... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

... the shutters, loads . ... We have shutter/receiver protection to protect the receivers when we transmit with one of our transmitters (sband,430, hf). ... this is also controlled by the 430 ch load/antenna switch. closed always wins . ... shutter - open,close, or query the receiver/radar shutters . ... When the 430 dome is being used, we want to close all shutters, but leave the 430 dome receiver under control of the ch load/antenna switch (above the oscilloscopes in receiver room). ... shutter close...

... As input, OFFAXIS takes a visibility dataset and a model of the source total intensity (Stokes I). Given this, it computes the expected off-axis effects (given its internal models of the effects), subtracts this from the data, and produces an output (nominally) corrected dataset. Key: vis Input visibility dataset. ... Key: out The name of the output, corrected, visibility dataset. ... The default is to apply these if they are available. nopol Do not apply any polarization leakage correction. ...

... The PGPLOT library routine PGIMAG is used to plot the image. The WCS library of Mark Calabretta is used to compute and plot the optional celestial coordinate grid (or tick-marks). read parameters; load the image ; find all null-valued pixels and set them to the minimum non-null image value; if (--withzclip) { calculate the effective minimum and maximum image values effMin and effMax by histogram clipping; } else { effMin = minval( image ); effMax = maxval( ...

Next: The boot process in Up: Boots And Shutdowns Previous: Boots And Shutdowns . The act of turning on a computer system and causing its operating system to be loaded is called booting . ... During bootstrapping, the computer first loads a small piece of code called the bootstrap loader , which in turn loads and starts the operating system. ... For PC's, the computer (its BIOS) reads in the first sector (called the boot sector ) of a floppy or hard disk. ...

. Next: Load metrology data Up: Access a data file Previous: Load point data Contents . CHAMELEON can read its own output file. Use A CCESS L OAD INTERFEROMETRY if you need to re-start CHAMELEON to work on averaged data. This will read all relevant objects in a .cha file, get a startable for the observed stars and compute derived quantities (C ALIBRATE A STROMETRY C ALC ). Configuration items can also be read separately using buttons A CCESS L OAD S YS C ONFIG . Christian Hummel 2015-04-28

... Obviously, the size of the cavern is of the order of the Schwartzman radius. ... Thus, consideration of the inverse effect of pulsar radiation on the properties of accreting plasma makes the ejection possible even when the Schwartzman radius is smaller than the capture radius. ... If the cavern radius , the condition at its boundary can be written as . ... Apart from magnetic dipole radiation, the cavern may also contain relativistic particles (which are also reflected from the cavern boundary). ...

... This section describes three functions which have been created to cleanup defects in images. The first two functions for cleaning rows and columns are particularly useful for CCD--images. ... These can often be removed with the commands: MODIFY/COLUMN INPUT OUTPUT [C or V] [columns] . ... This is particularly useful for removing the permanent defects which may exist in the CCD--frames and which cannot be removed by the MODIFY/COLUMN or MODIFY/ROW commands. ...

... This program will be a part of AATM-0.06 examples when this version is released. ... Comments regarding this example welcome at: // Bojan Nikolic b.nikolic@mrao.cam.ac.uk // # include string # include vector # include iostream # include fstream // Unfortunately the using statement below is required because of poor // desgin of the header files using namespace std ; # include ATMRefractiveIndexProfile.h # include ATMPercent.h # include ATMPressure.h # ...

... Wind Baffle Parameters . ... As part of this analysis, the volume, mass, center of gravity and mass moment of inertia of the telescope and optics support structure (OSS) were computed. ... The total moment of inertia of the circular floor panel, wind baffle and telescope in azimuth should be correct to 30% but is dependent on estimates of the mass of equipment supported below and above the circular floor panel. ... Table 8 : Masses and mass moments of inertia of the wind baffle components. ...

... As described in "Tabular Storage of STIS Data" on page 20-5 , raw time-tagged Sdata are stored in an event table which contains separate columns for the x and y pixel coordinates and the arrival time of each detected photon event. ... Generate a series of ACCUMulated images from user specified time intervals of data and then process the image(s) with calstis . ... The default behavior for inttag is to accumulate all events from the table, writing the results as one image set in the output FITS file....

