Measuring the cosmic web
| dc.bibliographicCitation.firstPage | 259 | eng |
| dc.bibliographicCitation.issue | 2 | eng |
| dc.bibliographicCitation.journalTitle | Baltic Astronomy | eng |
| dc.bibliographicCitation.volume | 20 | eng |
| dc.contributor.author | Müller, V. | |
| dc.contributor.author | Hoffmann, K. | |
| dc.contributor.author | Nuza, S.E. | |
| dc.date.accessioned | 2020-09-11T12:52:58Z | |
| dc.date.available | 2020-09-11T12:52:58Z | |
| dc.date.issued | 2011 | |
| dc.description.abstract | A quantitative study of the clustering properties of the cosmic web as a function of absolute magnitude and color is presented using the SDSS Data Release 7 galaxy survey. Mark correlations are included in the analysis. We compare our results with mock galaxy samples obtained with four different semi-analytical models of galaxy formation imposed on the merger trees of the Millenium simulation. The clustering of both red and blue galaxies is studied separately. | eng |
| dc.description.version | publishedVersion | eng |
| dc.identifier.uri | https://doi.org/10.34657/4273 | |
| dc.identifier.uri | https://oa.tib.eu/renate/handle/123456789/5644 | |
| dc.language.iso | eng | eng |
| dc.publisher | Vilnius : Lithuanian Astronomical Union | eng |
| dc.relation.doi | https://doi.org/10.1515/astro-2017-0290 | |
| dc.relation.issn | 1392-0049 | |
| dc.rights.license | CC BY-NC-ND 4.0 Unported | eng |
| dc.rights.uri | https://creativecommons.org/licenses/by-nc-nd/4.0/ | eng |
| dc.subject.ddc | 550 | eng |
| dc.subject.other | Cosmology: Observations - Cosmology: Theory | eng |
| dc.subject.other | Galaxies: Statistics | eng |
| dc.subject.other | Large scale structure of the Universe | eng |
| dc.title | Measuring the cosmic web | eng |
| dc.type | Article | eng |
| dc.type | Text | eng |
| tib.accessRights | openAccess | eng |
| wgl.contributor | AIP | eng |
| wgl.subject | Geowissenschaften | eng |
| wgl.type | Zeitschriftenartikel | eng |