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| COSMOS2015 214169 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST21:04:08 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2009ApJ...696..546S 
|
15 | D | 1 | 86 | 28 | Photometric properties of Lyα emitters at z∼4.86 in the COSMOS 2 square degree field. | SHIOYA Y., TANIGUCHI Y., SASAKI S.S., et al. | ||
|
2012ApJ...760..128M
|
15 | D | 1 | 235 | 51 | Lyα emission from high-redshift sources in COSMOS. | MALLERY R.P., MOBASHER B., CAPAK P., et al. | ||
|
2015ApJ...815...57U
|
16 | D | 1 | 306 | 7 | A correlation between Lyα spectral line profile and rest-frame UV morphology. | U V., HEMMATI S., DARVISH B., et al. | ||
| 2016ApJ...819...25K | 94 | D | F | 2 | 63 | 9 | Morphological properties of Lyα emitters at redshift 4.86 in the cosmos field: clumpy star formation or merger? | KOBAYASHI M.A.R., MURATA K.L., KOEKEMOER A.M., et al. | |
|
2018ApJ...858...77H
|
16 | D | 1 | 7945 | 125 | The DEIMOS 10k spectroscopic survey catalog of the COSMOS field. | HASINGER G., CAPAK P., SALVATO M., et al. | ||
|
2021ApJ...911...78O
|
17 | D | 1 | 181 | 17 | SILVERRUSH X: machine learning-aided selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS survey data. | ONO Y., ITOH R., SHIBUYA T., et al. | ||
|
2022ApJS..259...20H
|
17 | 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. | ||
|
2023ApJS..268...24K
|
17 | D | 1 | 289 | ~ | SILVERRUSH. XIII. A Catalog of 20,567 Lyα Emitters at z = 2-7 Identified in the Full-depth Data of the Subaru/HSC-SSP and CHORUS Surveys. | KIKUTA S., OUCHI M., SHIBUYA T., et al. |
