... Watchouts . ... Help . ... If you re-load it in xmmselect , its selection expression is not recognized, and is not applied in the generation of further scientific products. In order to overcome this problem, use the expression SELECTED in your xmmselect screening expression widget. ... For instance: SELECTED PI in [300:1500] . ... Pages maintained by SAS librarian . Any question about SAS should be addressed to the XMM-Newton help desk . Updated on: November 18, 2006 ...

The low pass digital filters (lpdf) were simulated in software. ... Generate an in band sine wave (amplitude=10) and process it through the lpdf for each decimation. Generate noise (with an rms of 10) and filter it with the 4 decimations. ... Page 1: filter for decimate=4,8,16,32, The dcGain is the integral over each filter divided by the decimation length. ... Page 2: pushing a sine wave through the filter. ... Bottom: (sine waves)/decimation after filtering. ... Page 3: filtering noise. ...

Start with a new grayscale image, white background black foreground. ... Filter/Pixelate/Crystallize , use setting of 10. ... Filter/Blur/Gaussian Blur with value of 2.0 . Image/Adjust/Curve . ... Image/Map/Invert . ... Mode/RGB Color . Image/Adjust/Hue/Saturation... , click Colorize and set Hue to -175. If u want some sparkles, then choose airbrush tool, white foreground color, go to Brushes Palette, click right arrow icon and load Assorted brushes (came with Photoshop) Then apply some. ...

... Обзор LPR фильтра. Впечатления от наблюдений с LPR фильтром. ... Характеристики цветных фильтров Baader-Planetarium . Мой перевод pdf- файла о фильтрах с сайта Baader-Planetarium (379 кб) . ...

... This method is called once when the filter is loaded. ... This method should return a flag word that specifies the filters capabilities. ... With CONVERT_TO_FLOAT, the filter is called with the image data converted to a FloatProcessor (3 times per image for RGB images). ImageJ will lock the image before calling this method and unlock it when the filter is finished. For PlugInFilters specifying the NO_IMAGE_REQUIRED flag and not the DONE flag, run(ip) is called once with the argument null . ...

... 5.4 The main control . ... 5.6 Filtering your data . ... blinking images . 4 Viewing Images and . ... 1.1.2 Converting Between Data . ... 3 Viewing and Comparing | ... 11.1 Image and Contours . ... 4.3 Multiple Contour Images | ... data converters . ... data formats . ... 1.1 Supported Data Formats . ... 3.2 View Control | ... header viewing . Viewing Header Information in . ... image formats . ... images . ... viewing headers . ... viewing multiple datasets . ... Make Data Control Panel . ...

... I have compiled a list of throughput filter curves from a variety of telescopes, instruments, and surveys. Click on the name of the filter to download it. The first line of each filter is the zeropoint for that filter. If the filter is in the AB system, it is listed as 0.0 (or in otherwords -48.55). ... Filter . Effective Wavelength . ... A_V . ... 0.987 . ... 0.050 . ...

... 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. ...

... ARC 3.5m | GFP . ... Install Appropriate Filters and Edit filters.txt file . Edit filters.txt file on aiscam@finesse in /home/aiscam/config . ... It also loads the filter info and the gfp.cfg settings including the calibration file for the appropriate course z-setting . aiscam: etalon in ;load etalon into optical path . ... aiscam: fpzero -w 4044.4 -1591.47 ;set fpzero with wavelength and central z . ... aiscam: time 40 . ... aiscam: file bias ;set filename for biases, no time needed . ...

pro loadfits common ws_comm,namobj,solar_r,bunit,angle,xscale,centr_x, $ nfield,dtype,tdim, xmas , ddata ,status, wscan , base ,draw, $ list, fl_load ,fl_iv,nfile, twoscn ,exbeg,exend,wlsfrq ;pro loadfits wscan =-1 fl_load =0 nfile=pickfile(TITLE='Select Binary FITS file',filter='*.fit') if nfile eq '' then goto,x_ end fxbopen, fid, nfile,1 fhdr =fxbheader(fid) ndate=fxpar( fhdr ,'DATE_OBS') nobj=fxpar( fhdr ,'OBJECT') solar_r=fxpar( ...

