... Limit of star magnitude. If you want to obtain best results, you should use reference stars not more dimly than limiting star magnitude of your telescope. Limiting star magnitude depends on time of an exposition also.) This value should be set as " maximum of star magnitude " in a dialog box " Extraction from catalogue". To find darkest stars in the frame, make the following: . ... Two star magnitudes (m1, m2 in two photometric systems) will be outputted in the window "Information". ...

arxiv:1203.6616 Кластеризация галактик в Спектроскопическом Обзоре Барионных Осцилляций SDSS-III: космологические приложения крупномасштабной двухточечной корреляционной функции (The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological implications of the large-scale two-point correlation function) . ... Authors: Jun Toshikawa et al. обзор arxiv:1203.3824 Первые звезды и галактики - основные принципы (The First Stars and Galaxies - Basic Principles) . ...

In the report, we will discuss the value distribution of the modified Mellin transform of the square of the Riemann zeta-function introduced and studied by A.Ivic, M.Jutila and Y.Motohashi. We will recall its analytical properties as well as some estimates and mean square estimates. After this, we will state continuous and discrete limit theorems in the sense of weak convergence of probability measures on the complex plane and in the space of meromorphic functions for this transform. ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . FileљList . ... python . ... mov . checkSegment.py . ... 11 љ @param[in] pA position of starting point at time t = 0 . ... 13 љ @param[in] pB position of ending point at time t = dt . ... 16 љ @param[in] doPos log test position? . ... 20 љ @param[in] axisLim axis limits (a tcc.base.AxisLim) . ... 36 љ Even if you request that position limits be checked, some paths . ... 63 љ # check position limits; expand the limit to include the starting position . ...

... The BL Lac objects found within DXRBS fall mostly in the range . ... A large fraction of the BL Lacs so far in our sample are at L X / L R < 10 -6.5 , the region of Figure 6 populated by LBLs. In this region of parameter space (to the left of the left-most dashed line in Figure 6), DXRBS includes objects up to two orders of magnitude fainter than the 1 Jy survey. ... For comparison, we have plotted the values for members of these three ROSAT-based surveys (DXRBS, HQS/RASS and RC) in Figure 7. ...

... The SUB and SUP elements are used for subscripts and superscripts respectively, and are preferably rendered in reduced font. ... Some times you will want to place superscripts to the left of a term. ... For instance: X<sub align=right>a</sub> <sup align=left>b</sup>Y X<sub align=right>a</sub>Y<sup align=left>b</sup> b both render to X Y a while X<sub align=right>a</sub><sup align=left>b</sup>Y b renders to X Y a . ... The ID, LANG and CLASS attributes for SUB and SUP are not used within MATH...

... Observations have received at the telescope AT-64 of the Crimean Astrophysical Observatory . GRB . ... RA(2000): 11h 45m 10.54s . DEC(2000): 17o 24' 34.44" . ... Filter: none . ... Date, time (UT) . Exposure . ... 2000.07.29 18:21:52 . 30 sec . ... RA(2000): 19h 58m 19.61s . DEC(2000): 23o 32' 35.15" . ... 120 sec . ... DEC(2000): 6o 20' 47.07" . ... 240 sec . ... DEC(2000): 51o 46' 34.93" . ... DEC(2000): -13o 04' 30" . ... DEC(2000): +55o 18' 25.0" . ... 2000-11-09T16:03:19 . ...

Full-Text Search . ... arXiv.org . astro-ph . ... SAI VO . Search sort results by Date Relevance . ... Whitespace-separated words are treated as AND ed. Show 10 50 100 articles per page in Full Compact mode . This page hosts a simple full-text search for arXiv.org scientific e-print archive. ... The service is operated under the policy allowing us to regularly download and index the metatada of articles submitted to arXiv.org through Open Archive interface. ... SAI MSU . ...

RTT150 . ... One of the image, obtained in the May, 2003, with Andor DW436 CCD. Cluster 1541+6626, filter R, exposure 15 minutes, the resolution is 1", limiting star magnitude is 23m, the field of view is 8' x 8'. At the left: image of cluster 0720+7132 (z=0.268) obtained in the beginning of November, 2002 with RTT-150 and AP-47P CCD. 25 minutes exposure in R. The resolution is 0.7" (angular size of the image element - 0.23"), limiting stellar magnitude is 23.5-24. ...

Address: 4A Lenin Street, Korolev, Moscow area 141070 Russia . Phone: (495) 513-86-55 . Fax: (495) 187-98-77; 513-86-20 . ... The information to be disclosed by the Corporation in accordance with the legal acts and other regulations governing securities market . ... CORPORATION | INTERNATIONAL SPACE STATION | SEA LAUNCH . LAND LAUNCH | UNIVERSAL SPACE PLATFORM | ... LAUNCHERS | ... Official WEB-site of S.P.Korolev RSC Energia . ...

