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Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд). / Kiyaev, V. I.; Zaplava, A. B.

в: ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. СЕРИЯ 1: МАТЕМАТИКА, МЕХАНИКА, АСТРОНОМИЯ, № 3, 2002, стр. 99-104.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Kiyaev, VI & Zaplava, AB 2002, 'Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд)', ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. СЕРИЯ 1: МАТЕМАТИКА, МЕХАНИКА, АСТРОНОМИЯ, № 3, стр. 99-104.

APA

Kiyaev, V. I., & Zaplava, A. B. (2002). Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд). ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. СЕРИЯ 1: МАТЕМАТИКА, МЕХАНИКА, АСТРОНОМИЯ, (3), 99-104.

Vancouver

Kiyaev VI, Zaplava AB. Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд). ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. СЕРИЯ 1: МАТЕМАТИКА, МЕХАНИКА, АСТРОНОМИЯ. 2002;(3):99-104.

Author

Kiyaev, V. I. ; Zaplava, A. B. / Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд). в: ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. СЕРИЯ 1: МАТЕМАТИКА, МЕХАНИКА, АСТРОНОМИЯ. 2002 ; № 3. стр. 99-104.

BibTeX

@article{f6b1fc1e52ba44cb8c5c48c38163b44a,
title = "Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд)",
abstract = "To connect the HIPPARCOS catalogue or any other space catalogues with the ICRF by the optical observations of the radio stars is of great importance. The description of a technique, which permits to achieve the 15-20 mas accuracy in measuring the radio stars with the help of the transit circles is made. In contrast to classical routines of differential observations where the number of the target stars is much more than the number of the standard stars, the situation is quite opposite in case of the radio star observations in the system of any catalogues. This is the crucial point of our method. We present the input catalogue containing 172 bright radio stars and 193 standard stars and the algorithm of observation which confirm the ability of the 'old' ground astrometric tools to be useful for the projects of modern astrometry. The program opens a new wide field of the activity for the classical instruments to support the new space astrometric mission.",
author = "Kiyaev, {V. I.} and Zaplava, {A. B.}",
note = "Copyright: Copyright 2017 Elsevier B.V., All rights reserved.",
year = "2002",
language = "русский",
pages = "99--104",
journal = "ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. МАТЕМАТИКА. МЕХАНИКА. АСТРОНОМИЯ",
issn = "1025-3106",
publisher = "Издательство Санкт-Петербургского университета",
number = "3",

}

RIS

TY - JOUR

T1 - Определение дифференциальных поправок к прямым восхождениям радиозвезд (часть III – Входной каталог для наблюдений радиозвезд)

AU - Kiyaev, V. I.

AU - Zaplava, A. B.

N1 - Copyright: Copyright 2017 Elsevier B.V., All rights reserved.

PY - 2002

Y1 - 2002

N2 - To connect the HIPPARCOS catalogue or any other space catalogues with the ICRF by the optical observations of the radio stars is of great importance. The description of a technique, which permits to achieve the 15-20 mas accuracy in measuring the radio stars with the help of the transit circles is made. In contrast to classical routines of differential observations where the number of the target stars is much more than the number of the standard stars, the situation is quite opposite in case of the radio star observations in the system of any catalogues. This is the crucial point of our method. We present the input catalogue containing 172 bright radio stars and 193 standard stars and the algorithm of observation which confirm the ability of the 'old' ground astrometric tools to be useful for the projects of modern astrometry. The program opens a new wide field of the activity for the classical instruments to support the new space astrometric mission.

AB - To connect the HIPPARCOS catalogue or any other space catalogues with the ICRF by the optical observations of the radio stars is of great importance. The description of a technique, which permits to achieve the 15-20 mas accuracy in measuring the radio stars with the help of the transit circles is made. In contrast to classical routines of differential observations where the number of the target stars is much more than the number of the standard stars, the situation is quite opposite in case of the radio star observations in the system of any catalogues. This is the crucial point of our method. We present the input catalogue containing 172 bright radio stars and 193 standard stars and the algorithm of observation which confirm the ability of the 'old' ground astrometric tools to be useful for the projects of modern astrometry. The program opens a new wide field of the activity for the classical instruments to support the new space astrometric mission.

UR - http://www.scopus.com/inward/record.url?scp=0038677718&partnerID=8YFLogxK

M3 - статья

SP - 99

EP - 104

JO - ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. МАТЕМАТИКА. МЕХАНИКА. АСТРОНОМИЯ

JF - ВЕСТНИК САНКТ-ПЕТЕРБУРГСКОГО УНИВЕРСИТЕТА. МАТЕМАТИКА. МЕХАНИКА. АСТРОНОМИЯ

SN - 1025-3106

IS - 3

ER -

ID: 5275581