... 000, 1ґ12 (2009) Printed 11 February 2010 A (MN L TEX style file v2.2) Analytical approximations of K -corrections in optical and near-infrared bands I1gor V. Chilingarian1 2 ,2,3 , Anne-Laure Melchior 1,4 and Ivan Yu. ... Received 2010 February 01; in original form 2009 August 14 ABSTRACT To compare photometric properties of galaxies at different redshifts, the fluxes need to be corrected for the changes of effective rest-frame wavelengths of filter bandpasses, called K -corrections. ... Table 1. ...

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... For full UV energy Euv (erg) radiated in TLE the corresponding number of photons of wavelength =300-400 nm (with average energy 3.5 eV) is: Nph=Euv/3.5в1.6 10-12 (1) We considered 2 options of the pinhole camera focal distance: 1. focal distance is short so that the circle of diameter 40 km is observed by one pixel and 2. focal distance is long so that the 40 km circle is observed in many camera pixels. ... Full energy released in UV in the atmosphere is determined by the pixel signal. ...

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... This area of ??the program is devoted to the study of the biological diversity of animals in various aspects. We study the taxonomic (mainly species) diversity 9 in types, at least 14 classes and at least 30 orders of multicellular animals. Research is conducted at two levels of diversity - global (family-to-type macrotaxa rank analysis according to the world fauna level) and local (subspecies-to genus taxa rank analysis as a part of the regional fauna and local natural communities). ...

526. CV of Alexander Moskovsky

527. Book review by Professor Teodor M. Atanackovic

528. New account