... Class . Use . ... Packages that use Roi . ... ImagePlus. roi . Methods in ij that return Roi . Roi . ... Methods in ij with parameters of type Roi . void . ... A subclass of ij.gui.Roi (2D Regions Of Interest) implemented in terms of java.awt.Shape. class . ... Methods in ij.gui with parameters of type Roi . ... Methods in ij.measure with parameters of type Roi . ... Methods in ij.plugin with parameters of type Roi . ... Methods in ij.plugin.filter with parameters of type Roi . ...

Next: Deleting Calibration Tables - Up: Calibration, the ATCA, and Previous: Copying Calibration Tables - . ... This task can list and plot antenna gain, bandpass, delay and leakage terms. ... Possibilities are gains ( i.e. the antenna gains), polarisation (the polarisation leakage terms), delays and bandpass . ... The select parameter behaves like the normal visibility selection parameter (see Section 5.5 ) - except that you are selecting gains rather than visibilities. ...

Appendix C. Display Device Names . ... A "display device name" is a string description that uniquely identifies a display device; it follows the format "<type>-<number>", for example: "CRT-0", "CRT-1", "DFP-0", or "TV-0". ... Display device names can be used in the MetaMode, HorizSync, and VertRefresh X config options to indicate which display device a setting should be applied to. ... That is why specifying the display device name is preferable. ... Appendix B. X Config Options . ...

... How to display images in IRAF using the display task. ... The most general IRAF task for displaying image data is the display task, the best choice for a first look at HST imaging data. ... Display the image with the IRAF display task, using the syntax appropriate for the file format (Chapter 2 explains how to specify GEIS groups and FITS extensions): tv> display fname.c0h [2] 1 (GEIS group 2) . ... If you want to display an image with high dynamic range, you may prefer to use logarithmic scaling. ...

Next: Command Syntax Up: MIDAS Data Structures Previous: Specifying Pixels in . In all MIDAS commands which accept images as parameters you can also provide subimages in the syntax specified above. For example, the command LOAD/IMAGE loads an image into the MIDAS display (window). ... Midas 567> LOAD/IMAGE mygalaxy . would try to display the whole 2-dim image mygalaxy.bdf , whereas . Midas 568> LOAD/IMAGE mygalaxy[@100,@200:@199,@299] . ...

OptInt PmWiki : Pm Wiki / Available Actions . Default actions . ... Cookbook actions . Page actions are applied to wiki pages, as a query string appended to the URL . ... displays dialog for setting/changing password of the specified page or group of pages, see passwords , see also $EnablePostAttrClearSession if you do not want to have the session cleared after validating change General use of passwords . ... display the specified page (default action if no ?action= is present) . ...

SAOtng supports display of photon event data contained in raw files, similar to its support for FITS Binary Table extensions (e.g., X-ray event lists). ... Because event files do not usually contain enough information to generate an image, we have adopted some conventions for specifying how to interpret the data in these files and for how to bin rows of events into images. To image an event file, it is first of all necessary to define the structure of the events in the event file. ...

... The various command lines for running the program are: . omgsource imageset=... newsrclistset=... newspectrumset=... spectrumplotset=.. For creating new source and spectrum list files (no parameters oldsrclistset oldspectrumset specified). The image stored in the image file specified by the parameter imageset is displayed without any source regions overlayed. ... The image stored in the fits file specified by the parameter imageset is displayed with the source regions overlayed. ...

... Restrictions ) are used. If specified form of output is EMP then astrometric equatorial coordinates are printed in the form usual for Ephemerides of Minor Planets, with formal precision of 0.01 minute of time in R.A. and 0.1 minute of arc in declination. ... It should be noted that the near-opposition ephemerides are not calculated for bodies/ points with numbers from –12 to 0 (in case they are included into task for computation of such ephemerides only their names are displayed in the results). ...

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