Star photometry on digitized astronegatives

V. M. Andruk; L. K. Pakuliak; V. V. Golovnia; S. V. Shatokhina; O. M. Yizhakevych; Y. I. Protsyuk; I. Eglitis; M. Eglite; L. V. Kazantseva; H. Relke; Q. X. Yuldoshev; M. M. Muminov

doi:10.15407/scine13.01.015

Institute of Astronomy

NASU - Main Astronomical Observatory
Nikolaev Astronomical Observatory
University of Latvia
Kyiv National Taras Shevchenko University
Walter-Hohmann-Observatory
Academy of Sciences of the Republic of Uzbekistan
Andijan State University

Research output: Contribution to journal › Article › peer-review

5 Citations (Scopus)

Abstract

This paper discusses the issues of characteristic curve restoration for astronegatives exposed in the wide range of expositions in U, B Johnson color bands using different telescopes. Photographic plates are digitized by Epson commercial scanners. Digitized images are processed in MIDAS/ROMAFOT software. The accuracy of characteristic curve restoration using photoelectric data is within the range 0,1-0,2m.

Original language	English
Pages (from-to)	15-23
Number of pages	9
Journal	Science and Innovation
Volume	13
Issue number	1
DOIs	https://doi.org/10.15407/scine13.01.015
Publication status	Published - 2017

Keywords

And image processing
Astronegatives
U and B stellar magnitudes

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10.15407/scine13.01.015

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@article{744d67a43db34c379c5ee200e9ad69fc,

title = "Star photometry on digitized astronegatives",

abstract = "This paper discusses the issues of characteristic curve restoration for astronegatives exposed in the wide range of expositions in U, B Johnson color bands using different telescopes. Photographic plates are digitized by Epson commercial scanners. Digitized images are processed in MIDAS/ROMAFOT software. The accuracy of characteristic curve restoration using photoelectric data is within the range 0,1-0,2m.",

keywords = "And image processing, Astronegatives, U and B stellar magnitudes",

author = "Andruk, \{V. M.\} and Pakuliak, \{L. K.\} and Golovnia, \{V. V.\} and Shatokhina, \{S. V.\} and Yizhakevych, \{O. M.\} and Protsyuk, \{Y. I.\} and I. Eglitis and M. Eglite and Kazantseva, \{L. V.\} and H. Relke and Yuldoshev, \{Q. X.\} and Muminov, \{M. M.\}",

note = "Publisher Copyright: {\textcopyright} 2017 ANDRUK, V.M., PAKULIAK, L.K., GOLOVNIA, V.V., SHATOKHINA, S.V., YIZHAKEVYCH, O.M., PROTSYUK, Yu.I., EGLITIS, I., EGLITE, M., KAZANTSEVA, L.V., RELKE, H., YULDOSHEV, Q.X., and MUMINOV, M.M.",

year = "2017",

doi = "10.15407/scine13.01.015",

language = "English",

volume = "13",

pages = "15--23",

journal = "Science and Innovation",

issn = "2409-9066",

publisher = "Publishing House Akademperiodyka",

number = "1",

}

TY - JOUR

T1 - Star photometry on digitized astronegatives

AU - Andruk, V. M.

AU - Pakuliak, L. K.

AU - Golovnia, V. V.

AU - Shatokhina, S. V.

AU - Yizhakevych, O. M.

AU - Protsyuk, Y. I.

AU - Eglitis, I.

AU - Eglite, M.

AU - Kazantseva, L. V.

AU - Relke, H.

AU - Yuldoshev, Q. X.

AU - Muminov, M. M.

N1 - Publisher Copyright: © 2017 ANDRUK, V.M., PAKULIAK, L.K., GOLOVNIA, V.V., SHATOKHINA, S.V., YIZHAKEVYCH, O.M., PROTSYUK, Yu.I., EGLITIS, I., EGLITE, M., KAZANTSEVA, L.V., RELKE, H., YULDOSHEV, Q.X., and MUMINOV, M.M.

PY - 2017

Y1 - 2017

N2 - This paper discusses the issues of characteristic curve restoration for astronegatives exposed in the wide range of expositions in U, B Johnson color bands using different telescopes. Photographic plates are digitized by Epson commercial scanners. Digitized images are processed in MIDAS/ROMAFOT software. The accuracy of characteristic curve restoration using photoelectric data is within the range 0,1-0,2m.

AB - This paper discusses the issues of characteristic curve restoration for astronegatives exposed in the wide range of expositions in U, B Johnson color bands using different telescopes. Photographic plates are digitized by Epson commercial scanners. Digitized images are processed in MIDAS/ROMAFOT software. The accuracy of characteristic curve restoration using photoelectric data is within the range 0,1-0,2m.

KW - And image processing

KW - Astronegatives

KW - U and B stellar magnitudes

UR - https://www.scopus.com/pages/publications/85091182693

U2 - 10.15407/scine13.01.015

DO - 10.15407/scine13.01.015

M3 - Article

AN - SCOPUS:85091182693

SN - 2409-9066

VL - 13

SP - 15

EP - 23

JO - Science and Innovation

JF - Science and Innovation

IS - 1

ER -

Star photometry on digitized astronegatives

Abstract

Keywords

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