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| CANDELS COSMOS F160W J100026.36+021346.7 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST17:51:45 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 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. | ||
2014ApJS..214...24S 
|
15 | D | 1 | 97940 | 733 | 3D-HST WFC3-selected photometric catalogs in the five CANDELS/3D-HST fields: photometry, photometric redshifts, and stellar masses. | SKELTON R.E., WHITAKER K.E., MOMCHEVA I.G., et al. | ||
|
2015ApJ...803...34B
|
16 | D | 1 | 10313 | 1045 | UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields. | BOUWENS R.J., ILLINGWORTH G.D., OESCH P.A., 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. | ||
|
2016ApJ...830...51S
|
16 | D | 1 | 67525 | 168 | The FourStar galaxy evolution survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z ∼ 3.5. | STRAATMAN C.M.S., SPITLER L.R., QUADRI R.F., et al. | ||
|
2017ApJS..228....7N
|
16 | D | 1 | 37352 | 95 | CANDELS multi-wavelength catalogs: source identification and photometry in the CANDELS COSMOS Survey Field. | NAYYERI H., HEMMATI S., MOBASHER B., 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. | ||
|
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. |