Here is a description of the Filter/Driver Pack Plus release from Aldus. ... The Macintosh Filter/Driver Pack Plus includes several new and updated filters, including import filters for Microsoft Works 3.0 and MacWrite Pro files, as well as the most recent LaserWriter driver, version 8.1.1. ... The Filter/Driver Pack Plus also includes a patcher utility which will update PageMaker 5.0 to version 5.0a. This patcher corrects a handful of reported customer problems. ...

WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Chapter 2: WFC3 Instrument Description > 2.3 Spectral Elements . ... 2.3.1 The Filter Selection Process . ... Both WFC3 channels are equipped with a broad selection of spectral elements. ... The UVIS channel has a selectable optical filter assembly (SOFA) that contains a stack of 12 filter wheels housing a total of 48 elements: 42 full-frame filters, 5 quad filters, and 1 UV grism. ...

CCD Forum Message . Forums: . Atm ћ Astrophotography ћ Blackholes ћ Blackholes2 ћ CCD ћ Celestron ћ Domes ћ Education . ... Discussion Forums | CCD Tips and Techniques | Post . ... Tri-Color Images . Forum List | ... Post Message | ... Login to Post . ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

... Apache HTTP Server Version 2.2 . ... This document describes the use of filters in Apache. ... The Filter Chain is available in Apache 2.0 and higher, and enables applications to process incoming and outgoing data in a highly flexible and configurable manner, regardless of where the data comes from. ... A wider range of applications are implemented by third-party filter modules available from modules.apache.org and elsewhere. ... There are two ways to use filtering: Simple and Dynamic. ...

... Apache HTTP Server Version 2.2 . ... This document describes the use of filters in Apache. ... The Filter Chain is available in Apache 2.0 and higher, and enables applications to process incoming and outgoing data in a highly flexible and configurable manner, regardless of where the data comes from. ... A wider range of applications are implemented by third-party filter modules available from modules.apache.org and elsewhere. ... There are two ways to use filtering: Simple and Dynamic. ...

Stellarium 0.12.3 . ... Classes . ... Renderer . ... StelQGLTextureBackend Class Reference . ... constructFromImage (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params, QImage &image) . Construct a StelQGLTextureBackend from an image. ... constructFromPVR (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params) . ... constructAsynchronous (class StelQGLRenderer *renderer, const QString & path , const TextureParams &params) . ... path . ...

... Meade Series 4000 Nebular Filters incorporate the very latest in interference coatings technology. ... Technical Basis of the Meade Broadband Nebular Filter: As shown in the transmission graph below, the Meade Broadband Nebular Filter strongly rejects the light of sodium- and mercury-vapor lights as well as natural airglow and auroral emissions. ... Meade Series 4000 Narrowband Nebular Filters . ... Meade Series 4000 Oxygen-III Nebular Filters . ... Meade Series 4000 Photo-Visual Color Filters . ...

TEST REPORT FOR P2PP V2.1.1beta3 ================================ A) CHECKING BUG FIXES SINCE V2.1.1beta2: 1/ Serialisation bug : P2PP is able to read the two V2.1 cache directories previously generated by Bkemp ==> BUG FIXED 2/ bug 1053, filter not cleared after having been set from RANGE keyword : the filter is correctly set for a paramfile parameter, and cleared if another paramfile is selected (within the same OB but another template, and for another OB). ... Acq template with file parameter. ...

... NOTE: Some of these operations generate new sets, if you run out of sets use Edit/Set operations (described below) to kill unneeded sets. ... Select the set on which the formula will operate, (set must be active, use File/Status to find the current state of sets). ... where (x,y,a,b,c,d) are defined as the x and y of the currently selected set and a,b,c,d are scratch arrays that can be used to perform operations between sets. ... Select the set. ... Select fitted curve or residuals to load. ...

MAKING THE PROFILES . First of all you are expected to load a FITS file ("FILE"-"LOAD"). ... By pressing the middle button you copy the profile from the first profile window to the second one. ... An example: first integral can correspond to the profile of active region and second integral can correspond to the profile of quiet chromospheric region. ... The second profile (which is subtracted from the first one) you extract after clicking on "SUBTRACT"-"MARK QUIET PROFILE" and marking the region. ...