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| [UTK2014] SSA22-Az14c , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST12:44:44 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
2014MNRAS.440.3462U 
|
15 | D | 1 | 157 | 23 | AzTEC/ASTE 1.1-mm survey of SSA22: Counterpart identification and photometric redshift survey of submillimetre galaxies. | UMEHATA H., TAMURA Y., KOHNO K., et al. | ||
| 2015ApJ...799...38K | 16 | D | 1 | 45 | 22 | NIR spectroscopic observation of massive galaxies in the protocluster at z = 3.09. | KUBO M., YAMADA T., ICHIKAWA T., et al. | ||
| 2015ApJ...815L...8U | 41 | X | 1 | 18 | 88 | ALMA deep field in SSA22: a concentration of dusty starbursts in a z = 3.09 protocluster core. | UMEHATA H., TAMURA Y., KOHNO K., et al. | ||
| 2016MNRAS.455.3333K | 488 | D | X C F | 11 | 25 | 15 | An extremely dense group of massive galaxies at the centre of the protocluster at z = 3.09 in the SSA22 field. | KUBO M., YAMADA T., ICHIKAWA T., et al. | |
| 2017ApJ...835...98U | 16 | D | 2 | 52 | 63 | ALMA deep field in SSA22: source catalog and number counts. | UMEHATA H., TAMURA Y., KOHNO K., et al. | ||
| 2017MNRAS.469.2235K | 1049 | D | X C | 26 | 20 | 5 | Bimodal morphologies of massive galaxies at the core of a protocluster at z = 3.09 and the strong size growth of a brightest cluster galaxy. | KUBO M., YAMADA T., ICHIKAWA T., et al. | |
| 2021ApJ...918...69U | 17 | D | 1 | 21 | 2 | ALMA observations of Lyα blob 1: multiple major mergers and widely distributed interstellar media. | UMEHATA H., SMAIL I., STEIDEL C.C., et al. | ||
| 2022ApJ...935...89K | 1985 | A | X C | 46 | 4 | 6 | An AGN with an Ionized Gas Outflow in a Massive Quiescent Galaxy in a Protocluster at z = 3.09. | KUBO M., UMEHATA H., MATSUDA Y., et al. | |
| 2025ApJ...985L...8U | 513 | A | D | X C | 11 | 12 | ~ | ADF22-WEB: Detection of a Molecular Gas Reservoir in a Massive Quiescent Galaxy Located in a z ≈ 3 Protocluster Core. | UMEHATA H., KUBO M. and NAKANISHI K. |
