... Name Designation ff ffi J (ffi J ) H (ffi H ) K (ffi K ) J \Gamma K H \Gamma K Nights a AS01­0 FS02 00 55 09.9 00 43 13 10.716 ( 0.005 ) 10.507 ( 0.010 ) 10.470 (0.003) 0.25 0.04 6,6,6 AS02­0 SAO054271 00 55 58.6 39 10 09 8.775 (0.006) 8.771 ( 0.012 ) 8.770 ( 0.009 ) 0.01 0.00 5,6,6 AS03­0 FS03 01 04 21.6 04 13 39 12.606 ( 0.011 ) 12.729 ( 0.008 ) 12.827 ( 0.013 ) ­0.22 ­0.10 6,6,6 AS04­0 FS04 01 54 37.6 00 43 01 10.555 (0.004) 10.301 ( ...

F(6 cm) Other Name ct/s erg cm -2 s -1 µJy FX/FR mJy # r B R Class z Catalogs WGAJ0011.2- 3620 0.002 1.73E - 14 0.003 -12.73 96 0.12 21.3 FSRQ 2.324 WGAJ0012.5- 1629 0.097 1.28E - 12 0.29 -10.53 50 0.62 17.7 FSRQ 0.151 1 WGAJ0015.5+ 3052 0.019 2.82E - 13 0.083 -11.37 89 0.62 16.3 17.2 FSRQ 1.619 0.023 3.16E - 13 0.095 WGAJ0029.0+ 0509 0.006 6.33E - 14 0.014 -12.71 377 0.00 19.3 18.1 FSRQ 1.633 WGAJ0032.5- 2849 ...

... The designations are given for each object along with J2000.0 coordinates, followed by three columns for each filter, containing the magnitude, the first standard deviation or scatter among data points, and the number of measurements N. The values reported for the magnitudes are weighted averages, using 1/(sigma)^2 weighting, where the sigmas are the internal photometric errors of individual measurements." ... 0.005 . ... 0.008 . ... 0.006 . ... 0.007 . ...

wmap7_spt_bao_h0 +clusters, stat. sys. omegabh2 0.02263 +- 0.00044 0.02247 +- 0.00043 +- 0.00005 ns 0.980 +- 0.012 0.975 +- 0.012 +- 0.002 logA 3.173 +- 0.036 3.153 +- 0.035 +- 0.007 omegal 0.729 +- 0.014 0.7478 +- 0.0076 +- 0.0068 omegadmh2 0.1133 +- 0.0032 0.1087 +- 0.0013 +- 0.0017 age 13.681 +- 0.086 13.707 +- 0.084 +- 0.008 omegam 0.271 +- 0.014 0.2522 +- 0.0076 +- 0.0068 sigma8 0.833 +- 0.024 0.798 +- 0.010 +- ...

Peremennye Zvezdy ( Variable Stars ) 28 , No. ... We present the results of our long-term ( 13 years) J and K photometry of the X-ray binary Cyg X-1. ... From the analysis of these observations together with optical photometry of Cyg X-1, we concluded that the variations of the binary's J and K brightness were ellipsoidal. ... 0.007 . ... 0.008 . ... 0.009 . ... Figure 2 displays variations of the J and K brightness of Cyg X-1 versus the orbital phase, from observations of 1995-2007. ...

... Digital systems . ... Standard Stars - CCD Photometry, Transformations and Comparisons . ... Figure 2: A typical sample of transformation relations to the Landolt standard system (1996 Nov. ... 0.006 . ... Landolt's natural GaAs u - b system is not very close to the standard U - B system and so it is likely that, because the transformations were made using a U - B colour term alone, systematic U - B differences exist for some kinds of stars namely, A-F stars, reddened B-A stars and giant A-F stars. ...

... 0.039 0.009 . ... 0.043 0.006 . 0.059 0.005 . 0.039 0.002 . 0.063 0.002 . 0.053 0.003 . 0.069 0.003 . 0.093 0.005 . 0.054 0.003 . 0.076 0.003 . ... 0.078 0.004 . ... 0.235 0.014 . ... 0.029 0.007 . ... 0.014 0.002 . ... 0.006 0.002 . ... 0.007 0.002 . ... 0.005 0.002 . ... 0.014 0.003 . ... 0.009 0.005 . ... 0.009 0.003 . ... 0.009 0.002 . ... 0.007 0.003 . ... 0.014 0.005 . ... 0.014 0.006 . ... 0.003 0.002 . ... 0.004 0.002 . ... 0.006 0.003 . ... 0.007 0.004 . ...

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 ...

... 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 ...

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

Computer Ephemeris for 2016 from DE200/LE200. Elements of the Partial Lunar eclipse - 18 Aug 2016. ...

... Astrometric Observations of the Second, Third, and Fourth Satellites of Uranus I. S. Izmailova, S. A. Korotkiib, M. V. Ereshkob, and A. V. Stepurab a Pulkovo Observatory of the Russian Academy of Sciences, Pulkovskoe shosse 65­1, St. Petersburg, 196140 Russia b Ka-Dar Observatory, 1-i Neopalimovskii per., ... ASTROMETRIC OBSERVATIONS 43 To determine the center coordinates and other parameters of a satellite or a star image, we solved a redundant system with the nonlinear least-squares method. ...

