... Optical Prescription . ... Radius=625. 000 Source at infinity s c s n a2 a4 a6 k 1 -8.889e-005 0.00 -1.00028 0.000e + 000 0.000e + 000 3.81e-022 -1.285e+ 000 2 -1.390e-004 -3644.44 1.00028 0.000e + 000 0.000e + 000 1.79e-019 -1.197e+001 3 0.000e + 000 3619.89 1.46080 2.321e-005 -1.173e-010 -7.87e-017 0.000e + 000 4 0.000e + 000 12.00 1.00028 0.000e + 000 0.000e + 000 0.00e+ 000 0.000e + ...

... RJMCMC Similar to Richardson Green 1997 Knowledge of the PSF makes things easier Insensitive to e.g. posterior for ten sources with = 3: Number of Components 9 10 11 12 0.141 0.222 0.220 0.157 0.022 0.029 0.027 0.021 Mean SD 7 0.029 0.018 8 0.058 0.019 13 0.082 0.014 Simulated Data Source region (2 SD) is about 28% of the area and contains about 41% of the observations Positions (-2, 0), (0, 1), (1.5, 0) with intensities ... Approximate the number of sources (2 in this case) 2. ...

... Глава 2 . ... Ссылка из Главы 4 ). ... 4.3 . ...

... Nearly all the sources have com­ plete data at 2.3, 3.9, 7.7 and 11.2 GHz; 40 sources have 21.7 GHz flux densities. ... Fluxes of the sources in the NCP region Name, S 0.325 # t S 1.4 # t S 2.3 # t S 3.9 # t S 7.7 # t S 11.2 # t S 21.7 # t Sp. index NVSS Jy, WENSS Jy, NVSS Jy Jy Jy Jy Jy # 0.325/11.2 J000943+772440 2.059 0.082 0.628 0.021 0.447 0.04 0.267 0.017 0.161 0.007 0.14 0.016 -- -- 0.76 J001236+854313 1.605 0.064 0.691 0.023 0.539 0.048 0.246 0.018 0.148 ...

Kepler-11 . KIC 6541920 . KOI-157 . ... открыта в 2011 году . 0.091+0.001 . 0.006+0.004 . 0.161+0.002 . 10.3039+0.001 . ... 0.107+0.001 . ... 0.256+0.002 . ... 0.155+0.001 . ... 0.278+0.002 . ... 0.004+0.007 . ... 0.195+0.002 . ... 0.373+0.002 . ... 0.25+0.002 . ... 0.466+0.004 . ... 0.297+0.002 . 118.3807+0.001 . ... 1 Уникальная система Kepler-11 - шесть транзитных планет в плотной упаковке . 2 Все 6 планет в системе Kepler-11 имеют низкую плотность ...

... SWXCS J000315-5255.2 . ... SWXCS J000324-5253.8 . ... SWXCS J002437-5803.9 . ... SWXCS J005500-3852.4 . ... SWXCS J011432-4828.6 . ... SWXCS J021705-5014.2 . ... SWXCS J021747-5003.4 . ... SWXCS J023924-2505.1 . ... SWXCS J035259-0043.7 . ... SWXCS J044144-1115.6 . ... SWXCS J062155-6228.6 . ... SWXCS J082113+3200.1 . ... SWXCS J084749+1331.7 . ... SWXCS J085524+1102.0 . ... SWXCS J090946+4157.2 . ... SWXCS J092729+3010.8 . ... SWXCS J092650+3013.8 . ... SWXCS J092719+3013.7 . ...

ФИЗИЧЕСКИЕ ДАННЫЕ . СПУТНИКОВ НЕПТУНА . ... спутника . ... 1.5 . ... 9] Обозначения: Название Название спутника GM Гравитационная постоянная, помноженная на массу спутника Радиус Радиус Плотность Средняя плотность Vo Видимая звездная величина в оппозиции V или R Альбедо Визуальное геометрическое альбедо . ... Neptune's ring system // Neptune and Triton / Ed. Cruikshank D.P. Tucson: Univ. ... 1991. ... Goguen J.D., Hammel H.B., Brown R.H. Photometry of Titania, Oberon, and Triton // Icarus. ...

. Computer Ephemeris for 2014 from DE200/LE200. Mean places of fundamental stars at J2014.5 # name m Sp paralax alpha dif mu(al) delta dif mu(dl) " h m s s s o ' " " " 902 Psc omega 4.01 F5 0.012 3.437 3.085 0.0103 65636.77 19.93 -1.15 903 Tuc epsilon 4.50 B9 0.000 39.621 3.084 0.0077 -652947.46 20.02 -0.24 904 Oct theta 4.78 K0 0.011 219.259 3.016 -0.0188 -765908.52 19.86 -1.77 1630 Psc 30 4.41 M3 0.043 242.249 3.077 0.0034 -55600.70 20.00 -0.41 905 Cet 2 4.55 A0 0.004 428.899 3.070 0.0018 -171519.15 20.03

# Band Reference Magnitude Error U 1 15.395 0.037 B 1 16.028 0.313 V 1 15.433 0.027 i 1 14.926 0.028 J 2 14.246 0.032 H 2 13.557 0.022 K 2 12.296 0.027 IRAC 1 1 10.402 0.022 IRAC 2 1 9.775 0.023 IRAC 3 1 8.206 0.024 IRAC 4 1 8.662 0.020 WISE 1 1 10.648 0.024 WISE 2 1 9.696 0.022 WISE 3 1 7.383 0.040

... Выходное напряжение: 220+8% В; . ... Max входное напряжение: 260 В; . Min входное напряжение: 140 В; . ... Цвет: желтый . Кардиганы . ... Цвет: светло-розовый . ... Цвет: черный . ... Цвет: Красный . ... Цвет: Черный . ... Цвет: розовый . ... Цвет: нельсон . ... Villeroy & Boch Ultimate BBQ Тарелка десертная, 21x20 см - Villeroy & Boch - Villeroy & Boch . ... Villeroy & Boch Petite Fleur Charm Емкость для хранения средняя, 25 см - Villeroy & Boch - Villeroy & Boch . ...

