GroupMtg.numbers-Program 12 Dec
CURRICULUM VITAE
Alexis Finoguenov (@finoguenov) / X
A Deficit Of Faint Red Galaxies In The Possible Large-Scale Structures Around The RDCS J1252.9-2927 Cluster At Z=1.24 | Masayuki Tanaka,Tadayuki Kodama,Masaru Kajisawa,Richard Bower,Ricardo Demarco,Alexis Finoguenov,Chris Lidman,Piero Rosati
Alexis Finoguenov — University of Helsinki
XMM-Newton surveys of X-ray galaxy groups Alexis Finoguenov MPE/UMBC+ S.Giodini, V.Allevato, M. Tanaka, A. Leauthaud, O. Ilbert, N.Cappelluti, J.Silverman, - ppt download
CCE - II Virtual Edition - 11 de novembro - YouTube
MeerKAT picks up shock wave extending 6.5m light years | ITWeb
OSEL.CZ - detail obr�zku
Ein alter Haufen im jungen Universum | Max-Planck-Institut für extraterrestrische Physik
Alexey Finogenov | People finder | University of Helsinki
Brightest group galaxies – II: the relative contribution of BGGs to the total baryon content of groups at z < 1.3 - UTUPub
Milena Oksanen - Sirkustaiteilija
PPT - COSMIC MAGNIFICATION the other weak lensing signal PowerPoint Presentation - ID:4711611
Alexis Finoguenov - Prof. - University of Helsinki | LinkedIn
Clustering, host halos, and environment of z 2 galaxies as a function of their physical properties
Suomen tähtitieteilijäseura ry
Vermisste Materie gefunden - wissenschaft.de
List of participants
Alexis Finoguenov - Prof. - University of Helsinki | LinkedIn
What IGM knows about the star-formation... An X-ray perspective.
Turbulence measurements in clusters of galaxies with XMM-Newton
