... INTERVAL TD C/S (mb) C/S ALMA-ATA 890929 3600 000000-010000 00 1209.74 677.8 1206.26 0.1 ALMA-ATA 890929 3600 010000-020000 00 1209.74 677.9 1207.13 0.2 ALMA-ATA 890929 3600 020000-030000 00 1206.19 678.2 1206.19 0.1 ALMA-ATA 890929 3600 030000-040000 00 1206.04 678.4 1207.78 0.2 ALMA-ATA 890929 3600 040000-050000 00 1208.32 678.4 1210.06 0.4 ALMA-ATA ...

... KTP Specifications Flatness Scratch/Dig Code Parallelism Perpendicularity Angle Tolerance AR Coating Wavefront Distortion Dimension Tolerance Clear Aperture /8 at 633nm 10/5 to MIL-O-13830A < 20 arc seconds 5 arc minutes < ± 0.5°, < ± 0.5° R < 0.2% at 1064nm and R < 1.0% at 532 nm < /4 at 633nm (W ± 0.1 mm) x (H ± 0.1 mm) x (L + 0.2 mm/- 0.1 mm) > 90% of central area Standard Products Part No. ...

Surface Scattering Angle Surface Point Source, Isotropic Emitter into Sphere 1 0.9 0.8 0.7 0.6 P["] 0.5 0.4 0.3 0.2 0.1 0 0 !/4 !/2 Scattering " 3!/4 ! MC: local line center resonant MC: local HG scattering, g=0.0 Analytic HG, g=-1/3

... Summary of reduced ISAAC fields . ... This data release includes eight fully reduced VLT/ISAAC fields in J,H,K s bands covering 50 arcmin 2 of the GOODS region in the Chandra Deep Field South (CDFS). ... 8 ISAAC fields) . ... The 8 ISAAC fields which are part of this data release are superimposed onto a SOFI image (J+K) (part of a previous EIS data release). ... In one case (GOODS field 11/J-band), for which not enough standard stars were available, the ZP was boostrapped from previous SOFI/EIS data...

... Superflat Correction of Data An example of space-dependent calibration errors combined with poor centering is shown in Figure 1, where the differential V photometry for three stars in a single field is plotted as a function of the position on the detector. ... 374 Manfroid, Royer, Rauw, and Gosset -0.05 a b c a b c 0 0.05 0 -0.05 0.1 0.2 0.3 0.4 0.5 a b c 0.6 0 0.2 0.4 0.6 0.8 a b c 1 0 0.05 0 0.1 0.2 0.3 0.4 x position 0.5 0.6 0 0.2 0.4 y position 0.6 0.8 1 Figure 1. ...

THE SUBSYSTEMS OF THE MILKY WAY HALO. ... A catalogue of homogeneous fundamental astrophysical parameters for 145 globular clusters is composed on the base of the data of compilative catalogue by Harris (1997) and from another literature. ... In addition, it has large rotation velocity ( V rot =77?33 km/s), appreciable radial and vertical metallicity gradients equal by value, and has the oldest average age (subsystem of the old halo). ... Characteristic parameter of globular cluster subsystems. ...

... DZ *= (+1.2 + 1.7) óãë. ñåê. ...  òå÷åíèå 40 ìèí. òåëåñêîï ñîïðîâîæäàë îáúåêò òîëüêî ïðîãðàììíûì âåäåíèåì (îáëà÷íîñòü) è ïðè ïîÿâëåíèè îáúåêòà íàáëþäàòåëü ââåë ïîïðàâêè êîððåêöèè (+ 0.1 è - 0.3 ) óãë. ñåê., íî äàæå è ýòè ïîïðàâêè áûëè óñòðàíåíû ñëåäóþùåé êîððåêöèåé ( ñì. ðèñ. 3 è òàáë. 2 è 3 ). ... Îòñþäà ìîæíî ñäåëàòü âûâîä, ÷òî ïðè íàáëþäåíèÿõ ñ ÏÇÑ-êàìåðîé ÏÔ ÁÒÀ íàêîïëåííàÿ îøèáêà ïðîãðàììíîãî âåäåíèÿ ÁÒÀ íå ïðåâûøàåò çíà÷åíèé (0.1 - 0.2) óãë. ñåê., òî-åñòü ˜ 0.1 ðàçìåðà èçîáðàæåíèé (âñå îöåíêè...

... The problems of complexity in coagulation: specification 1. ... Numerical experiments Task 1: Activation threshold Final clot density VS activation : model reduction Factor V is activated 7 6 7 6 No factor V activation Fibrin 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Fibrin 5 5 4 3 2 1 0 0.00 0.02 0.04 0.06 0.08 0.10 0.12 Activation Activation y= Ae ( Bx 1 ) y = Ax Final clot density VS activation : the experiment Fibrin clot density (a.u.) 1.0 0.8 0.6 0.4 0.2 ...

