Next: MOUNTING= 'FORK' Up: Horizon obstructions Previous: Getting the data . A character descriptor is needed to specify which of three possible formats is actually used: . MOUNTING : possible values are 'FORK' , 'GERMAN' , or 'ALTAZ' . ... In the case of an alt-azimuth mounting that displays only equatorial coordinates to the user, it would be more convenient to use the 'FORK' form of table, despite the actual mounting. ... The next three subsections describe these three forms. ...

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Name: GDSD_Wxxx Purpose: Write FITS data field File: gdsd_wfits.shl Category: GDS Author: J.P. Terlouw Use: CALL GDSD_Wxxx ( file_id, name, level, value, *error ) xxx can be REAL, DBLE, INT, LOG or CHAR, depending upon type of `value'. file_id = file identifier, CHARACTER name = name of FITS item. CHARACTER*8 level = coordinate word specifying the substructure at which the FITS item is to be written. INTEGER value = variable containing the data for the FITS record. ...

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• http://www.atnf.csiro.au/computing/software/gipsy/tsk/getval.dc1
• http://www.atnf.csiro.au/computing/software/gipsy/sub/gdsd_rxxx.dc2
• http://www.atnf.csiro.au/computing/software/gipsy/sub/dcdpos.dc3

... There is an opportunity to perform O-C calculations for objects which are absent in the data base of the package. Such objects can be described by orbital elements or by initial coordinates and velocities. ... On pressing Edit file button user has a possibility to look through the list of object elements or their coordinates and velocities to add or to change it. ... For example, the designations of objects in the list can occupy the last position in each line. ...

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• Keywords_289

Clear the screen and display a title at the top} display_title(++ TRANSFORMATION of CELESTIAL COORDINATES ++) {Set the delimiter to % so that commas can be used in the prompt string} set_delimiter(%) {Get the coordinates to transform from and into} ask_for_character ( Transform from which system [h,a,r,e,g]%hareg%c1) ask_for_character (........... to which system [h,a,r,e,g]%hareg%c2) new_line {Write an appropriate message depending on the ...

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On Systematic Differences in Individual Solutions and IERS Products Zinovy Malkin Institute of Applied Astronomy RAS, St. Petersburg, Russia 1 Present status Proper determination, modelling, and accounting for systematic differences between contributed series is of the great importance in compilation of the IERS products. ... Possible sources of systematic differences are: · Different reference systems (e.g. TRF, CRF, geopotential, time scale). ... 87 IERS Technical Note No. ...

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• http://www.gao.spb.ru/english/personal/malkin/publ/zm14e.pdf
• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf

FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 4: Observing with the FGS > 4.4 Transfer Mode Overview . ... 4.4.1 The FGS Response to a Binary . ... Figure 4.3 shows the changes in the observed FGS1r interferogram due to binary systems of varied separations and magnitude differences. In Figure 4.3 a we display the interferogram of a wide binary pair with component separations and magnitude differences of (200 mas, 1.0) respectively. ...

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• ACS Data Handbook
• Introduction
• CSPICE Routines: SCE2S_C

Convex chains for Schub ert varieties Valentina Kiritchenko (joint work with Evgeny Smirnov and Vladlen Timorin) In [4], we constructed generalized Newton polytopes for Schubert subvarieties in the variety of complete flags in Cn . Every such "polytope" is a union of faces of a Gelfand­Zetlin polytope (the latter is a well-known Newton­Okounkov body for the flag variety). ... A root space of rank n is a coordinate space Rd together with a direct sum decomposition Rd = R d 1 . ... Bott towers. ...

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• http://www.mccme.ru/tg2007/talks/Kac.pdf
• http://www.mccme.ru/tg2007/talks/Kumar.pdf

Position Switching Separation Tolerance with Arecibo in L-Band Travis McIntyre The University of New Mexico July 2010 Revised December 2013 Abstract The blocked telescope aperture at Arecibo creates standing waves in the bandpass around 1MHz. ... Test observations with Arecibo in L-Band show that position switching effectively removes standing waves for separations of one half FWHM or less. Standing waves remain for separations of one FWHM, increasing the rms of the baseline by 20%. ...

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• CIMA Source Catalogs
• nearFarField

... The European HST Archive has been moved to ESA's European Space Astronomy Centre ( ESAC ), Spain, where most of ESA's Space Science Archives are located and operated from. ... The Space Telescope European Coordinating Facility (ST-ECF), jointly operated by ESA and the European Southern Observatory ( ESO ) was, until the end of 2010, the European HST science facility, supporting the European astronomy community in exploiting the research opportunities provided by the Hubble Space Telescope. ...

