MUNICS S2F1 511 , the SIMBAD biblio

MUNICS S2F1 511 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:36:55


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in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2005MNRAS.357L..40S 2 9 74 The density of very massive evolved galaxies to z≃ 1.7. 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 26       D               1 10 233 Extremely compact massive galaxies at z ∼ 1.4. TRUJILLO I., FEULNER G., GORANOVA Y., et al.
2007MNRAS.374..614L 5 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 98       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 viz 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.
2015A&A...573A.110G 56       D     X         2 19 2 Lower mass normalization of the stellar initial mass function for dense massive early-type galaxies at z ∼ 1.4. GARGIULO A., SARACCO P., LONGHETTI M., et al.
2016A&A...592A.132G 136       D     X C       3 26 5 Ultramassive dense early-type galaxies: Velocity dispersions and number density evolution since z = 1.6. GARGIULO A., SARACCO P., TAMBURRI S., et al.

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