... Latyshev Yu.I., Pavlenko V.N., Nevelskaya J.E., Monceau P., "Micron scale stacked structures fabricated from BSCCO 2212 single crystal whiskers", Journal of Alloys and Compounds 1997, v.251, 236-239. ... Yu.I. Latyshev, V.N. Pavlenko, S.-J. Kim and T. Yamashita, "Collective motion of Josephson vortex lattice in long stacked junction fabricated from Bi-2212 whisker", Physica C, 362 (1-4) (2001) pp. ... R. Kleiner, F. Steinmeyer, G. Kunkel, P. Muller, Phys. Rev. Lett. ... I. Latyshev, Phys. Lett. ...

DIMM . ... 100 000 , 2007 ­ 2009 . ... S 0.2). ... 1 3 ) , D DIMM. s DIMM s= D r0 5/3 = 5 D 2 · l2,t , Kl,t (1 4 ) 1.0 S a 0.9 0.8 0.7 LE MTF SE MTF S a 0.6 0.5 0.4 0.3 0.2 0 1 2 3 4 5 6 5/3 7 8 9 10 s = (D/r0) . ... Smin > 0.45, Smin < 0.45, - DIMM, 7 - 8 . ... Smin > 0.45 ( ) Smin < 0.45 , . ... Smin > 0.3 7 l / 0.8 0.6 S o t 1.0 0.4 0.2 Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep Aug Jul Jun May Apr Mar Feb Jan Dec Nov Oct Sep 2008 2009 . ... 8 MASS/DIMM 2007 2009 , , , , . ...

... 673 Table Mountain Observatory, W rightwood. ... 703 Catalina Sky Survey. ... H 19.0 seconds of 0.0 0.5+ 0.8- 1.6+ 1.0+ 0.21.0- 0.11.2+ 1.00.2+ 0.0 0.4- 0.5+ 0.6- 0.41.6+ 0.1 + 0.6- 0.10.4- 0.50.5- 0.10.8- 1.91.4- 1.3- 15.89003 +0.55234657 -0.27174286 G 0.15 U9 arc 090818 151 0.1 + 0.4+ 090819 H26 0.0 0.4090818 B04 0.5+ 0.0 090819 695 1.1- 0.6+ 090818 151 0.1 + 0.6+ 090819 673 0.3- 0.0 090818 B04 0.6+ 0.0 090819 673 0.1 + 0.1090818 B04 0.5+ 0.0 ...

... The contribution of backgrounds in signal box is estimated using sideband region. data , Blinded Events / ( 0.025 ) 25 Events / ( 0.0275 ) P M data 30 P E data 25 P f f qq data = QE D 20 20 QE D ÇP + 15 15 10 Ç (1 - f QE D ) Ç Pq q + 10 5 5 (1 - fQE D - fqq Ç (1 - fQE D )) Ç P E 0 - 0.6 -0.5 - 0.4 -0.3 - 0.2 -0.1 -0 0.1 0.2 0.3 0.4 x: delta M 0 - 0.6 - 0.4 - 0.2 0 M 0.2 0.4 y: delta E E data , Blinded ... LF V tau decay s Olga Igonkina DPF 2004 12 ...

IPCC, 2013] , - [%], ( MODIS) [Miralles et al., ... 2002] (1-6 - ) [Myhre and Myhre, 2008] [/2] [IPCC, 2013] 1750-2011 . ... 1) SRES 2, CH4, N2O, CFC11, CFC12, (MOZART-2.0) + 2) HYDE 3.1 LUH (MESSAGE, IMAGE, AIM, MiniCAM) XX [K] ( GISS) -0.5 -0.2 0.2 -0.5 1 [/] ( UEA CRU) -5 -3 -1 1 3 5 [Brovkin et al., ... 2) : - () CO2 ( ) . ... F - 2 U = t F(t) dt = U(q CO2 , T g) a) U / qCO 2 b) U / T g C2 [ ., 2008] ­ ­ , ( q CO2) qCO2, -1 SRES A2 875 -1 (90 -1) SRES A1B 762 -1 (83 -1) SRES B2 669 SRES B1 615 . ...

... The data from the images during this period is as follows: 09_1846.fit sur,sig= 2669.5 8.8 plat,sig= 2682.6 7.9 P-S= 13.1 DT= 0.8 . 09_1852.fit sur,sig= 2666.5 8.0 plat,sig= 2679.2 8.1 P-S= 12.7 DT= 0.6 . ... 09_1912.fit sur,sig= 2659.9 8.4 plat,sig= 2669.5 8.1 P-S= 9.6 DT= 0.0 . ... The filenames are date_mst.fit; sur,sig give the mean level in the image of the surround and the noise. plat,sig give the mean level in the heated plate and its noise. ... noise: < 0.16 C-deg-(min)^0.5 . ...

