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| COSMOS2015 596366 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST19:37:41 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 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. | ||
2013A&A...556A..55I 
|
15 | D | 2 | 259207 | 819 | Mass assembly in quiescent and star-forming galaxies since z ≃ 4 from UltraVISTA. | ILBERT O., McCRACKEN H.J., LE FEVRE O., et al. | ||
| 2015MNRAS.452.1817B | 44 | X | 1 | 14 | 161 | The galaxy luminosity function at z~= 6 and evidence for rapid evolution in the bright end from z~=7 to 5. | BOWLER R.A.A., DUNLOP J.S., McLURE R.J., et al. | ||
|
2017MNRAS.472..772M
|
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. | ||
|
2018PASJ...70S..10O
|
16 | D | 1 | 365 | 182 | Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV luminosity functions at z ∼ 4-7 derived with the half-million dropouts on the 100 deg2 sky. | ONO Y., OUCHI M., HARIKANE Y., et al. | ||
| 2019ApJ...887..107F | 264 | D | X C | 6 | 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. | |
| 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. | ||
|
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. | ||
| 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. | ||
| 2024ApJ...963...51F | 18 | D | 1 | 50 | ~ | The Magellan M2FS Spectroscopic Survey of High-redshift Galaxies: The Brightest Lyman-break Galaxies at z ∼ 6. | FU S., JIANG L., NING Y., 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. |
