... This algorithm is designed to pick up sources that have either extents much greater than that of the points-spread function or any other sources that were not picked up by the point-source detection algorithm. ... nESources - the total number of extended-sources detected so far . ... eLevelImage - a two-dimension array that stores the pixels assigned to the extended-sources- each pixel assigned to the source is set equal to the number assigned to the source. ... x - stores the pixel index i . ...

... HST . ... Data . ... HST Overview . ... Cycle 24 Announcement . ... The header consists of engineering telemetry values, plus other information. ... The keyword PTSRCFLG (point source flag) should list either P for a point source or E for an extended source. The IRAF task listpixels under the images package can be used to look at the values of the SHP and UDL pixels. The following chart shows the correct value for SHP pixel #937 according to MODE and if the source is EXTENDED or POINT. ...

Next: Source Fitting and Positions Up: Image Analysis Previous: Image Statistics and Histograms . You might like to list some of the pixel values from a section of an image. ... Because it is always very difficult to format numbers in a way which suits every application, imlist gives you this job. You do this via the format keyword, into which you put a FORTRAN format specifier such as `1pe11.4', or `f7.2' etc. ... Display pixel values . ... Select region . ... Select display format . ...

Next: *tabplot* - Displaying a Up: Radial Profiles and Projections Previous: Radial Profiles and Projections . Obtain a radial distribution of counts for the source centered at x = 503, y = 513, in the data image xdata$snr.qp . The background is taken locally from an annulus outside the source region. ... Region descriptors can also be given on the command line, but they must be enclosed by quotes. xs> imcnts xdata$snr ``a 503 513 0 50 n=5'' . ...

... The generation of simulated sources whose physical properties are well understood is useful in assessing the functionality of point source analysis software. Qpsim is an IRAF/PROS task which will generate events from sources of given intensity, shape, and position and either overlay them on a flat background in a new QPOE file or inject them into an existing QPOE file. ... The simulated data can be a useful tool in calibrating point source analysis software. ...

... 389Voges+ IX/29 ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000) ============================================================================= ROSAT All-Sky Survey Faint source Catalogue (RASS-FSC) Voges W., Aschenbach B., Boller Th., ... The sources have a detection likelihood of at least 7 and contain at least 6 source photons. ... 0 Extraction radius 141-146 A6 --- PrioFlags [01] priority flags (8) 147 A1 --- PHA [ABCDb] PHA range of best detection (9) 149-152 F4.2 --- VigFactor ?= ...

The cal values for lband narrow were measured on 28jan02 in the early morning using the sky/absorber technique. ... Comparing phil's and karen's cal values. ... Fig 1 is the cal value in deg K versus frequency. ... fig top: The cal values in kelvins. black:karen, red:phil, green: old cal values (after correcting for 6%error). fig middle: ratio of "new" cal to old cal. black:karen's computations, red: phil's. fig bottom: Ratio of phil's cal values/ karen's cal values. ... Fig 1. ...

... Observatory . ... Science . ... Science Users Information > Data Handling and Products > Data Reduction FAQ > How do I interpret the SEQ TIME keyword values? ... Science Users Information . Observing Facilities . La Silla Paranal Observatory . ... Observing with ESO Telescopes . ... Science Data Products Forum . ... Science Archive Facility . ... ESO Data . ... ESO Data Access Policy . ... ESO Science Newsletter . ... For VISIR, the SEQ TIME keyword is set to the requested exposure time. ...

... The package stsdas.graphics needs to be loaded (to run imdisp_pos for getting # the NDC's of the display image) # set imtype="fits" # print " " print " *** Start of impol SPECIAL instrument demo *** " print " [stecf.impol and stsdas.graphics need to be loaded] " print " " # # (First delete any model reflection nebulae left over from previous demos) # print " Deleting any old demo files " imdel reflneb1*.fits verify=yes # # An input (intensity) image is required. ...

... 172 ] Briefly, the count rate at the detector from a source at a redshift z is . ... Figure 55 shows the ``Green functions'' for the double compact binary merging rate   evolution assuming no collapse anisotropy. ... Another way that diverse peculiarities in the - distribution induced by the sources evolution could arise is connected with a possible non-monotonic character of the star formation rate in galaxies. ... 22 ] Figure  56 shows two-dimensional cuts through the parameter space. ...

