... ppssumm will create these five HTML summary pages: . ... The product and processing information for the EPIC instrument. ... Each page will also link to the several pages created for any other instruments that took data in a given observation, as well as a link to the Observation Data File summary page. All of the information necessary to create a page will be read from the Observation summary (ascii file) and the Pipeline Processing Summary Index File (see [] for details). ...

Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...

... The analysis and reduction of the STIS flanking fields proceeded in similar fashion as for the imaging of the Main STIS Field. ... The DARK calibration reference file used in the CALSTIS data reduction steps was constructed using a 'delta-dark' image appropriate for the epoch of the flanking field observations. ... DRIZZLE drop-size used for the flanking fields was a "pixfrac" of 0.8. ... For information on the data reduction, please read first the technical information for the Main WFPC2 Field . ...

... It provides long range planning information to the scheduling team; it provides bright object, timing, and orientation information to the observation planning team; and it provides graphical description of the observations and their constraints. ... The GUI graphically displays the constraints that are computed by Spike and stored in the description files and in the database. ... BOAS processes all bright objects that have entered the database since the last time BOAS was run. ...

... Classes . ... Class List . ... casa . casa::HistTiledCollapser< T > . ... Generate histograms, tile by tile, from a masked lattice. ... HistTiledCollapser ( LatticeStatistics < T > *pStats, uInt nBins) . Constructor. virtual void . ... process ( uInt accumIndex1, uInt accumIndex3, const T *inData, const Bool *inMask, uInt inIncr, uInt nrval, const IPosition &startPos, const IPosition &shape) . ... template<class T > . ... virtual Bool casa::HistTiledCollapser < T >::canHandleNullMask . ...

. This diagram illustrates the boxes generated by a UL list with two LI list items. There are two parts to the illustration. The first shows the actual rendering of the boxes generated by the list elements. Background colors and border styles vary to delimit the box areas. The second shows the same rendering, but the content, padding, border, and margin edges of each box are shown explicitly. In particular, the illustration shows how vertical margins between the LI boxes collapse. Return to image.

Next: *timsort* Up: Timing Analysis Previous: Summary of tasks in . ... Events will be time ordered in the output file. xt> timsort xdata$snr psr ``c 503 513 24'' none A light curve is then generated and plotted so we can inspect the gross properties of the sample (the sequence of good-data intervals and gaps) and any source variability. xt> ltcurv psr none psr 500 xt> ltcplot psr_ltc Finding this sample satisfactory, we search for periodicity with a fast Fourier transform. ...

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

... Bojan Nikolic web pages (r. 329) . ... Building CASA . ... XML Schema for the tools description ( casa.xsd ) . These are my notes on how to create a new tool for CASA, in particular in this case a new tool to implement WVR phase correction. ... include <wvrphase_cmpt.h> . ... All of the files below need to be placed in the casa/code/xmlcasa/implement/synthesis directory and the tool will be built and accessible from Python. ... create (); wvrphase . ... How to create a new tool in CASA . ...

... Apache HTTP Server Version 2.2 . ... Default <base> assignment through a new map directive base . ... The directives can come in any order, but are processed in the order they are found in the imagemap file. base Directive . ... The base directive overrides ImapBase as set in a .htaccess file or in the server configuration files. In the absence of an ImapBase configuration directive, base defaults to http://server_name/ . ... The ImapBase directive sets the default base used in the imagemap files. ...

. Russion version . Last updated on May, 2008 . RadioAstron Mission .

makeflat -- makes flatfields corresponding to the output image of asncombine. makeflat association flatlist . ... ASCII file with list of flatfields as used by NICMOSlook. resolution . ... The ST-ECF tool NICMOSlook performs this task by determining the appropriate factor from narrow band flatfields. ... This task takes a list of flatfields in the same format as NICMOSlook, shifts and co-adds each of the flatfields in the list, and creates a new list which can be used as input for NICMOSlook. ...

... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....

... CREATE FULLTEXT MAPPING -- binds tokens and dictionaries . ... CREATE FULLTEXT MAPPING bind token of type lexemetypename and full-text dictionaries in given configuration cfgname . ... CREATE FULLTEXT CONFIGURATION testcfg LOCALE 'testlocale' LIKE russian_utf8; CREATE FULLTEXT CONFIGURATION =# CREATE FULLTEXT MAPPING ON testcfg FOR lword,lhword,lpart_hword WITH simple,en_stem; CREATE FULLTEXT MAPPING =# \dF+ testcfg Configuration 'testcfg' Parser name: 'default' Locale: 'testlocale' Token | ...

The Wideband Arecibo Pulsar Processor - File Format Page . WAPP files have three sections that appear sequentially in this order: an ASCII header description, the binary header, and finally the actual binary data. ... The WAPP realtime observation engine does not produce files larger that 2 Gbytes. At one time this represented a fundamental limit to Linux files. ... Each file will have it's own header, even when the files are simply continuations of a single observation. ... long int . ...

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

grdclip - Clipping of range in grdfiles. grdclip input _ file . grd -G output _ file . grd [ -Sa high / above ] [ -Sb low / below ] [ -V ] grdclip will set values < low to below and/or values > high to above . ... Sa Set all data[i] > high to above . Sb Set all data[i] < low to below . ... To set all values > 70 to NaN and all values < 0 to 0 in file data.grd, try: grdclip data.grd -G new_data.grd -Sa 70/NaN -Sb 0/0 -V gmt , grdlandmask , grdmask , grdmath , grd2xyz , xyz2grd . ...

... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...

dfos = Data Flow Operations System, the common tool set for QC . ... This page provides documentation about the process behind the PWV monitor . ... QC1 table ambient_PWV (store PWV); xshooter_telluric (to identify saturated telluric data) . dfos tools . ... The workspace UVES_STD is generated in the giraffe account, as defined in .dfosrc_UVES_STD . ... The tool help is available with option -h. It is called as a giraffe cronjob in four steps: for crires , visir , xshooter , and uves . ...

... 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. ...