... nlayc***solvefinishc***c*** Enter post processor and calculate the variance of the error weightedc*** with area.c***/post1setnsel,s, node ,,44fsum* get ,f01,fsum,fynsel,s, node ,,77fsum* get ,f02,fsum,fynallf01=-f01f02=-f02c*** aa00 = -1.468e-003 aa02 = -3.104e-006 aa04 = -4.111e-010 aa06 = 1.377e-015 c*** ab00 = 35.881ab02 = -0.00073173ab04 = 1.3682e-08ab06 = -4.0372e-14c*** vsum =0.0wsum=0.0* get ,y1, node ,528,u,yy1=( ...

October 17, 2010 ================ CDK125 and Nikon D3s Exposure of 0.001 seconds at ISO 1600 nikon_1287376892_moon_0p001s_1600iso.jpg was taken at Wed, 30 Jan 1974 00:28:09 GMT You can convert any unix time stamp to GMT (UTC) at this website: http://www.onlineconversion.com/unix_time.htm

Impact ­ Produced Exosphere of Europa A.A. Berezhnoy Sternberg Astronomical Institute, Moscow, Russia Equilibrium chemical composition of the impact-induced cloud 0.5 0.45 0.4 0.35 0.3 0.25 0.2 0.15 0.1 3000 3500 4000 T, K 4500 OH H2 5000 O 5500 H H2O Q 0.0045 0.004 0.0035 0.003 0.0025 0.002 0.0015 0.001 0.0005 0 2000 Na NaO H NaO 3000 T, K 4000 5000 1.E-01 2000 Q 1.E-02 1.E-03 1.E-04 T, K 2500 CO 3000 ... Previous detection of cometary impacts on Europa is very tentative. ...

... TRF - TRS. ITRS ITRF. ... TRS 1 TRS 2 X ( 2) = T1, 2 + 1, 2 R1, 2 X (1) IERS, ITRF2000 ITRF2005 Transformation parameters at epoch 2000.0 and their rates from ITRF2005 to ITRF2000 (ITRF2000 minus ITRF2005) T T T D 10 -9 1 2 3 R 1 R 2 R 3 mm 0.1 ± Rates ± 0.3 -0.2 0.3 mm - 0.8 0.3 0.1 0.3 mm - 5.8 0.3 -1.8 0.3 mas 0.000 0.012 mas 0.000 0.012 mas 0.000 0.012 0.40 0.05 0.08 0.05 0.000 0.000 0.000 0.012 0.012 0.012 (ITRF ) 20 40 2 10 ­9 12 ( ) 3-5 4- 20 3-8 25-30 1 / 1-3 / 10 / x, y z : (c...) : (c... ...

... Data It is now clear that fuzzballs are actually galaxies. ... Using the automatic telescope, we measured the redshifts and brightnesses of a large number of fuzzballs in all regions of the sky. ... Correlation between brightness and redshift Redshifts and Brightnesses 0.005 0.004 0.003 0.002 0.001 0 -0.001 0 -0.002 -0.003 -0.004 -0.005 Redshift of Fuzzball 500 1000 1500 2000 Brightness of Fuzzball The brightnesses and redshifts of all the fuzzballs measured are shown in this graph. ...

... 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 . ...

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

... 268, 274), ( P , 680, 710)) OSF_flat_pr=( ( n , 0, 10), ( T , 250, 285), ( P , 500, 750)) def applyPriors(obsmod, prior = None , log_pr= False ): Apply prior information to a model -- supports flat or log-flat priors : param obsmod: The base model : param prior : List of lists defining the prior ranges : param log_pr: If true, use log-priors if prior is ... If None assume pointing straight up :param sampler: Allow different samplers to be run. ...

ISSN 1561 8889. . 2009. . ... 1 2 3 3 i , , ESTEC, () « », , ARTEMIS ESA ( 7.2°) 70 . ... ARTEMIS OGS ESA [4, 8]. ... M = m [r a ] , M h = mh [rh a h ] , (2) (3) J = (r0)2 m , Jh = (r0h)2 mh , ISSN 1561 8889. ... Performance of satellite to ground communications link between ARTEMIS and the Optical Ground Station // Proc. SPIE. ... Investigation of Atmospheric Instability for Communication Experiments with ESA's Geostationary Satellite ARTEMIS // Kine matics and Physics of Celestial Bodies. ...

... Горизонты науки о Вселенной (Модераторы: Дмитрий Вибе , AlAn ) ? Давайте приколем инопланетян! :) . ... Рейтинг: +0/-0 . ... 19.05.2005 [11:05:30] ? ... Инопланетяне видят огонек, бегающий по . ... Записан . ... Ответ #1 : 19.05.2005 [13:27:11] ? ... А импульсные источники, которые дают импульс 1 мс -- не проблема, можно сделать и 1 нс. ... Цитата: Павел Фоменко от 19.05.2005 [11:05:30] Длина земного экватора L = 40 тысяч километров. ... Хорош прикол для инопланетян (которых поблизости Земли нет). ...

