ESO Imaging Survey V. Cluster Search using Color Data
| dc.creator | Olsen, L. F. | |
| dc.creator | Scodeggio, M. | |
| dc.creator | da Costa, L. | |
| dc.creator | Slijkhuis, R. | |
| dc.creator | Benoist, C. | |
| dc.creator | Bertin, E. | |
| dc.creator | Deul, E. | |
| dc.creator | Erben, T. | |
| dc.creator | Guarnieri, M. D. | |
| dc.creator | Hook, R. | |
| dc.creator | Nonino, M. | |
| dc.creator | Prandoni, I. | |
| dc.creator | Wicenec, A. | |
| dc.creator | Zaggia, S. | |
| dc.date | 1998-07-15 | |
| dc.date.accessioned | 2026-07-07T02:27:24Z | |
| dc.date.available | 2026-07-07T02:27:24Z | |
| dc.description | This paper presents 19 additional candidate clusters detected using the galaxy catalog extracted from the I-band images taken for the ESO Imaging Survey (EIS). The candidates are found over a region of 1.1 square degrees, located near the South Galactic Pole. Combined with the sample reported earlier, the number of candidates in the Southern Galactic Cap is now 54 over a total area of 3.6 square degrees. Images in V band are also available over 2.7 square degrees, and galaxy catalogs extracted from them over a uniform area of 2 square degrees have been used to further explore the reality of the I cluster candidates. Nearly all the I candidates with estimated redshifts <~ 0.5 are also identified in V. At higher redshifts, only rich candidates are detected in both bands. | |
| dc.description | 5 pages, 2 figures, submitted to Astronomy and Astrophysics Letters | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9807156 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9807156 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/12679 | |
| dc.subject | Astrophysics | |
| dc.title | ESO Imaging Survey V. Cluster Search using Color Data | |
| dc.type | text |