. To display the name of the system in the prompt: . 1. Use your editor to open your .tcshrc file and add the line: set prompt='%m %' . 2. Save the file and leave the editor. 3. Enter the command: source .tcshrc . This adds the new values to your working environment.

... 161 љ virtual bool addVertexShader ( const QString& source) = 0; . ... 184 љ virtual bool addVertexShader ( const QString& name, const QString& source) = 0; . ... 194 љ virtual void enableVertexShader ( const QString& name) = 0; . ... 306 љ virtual void setUniformValue_ ( const char * const name, const bool value) = 0; . ... 309 љ virtual void setUniformValue_ ( const char * const name, const int value) = 0; . ... 312 љ virtual void setUniformValue_ ( const char * const name, const float value) = 0;...

... SELECT file, title, rank(ts_vec, to_tsquery('create schema')) FROM postgresql_manual WHERE ts_vec @@ to_tsquery('create schema') ORDER BY rank(ts_vec, to_tsquery('create schema')) DESC LIMIT 5; file | title | ... CREATE SCHEMA | ... SELECT file, title, rank('{0, 0, 0.01, 0.99}',ts_vec_tb, to_tsquery('create aggregate')) FROM postgresql_manual WHERE ts_vec_tb @@ to_tsquery('create aggregate') ORDER BY rank('{0, 0, 0.01, 0.99}', ts_vec_tb, to_tsquery('create aggregate')) DESC LIMIT 5; file | ...

lsst.tcc љ 1.2.2-3-g89ecb63 . ... Files . FileљList . FileљMembers . ... python . ... msg . formatObjFields.py . ... 2 љ """!Format the values of data types found in the tcc.base.Obj, for key=value messages . ... 8 љ from .blockToKW import WriterFromBlock, FieldKW . ... 36 љ def formatChebyCoeff (chebyCoeff): . ... tcc.msg.formatObjFields.formatPVTList . ... tcc.msg.formatObjFields.MoveItemKW . ... tcc.msg.formatObjFields.makeObjBlockWriter . ... tcc.msg.formatObjFields.formatWrapPref . ...

... Clean . ... Flux Sign Expo . ... The map above is movable . The image is shown in significance with a squared root color map ranging from 0 to 25. ... Original shows mosaics with all data available. Flux map Error map Significance Exposure . Flux and error maps are in mCrab units. ... Exposure maps are in ksec. INTEGRAL/IBIS 9-year Galactic Hard X-Ray Survey* , A , Volume 545, id.A27 { NASA ADS | ... 7-year Galactic Bulge map , 2009 . 9-year Galactic survey , 2012 . ... Exposure . ...

... Forum: Character Device Drivers . Keywords: return values . Date: Fri, 25 Apr 1997 21:42:46 GMT . ... In this section I noticed the example foo_write function returns 0 all the time. ... the foo_write () function gets called indefinately. Furthermore, I have noticed that from the source of serial.c (from /usr/src/linux-2.0.0/drivers/char) always returns the number of characters transmitted. ... Also, why isn't there a DEFINITIVE list of return values for all functions? ...

J/MNRAS/429/2080 Lockman Hole 10C sources radio spectral indices (Whittam+ 2013) ================================================================================ The faint source population at 15.7 GHz. ... 2011, Cat. ... 2008, Cat. ... For 10C sources without a counterpart in the GMRT image, three times the local noise is included as an upper limit on the flux density at 610MHz. ... 1.4-GHz flux density value from NVSS catalogue, including upper limits for undetected sources 76 I1 --- f_SNVSS [0/1]? ...

... Field size . Object name . ... Map size . ... Field size: the approximate size of the map in the Y direction. ... Galaxies: . ... Galaxies, which size exceeds some value depending on the field and map sizes, are displayed with their real positional angles and sizes by 25m isophote. ... In the "tools" fields there are links to the several famous AVO (Astrophysical Virtual Observatory) resources: NED and Simbad databases and DSS2 (Palomar Digitized Sky Survey) images of the corresponding sky area. ...

This module provides for server-side imagemap processing. ... Configurable generation of imagemap menus. The lines in the imagemap files can have one of several formats: directive value [x,y ...] . ... The directives can come in any order, but are processed in the order they are found in the imagemap file. base Directive . ... Module: mod_imap . ... Its value is overridden by a default directive within the imagemap file. ... Its value is overridden by a base directive within the imagemap file. ...