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... This makes spatial event selection very hard of even impossible in cases where the object is too faint to clearly stand out against the X-ray background. movecalc takes an event table with aspect corrected X / Y coordinate columns (as generated by task attcalc ) and adds two new columns X_MOV / Y_MOV (different names can be specified via parameters xmovcol / ymovcol ) containing the corresponding coordinates in a reference frame that is centered on the moving object at all times. ...

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• Introduction

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• Correlating Spectral Data with Spatial Gain Variations
• *plcreate* -- Defining a Region
• The AstroStat Slog Blog Archive The chance that A has nukes is p%

Download Izmccd (~2.7 MB). ... a) a choice of the best mode of measurements of stars and objects ("Properties/Measurement"), . b) a choice of reference stars. ... 1) necessity of presence on an image of a plenty of stars (we recommend to apply this mode, if on the frame of reference stars is more 100) . ... Sx and Sy depend from residuals at all reference stars (reference stars are marked by blue color). ... These residuals are the image of the star a minus function of a profile for each pixel. ...

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The efficiency of interaction of radiation with a particle and hence its optical properties depend on the particle chemical composition, size, shape, structure, etc. ... Particle size expressed in units of the wavelength of incident radiation, together with chemical composition, most strongly affects the optical properties of a scatterer. ... There are many methods to solve the light-scattering problem for a homogeneous spheroid (our survey of the light-scattering methods see here ). ...

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Microsymposium 38, MS083, 2003 (A4 format) MERCURY: LOCAL VARIATIONS OF THE PHOTOMETRIC RELIEF. ... Because of trajectory and pointing angle constraints the planet could be observed from Mariner 10 only over a small range of phase angles between about 75o and 110o. Therefore the photometric investigations are restricted to measuring the distribution of brightness on the Mercurian disk. ... Raw versions of real-time processing pictures FDS 0000984 and FDS 0000986 were used (images 196 and 202). ...

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• http://selena.sai.msu.ru/Shev/Publications/m44_76_sinitsin_shevchenko.pdf
• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
• Morphological Catalogue Of The Craters Of Mars

... Packet Format . ... The TCC broadcasts UDP packets containing position information. ... Packet Header . ... int4 . ... double . ... pos, vel double . ... pos, vel, time double . ... See the TCC Message Keywords Dictionary for full definitions of most items in the "data" section of the packet. pos, vel double is a structure containing two doubles: "pos" and "vel"; it contains the same information as the TCC's "coordinates" (p,v,t triplets), but with time given by the "TAIDate" entry in the packet. ...

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• TUI:Telescope:Slew Window:Options:Mag PM
• TUI:Telescope:Slew Window
• lsst.tcc: python/tcc/axis/coordConvWithFP.py Source File

... In Spiral . Between spiral . ... Center of vortices . ... to density exterema . ...

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• Arrays and Strings
• Functions
• Character Classification and Conversion

... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...

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• Journal "Peremennye Zvezdy"
• Ocean Planet Pole To Pole
• Астронет > Ocean Planet Pole To Pole

... Explanations. Each row contains at 0h of Time Dynamical Terrestrial: month, day, apparent right ascension (hours, minutes, seconds), apparent declination (degrees, minutes, seconds), hour difference of declination (seconds), apparent radius (minutes, seconds), equation of time (hours, minutes, seconds), hour difference of equation of time (seconds), time of upper culmination of Sun (hours, minutes, seconds), change in moment of upper culmination when longitude changes on 1 hour to west (seconds). ...

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ESO Phase 3 Data Release Description Please start from this template when preparing the documentation for your ESO Phase 3 data release. ... Finally, the release description will be published as submitted - without further editing by ESO - to support the user community in utilizing the data. ... Please indicate if this is a catalogue data release. ... Data Reduction and Calibration Please address the following questions for scientific catalogue data, particularly in case of source catalogues: . ...

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• VLTI Calibrator Selection Help Page
• Fonts used in the guide
• FORS1 Photometric System Characterization

... Another significant contribution to the crystal energy of metals is the electron-ion interaction or the electron bandstructure energy (E BS ) which is defined by the interaction of valence electrons and the Brillouin zone (BZ) planes. ... The program BRIZ has been developed for 3D visualization of Brillouin zone configurations and intersections of BZ planes with a Fermi sphere[4]. ... 1.75 (electrons/atom). ... 4] Degtyareva V.F., Smirnova I.S.: BRIZ: a vizualization program for Brillouin zone ? ...

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