𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Predicting the clustering properties of galaxy clusters detectable by the Planck satellite

✍ Scribed by L. Moscardini; M. Bartelmann; S. Matarrese; P. Andreani


Book ID
104467509
Publisher
John Wiley and Sons
Year
2002
Tongue
English
Weight
188 KB
Volume
335
Category
Article
ISSN
0035-8711

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Investigations of clusters of galaxies.
✍ F.W. Baier; K. Fritze; H. Tiersch; R. Ziener πŸ“‚ Article πŸ“… 1991 πŸ› John Wiley and Sons 🌐 English βš– 1008 KB

The structure of the centre of the galaxy cluster A 1795 and its surroundings, representing different cluster components, has been investigated in several wavelength ranges. A preferred orientation deviating about 10 -20" from the north-south direction has been found for all cluster components. The

The clustering properties of Luminous Re
✍ X.F. Deng; S.Y. Zou; J.Z. He; P. Jiang; X.X. Tang; X.X. Qian πŸ“‚ Article πŸ“… 2008 πŸ› John Wiley and Sons 🌐 English βš– 191 KB πŸ‘ 2 views
On the detectability of distant clusters
✍ R. Von Berlepsch; H.-E. FrΓΆhlich; K.-H. Schmidt πŸ“‚ Article πŸ“… 1987 πŸ› John Wiley and Sons 🌐 English βš– 231 KB πŸ‘ 2 views

J-magnitude limits (KRON'S J) which have to be reached to detect a cluster of galaxies of given redshift (up to z background of field galaxies are given. Grenzreichweiten in KRONS J-Band werden angegeben, die mindestens erreicht werden mussen, sol1 sich ein Galaxienhaufen vorgegebener Rotverschiebu