... In 1976, Polyakov (1976) predicted the existence of ionospheric AlfvИn resonator (IAR), equivalent to the ionospheric waveguide , but operating in vertical direction with shear AlfvИn waves . ... Belyaev, P. P., S. V. Polyakov, V. O. Rapoport, and V. Y. Trakhtengerts, The fine structure of the radiation of an AlfvИn maser, Geomagn. ... Belyaev, P. P., S. V. Polyakov, V. O. Rapoport, and V. Y. Trakhtengerts, The ionospheric AlfvИn resonator, J. Atm. ... Space Physics Text Book of Oulu ...

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

. Diameter of circular antenna . 576 m . Number of antenna elements . 895 . Size of an element . 11.4 x 2 m . Geometrical area . 15000 m 2 . Effective area of full circle . 3500 m 2 . Wavelength range . 1 - 50 cm . Frequency range . 610 - 30000 MHz . Maximum angular resolution . 2 arcsec . Accuracy of coordinate determination . 1-10 arcsec . Flux density limit . 0.500 mJy . Absolute brightness temperature limit . 0.050 mK . Tracking time (South sector + Flat mirror) . 1-3 h . [RATAN-600 Homepage]

. To continue the work mark the row with data on wonted plate by sliding bar and click first on Plate in menu bar and then on Object list or on Plot of plate in drop-down menu. The first choice will result in displaying the list of minor planets within the limits of the plate, the second one leads to displaying the image of the plate with objects. But in both cases user should specify the magnitude limit above which the objects are not inserted into the list and not displayed in the plot.

... The one year crew. (image credit: NASA/Bill Stafford) . The тАЬOne Year CrewтАЭ has specific objectives to their mission all in a bid to find out if the human body and mind is capable of long missions to an asteroid, back to the Moon or even to Mars in the future. ... On-board the Russian space station Mir four cosmonauts clocked up more than a year in space in the 1980s and 1990s.€а (1942-) has the record for the longest single space flight of 437 days or 14 months in space in 1995. ...

Эта книга является плодом многолетней работы ряда американских ученых - членов Общества по исследованиям в области планетарного SETI (The Socity for Planetary SETI Search - SPSR). Авторов сборника объединила страсть к археологической разведке Марса. ... Книга состоит из 10 разделов, подробно описывающих историю открытия и исследований марсианских аномалий, в частности знаменитого "Лица Марса". ... Кроме "Лица", заслуживающими внимания сочтены и 12 других деталей ("Форт", "Город" и др.) ...

ATMoB "Double Star Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston ­ in particular, double, triple, and multiple stars. Introduction: Double, triple, and multiple stars are the "Rodney Dangerfields" of the night sky. ... W hile they can be observed under a variety of sky conditions, double stars ­ especially close ones ­ are best viewed on nights when the seeing is steady. ... The direction from a star to Polaris is north. ...

... OBJECT имя объекта MODEL тип модели спектров (пока 2 значения: PEGASE1 и GISSEL98) G_TYPE тип галактики (E, S0, Sa, Sb, Sc или Sd) FILT_MAG_STR список данных по фильтрам с ошибками, формируется как строка из заданных фильтров, например: FILT_MAG_STR="B=23.73+0.21 V=23.57+0.2 R=22.36 I=20.81" Z_FIXED заданное красное смещение z Z_LIMITS пределы поиска z, когда красное смещение неизвестно AGE_LIMITS пределы поиска возраста EXTINCTION ключ задания вычисления экстинкции в заданных фильтрах RA | ...

attach_mod schema - mssql $Id: attach_mssql_schema.sql,v 1.3 2003/01/29 11:43:58 acydburn Exp $ */ BEGIN TRANSACTION GO CREATE TABLE [phpbb_attachments_config] ( [config_name] [ varchar ] (100) NOT NULL , [config_value] [ varchar ] (100) NOT NULL ) ON [ PRIMARY ] GO CREATE TABLE [phpbb_forbidden_extensions] ( [ext_id] [ int ] IDENTITY (1, 1) NOT NULL , [extension] [char] (100) NOT NULL ) ON [ PRIMARY ] GO CREATE ...

RadioAstron AO-2 prop osal Submission dead line: 27 January 2014, 23:59 UT. ... Team contact name and e-mail address: Ivan Petrov (e-mail: Ivan.Petrov@gmail.com ) Total observing time request: 60 hrs Should be < 100 hours if GOT. ... Introduction -- providing concise background information necessary to assess the scientific merits of the research proposed; outlining the reasons for the project to constitute key science area for RadioAstron if the KSP-type is selected. ...