... Science User Portal . ... ESO, the European Southern Observatory . ... Travel and Contacts . Travel to ESO Headquarters . ... Survey Telescopes . ... Star Clusters . ... Stars@ESO . ... ESO Science Newsletter . ... ESO 3.6-metre telescope . ... The Comet€аMcNaught€а2007 . ... 12 A. This spectrum is typical for an incoming comet at Hyakutake's heliocentric distance, r = 1.52 AU (228 million kilometres) at the time of the observation. It shows that the comet continues to develop normally. ...

... Кресла . ... Размер: XS . ... Цвет: белый . ... Размер шлица: PZ2 ; . ... Цвет: Фиолетовый . ... Глубина: 90 . ... Цвет: черный . ... Цвет: серый . ... Размер INT: 54 . ... Глубина пропила: 90, . ... Макс. глубина пропила под углом 90њ: 90, . ... Размер площадки: 800x550, . ...

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

Determination of short-term proper motions of fast stars with Pulkovo Normal Astrograph. ... Khovritchev Laboratory of Astrometry and Stellar Astronomy of the Pulkovo Observatory, RAS, Saint-Petersburg Observations Normal Astrograph (D/F=33 cm/3.5m), CCD camera: S2C, FOV = 18x16 arcmin, Pixel size 900x900 mas Determination of the new proper motions of 413 LSPM stars 1 epoch : CCD-surveys and catalogs -- M2000, CMC14, 2MASS, SDSS DR7 2 epoch : CCD-observations with the ...

... Satellite data ] . SMIS ] . The program is designed to process the specific AVHRR instrument data for calculation and analysis of temperature fields on the sea surface and upper level of clouds. It performs brightness correction for visible channels with regards to clouds altitude. ... The program features a wide variety of classification algorithms (including two-dimensional histogram analysis) and enables to construct personal procedures for classification. ... Back to SMIS Home Page . ...

... Green and blue curves - CYGAM telescope (squares - no constraints on the angle a , triangles - a <0.5 0 ); red curve - EGRET telescope. Effective area versus photon incidence angle to relative the longitudinal telescope axis (squares - no constraints on the angle a , triangles - a <0.5 0 , spectral index g= 2). ... Angular resolution for normal to the axis X incidence versus source power law spectrum index (squares- no constraints on the angle a , triangles- a <0,5 0 ). ... CYGAM (PDF, 450 Kb) . ...

... Smear particle position & Energy Cluster merging tool New! ... Make 1 cluster from 1 particle by Cluster Cheater New! ... Tracks at Root FastMC Maintained by R.Dubois FullMC TrkMult Nent = 100 TrkMult Nent = 100 Mean = 37.84 RMS = 12.93 Mean = 48.35 RMS = 15.37 10 14 8 12 10 6 8 4 6 4 2 2 0 0 20 40 60 80 100 120 140 160 180 200 0 0 20 40 60 80 100 120 140 160 180 200 Charged Track multiplicity Tracks at Root FastMC 220 200 180 160 140 140 120 120 100 ...

... astro-ph . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . ... Quasar Variability in the Framework of Poissonian Models . ... It is shown that in this very general framework the well established anti-correlation between variability amplitude and wavelength can only be understood as an effect of an underlying spectral component which remains stable on long time-scales, and is redder than the variable component. ...

... Astrophysics Group . Research . Cosmic Microwave Background (CMB) . ... A significant fraction of the Astrophysics Group is involved in work on the Cosmic Microwave Background, both experimental and theoretical. We are currently operating the Arcminute Microkelvin Imager , an arcminute-scale survey telescope, and developing analysis techniques for the Planck satellite. ... 2013, Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge, CB3 0HE . ...

Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) · · Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...

... Shkredov Ilya Dmitrievich, report, 2010. ... In 2010 I wrote several papers : (with S. Yekhanin) Sets with large additive energy and symmetric sets , accepted to Journal of Combinatorial Theory, Series A, 8 pages. (with A. Fish) A note on non­trivial solutions of Vieta system of equations within any normal set , Combinatorics, Probability and Computing, 4 pages. (with T. Schoen) Additive properties of ... These sets are dual to so­called sets of large exponential sums. ...

... 0.015 0.01 0.005 0 -0.005 -0.01 -150 -100 -50 0 GLON [deg] 50 100 150 4. ... 0 GLON [ deg ] 50 100 150 ей ж и ей ж и зж 1 -1 -3 1 0 -1 -2 Residuals OFF 0.006 0.004 0.002 count rate [cpscorr] 0 -0.002 -0.004 -0.006 -0.008 -0.01 -0.012 - 150 - 100 -50 0 GLON [ deg ] 50 2 / ndf p0 61.04 / 58 -1.206e-06 ‘ 1.595e-04 Residuals OFF 0.006 0.004 count rate [cpscorr] 0.002 0 -0.002 -0.004 -0.006 -0.008 -0.01 2 / ndf p0 67.73 / 58 8.599e-06 ‘ 1.596e-04 100 150 - 150 - 100 -50 0 GLON [ ...

SLR Observations at the Quasar Network Stations I.Gayazov, V.Mitryaev, S.Smolentsev, I.Rahimov, A.Diyakov, V.Shpilevski, V.Pshenkin, Ya.Rets Institute of Applied Astronomy, Saint Petersburg, Russia WPLTN-2012 September 24 - 28, 2012 Saint Petersburg SLR systems installation at the Quasar observatories Observatory Zelenchukskaya Badary Stage Dome building System installation Testing Dome building System installation Testing Dome building ...

... Authors: T. Bohm et al. arxiv:1411.7032 19-мегапарсековое расстояние до сверхмассивной черной дыры в NGC 4151, определенное по "пылевому параллаксу" (A dust-parallax distance of 19 megaparsecs to the supermassive black hole in NGC 4151) . ... Authors: Patrick L. Kelly et al. arxiv:1411.4666 KOI-1299: красный гигант, взаимодействующий с одной из двух долгопериодических гигантских планет (KOI-1299: a red giant interacting with one of its two long period giant planets) . ... Authors: John Southworth . ...