... 8, ``Celestial Mechanics'', 2002 Rotation theory of celestial bodies: dynamical relations of the pole motion and nutation Yu. ... Problem By construction Earth rotation theory the studies of the precession--nutation motion and pole motion are considered usually separately. ... The angle Q between the polar axis of inertia and axis of rotation is small (of order 10 \Gamma6 ). ... The perturbation theory of the Earth rotation has been constructed in the elastic Andoyer and angle--action variables. ...

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• http://www.ipa.nw.ru/conference/2002/sovet/abstact/BORDOVIT.TEX.txt
• http://www.ipa.nw.ru/conference/2002/sovet/PS/BARYSHEV.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/BORDOVIT.PS

Subject of Astronomy. ... Celestial Sphere. ... Spherical Frames of Reference: Horisontal and Equatorial Coordinates, Ecliptical System. ... Transformation of Celestial Coordinates. ... Change of Object Coordinates as a Result of Diurnal Rotation of Celestial Sphere. Phenomenons, Which Lead to Celestial Coordinates Change. ... Motion of Equator, Ecliptic, and Their Poles. ... Diurnal Solar Motion on Different Latitudes. ... Time Equation. ... Apparent Motions and Configuration of Planets. ...

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• Spherical and Practical Astronomy

... Routine uvprobvr checks for the existence of a variable, and returns information about it. ... The following section of FORTRAN lists the variables present in a uv data set. character var*12,name*(?) integer iostat,tno,item call uvopen(tno,name,'old') call haccess(tno,item,'vartable','read',iostat) call hreada(item,var,iostat) dowhile(iostat.eq.0) call output(var(3:10)) call hreada(item,var,iostat) enddo call hdaccess(item,iostat) call uvclose(tno) . ...

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• Pulsar Group PmWiki/Page specific variables
• Keeping Track of UV Variables
• VLBI Wiki | PmWiki / Page-specific Variables

... 4. (a) Distribution of distance from the Galactic plane, (b) kinematic diagram, and (c) relation between metallicity and distance from the Galactic plane for RR Lyrae stars with [Fe /H ] > -0.95 . ... The solid line in the middle panel is a regression line, whose slope is determined by the subsystem?s rotation rate; the open circles and dashed line correspond to stars with [Fe/H] > -0.4, and the filled circles and dashed line to stars with -0.95 < [Fe/H] < -0.4. ... next figure | privious figure . ...

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OptInt PmWiki : Pm Wiki / Page specific variables . ... Page variables have the form {$ variable } , and can be used in page markup or in certain formatting strings in PmWiki. ... Prefixing the variable name with an asterisk (*) means the variable reflects the value related to the target page or main page. ... Namespaced} - spaced page name, as in "Page Variables" . ... Defines new Page Variable of name $CurrentSkin, which can be used in the page with {$CurrentSkin} (also for Conditional markup ). ...

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• OptInt PmWiki : Page specific variables
• OptInt PmWiki : PmWiki / Other Variables
• OptInt PmWiki : Other Variables

The ESA/ESO Astronomy Exercise Series 2 . The Distance to Messier 100 as Determined by Cepheid Variable Stars . ... The small variations in distance to the individual Cepheid variable stars in the Cloud are negligible compared with the much larger distance to the SMC. ... In this way Cepheid variable stars can be used as one of the 'standard candles' in the Universe that act either as distance indicators themselves or can be used to calibrate (or set the zero point for) other distance indicators. ...

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• ASP: Making Your Own Astronomical Camera

... CEPHEID VARIABLE STARS: A Cepheid variable or Cepheid is a member of a particular class of very luminous, massive variable stars with pulsation periods of 1-70 days. ... The relationship is calibrated using data collected from Cepheids whose distances are determined by other means. ... Browse through the 68 CCD fits images he sent you, using ds9 and locate the Cepheid variable. ... Image credits: ESA - "http://sci.esa.int/science-e-media/img/20/cepheid-variables.jpg" . ...

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• Philip Lah's Research

... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...

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• New Luminous Variable Star in M33

... В теме В разделе По форуму . ... Темы, интересные всем ? ... Научная панорама ? arxiv:0705.4195 VSOP: The Variable Star One-shot Project . предыдущая тема следующая тема . ... 0 Пользователей и 1 Гость просматривают эту тему. ... arxiv:0705.4195 VSOP: The Variable Star One-shot Project I. Описание проекта и первый релиз данных (VSOP: The Variable Star One-shot Project I. Project presentation and first data release) . ... VSOP - The Variable Star One-shot Project ( http://vsop.sc.eso.org/ ). ...

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Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Our BVR CCD photometric study of the globular cluster NGC 7006 permitted us to find two new suspected RR Lyrae variables. A cluster chart is presented with the position of known and suspected variables marked. ... According to the Catalogue of Variable Stars in Globular Clusters (Clement et al., 2001), it contains 76 variables, most of which are RR Lyrae variables, the RR1 to RR0 ratio being 8:55. ... for suspected and some of known variable stars. ...

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• Nearby Cepheid Variable RS Pup
• Астронет > Nearby Cepheid Variable RS Pup
• NGC 2261: Hubbles Variable Nebula

Chapter 11. Specifying OpenGL Environment Variable Settings . ... Several antialiasing methods are available and you can select between them by setting the __GL_FSAA_MODE environment variable appropriately. ... To see the available values for __GL_FSAA_MODE along with their descriptions, run: nvidia-settings --query=fsaa --verbose . The __GL_FSAA_MODE environment variable uses the same integer values that are used to configure FSAA through nvidia-settings and the NV-CONTROL X extension. ...

