... For a certain group of XMM PPS products (e.g. EPIC background maps, EPIC maximum-likelihood source lists, EPIC images, EPIC sensitivity maps) a list of commands is executed stored in an ascii file (hereafter check file). ... The tests include existence and parameter range checks for header key words and source tables columns of EPIC PPS Fits files. ... This check file performs existence and parameter range checks for EPIC PN, MOS1, MOS2 background maps in the energy bands 0,1,2,3,4 and 5. ...

... Classes . Files . ... casa . casa::FITSTableWriter . ... Private Member Functions | ... More... #include < FITSTable.h > . ... FITSTableWriter ( FitsOutput *file, const RecordDesc &description, const Record &maxLengths, uInt nrows, const Record &extraKeywords, const Record &units, Bool freeOutput= True , const Record &variableShapes= Record ()) . ... References row_p . ... BinaryTableExtension * casa::FITSTableWriter::bintable_p [private] . ... Record casa::FITSTableWriter::row_p [private] . ...

... example, note below the dramatic speedup in searching a 1 Gb file using an AND filter, even when one of the columns (pha) has no index : time fundisp \ huge.fits'[idx_activate=0,idx_debug=1,pha= 2348 4000 4000 1]' \ x y pha x y pha ---------- ----------- ---------- 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 3999.48 4000.47 2348 ... Currently, indexed filtering only works with FITS binary tables and raw event files. ...

MRO-ICD-CAM-1100-0108 FTTNAS-FTTA.odt Page 1 of 7 MRO FTT / NAS FLC ICD FTT / NAS Electronics to FTTA Controller ICD MRO-ICD-CAM-1100-0108 The Cambridge FTT Team Rev 1.0 9 May 2013 Cavendish Laboratory JJ Thomson Avenue Cambridge CB3 0HE UK MRO-ICD-CAM-1100-0108 FTTNAS-FTTA.odt Page 2 of 7 ICD Description ... 2.1 Signal definitions.. ... The analogue input interface in the FTT-NAS electronics interface is to accept the full range of output available, specifically: 1. ...

... The PC is interfaced with a high speed parallel card. ... Data is read from the radar interface hardware and sent over the VME bus to a MVME162 card. From the 162 card the data passes over the IP (Industry Pack) bus to a second high speed parallel card in the WAPP PC. ... WAPP Radar interface as tested , 5 megabytes/second . ... Stop the radar observation, in the vxWorks window . Kill the radar interface gui window . ... There remains a bug in the data taking with the WAPP radar interface. ...

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

... The routine processing of STIS data in the calibration ``pipeline" requires an interrelated set of software tasks and databases developed and maintained by many groups at STScI. We present the systems-level design of this calibration pipeline from the perspective of the STIS instrument group at STScI. We describe the multiple interfaces to the pipeline processes that the STIS group works across in an effort to provide for the routine calibration of STIS data. ... For example, the STIS group: . ...

... 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. ...

... For observations we selected all Case galaxies in the zone = - from the Case lists III, IV, V, VIII, XI, XII and XIII which were classified in the Case survey by some indication on presense of [O III ] 4959,5007 emission lines (vs - very strong, s - strong, m - medium, w - weak, w? - weak?) and which had not been observed yet. ... Аdditionally nine Markarian galaxies in the same sky region were observed in hope to have better completeness in picking up all probable BCGs. ...

... Abstract Retrieve the current short error message, the explanation of the short error message, or the long error message. ... The choices are: The current short error message, the explanation of the short error message, or the current long error message. ... Most CSPICE short error messages have corresponding explanation text. ... Not all errors have long error messages. ... Get explanation text for the current short message and print it: ./ getmsg_c ( "EXPLAIN", MSGLEN, msg ); [Output message] . ...

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: . ...

... The nodes defined by the specified region and lattice spacing will be set equal to one of three possible values depending on whether the node is outside, on the polygon perimeter, or inside the polygon. ... The xy-files simply represent data point locations and the mask is set to the inside or outside value depending on whether a node is within a maximum distance from the nearest data point. ... Default is grid registration]. ... S Set nodes depending on their distance from the nearest data point. ...

This section is currently based solely on the Miniature Card specification v1.1. Address A0 to A24 are the address bus lines that can address up to 32 Mwords (64 MBytes). The Miniature Card specification does not require the Miniature Card to decode the upper address lines. A 2 Mbyte Miniature Card that does not decode the upper address lines would repeat its address space every 2 Mbytes. ... Data lines D0 through D15 constitute the data bus. ... Voltage Sense 1 signal. ...

SAI VO . ... SAI CAS . ... Web Services . Catalog Access Services . ... SAI VO Wiki . ... Program Access . SAI CAS Wiki . SAI Web Services . ... DSS Mirror . ... We provide an implementation of IVOA standard Simple Image Access Protocol interface to our DSS mirror. Service metadata is available here . Currently, we provide the atlas service only, which returns the list of original DSS images intersecting the requested sky area. ... SAI MSU | ...

... Reference ID: IRIG . Driver ID: IRIG-TPRO . ... Features: KSI/Odetics device driver (required) . This driver supports the KSI/Odetics TPRO and TPRO-SAT IRIG-B Decoder, which is a module connected directly to the SBus of a Sun workstation. ... Using the TPRO interface as a NTP reference clock provides precision time only to xntpd and its clients. ... Specifies the time offset calibration factor, in seconds and fraction, with default 0.0. time2 time . ... Not used by this driver. flag2 0 | ...

This diagram shows the effect of the 'collapse' value of the 'border-collapse' property. ... The left and right content, padding, border, and margin areas of each cell are labeled by rotated text above each of the areas. Each (red, dotted) grid line bisects the border between two cells. The table width is indicated below the cells as encompassing all the left and right content, padding, border, and margin areas of the cells, except for the cells that touch the sides of the table. ...

Ground Support of RadioAstron . Control and Tracking Stations . RadioAstron satellite control (command transmission, telemetry, orbit measurements) will be conducted from Evpatoria and Bear Lake control stations. ... Coarse orbit measurements will be carried out from control stations. Each measurement takes ten minutes. ... Orbit measurements at tracking stations give only radial component of spacecraft velocity but the measurements are going continuously during observing sessions. ...

The MOD and IOPT parameters value depend of the external magnetic field model (MOD), used during magnetic mapping and IOPT version (IOPT = Kp + 1), see the table: . MOD . External model . IOPT range . ... N.A.Tsyganenko, Planet. Space Sci., ... N.A. Tsyganenko, A magnetospheric magnetic fields model with a warped Tail current sheet: Planet. Space SCI., ...

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 . ...

Stellarium 0.12.3 . ... StelTextureNew Class Reference . ... Get a human-readable message describing the error that happened during loading (if any). ... A texture can be in one of 4 states, depending on how it is loaded. These are Uninitialized, Loading, Loaded, Error. ... If load mode specified with createTextureBackend is Normal, it is immediately loaded (internally, it's in Loading state), and one createTextureBackend is done, its state changes to Loaded on success or Error if loading failed. ...