ACS/HRC AOA Test: X-Astigmatism v. Time 0.012 0.011 0.010 0.009 0.008 0.007 0.006 0.005 X-Astigmatism 0.004 0.003 0.002 0.001 0.000 -0.001 -0.002 -0.003 -0.004 -0.005 -0.006 17.00 17.25 17.50 17.75 18.00 18.25 18.50 18.75 19.00 19.25 19.50 19.75 20.00 20.25 20.50 AOA Test (Orbit 1) AOA Test (Orbit 2) Hours (Day 2005.142)

Peremennye Zvezdy ( Variable Stars ) 33 , No. ... We present our discovery a new variable star USNO-A2.0 1350-17086180 from observations at the Astrotel-Caucasus Observatory. ... The numbers of observations on each of the observing nights are presented in Table 1; the observations are attached to the html version of this paper. ... Numbers of observations . ... No. observations . ... 0.001 . ... 0.000 . ... 0.003 . ... 0.004 . ... 0.002 . ... 0.005 . ...

... Computation: RJMCMC Similar to Richardson Green 1997 Knowledge of the PSF makes things easier Insensitive to the prior on k e.g. posterior when k = 10 and = 3: Posterior of number of sources (k) 8 9 10 11 12 0.058 0.141 0.222 0.220 0.157 0.019 0.022 0.029 0.027 0.021 Mean SD 7 0.029 0.018 13 0.082 0.014 Used posterior probabilities given by 10 chains 6 / 30 Example Region occupied by the three ... 28 / 30 XMM data spectral distribution 29 / 30 Four models 30 / 30 ...

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Revs - number of orbits of dust from ejection to 2014 . Ep - ejection epoch (year) . Da0 large particles . rE-rD - distance of the dust trail node from Earth's orbit (Earth radius=0.00004AU) (Impact radius=0.00005AU) (trail widths can easily be a few Earth diameters, depending on ejection velocities) . fM - estimate of the along-trail dispersion. ... Year Mo Da . ... Revs . ... Da0 . ... 0.001 . ... 0.000 . ...

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 ...

J1407+284 2.26.10 4 2.28.10 4 2.30.10 4 2.32.10 4 2.34.10 4 2.36.10 4 Heliocentric Velocity (Km/s) ­0.001 0.000 0.001 0.002 0.003 Fractional Absorption 22600 22800 23000 23200 23400 23600 Heliocentric Velocity (km/sec) -0.001 0.001 0.002 0.003 0.0 Fractional Absorption J1407+284

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

An X-ray/radio sample of Active Galactic Nuclei Nuria Fonseca Bonilla Tutor: Stefano Bianchi Matteo Guainazzi An X-ray/radio sample of Active Galactic Nuclei Brief introduction Results Conclusions An X-ray/radio sample of Active Galactic Nuclei 1. ... Classification of AGN radio loud (powerful jets): e.g: radio galaxies, quasars, blazars... radio quiet radio quiet quasars (RQQs) Veron `06: MABS < -23 Seyfert Veron `06: MABS > -23 An X-ray/radio sample of Active Galactic Nuclei 3. ...

... 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 . ...

Тема : Астероид 2010 AL30 (Apollo) 13 января 2010 года в 0.3 LD от Земли .. Показать сообщение отдельно . 12.01.2010, 23:03 . ... Астероид 2010 AL30 (Apollo) 13 января 2010 года в 0.3 LD от Земли .. 2010 AL30, MPEC 2010-A63 . 2010 AL30 (астероид, Earth MOID=0.0 LD, H=27.2 ~12m), 10 - 14 метров, по внутренней орбите, меньше трети расстояния Земля - Луна .. Открыт LINEAR 10 января 2010 года в 06:34 UTC .. Последние наблюдения 12 января 2010 года в 11:41 UTC Magdalena Ridge Obs. ...

... 01.01.2008 . ... 1.0916 . 0.001 . ... 0.000 . ... 1.0466 . ... 1.0471 . ... 0.023 . ... 0.010 . ... 1.0506 . ...

... 60 спутников в порядке удаления от планеты) . ... Спутник . ... 128 000 . 0.3 . ... 129 000 . ... 181 400 . ... 671 100 . ... 0.000 . ... 1 070 400 . ... 1 882 700 . ... 7 507 000 . ... 11 165 000 . ... 11 461 000 . ... 11 717 000 . ... 11 741 000 . ... 12 555 000 . ... S/2003 J20 Carpo . ... 17 056 000 . ... S/2003 J3 . ... S/2003 J12 . ... S/2001 J10 Euporie . ... 19 394 000 . ... 20 216 000 . ... S/2003 J18 . ... 20 700 000 . ... S/2003 J6 Helike . ... 20 979 100 . ... 21 000 000 . ... Юпитер | ...

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

... 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. ...

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. ...

... 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. ...

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 ...

Next: Observations and data reduction Up: On the metallicities of Previous: On the metallicities of . Since the discovery of low metallicity gas in H II regions of Blue Compact Galaxies (BCGs) by Searle & Sargent (1972), a debate lasting for decades on possible existence of local truly young galaxies is still continuing. ... In particular, we reobserved two BCGs presented in the K? list - UM 133 and UM 382. ... UM 133 . UM 382 . ... 3868 [Ne III] .. ... 1.000 0.017 . ... 0.017 0.001 . ...

МОДЕЛЬ тени HENOUX 1969 J.C.Henoux Astron. ... 2,288-308 ( 1969 ) COLUMNS 6 LINES 25 TAU LGT TETA TEMP LGPE LGPG LGPH LGPH2 ---------------------------------------------- T5000 Theta lg(Pe) lg(Pg) lg(PH) lg(PH2) 0.00001 1.600 -3.00 2.60 2.56 0.56 0.0001 1.540 -2.20 3.20 3.16 1.20 0.0003 1.510 -1.83 3.50 4.45 1.65 0.0006 1.495 -1.58 3.64 3.59 1.90 0.0008 1.490 -1.44 3.72 3.67 2.00 0.001 1.480 -1.36 3.80 3.72 2.10 0.003 1.455 -1.09 4.08 4.00 ... 1.035 1.20 5.78 5.73 3.98 6. ...

ON ;connect points /sd ON ;dashed lines /sb OFF ;bar /se x OFF ;X-error bars /se y OFF ;Y-error bars /tr 150 ;# pts in computed curve /or x 0.001 100 ;set computing range /td xy ;define the columns /ac y=8*10^9*x^1.5 ;file or eqn /sr c 1 ;restyle eqn curve /sa m 2 2 ;mark, dash color for column 2 /sd OFF ;dashed lines /tr 150 ;# pts in computed curve /or x 0.001 100 ;set computing ...