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[CLM2003] J022802.97-041618.3 , the SIMBAD biblio (24 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST04:25:56 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
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 | 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 | 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 | 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 | 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 | 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 | 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. |