THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE

We describe the database of CCD- observations conducted withMeridian Axial Circlein 2001-2003. Inthat time it was equipped with a ISD017AP CCD having 1040x1160 pxs, 16 mkm pixel size and 1.394" per pixel scale.which is the component of UkrVO astro-information resource. We developed the software...

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Main Author: A. Zolotukhina
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2013-11-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/83753
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author A. Zolotukhina
author_facet A. Zolotukhina
author_sort A. Zolotukhina
collection DOAJ
description We describe the database of CCD- observations conducted withMeridian Axial Circlein 2001-2003. Inthat time it was equipped with a ISD017AP CCD having 1040x1160 pxs, 16 mkm pixel size and 1.394" per pixel scale.which is the component of UkrVO astro-information resource. We developed the software for management and accumulation of these and new data, which will be used to create a catalogue for clarification of coordinates of faint stars. We note that the MAC is a refractor (D=180 mm, F=2.3 m) which is used now in a CCD astrometric survey of the equatorial zone.
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spelling doaj.art-a9cfbb0863b94549883019a27d2750232022-12-22T03:15:48ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152013-11-0126223923910.18524/1810-4215.2013.26.8375383753THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCEA. Zolotukhina0Main Astronomical Observatory NAS of UkraineWe describe the database of CCD- observations conducted withMeridian Axial Circlein 2001-2003. Inthat time it was equipped with a ISD017AP CCD having 1040x1160 pxs, 16 mkm pixel size and 1.394" per pixel scale.which is the component of UkrVO astro-information resource. We developed the software for management and accumulation of these and new data, which will be used to create a catalogue for clarification of coordinates of faint stars. We note that the MAC is a refractor (D=180 mm, F=2.3 m) which is used now in a CCD astrometric survey of the equatorial zone.http://oap.onu.edu.ua/article/view/83753virtual observatorymeridian axial circleccd-archive
spellingShingle A. Zolotukhina
THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
Odessa Astronomical Publications
virtual observatory
meridian axial circle
ccd-archive
title THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
title_full THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
title_fullStr THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
title_full_unstemmed THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
title_short THE KYIV MERIDIAN AXIAL CIRCLE’ OBSERVATIONAL ARCHIVE AS THE UKRVO SCIENTIFIC RESOURCE
title_sort kyiv meridian axial circle observational archive as the ukrvo scientific resource
topic virtual observatory
meridian axial circle
ccd-archive
url http://oap.onu.edu.ua/article/view/83753
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