... разработка теории и методов расчета лучевых дифференциалов первого, второго и третьего порядков в градиентных оптических системах; . ... разработка методов расчета геометрических аберраций второго и третьего порядка осесимметричных оптических систем, содержащих асферические поверхности и градиентные среды типа "псевдоаксикон"; . ... получены формулы для расчета смещения изображения и геометрических аберраций второго порядка в градиентных оптических системах с малыми нарушениями осевой симметрии; . ...

... Парад планет 21.12.1997 Юпитер Венера Марс Пленка (PFG 400) Pro Foto || 400 Kodak фото Сергея Королькова . Парад планет 21.12.1997 Уран Венера Марс t=1 мин. Royal Gold 1000 150 Обьектив Гелиос f=58 + 2 конвертора фото Сергея Королькова . ... Парад планет (Венера Марс Уран) 22.12.97 Таир 3с. 1/4.5 f=300 мм 1 мин Kodak Royal 1000 . Парад планет (Юпитер и Марс) 21.01.98 БВТ 500 f=5000 мм 1/10 1 сек Kodak royal 1000 ...

... For reliable estimation of the accuracy of asteroid CCD observations we usually consider from ten or more various NUMBERED MINOR PLANETS (NMPs) observed during several nigths per month (more then 50 positions). ... They can be considered as an indicator of accuracy of the CCD positional observations with given MPC code. ... For any NUMBERED minor planet the (O-C) values must be zero if the errors of observations and the errors of its theory are absent. ...

WGN, the Journal of the IMO XX:X (200X) 1 General Relativistic Precession in Meteoroid Orbits A. Sekhar1 ,2 1 There are only very few past works related to the application of general relativity in the orbital evolution of small solar system bodies. ... However the maximum r ( 2 в 10-3 AU (1 - e cos )2 in 1 kyr) is exhibited by Daytime Arietids due to low q The values of and r given in Table 1 and 2 and low a compounded by the favourable value in . ... It can depend on for a constant value of . ...

The Astrophysical Journal, 794:97 (21pp), 2014 October 20 C doi:10.1088/0004-637X/794/2/97 2014. The American Astronomical Society. All rights reserved. Printed in the U.S.A. A FULLY BAYESIAN METHOD FOR JOINTLY FITTING INSTRUMENTAL CALIBRATION AND X-RAY SPECTRAL MODELS Jin Xu1 , David A. van Dyk2 , Vinay L. Kashyap3 , Aneta Siemiginowska3 , Alanna Connors5 , Jeremy Drake3 , Xiao-Li Meng4 , Pete Ratzlaff3 , and Yaming Yu1 2 1 Department of Statistics, University of California, Irvine, Irvine, CA 92697-1250,

... After matching image point sources to ob jects in each of the catalogs and fitting world coordinate systems to them using the IMWCS program, we find mean residuals between observed and catalog star positions of between 0. 09 and 0. 25 for the latest catalogs. ... Unix shell scripts written for each catalog set up an initial FITS header for each of the 1728 images with the center being the mean position of the ob jects found in that image. ... Catalog Fits of Various Catalogs to 1728 Images. ...

Mon. Not. R. Astron. Soc. 349, 1397­1418 (2004) doi:10.1111/j.1365-2966.2004.07619.x The 2dF QSO Redshift Survey ­ XII. The spectroscopic catalogue and luminosity function S. M. Croom,1 R. J. Smith,2 B. J. Boyle,1 T. Shanks,3 L. Miller,4 P. J. Outram3 and N. S. Loaring4,5 1 2 3 4 5 Anglo-Australian Observatory, PO Box 296, Epping, NSW 1710, Australia Astrophysics Research Institute, Liverpool John Moores University, Twelve Quays House, Egerton Wharf, Birkenhead CH41 1LD Department of Physics, University of