Mobile Device to Digitize the photographic plates: first results Grosheva E.A., Izmailov I.S., Khrutskaya E.V. Pulkovo Astronomical Observatory, Russian Academy of Sciences, St. Petersburg, Russia Abstract -- The first results of astrometrical reduction for 40 Saturn and Pluto's plates are presented. ... This method of digitization and astrometric reduction of photographic plates using a digital camera is developed due to the problem of plate archive transportation to the high-tech measuring machines. ...

... ------------------------------------------------------------------------------------- 01 12 19:48 104 Klymene 09:17.22 +20 08.3 12.5 280 22 NGC 2809 13.0 G 157 130 -0.05 01 13 08:42 305 Gordonia 02:53.67 +13 01.5 13.5 94 343 NGC 1134 12.1 G 112 133 -0.03 01 13 11:44 104 Klymene 09:16.77 +20 10.9 12.5 73 202 NGC 2804 12.9 G 157 138 -0.03 02 15 05:14 113 Amalthea 10:01.66 +15 50.9 11.2 272 30 NGC 3094 12.3 G 176 166 ... Астрокалендарь 2010 ...

Data on the Objects "Crater" . ... Crater . ... 16.00 . ... log L K . ...

... 53, Moscow, 119991 Russia 2 MoscowPhysicotechnical Institute, Dolgoprudnyi, Moscow oblast, 141700 Russia Received June 15, 2004 ° Abstract--We present a catalog of 100 lines in the wavelength range 280­330 A detected by the RES-C spectroheliograph in solar active regions and flares during the SPIRIT experiment aboard the CORONAS-F orbital station. ... The line intensities recorded during the X3.4 (GOES) solar flare of December 28, 2001, are given. ... The Ca XVIII 302.19 A line is observed. ...

In the Table below the masses of some asteroids which were determined during the last years are listed. ... The listed values were determined from observations of many test bodies by the weighted least square fit for one perturbing mass and corrections to the orbit elements of all used test bodies. ... based on the observations of 98 asteroids (including 50278) with the values of standard error of mass determination less than 3.0 10 -11 M Sun . ... Mass . ... 3) Mass 121 : 0.74 x 10 -11 M Sun ; . ...

... 4 - Dhofar (Dh) 287. ... Dh 287 , KREEP . ... Taylor, 1982) . ... Dh 287 : Dh 287A (95%) Dh 287B (5%). ... Demidova S.I., Nazarov M.A., Anand M., Taylor L.A. A lunar regolith breccia Dhofar 287B: A record of lunar volcanism // Meteorit. ... Anand M., Taylor L.A., Misra K.C., Demidova S.I., Nazarov M.A. KREEPy lunar meteorite Dhofar 287A: A new lunar mare basalt // Meteorit. ... Demidova S.I., Nazarov M.A., Anand M., Taylor L.A. Clast population of lunar regolith breccia Dhofar 287B // Lunar Planet. ...

. Bright Supernovae - 2007 . This data comes from IAU Circulars and occasionally more data will be provided on IAU 's Astronomical Headlines page. An archive of the 2007 updates to this page is available. This is a list of the supernovae discovered in 2007. For supernovae which are still visible, please look at the main page for the latest data. Note that Extra galactic Novae have been moved to a special Extra galactic novae page . For more information, you can look at the following Supernova Catalogs: .

... 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 ...

... Orientation dependence of the grain boundary diusion Arrhenius parameters The temperature dependence of 195Au GB diusion of all bicrystals is shown in Figs 5(a)±(d) in Arrhenius coordinates. ... Structure dependence of Au and Cu GB diusion in Cu bicrystals The orientation dependence of GB diusion in the tilt angle range 33X218Y36X538 indicates a cusp of sdDGB and maxima of Arrhenius parameters, as determined from the lower temperature data, in the vicinity of the S 5 CSL GB, see Figs 3 and 6. ...

... The set of D30 new, unпltered CCD observations delineate the early rise behavior of SNe Ia 18 to 10 days before maximum. ... Using a variety of light-curve shape methods, we пnd the rise time to B maximum for an SN Ia with *m (B) \ 1.1 mag and peak M \[19.45 mag to be 19.5 ^ 0.2 days. ... OBSERVATIONS 2.1. ... 118 V B mag 20 -20 -10 0 10 Age (Days) 20 FIG. 4.хL eft : Observed V -band light curves for 10 SNe Ia including rise-time observations transformed from unпltered CCD measurements. ...

TOPEX/Poseidon Jason-1 , , 14-17 2005 . ... 14-17 2005 . ... 110° 90°W. , , 14-17 2005 . ... 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 110°W. , , 14-17 2005 . 25° 25° 30° 30° 35° 35° 40° 40° 1.1993 1.1994 1.1995 1.1996 1.1997 1.1998 1.1999 1.2000 1.2001 1.2002 45° 1.2003 45° -0 .05 -0 .03 -0 .01 0 .01 0 .03 0 .05 0 .07 0 .09 / - 100°W. , , 14-17 2005 . ...

