VLT and NTT Observations of Two EIS Cluster Candidates. Detection of the Early-Type Galaxies Sequence at z~1
| dc.creator | da Costa, L. | |
| dc.creator | Scodeggio, M. | |
| dc.creator | Olsen, L. F. | |
| dc.creator | Nonino, M. | |
| dc.creator | Rengelink, R. | |
| dc.creator | Bender, R. | |
| dc.creator | Franx, M. | |
| dc.creator | Jorgensen, H. E. | |
| dc.creator | Renzini, A. | |
| dc.creator | Rosati, P. | |
| dc.date | 1999-01-19 | |
| dc.date.accessioned | 2026-07-07T02:30:04Z | |
| dc.date.available | 2026-07-07T02:30:04Z | |
| dc.description | Optical data from the ESO VLT-UT1 Science Verification observations are combined with near-infrared data from SOFI at the NTT to obtain optical-infrared color-magnitude diagrams for the objects in the fields of two EIS cluster candidates. In both cases, evidence is found for a well-defined sequence of red galaxies that appear to be significantly more clustered than the background population. These results suggest that the two systems are real physical associations. The (R-Ks), (I-Ks) and (J-Ks) colors of the red sequences are used, in conjunction with similar data for spectroscopically confirmed clusters, to obtain redshift estimates of z ~ 0.9 and z ~ 1.0 for these two systems. These results make these EIS cluster candidates prime targets for follow-up spectroscopic observations to confirm their reality and to measure more accurately their redshift. | |
| dc.description | 6 pages, 5 figures, to appear in Astronomy & Astrophysics (Special Letters Edition on "First Science with the VLT") | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9901248 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9901248 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/13705 | |
| dc.subject | Astrophysics | |
| dc.title | VLT and NTT Observations of Two EIS Cluster Candidates. Detection of the Early-Type Galaxies Sequence at z~1 | |
| dc.type | text |