... Коллекция: Весна-лето 2016 . ... Платье Olivegrey. Цвет: . Сезон: Весна-лето 2016. ... Первые ложечка и вилочка Вашего малыша в удобном футляре. ... Примерный вес изделия - 3.365 гр., вставки: 24 бриллиантов, суммарный средний вес камней 0.048 карат, цвет 3, чистота 5, 1 изумруд, суммарный средний вес камней 0.7 карат, цвет 3, чистота 3. ... Цвет: металлик . Материал: металл . ... Цвет: синий . ... Материал верха: искусственная кожа, текстиль . ... Ложки для салата mayer&boch 24177, 2 шт., ...

... Some equations, identities or formulas contain small quantities , and these can be made much simpler and easier to use by sacrificing a little accuracy. ... When we derive squares, 3rd powers, 4th powers etc. of numbers larger than 1 , the results are always bigger , while for numbers smaller than 1 , the results are always smaller . ... power . ... number . ... The above also holds for negative numbers, if one understands "bigger" and "smaller" to refer to the absolute value (the value without sign...

... 0.3-10 . ... PANTER . ... FM2): 12 . ... FM1, FM2 FM3* , 1.49 8.05 FM1, 2 FM2, 2 FM3, 2 **, 2 164.6 72.9 158.9Б1.1 69.2Б0.6 161.0Б0.8 69.5Б0.6 162.5Б1.1 62.1Б0.4 * PANTER () PSPC , . ... FM1 FM2 3.5% 2.2% 1.5 . ... HEW ) 25 1.7 3 3 3.5 ~1.2' (2) (E/E) ROSAT PSPC HRI ASCA GIS SIS SAX LECS MECS PDS -. doc 0.1-2.4 0.1-2.4 0.7-10 0.5-10 0.1-10 1.3-10 15-300 220 1.5 95 1.2 300 2 280 2 56 2 150 6 500 60 43% 0.9 7% 7 2% 7 8% 6 8% 6 15% 60 13 HPGSPC XTE PCA HEXTE JET-X SODART LEPC HEPC SIXA MART ...

Hide Zen home . ... Index . ... q3c_ang2ipix x2013; converts spatial coordinates (ra,dec) to the ipix value . ... Suppose, you have table with spatial coordinates - ra and dec columns. ... To perform the query around ra0=2 and dec0=3 with radius0=1 from the table mytable you can do: # select * from mytable where q3c_radial_query(ra, dec, 2, 3, 1); . ... Assuming that we have a huge table "table2" with created ipix index and with ra and dec columns and the smaller one "table1" with ra and dec columns. ...

Диоды выпрямитиельные КДС111 - КД128 . Диод . ... 0.2/0.5 . ... 100/300 . ... 75/100 . ... 0.001/0.05 . ... 100/100 . ...

g - GaAs/Alx Ga1-x As , . ... 1.2 g - GaAs/Alx Ga1-x As . ... GaAs/Alx Ga1-x As , 5 [001] D2d . ... g = g , g = g ), g ^ [001], [110], [110]. ... g - h : Ї g= 2 2 2 gz z cos2 + gxx sin2 cos2 + gyy sin2 sin2 (1.5) (1.6) h = µB B Ї 2 2 2 gz z cos2 + gxx sin2 cos2 + gyy sin2 sin2 , g - 7 1.3 g - . ... 3.5 ). 1.5 g ( ): 2 2 g 2 () = gxx cos2 + gyy sin2 (3.3) ( ) 3.3 , g [001], [110] [110] . ... Science 306,1910 (2004) [2] C. Kallin and B. I. Halperin Phys. Rev. B 30, 5655 (1984) [3] Jongso o Yo on et al., ...

Initial orbit determinations of NEO-2005 with Pulkovo AMP-method O.P. Bykov Central Astronomical Observatory of RAS, Russia, 196140, Saint-Petersburg, Pulkovskoye shosse 65/1 Abstract Pulkovo Apparent Motion Parameters Method (the AMP-method) was proposed by prof. A.A.Kiselev and developed by his colleagues for initial orbit determinations of Artificial Earth Satellites, Space Debris, Asteroids, and Comets on the base of very short observational arc. ... Table 4 Apparent Motion Parameters for 2005 EE. ...

­556 DOI 10.1007/s00190-008-0265-2 ORIGIN AL AR TICLE On comparison of the Earth orientation parameters obtained from different VLBI networks and observing programs Z. Malkin Received: 25 March 2008 / Accepted: 22 August 2008 / Published online: 13 September 2008 © Springer-Verlag 2008 Abstract In this paper, a new geometry index of very long baseline interferometry ( VLBI ) observing networks, the volume of network V , is examined as an indicator of the ...

... We present a new technique to segregate old and young stellar populations in galactic spectra using machine learning methods. We used an ensemble of classifiers, each classifier in the ensemble specializes in young or old populations and was trained with locally weighted regression and tested using ten-fold cross-validation. ... In this work we propose a Machine Learning (ML) method to determine the age of stellar populations in synthetic galactic spectra. ... Combine results in an ensemble. ...

... 2 Measurement of PMTs counting characteristics and selection of op erating p oint To select the operating point of the PMT, that is the optimal values of the high voltage supply and pulse discrimination threshold, the command run counting=hv value is provided in the program mass. ... Starting with the minimum voltage (say 550 V) run command run counting=550 for the measurement execution. ... It is recommended to take measurements for the set of values of 0.4, 0.6, 0.8, 1.0. ...