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. Comment on J0126-0123 . No detection: this object has been studied with the Molonglo telescope at 408 MHz (Schilizzi & McAdam 1975) as a source with a size between 2 and 5 . It is near an Abell cluster (Owen & Ledlow 1997). The data could be confused with a strong radio source (3C 40) identified with a pair of galaxies at z=0.018, 170" from our field center. VLBApls home page . Last modified: 16 Oct 2000

... 00 30 50 20 40 00 30 00 30 00 30 30 Sunrise Registration of participants Opening of the conference and Memorial Coffee break Plenary session « i i i .. Group photo Lunch Section sessions Coffee break Section sessions Dinner Guitar concert Shevchenko memorial « » ( ) Sunset Welco me Party Tuesday, 19.08.2014 Sunrise Plenary session Coffee break Plenary session Lunch Section sessions Coffee break Section sessions Dinner : , " Sunset 20.03 21.00 ­ 23.00 06.00 09.30 ­ 11. 11.00 ­ 11. ...

... 13, Moscow 119992, Russian Federation, e-mail: busarev@sai.msu.ru; 2 Research Institute Crimean Astrophysical Observatory, p/o Nauchnyi, Crimea 334413, Ukraine, e-mail: prok@crao.crimea.ua Summary: We propose a combined method of astronomical investigations of small or distant planets incorporating registration of a set of integral spectra of an object and their frequency analysis. ... An application of the method is shown on example of asteroid 21 Lutetia. ... 6] Busarev V. V. (2002), Solar Sys. ...