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| [APS2019] 5 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:16:06 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
1992ApJS...78....1D 
|
1977 | 309 | Spectroscopy of galaxies in distant clusters. IV. A catalog of photometry and spectroscopy for galaxies in seven clusters with O.35<z< 0.55 | DRESSLER A. and GUNN J.E. | |||||
|
2003ApJ...591...53T
|
2218 | 326 | A wide-field Hubble Space Telescope study of the cluster Cl 0024+16 at z=0.4. I. Morphological distributions to 5Mpc radius. | TREU T., ELLIS R.S., KNEIB J.-P., et al. | |||||
|
2005ApJ...634..977M
|
15 | D | 1338 | 69 | A Wide-Field Hubble Space Telescope survey of the cluster Cl 0024+16 at z=0.4. III. Spectroscopic signatures of environmental evolution in early-type galaxies. | MORAN S.M., ELLIS R.S., TREU T., et al. | |||
|
2007ApJ...671.1503M
|
15 | D | 1 | 1763 | 183 | A wide-field survey of two z ∼ 0.5 galaxy clusters: identifying the physical processes responsible for the observed transformation of spirals into S0s. | MORAN S.M., ELLIS R.S., TREU T., et al. | ||
|
2015A&A...578A..30S
|
16 | D | 1 | 169 | 3 | GLACE survey: OSIRIS/GTC tuneable filter Hα imaging of the rich galaxy cluster Zw Cl0024.0+1652 at z=0.395. I. Survey presentation, TF data reduction techniques, and catalogue. | SANCHEZ-PORTAL M., PINTOS-CASTRO I., PEREZ-MARTINEZ R., et al. | ||
|
2018ApJ...856...15L
|
16 | D | 1 | 62 | 8 | Evolution of the stellar mass-metallicity relation. I. Galaxies in the z ∼ 0.4 cluster Cl0024. | LEETHOCHAWALIT N., KIRBY E.N., MORAN S.M., et al. | ||
|
2019MNRAS.485.1528A
|
16 | D | 1 | 233 | ~ | A morphological study of galaxies in ZwCl0024+1652, a galaxy cluster at redshift z ∼ 0.4. | AMADO Z.B., POVIC M., SANCHEZ-PORTAL M., et al. | ||
|
2021MNRAS.501.2430B
|
17 | D | 1 | 81 | ~ | GLACE survey: Galaxy activity in ZwCl0024+1652 cluster from strong optical emission lines. | BEYORO-AMADO Z., SANCHEZ-PORTAL M., BONGIOVANNI A., et al. |