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• Debugging and Tracing

... We have compared visualized fields of GSC and USNO A1.0 catalog with unpublished photographic finding charts that were sent by L. Plaut to the compilers of the GCVS. ... 7-15 A9 --- GCVS GCVS or NSV name 17-25 F9.4 --- GSC GSC number 26 A1 --- NoteFlag *Nonstar (GSC) flag 28-29 I2 h RA2000GSC.h Hours RA (GSC), equinox 2000.0 31-32 I2 min RA2000GSC.m Minutes RA (GSC), equinox 2000.0 34-38 F5.2 s RA2000GSC.s Seconds RA (GSC), equinox 2000.0 40 A1 --- DE2000GSC.- ... Plaut, L., 1966, Bull. ...

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• General Catalogue of Variable Stars: Homepage.
• Future Prospects of Variable-Star Catalogues
• General Catalogue of Variable Stars: classification.

lsst.tcc   1.2.2-3-g89ecb63 . ... Namespaces . Classes . ... Namespace List . Namespace Members . All   Classes   Namespaces   Files   Functions   Variables   Typedefs   Enumerations   Enumerator   Macros   Pages . ... rotate . ... tcc.cmd.rotate Namespace Reference . def  . ... list  . all__ = ["rotate"] . def tcc.cmd.rotate.rotate . ... Definition at line 13 of file rotate.py . list tcc.cmd.rotate.__all__ = ["rotate"] . ...

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• Student Research at Manastash Ridge Observatory
• lsst.tcc: python/tcc/cmd/rotate.py File Reference
• lsst.tcc: tcc.parse.getPVTList Namespace Reference

README for XFree86 on OS/2 : Adding Variables to CONFIG.SYS . ... ETC . Set to an ETC directory. Normally, this is already set to the ETC directory of the TCP/IP code, such as SET ETC=C:\TCPIP\ETC For Warp 4 and later, this may point to the \MPTN\ directory. ... Normally you will set this variable to the same value as the HOSTNAME variable and simply add a :0.0 after it, such as SET DISPLAY=myhost:0.0 Read the X11 man page on the exact meaning of these postfixes and other options. ...

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• Additional problems at the transition
• Specifications
• ApSA courses

... The particular variables it is concerned with are tick , which is the number of microseconds added to the system time during a clock interrupt, tickadj , which sets the slew rate and resolution used by the adjtime system call, and dosynctodr , which indicates to the kernels on some machines whether they should internally adjust the system clock to keep it in line with time-of-day clock or not. ... Set the kernel variable tickadj to an internally computed "optimal" value. -t tick . ...

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• Miscellaneous Options
• APOD: 2013 September 9 - Nearby Cepheid Variable RS Pup
• APOD: October 20, 1999 - NGC 2261: Hubbles Variable Nebula

PCA Analysis of MaNGA Sky Spectra Meng Gu What is PCA Set of observations of possibly correlated variables Set of values of linearly uncorrelated variables (PCs) Straightforward & Has been applied to astro. spectra for many purposes. QSO-PCA Bailey 2012 Why PCA in Sky Subtraction To deal with complex and ever-changing telluric featu L s el One Body ree,vPCA method is promising! ... 0.Body Level Three 2<mean flux<0.2 2.Variance dy thevel F<0.8 Bo of Le flux our 3. ...

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• The AstroStat Slog variable selection
• Funtools Environment Variables
• XPA Access Control

... This chapter discusses values that JavaScript recognizes and describes the fundamental building blocks of JavaScript expressions: variables and literals. ... So, for example, you could define a variable as follows: . var answer = 42 And later, you could assign the same variable a string value, for example, . ... These are fixed values, not variables, that you literally provide in your script. ... A string literal is zero or more characters enclosed in double ( " ) or single ( ' ) quotation marks. ...

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• Function Specification
• All Sky Catalog at 2.7 GHz
• Principal Components Analysis

The period of this variable was first determined by Tony Vanmunster (Center of Backjard Astrophysics). We have taken the observations with CCD ST-7 and 60-cm reflector of SAI Crimean station. ... The longest set was taken at night of 2000 February 12 including 291 R 60 second long frames with the magnitude limit of 18. Summing all these frames in a single one I have taken a "deep sight" of this region having the limit of 21.7R. The effective exposition is 4 h. 51 m. Look at this frame! ...

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• Further Data Types
• LWN: Driver porting: per-CPU variables

. · . Международная конференция   к 100-летию Б.В. Кукаркина . · Сотрудники отдела . · Семинар по Звездной астрономии . · Наша научная работа . · Общий Каталог Переменных Звезд . · Каталог рассеянных скоплений . · Наши учителя . · Избранные публикации . · Педагогическая и популяризаторская деятельность . · Наши интернет-ресурсы и другие полезные ресурсы . · Ссылки на каталоги и базы данных . · Фотогалерея . Присылайте Ваши вопросы и комментарии Ольге Дурлевич p >

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• Division of the Galaxy and Variable Stars
• Shugarov's Home Page

... Some data selection widgets for plotting display more indices than needed for some of the plot variables in order to avoid recycling of the data selection widget if the variables change. ... They are organized by class, even though, strictly speaking, an plot class refers only to a specific selection of variables listed in a plot selection widget. ... Also note that the IDL variables in italic font denote a derivation from this variable, i.e. the data is not exactly identical to the variable...

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• Adding plot variables
• Table of Contents
• OT V.1.4.1 installation instructions