... We investigate the extent to which the Wilson­Bappu relationship holds for chromospherically active binaries using the Mg ii h&k lines of 41 RS CVn stars observed with IUE. ... The line width does however depend on the column mass at the transition region boundary showing increased line width at lower column mass. There is also a depen­ dence on the column mass adopted for the temperature minimum, however, the major and dominant parameter is the surface gravity scaling as g \Gamma1=4 . ...

... Зор? до 2.5 зоряно? величини . ... Паралакс . ... F2 III . ... Ведмедиц? ... Великого Пса ( Мурз?м ) . ... Великого Пса ( Сир?ус ) . ... Великого Пса ( Адара ) . ... Астроном?чна одиниця (а.о.): . ... Тобто р?чний паралакс св?тила це кут, п?д яким з цього св?тила видно середн?й рад?ус земно? орб?ти. ... В?н означа?, на ск?льки зоряних величин зоря в короткохвильов?й д?лянц? спектра яскрав?ша (слабша), н?ж у довгохвильов?й. Прийнято, що B V = 0 для з?р спектрального класу A0 головно? посл?довност?. ...

Коломна-2008: Влияние факторов, связанных с методикой расчета . ... Таблица 1 Коэффициент уменьшения концентрации пыли от взрывных работ на Приокском карьере (источник 6019_1) при учете перехода от шлейфа к клубу длительностью 500 с. Цветокод: красный цвет = 1 (нет уменьшения) . ... Таблица 5 Влияние размера частиц пыли (он предполагается одинаковым) на концентрации для склада пылящих материалов 6008 (Щуровский цемзавод). ... Таблица 7 Влияние средней неровности поверхности на оседание пыли. ...

... 15318 B9III 4.279 -0.056 -0.107 -0.023 -0.063 xi Cet "bs1544" 04 50 36.7 08 54 01 J2000.0 ! ... 34 239 sdG 11.225 0.488 -0.058 0.295 0.587 -0.030 -0.245 H "VMa2" 00 49 10 +05 23.4 J2000.0 ! 0046+051 LHS 7 DZ7 12.382 0.550 0.006 0.255 0.499 0.0812 -2.722 O "LTT1020" 01 54 48 -27 28.7 J2000.0 ! ... 2317-054 sdO 11.846 -0.304 -1.153 -0.133 -0.325 H,O !! ! ... 00 47 03.6487 -11 52 21.558 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-12" 00 52 15.3737 -10 39 48.039 J2000.0(1999.5) 0.0 0.0 0.0 0.0 "BD-11" ...

... 000, 1­17; (2005) Printed 28 March 2006 A (MN L TEX style file v2.2) The star formation history of early-type galaxies as a function of mass and environment M.S. Clemens1 , A. Bressan 1 2 3 4 1,2 INAF-Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio, 5, 35122 Padova, Italy. ... We calculate the Lick indices for the entire sample and correct for aperture effects and velocity dispersion in a model independent way. ... 2005). ... The mean velocity dispersion is higher in denser environments...

... Column (5) is the heliocentric velocity at which the HI emission was observed. ... 1: New emission -only HI spectra 20 IRAS 20093+0536 0.060 0.012 0.050 IRAS 20230+1024 0.055 IRAS 20415+1219 0.050 Flux Density (Jy) Flux Density (Jy) Flux Density (Jy) 7400 7600 7800 8000 Heliocentric Velocity (km/s) 8200 8400 0.010 0.045 0.040 0.008 0.040 0.030 0.006 0.020 0.004 0.035 0.030 0.025 4500 5000 5500 Heliocentric Velocity (km/s) 6000 7200 4000 4200 4400 4600 4800 Heliocentric ...

... 0.0 Azov | ... 180 | ... 189 | ... 176 | ... 0.0 Artem | ... 0.0 Acbest | ... 181 | ... 188 | ... 0.0 Belovo (Kemer.) ... 0.0 Beloretsk | ... 179 | ... 0.0 Bodajbo | ... 0.0 Bol'shoj Kamen' | ... 0.0 | ... 183 | ... 178 | ... 0.0 Vladikavkaz | ... 175 | ... 0.0 Daurskoe | ... 0.0 Ertarskii | ... 0.0 Zlatoust (Cheljab.) ... 0.0 Ivdel' | ... 0.0 Kirovgrad | ... 0.0 Kolpashevo | ... 0.0 Krasnokamsk | ... 0.0 Lys'va (Perm.) ... 0.0 Nazarovo | ... 0.0 Never | ... 0.0 Nevinnomysk | ... 0.0 Neftekamsk | ...

Kepler-60 . KOI-2086 . KIC 6768394 . ... 0.016+0.003 . ... планеты . ... наклонение орбиты планеты i . ... открыта в 2012 году . ... 0.013+0.002 . ... 0.012+0.003 . 0.17+0.013 . ... 0.013+0.003 . ... Орбиты планет отрисованы в предположении нулевого эксцентриситета. Средняя плотность планеты b оценивается в 4.6 +1.4/-1.1 г/куб.см, планеты c - в 3.06 +1.14/-0.86 г/куб.см, планеты d - в 2.9 +1.0/-0.8 г/куб.см. ... 1 Kepler-60: три нептуна на очень близких орбитах ...