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The MAGIC project – III. Radial and azimuthal Galactic abundance gradients using classical Cepheids

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.510 (2), p.1894-1901

2022

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Phenomenological modeling of the light curves of algol-type eclipsing binary stars

Astrophysics, 2012-12, Vol.55 (4), p.536-550

Andronov, I. L.

2012

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Variability of the Rotation Period of the White Dwarf in the Magnetic Cataclysmic Binary System EX Hya

Astrophysics, 2013-12, Vol.56 (4), p.518-530

2013

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Multiple timescales in cataclysmic binaries : The low-field magnetic dwarf nova DO Draconis

Astronomy and astrophysics (Berlin), 2008-08, Vol.486 (3), p.855-865

2008

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Polarimetric Standards: Calibration and Variability

Kinematics and physics of celestial bodies, 2023-10, Vol.39 (5), p.294-299

2023

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Orbital and spin variability of the intermediate polar BG CMi

Astronomy and astrophysics (Berlin), 2005-10, Vol.441 (2), p.663-674

2005

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ODESSA SCIENTIFIC SCHOOL OF RESEARCHERS OF VARIABLE STARS: FROM V.P.TSESEVICH (1907-1983) TO OUR DAYS

Odessa astronomical publications, 2017-12, Vol.30, p.252-255

Andronov, I. L.

2017

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Discovery of a bright X-ray transient in the Galactic Center with XMM-Newton

Astronomy and astrophysics (Berlin), 2005-01, Vol.430 (1), p.L9-L12

2005

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Astroinformation resource of the Ukrainian virtual observatory: Joint observational data archive, scientific tasks, and software

Kinematics and physics of celestial bodies, 2012-04, Vol.28 (2), p.85-102

2012

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The unique magnetic cataclysmic variable V1432 Aql (Research Note) : Third type of minima and synchronization

Astronomy and astrophysics (Berlin), 2006-06, Vol.452 (3), p.941-944

2006

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PHASE PLANE ANALYSIS OF THE PHOTOMETRICAL VARIATIONS OF LONG-PERIOD VARIABLES

Odessa astronomical publications, 2017-11, Vol.30, p.93-97

2017

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Photometric study of the unusual binary system vsx j052807.9 + 725606

Astrophysics, 2011-09, Vol.54 (3), p.392-402

2011

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STATISTICALLY OPTIMAL MODELING OF FLAT ECLIPSES AND EXOPLANET TRANSITIONS. THE “WALL-SUPPORTED POLYNOMIAL” (WSP) ALGORITMS

Odessa astronomical publications, 2017-12, Vol.30, p.57-62

2017

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PERIOD VARIATIONS AND POSSIBLE THIRD COMPONENTS IN THE ECLIPSING BINARIES AH TAURI AND ZZ CASSIOPEIAE

Odessa astronomical publications, 2018-10, Vol.31, p.103-109

2018

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EFFECTS OF THE MASS TRANSFER AND PRESENCE OF THE THIRD COMPONENTS IN CLOSE BINARY STELLAR SYSTEMS

Odessa astronomical publications, 2017-11, Vol.30, p.135-139

2017

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Comparative Analysis of Phenomenological Approximations for the Light Curves of Eclipsing Binary Stars with Additional Parameters

Astrophysics, 2017-03, Vol.60 (1), p.57-69

2017

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Nova-like cataclysmic variable TT Arietis QPO behaviour coming back from positive superhumps

Astronomy and astrophysics (Berlin), 2009-03, Vol.496 (3), p.765-775

2009

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Variability of long-period pulsating stars. I. Methods for analyzing observations

Astrophysics, 2006-07, Vol.49 (3), p.370-385

2006

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Capture radius and synchronization of the white dwarf in the unique magnetic cataclysmic system V1432 Aql

Astrophysics, 2007-01, Vol.50 (1), p.105-124

2007

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REVISION OF THE PHENOMENOLOGICAL CHARACTERISTICS OF THE ALGOL-TYPE STARS USING THE NAV ALGORITHM

