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Determining Cosmic Microwave Background Structure from Its Peak Distribution
Kashlinsky et al. 2001 The Astrophysical Journal Letters 557 L1.
Caption: Fig. 2.
All‐sky distribution of pixels with ﹩\nu =2﹩ for the SCDM model
© 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
