Preliminary Results from the ESO Slice Project (ESP)
| dc.creator | Vettolani, G. | |
| dc.creator | Zucca, E. | |
| dc.creator | Cappi, A. | |
| dc.creator | Merighi, R. | |
| dc.creator | Mignoli, M. | |
| dc.creator | Stirpe, G. | |
| dc.creator | Zamorani, G. | |
| dc.creator | Collins, C. | |
| dc.creator | MacGillivray, H. | |
| dc.creator | Balkowski, C. | |
| dc.creator | Alimi, J. | |
| dc.creator | Blanchard, A. | |
| dc.creator | Cayatte, V. | |
| dc.creator | Felenbok, P. | |
| dc.creator | Maurogordato, S. | |
| dc.creator | Proust, D. | |
| dc.creator | Chincarini, G. | |
| dc.creator | Guzzo, L. | |
| dc.creator | Maccagni, D. | |
| dc.creator | Scaramella, R. | |
| dc.creator | Ramella, M. | |
| dc.date | 1993-12-14 | |
| dc.date.accessioned | 2026-07-07T02:19:01Z | |
| dc.date.available | 2026-07-07T02:19:01Z | |
| dc.description | We present the first results of a galaxy redshift survey, ESO Slice Project (ESP), we are accomplishing as an ESO Key--Project over about 40 square degrees in a region near the South Galactic Pole. The limiting magnitude is $b_J = 19.4$. Up to now $\sim 85\%$ of the observations has been completed and $\sim 65\%$ of the data has been reduced providing $\sim 2000$ galaxy redshifts. We present some preliminary results concerning the large scale galaxy distribution, the luminosity function and the properties of galaxies with spectra showing prominent emission lines. | |
| dc.description | Proc. of Schloss Rindberg workshop (October 1993) Studying the Universe with Clusters of Galaxies Plain TeX, figures upon request (contact zucca@astbo1.bo.cnr.it) BAP 12-1993-042-IRA | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9312029 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9312029 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/9707 | |
| dc.subject | Astrophysics | |
| dc.title | Preliminary Results from the ESO Slice Project (ESP) | |
| dc.type | text |