... ACS/WFC File Suffixes, Primary Header Keywords, and Location of New Reference Files . ... News and . ... ACS ETC . ... Reference Files . ... ACS ISRs . ... File Suffix . ... Header Keyword . ... File containing CTE correction parameters. ... The PCTETAB reference table, as well as the DKC files, are now listed on the ACS Dynamic Reference file pages. A summary of both types of reference files is located at the bottom of: http://www.stsci.edu/hst/observatory/cdbs/SIfileInfo/ACS/reftablequeryindex . ...

... NOTE that this call also sets the state of the cal to the returned instrument. The and are obtained from respectively from the INSTRUME and DATE-OBS keywords of the dataset header. The is read from the RA_PNT , DEC_PNT and PA_PNT keywords (this is actually wrong, since the instrument attitude is what should be stored in these, not the spacecraft attitude). The boresight is then obtained for the exposure start time, and calculated by applying the boresight rotation to . ...

... For reducing data from ESO instrumentation it is assumed that the FITS headers conforms the standards set by the document ``ESO Archive, Data Interface Requirements''. ... As an example, in the ESO case the exposure type is stored in the ESO hierarchical FITS keyword `HIERARCH ESO GEN EXPO TYPE'. ... To fill the CCD keywords with the telescope and instrument setup parameters, like name of the telescope, CCD used, read-out noise, frame size, etc. the command LOAD/CCD can be used. ...

Next: Three-dimensional Data Analysis in IRAF and ZODIAC+ . ... A data analysis system has been developed at SRON, which has been designed to allow rigorous control of the quality of its processed data products. ... This means recording all parameters of all steps which lead to the establishment of the final data products (Figure 1 ). ... Figure: A processing pipeline is a sequence of tasks with several input/output files and parameters, which pass data from one task to the next. ...

Sherpa Aneta Siemiginowska 1 SHERPA CIAO's Modeling and Fitting Application Aneta Siemiginowska CXC Astrostatistics Workshop, HEAD meeting , New Orleans, Septemter 2004 Sherpa Aneta Siemiginowska 2 Modeling and Fitting Software XSPEC - analysis of 1D X-ray data (imaging + grating) ISIS and Pint of Ale- primarily for analysis of highresolution (ie grating) X-ray data ... Jointmode data: spatialspectral, spatialtiming Use scripts based on Sherpa only commands. ...

Program: CREATE Purpose: Creates a SET (and subsets) Category: UTILITY File: create.shl Author: K.G. Begeman Keywords: OUTSET= Name of set to create. ... N] This keyword is asked only when the set you want to create already exists. ... This item will be put in the header and will determine the coordinate system CTYPE1= Enter axis name of first axis [stop axis input] For the n_th axis the keyword will be CTYPEn=, like all the following keywords NAXIS1= Size of axis in grids. ...

... STScI has undertaken a project to place all HST keyword information in one source, the keyword database, and to provide a mecha­ nism for making this keyword information accessible to all HST users, the keyword dictionary, which is a WWW interface to the keyword database. ... Along with form­ ing the headers for the science data, most keyword values are ingested into HST archive catalog fields where they are accessible for archive searches and data characterization. ...

splitxyz - filter to divide (x,y,z[, distance ,heading]) data into (x,y,z) track segments . splitxyz [ xyz [ dh ] file ] -C course _ change [ -A azimuth / tolerance ] [ -D minimum _ distance ] [ -F xy _ filter / z _ filter ] [ -G gap _ distance ] [ -H [ nrec ] ] [ -M ] [ -N namestem ] [ -S ] [ -V ] [ -Z ] [ -: ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] ... If xy _ filter is non-zero, the data is first divided into segments and then the x,y values of each segment are filtered separately. ...

RADIOASTROPHYSICAL DEPARTMENT  INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . ... Radioastrophysical Department , Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Science. ... Head of Laboratory dr. Gubin A.V. LABORATORY of INFORMATION SUPPLY and METHODOLOGY of RESEARCH . ... Head of Observatory Kitsanov S.V. SIBERIAN SOLAR RADIO TELESCOPE . Siberian solar radio telescope data at 5.7 GHz in I SOHO EIT 171 SOHO EIT 195 SOHO EIT 304 MDI Continuum MDI Magnetogram . ...

... The instrument modes and arms should be indicated and described, and the keywords that distinguish between different modes should be indicated (usually INS.MODE is used if it is a mode and OCS keys are used in case it is related to an arm). ... Raw frames The format of the raw frames for each mode and arm should be described. ... The design should be checked on pre-processing or processing, which involves products only (no trigger via raw frames). ... QC parameters. ...