Odessa astronomical publications, 2016-06, Vol.28 (2), p.181-185

2016

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UkrVO Astroinformatics Software and Web-services

Proceedings of the International Astronomical Union, 2016-10, Vol.12 (S325), p.361-366

2016

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A TECHNIQUE FOR SIMULTANEOUS MEASUREMENT OF CIRCULAR AND LINEAR POLARIZATION WITH A SINGLE-CHANNEL POLARIMETER

Odessa astronomical publications, 2016-12, Vol.29, p.74-77

2016

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ASYMPTOTIC PARABOLA” FITS FOR SMOOTHING GENERALLY ASYMMETRIC LIGHT CURVES

Odessa astronomical publications, 2016-06, Vol.28 (2), p.158-160

2016

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Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch

Astrophysics, 2007-01, Vol.50 (1), p.76-82

2007

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Variability of long-period pulsating stars. II. Additional parameters for classifying stars

Astrophysics, 2006-10, Vol.49 (4), p.506-522

2006

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The MAGIC project – III. Radial and azimuthal Galactic abundance gradients using classical Cepheids

Phenomenological modeling of the light curves of algol-type eclipsing binary stars

Variability of the Rotation Period of the White Dwarf in the Magnetic Cataclysmic Binary System EX Hya

Multiple timescales in cataclysmic binaries : The low-field magnetic dwarf nova DO Draconis

Polarimetric Standards: Calibration and Variability

Orbital and spin variability of the intermediate polar BG CMi

ODESSA SCIENTIFIC SCHOOL OF RESEARCHERS OF VARIABLE STARS: FROM V.P.TSESEVICH (1907-1983) TO OUR DAYS

Discovery of a bright X-ray transient in the Galactic Center with XMM-Newton

Astroinformation resource of the Ukrainian virtual observatory: Joint observational data archive, scientific tasks, and software

The unique magnetic cataclysmic variable V1432 Aql (Research Note) : Third type of minima and synchronization

PHASE PLANE ANALYSIS OF THE PHOTOMETRICAL VARIATIONS OF LONG-PERIOD VARIABLES

Photometric study of the unusual binary system vsx j052807.9 + 725606

STATISTICALLY OPTIMAL MODELING OF FLAT ECLIPSES AND EXOPLANET TRANSITIONS. THE “WALL-SUPPORTED POLYNOMIAL” (WSP) ALGORITMS

PERIOD VARIATIONS AND POSSIBLE THIRD COMPONENTS IN THE ECLIPSING BINARIES AH TAURI AND ZZ CASSIOPEIAE

EFFECTS OF THE MASS TRANSFER AND PRESENCE OF THE THIRD COMPONENTS IN CLOSE BINARY STELLAR SYSTEMS

Comparative Analysis of Phenomenological Approximations for the Light Curves of Eclipsing Binary Stars with Additional Parameters

Nova-like cataclysmic variable TT Arietis QPO behaviour coming back from positive superhumps

Variability of long-period pulsating stars. I. Methods for analyzing observations

Capture radius and synchronization of the white dwarf in the unique magnetic cataclysmic system V1432 Aql

REVISION OF THE PHENOMENOLOGICAL CHARACTERISTICS OF THE ALGOL-TYPE STARS USING THE NAV ALGORITHM

UkrVO Astroinformatics Software and Web-services

A TECHNIQUE FOR SIMULTANEOUS MEASUREMENT OF CIRCULAR AND LINEAR POLARIZATION WITH A SINGLE-CHANNEL POLARIMETER

ASYMPTOTIC PARABOLA” FITS FOR SMOOTHING GENERALLY ASYMMETRIC LIGHT CURVES

Variability of long-period pulsating stars. III. Changes in the parameters of humps at the ascending branch

Variability of long-period pulsating stars. II. Additional parameters for classifying stars

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