Statistics of sunspot activity . The sunspot indices . ... The solar regions . ... 2013 . ... Solar activity in 2013 . Visual indices of solar activity by author's observations . Average by . ... 0.25 . ...

... ÑÀÒÓÐÍ . ... Ñóïóòíèêè Ñàòóðíà : . ... Óïðîäîâæ öüîãî ïåð?îäó Ñàòóðí ç'ÿâëÿòèìåòüñÿ íà íåá? â?äðàçó ï?ñëÿ çàê?í÷åííÿ âå÷?ðí?õ ïðèñìåðê?â. Ó ïåðø?é äåêàä? ñ?÷íÿ â?í ñïîñòåð?ãàòèìåòüñÿ äî ðàíêîâèõ ïðèñìåðê?â, òîáòî ö?ëó í?÷ - òðèâàë?ñòü âèäèìîñò? ïåðåâèùóâàòèìå 14 ãîä. ?ç ÷àñîì âîíà øâèäêî çìåíøóâàòèìåòüñÿ (á?ëüø í?æ íà 2 ãîä ùîì?ñÿöÿ) óíàñë?äîê çá?ëüøåííÿ òðèâàëîñò? ñâ?òëî? ÷àñòèíè äîáè òà çì?ùåííÿ ìîìåíò?â çàõîäó ïëàíåòè íà á?ëüø ðàíí? ãîäèíè (íà ïî÷àòêó òðàâíÿ Ñàòóðí çàõîäèòèìå âæå áëèçüêî ï?âíî÷?)...

. Home . Structure of Data . Description . Catalog . Publications . VO . ÞÁ 2000 . 10:48:55.7 . ÞÄ 2000 . -59:02:58 . l . 287.742 . b . 0.161 . diameter . 3.0' . (m - M) 0 . 13.4 0.3 . distance . 4790 710 pc . E(B - V) . 0.76 0.05 . log(t) . 9.25 0.1 . (J, J-H) isochrone VOTable . 2MASS data VOTable . Developed by the Team . Send us your questions or feedback

... We present preliminary results from two programs to image the host galaxies of radio-quiet quasars in 1.6 micron light using NICMOS camera 2 on HST. The high redshift program consists of QSOs covering the redshift range 0.8 < z < 4.4 and a range of QSO luminosities. Of the six objects for which data have been obtained the results range from no host galaxy detected, to an obvious galaxy with an interacting companion, to a possible high redshift galaxy cluster. ...

Êëóá Ñêåïòèêîâ] [Êîíôåðåíöèÿ] . ... Êèâè : Ïðàãìàòèçüìó, âíåñòè! Óâàæàåìûé Àðòåì, äåëî â òîì, ÷òî òåîðåìà ñî ñïè÷å÷íûì êîðîáêîì íå ðàáîòàåò, è íå ïðèçâàíà ðàáîòàòü. ... 27-Íîÿ (10:26) . ... Àðòåì Ñàìîöåëü? ... Þðèé Òèõîíðàâîâ Ñàìîñðåäñòâî 27-Íîÿ (18:08) . ... 29-Íîÿ (20:53) Êèâè re: Þðèþ Òèõîíðàâîâó î "âñåìîãóùèõ êîðîâàõ" 27-Íîÿ (03:45) Àðòåì Ïðîâåðèë.. ... 27-Íîÿ (11:29) Àðòåì re: Ïðàãìàòèçüìó, âíåñòè! 27-Íîÿ (13:48) Ïðîõîæèé re: Ïðàãìàòèçüìó, âíåñòè! ... 27-Íîÿ (21:39) Àðòåì Àãà! ...

... Ãëàâíàÿ Àñòðîíîìèÿ Ôîòîãðàôèè Ðåêîðäû Ôîðóì Ãîñòåâàÿ êíèãà . Àçáóêà . ... Ñòàòüè ïî àñòðîíîìèè . Âàø ïóòåâîäèòåëü â ìèðå àñòðîíîìèè . ... Ïðè ñîçäàíèè ñàéòà èñïîëüçîâàíû ìàòåðèàëû èç êíèãè Äàíëîï Ñ. "Àçáóêà çâåçäíîãî íåáà" 1990ã. Ôîòîãðàôèè âçÿòû èç . ... Ñòàòüè è ðåôåðàòû ïî Àñòðîíîìèè / Àñòðîíîìè÷åñêèå Òàáëèöû / Õàðàêòåðèñòèêè ñèñòåì ïëàíåòàðíûõ êîëåö . ... 0.1) . ... Èñòîðèÿ Àçáóêè. ...