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41. http://site2010.sai.msu.ru/static/doc/VKornilov_site2010.pdf
Sternberg astronomical institute activities on site testing programs review Victor Kornilov comprehensive/characterization/of/astronomical/sites > kislovodsk/russia/2010/october/4-9 > Introduction This presentation responds on our activity in 5 last years only, inspite of that in SAI site testing researches have been started many years ago. ... More detailed discussion is devoted to MASS and DIMM measurements processing, some additional effects which were taken in account in last year. ...
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Ссылки http://site2010.sai.msu.ru/static/doc/VKornilov_site2010.pdf -- 2488.3 Кб -- 18.10.2010
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42. http://astrometric.sai.msu.ru/articles/Shokin.pdf
... catalogues -----------------------------------------------------------------------577 * 5 00 14.355 -68 54 32.23 1 m fs HV12517 OGLE LMC_SC15 35181 619 5 00 46.136 -69 04 54.40 1 m fs HV5534 OGLE LMC_SC15 81394 626 5 00 55.870 -68 26 20.71 DMA HV2260 634 5 01 05.149 -68 27 05.78 DMA HV2263 635 * 5 01 00.386 -69 03 42.97 DMA HV12524 693 * 5 01 54.611 -68 54 14.06 DMA HV885 OGLE LMC_SC15 148920 700 5 02 01.463 -68 35 02.53 ... The star images were measured on two plates of the astrograph...
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Ссылки http://astrometric.sai.msu.ru/articles/Shokin.pdf -- 114.3 Кб -- 21.11.2000
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43. http://kcor.sai.msu.ru/arXiv1002.2360.pdf
... 000, 112 (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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Ссылки http://kcor.sai.msu.ru/arXiv1002.2360.pdf -- 1631.3 Кб -- 12.02.2010
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44. http://astra.prao.psn.ru/Molotov/Webpage/INFO/lfvn_en.pdf
... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (122 GHz) spectra obtained on the RATAN600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...
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Ссылки http://astra.prao.psn.ru/Molotov/Webpage/INFO/lfvn_en.pdf -- 301.6 Кб -- 16.09.2004
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