. This diagram shows a small table with three transparent cells and illustrates how their final background is determined. The table consists of two rows. Four (labeled) cells lie in the first row, but the second cell spans the first and second row. The first, third, and fourth cells of the second row are "empty". Each non-empty cell has a red background and a double black border. Each empty cell has the table's background color (specified as #ff0) as its own. Return to image.

... 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 # ...

... This task constructs the PPS product OM OSW FITS source timeseries from two rate files (source and background) produced by separate runs of EVSELECT on a tracking-shifted, QE-corrected OM fast-mode event-list. ... The counts measured in the source and `background` regions, together with the PSF function evaluated over the corresponding regions, are used to set up equations which are then solved to yield source and background rates evaluated for the nomimal coincidence-loss region (r=12 pixels). ...

Next: Echelle Reduction Method Up: No Title Previous: Example . This Chapter provides the basic information necessary to understand the echelle љ package implemented in MIDAS . ... Tutorial examples are available in the system (command TUTORIAL/ECHELLE ) and are also included in the Appendix so that users without previous experience in MIDAS could become familiar with the calibration procedures. ... The methods described here are generally sufficient to cover a wide range of echelle formats. ...

grdgradient - Compute directional derivative or gradient from 2-D grd file representing z(x,y) grdgradient in _ grdfile -G out _ grdfile [ -A azim [/ azim2 ] ] [ -D [ c ][ o ][ n ] ] [ -L flag ] [ -M ] [ -N [ e ][ t ][ amp ][/ sigma [/ offset ]] ] [ -S slopefile ] [ -V ] grdgradient may be used to compute the directional derivative in a given direction ( -A ), or the direction ( -S ) [and the magnitude ( -D )] of the vector gradient of the data. ... If amp is not given, default amp = 1. ...

... A top-level object used to access Java classes from within JavaScript code. ... The java , netscape , and sun properties represent the packages java.*, netscape.*, and sun.* respectively. ... For example, you can access a constructor of the Frame class as follows: var theFrame = new Packages.java.awt.Frame(); For convenience, JavaScript provides the top-level netscape , sun , and java objects that are synonyms for the Packages properties with the same names. ... Any class in the Java package sun.* ...

The database contains references to the papers, data files and links to the Internet resources related to measurements and calculations of the optical constants in the wavelength interval from X-rays to radio domain. ... References to some useful books and reviews on the subject (e.g. the classical handbooks edited by E.D.Palik) and links to Internet collections of optical constants and personal WWW pages with related software were also placed in the database. You have arrived at our welcome page. ...

... Classes . ... casa::SparseDiffX< T > . ... The function, with fixed parameters a,b: template class T class f { public : T operator ()( const T x) { return a_p*a_p*a_p*b_p*b_p*x; } void set ( const T a, const T b) { a_p = a; b_p = b; } private : T a_p; T b_p; }; // The specialized function template class f SparseDiffX Double { public : T operator ()( const T x) { return a_p*a_p*a_p*b_p*b_p*x; } void set ( ... Referenced by casa::SparseDiffX< T >::operator=() . ...

asncombine -- Process and combine images in one or two NICMOS associations asncombine association . ... set to yes to include error planes in co-added images error. background . ... This is useful to use different background subtractions for different images. fheader . set to yes in order to multiply the background by the value of keyword "factor" in the image header. ... Set to yes to use quadrants statistics save in the image header from previous runs of asncombine. regquad1 . ...

... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...

trackingtime- compute LST rise, transit, and set times for sources as well as time in the keyhole . trackingtime {--help --lim --sort --usecalib --usepsr --usex102 --usefluxgt1 --zamax=zamax --zamin=zamin --exclnorise} srcfile srcfile name of cima source file to process. ... exclnorise exclude sources that never rise. trackingtime is a shell script that calls idl routines to process the srcfile and output the lst rise, transit, and set times for each source in the file. ... Source Rises | ...