKINS S.M., FENG Y., DI MATTEO T., et al.
2017MNRAS.472..772M viz 16       D               1 48 66 Spectroscopic properties of luminous Ly α emitters at z ~= 6-7 and comparison to the Lyman-break population. MATTHEE J., SOBRAL D., DARVISH B., et al.
2018A&A...609A.130L viz 2 50 132 The [CII] 158 µm line emission in high-redshift galaxies. LAGACHE G., COUSIN M. and CHATZIKOS M.
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 18       D               3 41 108 Kiloparsec-scale gaseous clumps and star formation at z = 5-7. CARNIANI S., MAIOLINO R., AMORIN R., et al.
2019ApJ...871..109P 138       D     X         4 28 1 Multiband optical and near-infrared properties of faint submillimeter galaxies with serendipitous ALMA detections. PATIL P., NYLAND K., LACY M., et al.
2019MNRAS.487.3007K 18       D               1 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., et al.
2019ApJ...881..124M 17       D               3 37 73 Resolved UV and [C II] structures of luminous galaxies within the epoch of reionization. MATTHEE J., SOBRAL D., BOOGAARD L.A., et al.
2019ApJ...887..107F 183       D     X C       4 20 93 First identification of 10 kpc [C II] 158 µm halos around star-forming galaxies at z = 5-7. FUJIMOTO S., OUCHI M., FERRARA A., et al.
2019PASJ...71...71H 144       D     X         4 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.
2020ApJ...889...98M 305       D     X         8 6 ~ Investigating overdensities around z > 6 galaxies through ALMA observations of [C II]. MILLER T.B., CHAPMAN S.C., HAYWARD C.C., et al.
2020A&A...637A..32B 16       D               4 50 30 Observational and theoretical constraints on the formation and early evolution of the first dust grains in galaxies at 5 < z < 10. BURGARELLA D., NANNI A., HIRASHITA H., et al.
2020A&A...637A..84P 17       D               1 32 48 The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies. PENSABENE A., CARNIANI S., PERNA M., et al.
2020ApJ...896...93H 18       D               1 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.
2020A&A...641A.168N viz 16       D               1 48 34 The gas, metal, and dust evolution in low-metallicity local and high-redshift galaxies. NANNI A., BURGARELLA D., THEULE P., et al.
2022A&A...664A..73B viz 17       D               1 113 8 The ALMA-ALPINE [CII] survey. The star formation history and the dust emission of star-forming galaxies at 4.5 < z < 6.2. BURGARELLA D., BOGDANOSKA J., NANNI A., et al.
2022MNRAS.517.5642E 102       D     X         3 31 29 The REBELS ALMA Survey: efficient Ly α transmission of UV-bright z ≃ 7 galaxies from large velocity offsets and broad line widths. ENDSLEY R., STARK D.P., BOUWENS R.J., et al.
2023MNRAS.518..691J 44           X         1 34 4 Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations. JONES G.C., MAIOLINO R., CIRCOSTA C., et al.
2023A&A...679A.131R viz 44         O X         1 138 ~ Diagnosing the interstellar medium of galaxies with far-infrared emission lines II. [C II], [O I], [O III], [N II], and [N III] up to z = 6. RAMOS PADILLA A.F., WANG L., VAN DER TAK F.F.S., et al.
2024MNRAS.528..499L 18       D               1 192 ~ [C II] 158 μm emission as an indicator of galaxy star formation rate. LIANG L., FELDMANN R., MURRAY N., et al.
2024A&A...684A..84S 45           X         1 36 ~ JADES: The production and escape of ionizing photons from faint Lyman-alpha emitters in the epoch of reionization. SAXENA A., BUNKER A.J., JONES G.C., et al.
2024ApJ...971..161M 18       D               2 39 ~ SERENADE. II. An ALMA Multiband Dust Continuum Analysis of 28 Galaxies at 5 < z < 8 and the Physical Origin of the Dust Temperature Evolution. MITSUHASHI I., HARIKANE Y., BAUER F.E., et al.
2024MNRAS.534.2062V 18       D               1 72 ~ Characterising the contribution of dust-obscured star formation at ≳ 5 using 18 serendipitously identified [C II] emitters. VAN LEEUWEN I.F., BOUWENS R.J., VAN DER WERF P.P., et al.

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