This module provides for the customization of HTTP response headers. ... This module provides a directive to control the sending of HTTP headers. ... Header . ... Syntax: Header set|append|add header value . ... Module: mod_headers . This directive can replace, merge or remove HTTP response headers during 1xx and 2xx series replies. ... set . The response header is set, replacing any previous header with this name . ... The response header is appended to any existing header of the same name. ...

МОСКОВСКИЙ ЦЕНТР . НЕПРЕРЫВНОГО МАТЕМАТИЧЕСКОГО ОБРАЗОВАНИЯ . ... Механико-математический факультет МГУ ( в 2000 2010 см также MM-online ) . ... Институт лингвистики РГГУ . ... Школы города Москвы . ... Школа ?179 при МИОО . ... Специализированный учебно-научный центр МГУ (СУНЦ МГУ, школа им. А. Н. Колмогорова, бывш. ... Кировский Центр дополнительного образования ?Одаренный школьник? Центр развития дополнительного образования имени Бернулли (Краснодар) . ... Летняя экологическая школа (ЛЭШ) . ...

For all keywords that contain a red and a blue value, the blue value comes first. ... The full pathname, but without the trailing "b.fit" and "r.fit", that would be given to the next exposure if the basename argument is not given to the expose command. ccdHeaters=float,float . ... bluelambda2=float [M] . The center wavelength for the given grating: the 1 or 2 indicates the grating bay. The bluelambda and redlambda keywords match one set of these, depending on the position of the turret. ...

... Orion: Head to Toe . ... Explanation: Cradled in cosmic dust and glowing hydrogen, stellar nurseries in Orion the Hunter lie at the edge of a giant molecular cloud some 1,500 light-years away. ... To its left are the Horsehead Nebula , M78 , and Orion's belt stars. Sliding your cursor over the picture will also find red giant Betelgeuse at the hunter's shoulder, bright blue Rigel at his foot, and the glowing Lambda Orionis ( Meissa ) nebula at the far left, near Orion's head. ...

... The LH or list header element is used to provide a title for a list. ... An SGML identifier used as the target for hypertext links or for naming particular elements in associated style sheets. ... This is one of the ISO standard language abbreviations, e.g. "en.uk" for the variation of English spoken in the United Kingdom. ... The language attribute is composed from the two letter language code from ISO 639, optionally followed by a period and a two letter country code from ISO 3166. CLASS . ...

... Keywords: head.S . ... In the "Tour of the Linux kernel source" section there is reference to boot/head.S. I did a find on the source, this is a list of the "head.S"'s in the source: ./arch/i386/boot/compressed/head.S ./arch/i386/kernel/head.S ./arch/alpha/boot/head.S ./arch/alpha/kernel/head.S ./arch/sparc/kernel/head.S ./arch/mips/kernel/head.S ./arch/ppc/kernel/head.S ./arch/ppc/boot/compressed/head.S ./arch/m68k/kernel/head.S Obviously, there is a different one for each architecture. ...

... IKI STRUCTURE . ... Dr. Evgeny Lupian , Earth remote sensing projects support . ... Ilya Chulkov , instrument design and development . ... head - Prof. Dr. Nikolai Erokhin Theoretical and numerical approach to study Earth and space multi scale phenomena, such as tornadoes, plasma waves and Earth-ionosphere-magnetosphere interactions. ... Very Long Base Interferometry Integrated Departments Onboard and Special Instruments R head - Ilya Chulkov Complete cycle of instrument development . ...

OptInt PmWiki . Pm Wiki / . Edit Page | ... MROI Delay Line Design Contract . ... MROI DL Design Contract Private Material . ... Group Headers . Wiki groups | ... Group headers allow authors to create groups with custom headers and footers without having to coordinate with a wiki administrator . ... You can also set the variable $GroupPrintHeaderFmt and $GroupPrintFooterFmt in the same way as $GroupHeaderFmt and GroupFooterFmt in order to change the header used when action=print . ...

AO Home AO Astronomy Schedule Receivers CIMA AO IDL . IDL is the recommended data-reduction package for Arecibo spectral-line data. The different back-ends produce different data format. ... Mock spectrometer standard FITS format headers . Mock spectrometer PSRFITS format headers . WAPP CIMAFITS format headers . Interim Correlator IDL headers . ... Search WAPP data . ... How to fix WAPP FITS files taken with doppler tracking in order to read them with standard FITS readers . ...

... Animation . Arrow . ... I created the first animation by running Script-Fu / Animators / Fire on the head of an arrow. ... I merged the animation with the background image, and specified a final X offset of -128 (the background is 128 pixels wide). This results in an animation with a nice moving background. Note that you can also use a background that is wider than the image, as long as you specify the width of the background for the final X offset if you want the final animation to loop. ...