[CLM2003] J022802.97-041618.3 , the SIMBAD biblio

[CLM2003] J022802.97-041618.3 , the SIMBAD biblio (24 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST04:25:56


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Title First 3 Authors
2003A&A...405L..19C 2 5 40 Discovery of a z = 6.17 galaxy from CFHT and VLT observations. CUBY J.-G., LE FEVRE O., McCRACKEN H., et al.
2015ApJ...807..180W 1253       D S   X C       30 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.
2017MNRAS.465.3475W 342       D     X C       8 4 6 Dust evolution processes in normal galaxies at z > 6 detected by ALMA. WANG W.-C., HIRASHITA H. and HOU K.-C.
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.
2017ApJ...847...21F 98       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.
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 248           X   F     5 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 17       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.
2019MNRAS.487.3007K 19       D               2 26 66 Kinematics of z >= 6 galaxies from [C II] line emission. KOHANDEL M., PALLOTTINI A., FERRARA A., 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.
2019ApJ...887..107F 21       D               1 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 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.
2020ApJ...889...98M 528       D     X C       12 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 17       D               1 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 18       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 19       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 17       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.
2022ApJS..259...20H viz 18       D               1 1042 83 GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. HARIKANE Y., ONO Y., OUCHI M., et al.
2022MNRAS.517.5642E 108       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.
2023A&A...673A.153P 205       D       C F     4 12 1 ALMA hints at the presence of turbulent disk galaxies at z > 5. PARLANTI E., CARNIANI S., PALLOTTINI A., et al.
2023A&A...679A.131R viz 93         O X         2 138 ~ 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.

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