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Citation: A. Kashlinsky et al., Determining cosmic microwave background structure from its peak distribution, ASTROPHYS J, 557(1), 2001, pp. L1-L5

Authors: Kashlinsky, A Odenwald, S

Citation: A. Kashlinsky et S. Odenwald, Looking behind the stars, SCIENCE, 289(5477), 2000, pp. 246-247

Authors: Kashlinsky, A Atrio-Barandela, F

Citation: A. Kashlinsky et F. Atrio-barandela, Measuring cosmological bulk flows via the kinematic Sunyaev-Zeldovich effect in the upcoming cosmic microwave background maps, ASTROPHYS J, 536(2), 2000, pp. L67-L71

Authors: Kashlinsky, A Odenwald, S

Citation: A. Kashlinsky et S. Odenwald, Clustering of the diffuse infrared light from the COBE DIRBE maps. III. Power spectrum analysis and excess isotropic component of fluctuations, ASTROPHYS J, 528(1), 2000, pp. 74-95

Authors: Jimenez, R Kashlinsky, A

Citation: R. Jimenez et A. Kashlinsky, Galaxy evolution, deep galaxy counts, and the near-infrared cosmic infrared background, ASTROPHYS J, 511(1), 1999, pp. 16-33

Authors: Kashlinsky, A

Citation: A. Kashlinsky, Determining Omega from the cluster correlation function, PHYS REPORT, 307(1-4), 1998, pp. 67-73