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The paper contains the preliminary result description of the photometric observations of the Moon surface during the total lunar eclipse of June, 15, 2011 conducted in southern Russia and Ukraine in t...
At present, the precision of deep ultraviolet photometry is somewhat limited by the dearth of faint ultraviolet standard stars. In an effort to improve this situation, we present a uniform catalog of ...
We measure secondary eclipses of the hot giant exoplanets CoRoT-1 at 3.6 and 4.5 μm, and CoRoT-2 at 3.6 μm, both using Warm Spitzer. We find that the Warm Spitzer mission is working very well for exop...
The nearby Lynx-Cancer void is a good laboratory to study the effect of very rarefied environment on the evolution of the least massive dwarf galaxies. A recently compiled sample of this void’s galaxi...
New grids of Atlas9 models have been calculated using revised convection parame-ters and updated opacity-distribution functions, for chemical compositions intended to be representative of solar, [M/H]...
We present the results of BV RI photometry and classification of 53 un-usual asteroids, including 35 near-Earth asteroids (NEAs), 6 high eccentric-ity/inclination asteroids, and 12 recently-identified...
Aims. To develop a method to determine distances to molecular clouds using JHK near-infrared photometry.Methods. The method is based on a technique that aids spectral classification of stars lying tow...
We present a large collection of photometric data on the Blazar PKS 0537-441 in the VRIJHK bands taken in 2004−2009. At least three flare-like episodes with months duration, and >3 mag amplitu...
Context. Parallel analysis of the large-scale morphology and local environment of matched active and control galaxy samples plays an important role in studies of the fueling of active galactic nuclei.
We explore methods to improve the estimates of star formation rates and mean stellar population ages from broadband photometry of high redshift star-forming galaxies. We use synthetic spectral templat...
Asteroseismology of stars in clusters has been a long-sought goal because the assumption of a common age, distance and initial chemical composition allows strong tests of the theory of stellar evoluti...
Old main-sequence turnoff photometry in the SMC。
Low-Resolution Spectroscopy and uvby&beta Photometry of Selected Stars in Haffner 18。
CCD photometry of M92     CCD photometry  M92       2009/6/25
CCD photometry of M92。
uvby -β Photometry of the RR lyrae star AC and。

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