... Piles of scrap metal and barrow-loads aof ashтАж . Sidebar Left . Sidebar Top . No Sidebar . Sidebar Bottom . Sidebar Right . ... Title: Piles of scrap metal and barrow-loads aof ash begin to grow in the courtyard. ... Piles of scrap metal and barrow-loads aof ash begin to grow in the courtyard. ...

... When the computer loads a boot sector on a normal Linux system, what it loads is actually a part of lilo, called the ``first stage boot loader''. ... This reads the configuration file /etc/lilo.conf and writes the boot loaders, and information about the operating systems it can load, to the hard disk. ... The configuration file for lilo is /etc/lilo.conf . ... It is easy enough to get something wrong and screw up your master boot record and make your system unuseable. ... Set up lilo on a floppy...

ON THE IMPACT OF THE GALACTIC ABERRATION ON VLBI-DERIVED PRECESSION MODEL Z.M. MALKIN Pulkovo Observatory Pulkovskoe Ch. ... Corrections to adopted precession rate are usually computed from the linear trends in long-term time series of celestial pole offset (CPO), which are the differences between the measured and the theoretical coordinates of the celestial pole. ... CONCLUSIONS We have estimated the impact of GA on parameters of precession-nutation model derived from VLBI observations. ...

This annotated example walks a user through a PINTofALE session using predominantly .par files where available. ... read in line and continuum emissivity databases, . compute a theoretical spectrum, . spectral browsing using SHOW_LINE . ... Carole Jordan type" plot!) in_flx=fitlines_fstr.flx @potem_tool.par ; plot the output EM curves @plotem.par ;NOTE: ; the emission measures are in the IDL save file !ARDB+'example_5.save' ;save,file=!ARDB+'example_5.save',out_LOGT,out_EM,out_multid . ...

... Cost­E#ective System Management Skip Schaller Steward Observatory, University of Arizona, Tucson, AZ 85721 Abstract. Quality system management of computer workstations for as­ tronomy can be achieved with relatively small manpower requirements, if the right cost­e#ective administrative design decisions are made. ... The system is designed so that one doesn't depend on four or more hosts, (such as a software server, cpu server, data file server, font server, etc.) to get work done. ...

... SETI@home consists of a receiving Arecibo antenna, a professional team (PT), and a two-way Internet connection between the PT and an army of S@h users, who load from the S@h server special software for digital signal processing. ... Thereby, METI@home will consist of several originators, which may load via Internet from a M@h server special software for the creation of analog and digital messages. ... ETI as a Source of Information . ... Main Internet Server . ... ETI as a Customer of Information . ...

Manual of F.A.M.A. (Fast Automatic MOOG Analysis) V 4.0 April 2013 Laura Magrini INAF Osservatorio di Arcetri The idea of this program is to do in an automatic way what usually is done by hand, i.e., running MOOG several times trying to minimize the trends of iron abundances versus EP (thus setting the effective stellar temperature) and EW (deriving the correct microturbolence value), and the difference between FeI and FeII (obtaining the surface gravity). ...

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ClassљList . ... StelHTTPTextureLoader Class Reference . Texture loader that loads an image from the web. More... #include < StelTextureLoader.hpp > . voidљ . ... Emitted when image loading is finished, sending loaded image. ... Abort texture loading (for example when destroying a texture that's still loading). ... Move the loader to its thread (after setting up image loading). ... URL of the image to load the texture from. delay . ...

... Home About Meade Product Information Dealer Locator Customer Support Investor Relations Dealer Support Employment Opportunities Site Map . Meade Instruments Corp. ... Meade Autostar Supplementary Software Downloads . ... To upgrade your Autostar first click on the link below to download the Autostar Update (ASU) Client Application for Windows. ... The most recent versions of AutoStar Update automatically check for the newest versions of the AutoStar Updater and download it if necessary. ...