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| COSMOS2015 431680 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:06:59 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2010MNRAS.401..933M | 93 | D | F | 3 | 14 | 106 | High-redshift elliptical galaxies: are they (all) really compact | MANCINI C., DADDI E., RENZINI A., et al. | |
| 2012ApJ...755...26O | 16 | D | 1 | 37 | 129 | Deep near-infrared spectroscopy of passively evolving galaxies at z ≳ 1.4. | ONODERA M., RENZINI A., CAROLLO M., et al. | ||
2013ApJS..206....8M 
|
15 | D | 1 | 208367 | 332 | A public Ks-selected catalog in the COSMOS/ULTRAVISTA field: photometry, photometric redshifts, and stellar population parameters. | MUZZIN A., MARCHESINI D., STEFANON M., et al. | ||
|
2013A&A...556A..55I
|
15 | D | 1 | 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. | ||
| 2015ApJ...806L..20S | 1638 | S X C | 40 | 14 | 10 | A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43. | SARGENT M.T., DADDI E., BOURNAUD F., et al. | ||
| 2015ApJ...808..161O | 17 | D | 1 | 26 | 94 | The ages, metallicities, and element abundance ratios of massive quenched galaxies at z = 1.6. | ONODERA M., CAROLLO C.M., RENZINI A., et al. | ||
|
2020ApJ...905..103X
|
16 | D | 1 | 21135 | ~ | A large massive quiescent galaxy sample at z ∼ 1.2. | XU H., DAI Y.S., HUANG J.-S., et al. | ||
|
2022ApJ...925...34C
|
17 | D | 1 | 208670 | 12 | Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey. | CUTLER S.E., WHITAKER K.E., MOWLA L.A., et al. | ||
| 2024MNRAS.527.9529L | 18 | D | 1 | 26 | ~ | High dust content of a quiescent galaxy at z ∼ 2 revealed by deep ALMA observation. | LEE M.M., STEIDEL C.C., BRAMMER G., et al. |