Minor Planet 2000 EW70 Date UT R.A. (2000) Dec. ... 2000 Mar 16 0h 12 25.30 - 7 12.5 0.051 1.044 166.4 15.8 Vir 2000 Mar 16 6h 12 24.62 - 6 48.1 0.049 1.043 167.1 15.7 Vir 2000 Mar 16 12h 12 23.90 - 6 22.3 0.048 1.042 167.7 15.6 Vir 2000 Mar 16 18h 12 23.14 - 5 55.0 0.047 1.041 168.4 15.5 Vir 2000 Mar 17 0h 12 22.33 - 5 25.9 0.045 1.039 169.1 15.4 Vir 2000 Mar 17 6h 12 21.47 - 4 54.9 0.044 1.038 169.8 15.3 Vir ...

... 19 февраля 155 года было видно частное (тип Pe) затмение с максимальной фазой 0.007 в 09:01 UT в точке с коодинатами 70.8 северной широты 4.7 западной долготы. ... 20 марта 155 года было видно частное (тип P) затмение с максимальной фазой 0.629 в 21:00 UT в точке с коодинатами 71.9 южной широты 41.2 западной долготы. ... 14 сентября 155 года было видно частное (тип P) затмение с максимальной фазой 0.562 в 12:20 UT в точке с коодинатами 71.7 северной широты 96.4 восточной долготы. ... Поиск затмений ...

Orbital Data and Parent Star Data for: HD83443__ b . ... Orbital eccentricity . ... Stellar mass . ... Stellar T_eff . Kelvin . ... Planetary T_eff . ... Stellar Radius . ... Predicted Planetary Radius (w/o core) . ... T_circ (w/o core) . Gyr . ... T_damp (w/o core) . ... Bodenheimer, Laughlin, and Lin 2003, Astrophysical Journal, v. 592, 555-563. ... Adams and Laughlin 2006, ApJ : link . ...

LONG-TERM FREQUENCY HISTORY OF THE BE/X-BINARY SYSTEM SAX J2103.5 + 4545 A. Camero Arranz1 , C. A. Wilson2 , M. H. Finger3 , and V. Reglero 1 2 4 GACE, ICMUV, Univ. de Valencia,P.O. Box 20085, 46071 Valencia ... Spain, E-mail: Victor.Reglero@uv.es ABSTRACT We have carried out a long-term pulse-timing analysis of the transient X-ray pulsar SAX J2103.5 + 4545 using data from the INTEGRAL and the RXTE missions ... The 2-10 keV RXTE PCA fluxes. ... Orbital solution for SAX J2103.5+4545. ...

... An Electronic Version of Volume I of the General Catalogue of Variable Stars with Improved Coordinates N. N. Samus'1,2 , * , V. P. Goranskii2 , O. V. Durlevich2 , A. V. Zharova2 , E. V. Kazarovets1 , E. N. Pastukhova1, M. L. Hazen3 , and T. M. Tsvetkova Institute of Astronomy, Russian Academy of Sciences, ul. ... Subsequently, we are planning to publish new versions of the GCVS Volumes II and III, as well as of the catalog of suspected variable stars (the NSV catalog). ... Stars, No. ... Stars Obs. ...

... Kopylov, A.I., Kopylova, F.G. "Structure of galaxy groups and clusters and measurement of their masses", . ... Kopylova, F.G., Kopylov, A.I. "Peculiar motions of galaxy clusters and groups in the Hercules and Leo supercluster regions", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Leo supercluster", . ... Kopylova, F.G., Kopylov, A.I. "Analysis of the properties of clusters of galaxies in the region of the Ursa Major supercluster", . ...

... A02: Ткни "рукой" в угол экрана. ... 20011 - Attacked By Super Robo-Bitch 69869 - Space bar 90210 - Colony 53284 - Green Planet with Asteroids (Goliath) 41666 - Genetix 91001 - Uninhabited Planet 01015 - Uninhabited Planet 44091 - Uninhabtied Planet 81100 - Uninhabited Planet (Goliath) 54671 - Uninhabited Planet Лети по ним подряд. ... A12: Иди на картинку, где дерево переброшено через пропасть. ... A14: Возьми пульт дистационного управления, который тебе дал Cliffy и используй его на себя. ...

... 337, 275­292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...

... Asteroids 10 Hygiea, 135 Hertha, and 196 Philomela: Heterogeneity of the Material from the Reflectance Spectra V. V. Busarev Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow, 119992 Russia Received December 21, 2009 Abstract--The reflectance spectra of asteroids 10 Hygiea (C type), 135 Hertha (M type), and 196 Philomela (S type) are obtained in a range of 0.40­0.91 µm with different time intervals. ... 2008). ... Asteroids, Comets, Meteors 2008, Baltimore, 2008. ...

... The Thickness of Stellar Disks in Early-type Galaxies E. M. Chudakova* and O. K. Sil'chenko ** Sternberg Astronomical Institute, Lomonosov Moscow State University, Moscow, Russia Received August 19, 2013; in final form, October 30, 2013 Abstract--We suggest and justify a new photometric method enabling the derivation of the relative thickness of a galactic disk from the two-dimensional surface-brightness distribution of the galaxy in the plane of the sky. ... The galaxies are non-interacting. ...