Stellarium 0.12.3 . ... StelGeometryBuilder Class Reference . ... buildCircle ( StelVertexBuffer < VertexP2 > *vertexBuffer, const float x, const float y, const float radius, const int segments=128) . ... buildCylinder ( StelVertexBuffer < VertexP3T2 > *const vertexBuffer, const float radius, const float height, const int slices, const bool orientInside=false) . ... Build a fisheye-textured sphere. ... Build a flat texture mapped ring with 3D coordinates (for example for planet's rings) More.. ...

Astronomical Data Analysis Software and Systems XIII ASP Conference Series, Vol. 314, 2004 F. Ochsenbein, M. Al len, and D. Egret, eds. A Domino-based Virtual Observatory Service for the HI Parkes All Sky Survey D. G. Barnes and T. N. Stenborg School of Physics, The University of Melbourne, Parkvil le, VIC 3010, Australia Abstract. ... HICAT Virtual Observatory Service on Domino The HICAT Domino database currently stores 4,329 source documents, each with 172 data fields. ...

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

T he Siding Spring Survey (SSS) is a Near-Earth Object search program that utilises the 0.5-m Uppsala Schmidt Telescope at Siding Spring Observatory, N.S.W., Australia. ... The mission of the Siding Spring Survey is to contribute to the inventory of near-earth objects (NEOs), or more specifically, the potentially hazardous asteroids (PHAs) and comets (PHOs) that may pose a threat of impact and thus harm to civilization. ... Based on the CSS Mission page . ... Siding Spring Survey Main Page . ...

... Лекция 2 (40 K) | Лекция 3 (37K) | Лекция 4 (39K) | Лекция 5 (43K) | Лекция 6 (47K) | Лекция 7 (32K) | Лекция 8 (54K) | Лекция 9 (41K) | Лекция 10 (45K) | Лекция 11 (38K) | Лекция 12 (44K) | ... Postscript-файл (36 K) | ... Алгоритмическая сложность и класс P . ... Вероятностное вычисление и класс BPP . ... Идея квантового вычисления. ... Определение и простейшие свойства квантового вычисления. ... Вычисление, устойчивое к ошибкам (классическое и квантовое). ...

... Jan . Feb . ... Apr . ... Jun . Jul . Aug . ... Dec . ... To read availability charts user should know the descriptor (the three-letter "name") of the KP subset of interest. ... Plot resolution is exactly one pixel per hour. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

There are some variables which are set internally by the shell and which are available to the user: Name Description . ... 0 the name of the command currently being executed. $# the number of positional arguments given to this invocation of the shell. $? the exit status of the last command executed is given as a decimal string. ... For example '1 2' 3 becomes "1 2 3" . is identical to the arguments received by the shell, the resulting list of words completely match what was given to the shell. ...

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Here we present the ionospheric parameters variations for quiet conditions. ...

. < Previous Figure < Main Page < Next Figure . The same as in Fig. 1. Note the two DIBs around 6400A seen only in hot stars because of stellar contamination in late B supergiants. Note the varying intensity ratios of the three weak features between 6440 and 6450 A. < Download average spectrum of o Per . < Download average spectrum of reddened stars . < Previous Figure < Main Page < Next Figure .

... 403] Running number 2 --- Name Object name 3 deg Ra Right Ascension J2000 (degrees) 4 deg Dec Declination J2000 (degrees) 5 --- Mark Spatial confusion (Note 1) 6 mCrab Flux 17-60 keV flux (Note 2) 7 mCrab Error 1 sigma flux error 8 --- Range Revolution range (Note 3) 9 --- Type Source type (Note 4) 10 --- ExType Expected source type 11 --- Refs Reference number in table 2 (Note 5) 12 --- Notes additional notes and/or alternative source names. ... Note (2): Time-averaged source flux in mCrab units. ...

... The Earth orientation parameters UT1 and polar motion (x pol ; y pol ) are relat­ ed with the values of UT0 and VOL obtained from the LLR analysis for a station with geocentric longitude and latitude (–; OE) by the following expression: 7 UT0 \Gamma UTC = UT1 \Gamma UTC + (x pol sin – + y pol cos –) tan OE 15 V OL = x pol cos – \Gamma y pol sin – At least four normal points for each station--reflector pair at one day were accepted for the diurnal UT0 estimations. ...

