Search Results - "Belskaya, Irina N."

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  1. 1

    Updated taxonomy of trans-neptunian objects and centaurs: Influence of albedo by Belskaya, Irina N., Barucci, Maria A., Fulchignoni, Marcello, Dovgopol, Anatolij N.

    Published in Icarus (New York, N.Y. 1962) (01-04-2015)
    “…•We present updated classification of 258 trans-neptunian objects and centaurs based on their visible and near-infrared colors.•Increasing quality of color…”
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    Journal Article
  2. 2

    Asteroid observations at low phase angles. IV. Average parameters for the new H , G 1 , G 2 magnitude system by Shevchenko, Vasilij G, Belskaya, Irina N, Muinonen, Karri, Penttilae, Antti, Krugly, Yurij N, Velichko, Feodor P, Chiorny, Vasilij G, Slyusarev, Ivan G, Gaftonyuk, Ninel M, Tereschenko, Igor A

    Published in Planetary and space science (01-04-2016)
    “…We present new observational data for selected main-belt asteroids of different compositional types. The detailed magnitude-phase dependences including small…”
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  3. 3

    Polarimetry and BVRI photometry of the potentially hazardous near-Earth Asteroid (23187) 2000 PN9 by BELSKAYA, Irina N, FORNASIER, Sonia, KRUGLY, Yurij N

    Published in Icarus (New York, N.Y. 1962) (01-05-2009)
    “…The results of V-band polarimetric observations of the potentially hazardous near-Earth Asteroid (23187) 2000 PN 9 at large phase angles are presented as well…”
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  4. 4

    A three-parameter magnitude phase function for asteroids by Muinonen, Karri, Belskaya, Irina N., Cellino, Alberto, Delbò, Marco, Levasseur-Regourd, Anny-Chantal, Penttilä, Antti, Tedesco, Edward F.

    Published in Icarus (New York, N.Y. 1962) (01-10-2010)
    “…We develop a three-parameter H, G 1, G 2 magnitude phase function for asteroids starting from the current two-parameter H, G phase function. We describe…”
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  5. 5

    Polarimetry of main belt asteroids: Wavelength dependence by Belskaya, Irina N., Levasseur-Regourd, Anny-Chantal, Cellino, Alberto, Efimov, Yuriy S., Shakhovskoy, Nikolay M., Hadamcik, Edith, Bendjoya, Philippe

    Published in Icarus (New York, N.Y. 1962) (2009)
    “…New UBVRI polarimetric observations of ten asteroids, including space mission targets 1 Ceres and 21 Lutetia, are presented. These observations were obtained…”
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  6. 6
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  8. 8

    Opposition polarimetry and photometry of S- and E-type asteroids by Belskaya, Irina N, Shevchenko, Vasilij G, Kiselev, Nikolaj N, Krugly, Yurij N, Shakhovskoy, Nikolaj M, Efimov, Yurij S, Gaftonyuk, Ninel M, Cellino, Alberto, Gil-Hutton, Ricardo

    Published in Icarus (New York, N.Y. 1962) (01-12-2003)
    “…The first results of the observational program devoted to simultaneous investigation of asteroid polarimetric and photometric opposition phenomena are…”
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  9. 9

    Asteroid observations at low phase angles. IV. Average parameters for the new H, G1, G2 magnitude system by Shevchenko, Vasilij G., Belskaya, Irina N., Muinonen, Karri, Penttilä, Antti, Krugly, Yurij N., Velichko, Feodor P., Chiorny, Vasilij G., Slyusarev, Ivan G., Gaftonyuk, Ninel M., Tereschenko, Igor A.

    Published in Planetary and space science (01-04-2016)
    “…We present new observational data for selected main-belt asteroids of different compositional types. The detailed magnitude–phase dependences including small…”
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    Journal Article
  10. 10

    The potentially hazardous Asteroid (214869) 2007 PA8: An unweathered L chondrite analog surface by Fornasier, S., Belskaya, I.N., Perna, D.

    Published in Icarus (New York, N.Y. 1962) (01-04-2015)
    “…•We present the results from polarimetry and spectroscopy of the PHA 214869 (2007 PA8).•The spectra reveal that 2007 PA8 is a Q-type.•Spectral parameters and…”
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  11. 11
  12. 12

    Polarimetry and BVRI photometry of the potentially hazardous near-Earth Asteroid (23187) 2000 PN 9 by Belskaya, Irina N., Fornasier, Sonia, Krugly, Yurij N.

    Published in Icarus (New York, N.Y. 1962) (2009)
    “…The results of V-band polarimetric observations of the potentially hazardous near-Earth Asteroid (23187) 2000 PN 9 at large phase angles are presented as well…”
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    Journal Article
  13. 13

    Asteroid photometric and polarimetric phase curves: Joint linear-exponential modeling by Muinonen, K., Penttilä, A., Cellino, A., Belskaya, I. N., Delbò, M., Levasseur-Regourd, A. C., Tedesco, E. F.

    Published in Meteoritics & planetary science (01-12-2009)
    “…— We present Markov‐Chain Monte‐Carlo methods (MCMC) for the derivation of empirical model parameters for photometric and polarimetric phase curves of…”
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  14. 14

    Opposition Effect of Kuiper Belt Objects: preliminary estimations by Belskaya, Irina N, Barucci, Antonella M, Shkuratov, Yurij G

    Published in Earth, moon, and planets (01-06-2003)
    “…Information on the surface structure of the Kuiper Belt objectscan be obtained from studies of their opposition brightening.Although KBOs are observed at a…”
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  15. 15

    The F-type asteroids with small inversion angles of polarization by Belskaya, I.N., Shkuratov, Yu.G., Efimov, Yu.S., Shakhovskoy, N.M., Gil-Hutton, R., Cellino, A., Zubko, E.S., Ovcharenko, A.A., Bondarenko, S.Yu, Shevchenko, V.G., Fornasier, S., Barbieri, C.

    Published in Icarus (New York, N.Y. 1962) (01-11-2005)
    “…UBVRI polarimetric observations carried out in 1997–2004 for the F-type Asteroids 302 Clarissa, 419 Aurelia, 704 Interamnia, and 762 Pulcova (V band only) are…”
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  16. 16

    Asteroid observations at low phase angles by Shevchenko, Vasilij G., Chiorny, Vasilij G., Gaftonyuk, Ninel M., Krugly, Yury N., Belskaya, Irina N., Tereschenko, Igor A., Velichko, Fiodor P.

    Published in Icarus (New York, N.Y. 1962) (01-08-2008)
    “…The results of photometric observations of eight main-belt asteroids with low surface albedo are presented. The magnitude–phase dependences including low phase…”
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  17. 17

    Phase integral of asteroids by Shevchenko, Vasilij G, Belskaya, Irina N, Mikhalchenko, Olga I, Muinonen, Karri, Penttilä, Antti, Gritsevich, Maria, Shkuratov, Yuriy G, Slyusarev, Ivan G, Videen, Gorden

    Published 23-05-2019
    “…A&A 626, A87 (2019) The values of the phase integral q were determined for asteroids using (i) a numerical integration of the brightness phase functions over a…”
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