... Date UTC R.A Dec. Distance V.Mag Phase Elong. muRAcosDE muDE Dist_dot h m s h m s o ' au. o o /s /s km/s 8 25 2012 5 32 1.00 22 15 7.44024 -11 30 24.9922 28.984184693 7.83 0.03 179.05 -0.1064E-02 -0.4142E-03 0.69822 8 26 2012 5 32 1.00 22 15 1.18460 -11 31 0.7539 28.984735705 7.83 0.06 178.18 -0.1064E-02 -0.4136E-03 1.20977 8 27 2012 5 32 1.00 22 14 54.93292 -11 31 36.4593 28.985581959 7.83 0.09 177.23 -0.1063E-02 -0.4129E-03 1.72060 8 28 ...

... Глава 2 . ... Ссылка из Главы 4 ). ... 0015+0501 . ... 0105+0501 . ... 19000 .008 . ... 3000 .010 . ... 450 .008 . ... 4000 .008 . ... 0444+0501 . ... 3000 .0502 . ... 3000 .011 . ... 0.64 . ... 3000 .014 . ... 12000 .008 . ... 1429+0501 . ... 1436+0501 . ... 3000 .034 . ... 500 .008 . ... 3000 .1613 . ... 1646+0501 . ... 1000 .008 . ... 3000 .0040 . ...

... Four types of galaxy environments are considered: clusters, centers of groups, other places in groups, and the field. ... In order to check whether the mean ages of the stellar populations depend on environment density monotonically, as the hierarchical par­ adigm predicts, in this work I consider four types of environment separately: the cluster galaxies, the brightest (central ) galaxies of groups, the second­ranked group members, and the field galaxies. ... Group center SB(rs)0# 204 637 1996 Oct ...

Общая Астрономическая Конференция > Форумы общей направленности > Общий форум любителей астрономии > Точность любительских позиционных ПЗС наблюдений . ... Просмотр полной версии : Точность любительских позиционных ПЗС наблюдений . ... Публикую здесь письма с обработкой моих ПЗС наблюдений астероидов, в первую очередь потенциально опасных для Земли. ... 7495 114 2000 11 18.857320 4 44 36.739 0.08 +23 29 21.67 -0.09 18.9 27 . 7495 114 2000 11 18.875220 4 44 35.829 0.22 +23 29 17.51 0.16 18.2 24 . ...

... Лейтен 726-8 . Расстояние от Земли: . ... Название звезды, ее тип: . Лейтен 726-8 A, красный карлик M6V . Масса звезды, ее радиус: . ... Название второй звезды, ее тип: . UV Кита, красный карлик M4V . Масса второй звезды, ее радиус: . ... 2.1 - 8.8 астрономических единиц . ... 0.007 астрономические единицы . ... Описание изображения: На этом изображении мы видим два тусклых солнца на небе во время их наибольшего сближения в 2.1 астрономические единицы между ними. ...

... Exposure Time Calculator (ETC) . Survey processing . ... VISTA is a 4-m class wide field survey telescope for the southern hemisphere, equipped with a near infrared camera (1.65 degree diameter field of view at VISTA's nominal pixel size) containing 67 million pixels of mean size 0.34 arcsec and available broad band filters at Z,Y,J,H,K s and a narrow band filter at 1.18 micron. A wide field visible camera, if constructed, could also be used on VISTA. ... Tile . ... ESO VISTA Public Surveys . ...

Data online as files and in interactive forms in SPIDR The present catalogue contains information of avalability in WDC for STP,Moscow of data on neutron component of the cosimc ray intensity (corrected for pressure) in computer-readable form from 1957 --------------------------------------------------------------------- | ... USA | ... 0.00 | CANADA | ... FSU- Kaz.| ... FSU- Rus.| ... AUSTRALIA | ... ANTARCTICA | ... FRG | ... FSU- Ukr.| ... FSU- Uzb.| ... FSU- Geo.| ...

... Number 5721 . ... 8 August 2006 . ... Data file: 5721-t3 . ... IBVS No. ... 2000.0 Max Min Type References h m s o ' m m 780217 V1675 Ori 05 34 23.8 -05 08 16 13.70 ( 0.08 ) Ic INB 072 USNO 780218 V1676 Ori 05 34 23.9 -05 15 40 11.19 ( 0.16 Ic) J INB 072 USNO 780219 V1677 Ori 05 34 24.3 -06 06 56 12.96 ( 0.10 ) Ic INB 072 USNO 780220 V1678 Ori 05 34 25.3 -04 54 39 13.24 ( 0.09 ) Ic INB 072 USNO 780221 V1679 Ori 05 34 26.1 -06 15 33 15.64 ( 0.14 ) Ic INB ... Sgr . ... Ori...

... First Estimate of the Value of the Instrumental Polarization of the RadioAstron Space Radio Telescope Using the Results of an Early Scientific Program for Observing Active Galactic Nuclei I. N. Pashchenko, Yu. ... For this, it is necessary to construct a joint distribution of the observational data and unknown parameters, including both instrumental effects and the parameters of the observed source. ... Unknown parameters. ... Thus, the probability model used is based on the linear model of leakage....