1998/07/15 by L. F. Olsen, M. Scodeggio, Olsen, L. F. +27
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9807156
5 pages, 2 figures, submitted to Astronomy and Astrophysics Letters
arxiv created 1998/07/15 · openalex publication_date 1998/07/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
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