... The Spectrum Extraction window is activated by clicking on the button in the Main window and contains options for fitting the sky and extracting spectra. ... The window provides two buttons and for an interactive definition of the limits of the sky and the object. Clicking one of the these buttons activates a cursor in the display window. ... The name of the resulting sky file is defined in the text field Sky (image or constant): which includes the default value sky . ...

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• A VLA Survey of the First Quadrant of the Galactic Plane at 1.5
• THE TEXAS SURVEY: THE PRELIMINARY

MAKING THE PROFILES . First of all you are expected to load a FITS file ("FILE"-"LOAD"). ... By pressing the middle button you copy the profile from the first profile window to the second one. ... An example: first integral can correspond to the profile of active region and second integral can correspond to the profile of quiet chromospheric region. ... The second profile (which is subtracted from the first one) you extract after clicking on "SUBTRACT"-"MARK QUIET PROFILE" and marking the region. ...

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... 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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... Analysis of in-orbit data closely follow the CSL data analysis. Stars with known astrometric positions are matched with their image centroids. ... The measured position, the expected position and the offset between the measured and expected positions are calculated and written into a file. ... select catalogued positions for different observations/pointings (e.g. positions of objects in photometric sequence) . ... The new distortion map was generated from in-flight observations of the G153 field. ...

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• User-level errors and warnings

... An FGS astrometry dataset contains all the steps in the target acquisition and tracking sequence. ... To accomplish this task, the DF 224 slews the FGS's IFOV to the expected position of the target within its pickle. ... Once the IFOV arrives at the expected position of the star, the DF 224 delegates control of the FGS to its FGE, which attempts to locate and to track the star by implementing its Search, CoarseTrack, and FineLock algorithms. ... Tracking of the star in FineLock. ...

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• http://www.stsci.edu/ftp/documents/archive-manual/11_dmfstructure.txt
• Future Calibrations, Calibration by Observers, and Calibration Outsourcing
• CSPICE Routines: ORDC_C

... NEWS . WHEN : typically 3 weeks before the official deadline , i.e. date by which the new DFS release has to be operational on the mountain. ... complete list of performed tests. ... description of the new bugs raised during this Integration phase. ... HOW: Integration Acceptance meeting at DFS level with: . ... If needed, specific Integration acceptance meetings at DFS project level and SCCB meetings may be organized to prepare this Integration acceptance meeting. Before this meeting, . ...

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• The plot selection widget
• QA rules: DFS commissioning acceptance
• DFS Commissioning: integration procedure

... To run the <LAYER> version of the example, select: flower.htm . ... However, if the page had several layers with absolute positions, and you wanted to place another layer in a relative position to one of the existing layers, you could use inline JavaScript to calculate the value for LEFT or TOP . ... In this example, there is really no need to use inline JavaScript to position the last flower layer, since you could just let the TOP value default to its natural value, as in the other flower layers. ...

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... to_tsquery( [ configuration , ] querytext text) RETURNS TSQUERY . ... Query rewriting is a set of functions and operators for tsquery type. ... We'll expand query supernovae using table-driven rewriting rules. =# create table aliases (t tsquery primary key, s tsquery); =# insert into aliases values(to_tsquery('supernovae'), to_tsquery('supernovae|sn')); =# select rewrite(to_tsquery('supernovae'), 'select * from aliases') && to_tsquery('crab'); ?column? --------------------------------- ( 'supernova'...

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• Further Information and Bibliography
• APOD: 2006 March 13 - Z Machine Sets Unexpected Earth Temperature Record
• APOD: 2015 May 31 - Supernova 1994D and the Unexpected Universe

... Acronyms and Abbreviations AMOS Advanced Mechanical and Optical Systems (UTM vendor) EIE FTT FLC ICD ISS European Industrial Engineering (UTE vendor) Fast Tip-Tilt First Light Camera Interface Control Document Interferometer Supervisory System NAS NMT NOT TBC TBD UT UTE UTM Narrow-field Acquisition System New Mexico Tech Nasmyth Optical ... Interface design description 2.5 FTT/NAS to ISS ICD This ICD describes the software interfaces of the FTT/NA system to the ISS. ...

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• http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/uploads/MROIDelayLine.InterfaceControl/INT-406-VEN-0013.pdf
• Some notes on the GNU toolchain Bojan Nikolic web pages (r. 329)
• Bojan Nikolic -- Compiling CASA revisited

... JavaScript 1.2: added name , text , x , and y properties Using the HTML A tag or calling the String.anchor method. The JavaScript runtime engine creates an Anchor object corresponding to each A tag in your document that supplies the NAME attribute. It puts these objects in an array in the document.anchors property. ... A string specifying the anchor's name. text . ... The horizontal position of the anchor's left edge, in pixels, relative to the left edge of the document. y . ... Anchor . ...

