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| MUNICS S7F5 45 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST18:04:04 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2003A&A...398..127S | 3 | 3 | 35 | Massive z∼1.3 evolved galaxies revealed. | SARACCO P., LONGHETTI M., SEVERGNINI P., et al. | ||||
| 2005MNRAS.361..897L | 10 | 29 | Dating the stellar population in massive early-type galaxies at z∼ 1.5. | LONGHETTI M., SARACCO P., SEVERGNINI P., et al. | |||||
| 2006MNRAS.373L..36T | 22 | D | 1 | 10 | 233 | Extremely compact massive galaxies at z ∼ 1.4. | TRUJILLO I., FEULNER G., GORANOVA Y., et al. | ||
| 2007MNRAS.374..614L | 3 | 12 | 139 | The Kormendy relation of massive elliptical galaxies at z ∼ 1.5: evidence for size evolution. | LONGHETTI M., SARACCO P., SEVERGNINI P., et al. | ||||
| 2009MNRAS.392..718S | 16 | D | 2 | 35 | 79 | The population of early-type galaxies at 1 < z < 2 - new clues on their formation and evolution. | SARACCO P., LONGHETTI M. and ANDREON S. | ||
| 2009ApJ...695..101D | 97 | D | F | 4 | 19 | 289 | Red nuggets at z ∼ 1.5: compact passive galaxies and the formation of the Kormendy relation. | DAMJANOV I., McCARTHY P.J., ABRAHAM R.G., et al. | |
| 2011MNRAS.412.2707S | 15 | D | 1 | 28 | 44 | Constraining the star formation and the assembly histories of normal and compact early-type galaxies at 1 < z < 2. | SARACCO P., LONGHETTI M. and GARGIULO A. | ||
2011ApJ...739L..44D 
|
15 | D | 1 | 417 | 135 | Red nuggets at high redshift: structural evolution of quiescent galaxies over 10 Gyr of cosmic history. | DAMJANOV I., ABRAHAM R.G., GLAZEBROOK K., et al. | ||
| 2022MNRAS.514.3410H | 43 | X | 1 | 152 | 7 | Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets. | HON D.S.-H., GRAHAM A.W., DAVIS B.L., et al. |
