
handle: 10261/384565
In this work we show how well can the cosmological parameters be constrained using galaxy cluster data. We also show how in the process of fitting the model which attempts to describe the data it is possible to get some information about the cluster scaling relations T − M and Lx −T. Among other conclusions we found that only low density universes (Ω ≈ 0.3 with or without Λ) are compatible with recent data sets. These constraints will be improved with future SZ data.
This work has been supported by the Spanish DGESIC Project PB98-0531-C02-01, FEDER Project 1FD97-1769-C04-01, the EU project INTAS-OPEN-97-1192, and the RTN of the EU project HPRN-CT-2000-00124. JMD acknowledges support from a Spanish MEC fellowship FP96-20194004 and financial support from the University of Cantabria.
Peer reviewed
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 0 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