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• mod_proxy_ftp - Apache HTTP Server
• APOD: December 30, 1998 - Supernova 1994D and the Unexpected Universe
• APOD: 2000 March 12 - Supernova 1994D and the Unexpected Universe

... Plot vectors may be generated in several ways: . a. You may read the vectors from a file using the read command The file is expected to be an ASCII file of columns of numbers (separated by spaces or commas). You define the file to SM using the data command, and associate a column or row of numbers with a SM vector using the read command. ... I can also read a row from the file, instead of a column, by saying read row x 1 Note that the vector is defined by the read command. ...

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• kpvslice: interactive position-velocity slicing
• USNO/ATNF_VLBI
• casacore: casa/Containers/SimOrdMap.h File Reference

... Documentation for the Python objects defined by the project is divided into separate pages for each package, module, and class. The API documentation also includes two pages containing information about the project as a whole: a trees page, and an index page. ... A description of the package. ... A summary of the classes defined by the package. ... The module contents frame contains a list of every submodule, class, type, exception, function, and variable defined by a module or package. ...

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... Using a simple 2-D Gaussian Point Spread Function (PSF) on a constant (flat) sky background, I derive a theoretical photometric and astrometric performance model for analytical and digital PSF-fitting stellar photometry. ... The photometric performance is maximized when either the effective background area or the effective-background-level measurement error is minimized. ... An important, but frequently ignored, noise source is the uncertainty of the measurement of the effective background level ( )...

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• ADASS 2003 Conference Proceedings
• Heuristic Estimates of Weighted Binomial Statistics for Use in Detecting Rare
• Pipeline Processing of Data in the VLT Era

stable spacetime manifold Expected to propagate at speed of light Expected to have 2 independent polarizations Sources ­ ­ ­ ­ http ://www.johnstonsarchive.net/relativity/pictures.html Unmodeled bursts Binary Coalescence Periodic Sources Stochastic Background http ://mucholderthen.tumblr.com/post/55970198303/gravitational-waves-patterns-in-space-time-a 3 LIGO-VIRGO Interferometer Gaussian Noise: Coherent Signal vs. ...

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• Spatial Region Coordinates
• Vertical Structure of the Secondary: Hydrostatic Model
• The AstroStat Slog Blog Archive [Jobs] postdoc position at UC Berkeley

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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• http://www.naic.edu/alfa/ealfa/meeting2/handouts/ultra_precursor.pdf
• http://www.naic.edu/~phil/hardware/vertex/sharemegsvertex/ocu/pcr/mscv51/bin/C1.ERR
• ALFA Diode Temperature-Explanatory Notes

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

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• TRAXY (V0.4) --- Dec99 --- TRAXY (V0.4)
• TRANBACK (V0.2) --- Dec99 --- TRANBACK (V0.2)

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... ISS Russian Segment . ... Consolidated study of the ISS dynamic characteristics; parameters defining a space position of scientific devices and attitude sensors with respect to the station hull deformation; parameters of magnetic and microgravity disturbances on board the station. ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

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... Z Machine Sets Unexpected Earth Temperature Record . ... Credit: Z Machine Collaboration , Sandia National Lab , Lockheed Martin , NNSA, DOE Explanation: Why is this plasma so hot? ... What is known for sure is that the Z Machine running at Sandia National Laboratories created a plasma that was unexpectedly hot. The plasma reached a temperature in excess of two billion Kelvin , making it the hottest thing ever in the history of the Earth and, for a brief time, hotter than the interiors of stars. ...

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• Астронет > Z Machine Sets Unexpected Earth Temperature Record
• XWare > APOD

The first field of each line starts at 0 (zero); the second is 1 (one) and so on. To define which field to sort on you give the position of the field at which to start the sort followed by the position at which to end the sort. The position at which to start the sort is given as the number of fields to skip to get to this position. ... tells sort to skip the first two fields. The position at which to stop the sort is given as the number of the field at the end of which the sort stops. ...

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• Horizontal Tabs
• To define the 'region'
• Defining files with wildcard characters

... ClassљList . ... ClassљMembers . SphericalRegion Member List . ... contains (const SphericalRegion *r) const . ... contains (const SphericalRegionP r) const (defined in SphericalRegion ) . ... contains (const Vec3d &p) const (defined in SphericalRegion ) . ... contains (const SphericalPolygon &r) const (defined in SphericalRegion ) . ... contains (const SphericalConvexPolygon &r) const (defined in SphericalRegion ) . ... contains (const SphericalCap &r) const (defined in SphericalRegion ) . ...

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• Member List
• Stellarium: core/StelSphereGeometry.hpp File Reference