... Фонокартридж Tuscany Gold имеет самые высокоточные микрокатушки, когда либо производимые Gold Note.Сверхкороткий и предельно жесткий кантилевер из бора способствует абсолютно правильному следованию алмаза в виниловой канавке и передаче максимального количества информации на микрокатушки.В Tuscany Gold используется самарий-кобальтовый магнит, один из самых мощных в мире.Обновленный корпус Tuscany Gold из сплава дюралюминия 7050 заполнен полужидким полимером обеспечивает контроль вибраций для.. ...

... SPECTRAL ANALYSIS OF sdB-He STARS FROM THE SDSS A. Ahmad , C. Winter and C. S. Jeffery Armagh Observatory, Col lege Hil l, Armagh BT61 9DG. ... We present spectral classification and physical parameters of a sample of "helium-rich" sdB-He stars from spectra obtained from the SDSS archive. ... In this study we used an artificial neural network (ANN) to classify spectra of sdB-He stars from the SDSS and to derive fundamental atmospheric parameters. ... Position of sdB-He stars on the log g - T 5. ...

... Exposure Time Calculator (ETC) . ... ESO - Public Surveys . ... the recommended values to use for DIT, . ... Detector on-chip integration (DIT): seconds. to your chosen value - a separate page gives recommended values to use for DIT - for modes 1 and 2 below you may wish to start with the maximum recommended values as these will minimize the effect of read noise (a total object exposure of Y secs with DIT=X secs will produce Y/X lots of read noise) and give you a lower limit on the time needed. ...

. RC-archive . RC1322+0449 . RC1333+0452a . RC1333+0452b . RC1339+0445 . RC1347+0441 . RC1357+0453 . The R-band contours (BTA) superposed . on 1465MHz image (VLA) ps . The map (1465MHz,VLA) superposed . on the R-band image (BTA) ps . The R-band contours (BTA) superposed . on the FIRST image ps . The map (FIRST survey) superposed . on the R-band image (BTA) ps . Last updated 30 Oct 2001

... Class . ... METHOD . ... java.lang.Object ij.plugin.filter.UnsharpMask . ... public class UnsharpMask . ... Unsharp masking subtracts a blurred copy of the image and rescales the image to obtain the same contrast of large (low-frequency) structures as in the input image. ... This method is invoked by a Generic Dialog if any of the inputs have changed (CANCEL does not trigger it; OK and running the dialog from a macro only trigger the first DialogListener added to a GenericDialog). void . ...

tranback -- Transform an X,Y position from output to input pixel position using the same conventions as drizzle tranback xout yout . xout = 400 [real] . ... The X dimension of the input image (this is used to determine the centre which is the origin of the transformations). (nyin = 800) [real] . ... If "output" the input image center is mapped to the center of the output grid, rotated about that center and then shifted along the grid of the output image. ...

AUTOMATIC STATION OF ECOLOGICAL CONTROL . ... BASIC PERFORMANCE SPECIFICATION . STATE OF ASEC DEVELOPMENT . AIR POLLUTION MONITORING . ... OF MEASURING CHANNELS . ... unit of measurement . ... Nitric oxide (NO) concentration, . ... power measured by ASEC . ... In particular, RSC Energia finalizes its work on measurement systems designed to measure dust, volumetric activity of radioactive gases and aerosols and other environmental parameters. ... Official WEB-site of S.P.Korolev RSC Energia . ...

SPECTRUM ANALYZER OF MAGNETIC PHENOMENA SAMW . Spectrum analyzer allows onboard computation of electromagnetic waves spectra registered (observed) in the ionosphere and magnetosphere in the ELF/VLF frequency band. ... It consists of magnetic antenna, preamplifier, 16 bit sigma delta AD converter, DSP processor and telemetry interface. ... The channels of lower frequencies are averaged and transmitted with lower repetition rate so the telemetry volume is reduced. ... Dynamic range: 90 dB . ...