... RDS . ... Calculates PSF correction for Timing/Burst. ... Rudimetary support has been added for spatial masks. ... 29 Oct 2002 . ... The Q.E. is applied for each detector map position. ... Added description for out-of-time event corrections. ... 03 Nov 2000 . ... Renumbered versions in Change History section. ... Updated description to reflect current functionality, specifically the detector map implementation and encircled energy correction. ... Added description for detector map feature. ...

... Create a list widget. listw_bind . ... void listw_bind (KListWidget list, KPixCanvas canvas) . ... Only one list widget may be bound per pixel canvas. void listw_destroy (KListWidget list) . ... void listw_get_attributes (KListWidget list, .. ... The attribute notify function will be called whenever the list widget attributes are changed (see listw_set_attributes ). ... flag listw_PROTO_position_func (KListWidget list, unsigned int index, unsigned int event_code, void *e_info, void **f_info) . ...

Next: Mass change Up: Evolutionary Scenarios of Binary Previous: Stellar Winds From Normal . As mentioned earlier, the duration of the binary evolutionary stage (say, I+I) is determined by the faster evolving component , where is the time each component spends at the corresponding evolutionary stage. ... Next, we should calculate the mass change for the slower evolving companion, the orbital semi-major axis and the eccentricity. Mass change . Semi-major axis change . ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

polimodel -- Produce model linear polarization and position angle images . ... Whether to apply random errors to output polarization and position angle values. seed = "" [integer] . ... This task produces a model linear polarization image and corresponding position angle image from an input image assumed to represent intensity (Stokes I parameter). ... A threshold for the input image can be defined such that polarization and position angle are not computed for input values less than this threshold. ...

... WFPC2 Header Changes due to OPUS 10.0 Update . ... Data . ... WFPC2 Home . ... OPUS 10.0 includes a major change for the WFPC2 and FOC science data processing pipelines in OPUS. ... FITS standard TELESCOP keyword is added to all headers. ... The header positions of the DATE, FILETYPE, INSTRUME, and EQUINOX keywords have changed. ... How to identify OPUS 10.0 headers for WFPC2 and FOC: . FLTSWVER and OPUS_VER keywords, which are in the STIS and NICMOS FITS spt headers, are not in WFPC2 or FOC shh. ...

Region markers can be moved, resized, rotated, zoomed, deleted, and can change geometric type. ... For example, markers placed on astronomical catalog positions should be fixed so that one cannot accidentally move them off the specified position. ... Parameters can be fixed using the fix option of the regions public access point (for fixing classes of markers) or by means of a fix keyword in the definition of an externally loaded marker. ... In the command: echo "regions fix all -position -size" | ...

... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...

... Binary orbits in the acceleration/period plane . Circular Orbits . ... We first present the equations for the period and acceleration of a pulsar in an eccentric binary system as a function of its position in the orbit. ... In Freire, Kramer & Lyne (2001) (from where most of this text and following equations are taken), we describe in more detail how circular binary orbits can be determined from the observed periods and accelerations of the pulsar. ... where is the orbital period of the binary. ...

... New version of magnetic field data (descriptor "itm") is now available with small corrections in offsets and attitude coverage. ... Full set of INTERBALL-TAIL AKR radiointensity KP for AKR instrument is now available (descriptor "ita"). ... KP data availability plots are created. ... Magnetic field data (descriptor "itm") after 1st January, 1998 are recomputed with corrected Bx_GSE offset (this was just 0.5 nT correction). ... CDF files for plasma wave KP are now available (descriptor "itw"). ...

Next: Column label: LAT Up: Permanent telescope parameters Previous: Column label: DIAM . This is the longitude of the telescope, measured in decimal degrees east from Greenwich. ... The older versions of the Astronomical Almanac gave west longitudes. For photometric data reduction, an accuracy of about 0.003 degree (about 20 arcsec) is required. Current volumes of the Astronomical Almanac give positions to 0.1 arc minute, which is adequate for our purposes. ...

On 1 February 2002 this Mirror was upgraded from NVSSlist v2.10 to NVSSlist v2.17 . ... This form searches the source catalog produced by the NRAO/VLA Sky Survey (NVSS). ... Object name [optional] : . ... Search radius and verification halfwidth in arcseconds [Optional] : . ... Enter a list of positions to search: . ... The contents of the NVSS source catalog and the techniques used by NVSSlist to derive error estimates and other parameters are described here. ...

... Impact of Covariance Information on the Orientation Parameters Between Radio Source Position Catalogs, IVS 2012 General Meeting Proceedings, p.339­341 http://ivscc.gsfc.nasa.gov/publications/gm2012/sokolova.pdf Impact of Covariance Information on the Orientation Parameters Between Radio Source ... IVS Analysis Centers provide these catalogs in a standard IERS format, where together with radio source positions and other relevant information, RA/DE correlations are reported. ...

Hide Zen home . ... Here, <b>1#2</b> denotes 1st extent begins from 2nd position and . hidden words, which is controlled by the 3rd parameter (how many words we leave in extent from the beginning). First example could be . ... hidden words, controlled by the 3rd parameter (how many words we leave in extent from the beginning). ... Here, 1#2 denotes 1st extent begins from 2nd position, x2026; - hidden words, controlled by the 3rd parameter (how many words we leave in extent from the beginning). ...

As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...

... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...

Contact Russet McMillan (primary) or your Observing Specialists (secondary) for additional information. Contact Jack Dembicky for web page errors, corrections, ommisions, or additions. This page last updated: July 6, 2004 - JMD . This page last checked: September 14, 2003 - JMD . Configuring TUI to use the Echelle . Setting up the Echelle exposure parameters . Taking your Calibration lamps . ... Setting up multiple exposures . ... Stopping an exposure (discarding data) . ...

The HyperNews Linux KHG Discussion Pages . Forum: The Linux Kernel Hackers' Guide . Date: Thu, 15 May 1997 08:10:29 GMT . From: < demiguel@robot3.cps.unizar.es > . I need to find the tunable parameters of the linux kernel, bue i cant find them (filesystems, processes, swapping,...) . I would like to know if there is any files such as mtune, or dtune is System V where you can change the main tunable parameters. Thank you everybody!! . Messages . 1. Kernel tunable parameters by Jukka Santala .

Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...

... The previous example, Chapter 12, "Expanding Colored Squares Example," illustrates how to expand and contract the clipping region of a layer without changing the wrapping width of the layer. This example illustrates how to capture mouse events so that the user can make a layer's wrapping width wider or narrower by dragging the mouse. ... how to capture mouse events for a layer . how to change the wrapping width of a layer by using the load() function . ... Capturing Events for the Layer . ...