... The task makes use of a source-list produced by running omdetect on the same image. ... Parameter Mand Type Default Constraints set yes string OM image le with grism spectra aligned with respect to the columns of the image ( output from omg- prep). xmmsas 20060628 1801-7.0.0 XMM-Newton Science Analysis System Page: 2 sourcelistset yes string Source list ( output from omdetect) outset yes string Output spectra le region le no string Name of the ASCII (input) ...

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• http://xmm.vilspa.esa.es/sas/6.1.0/doc/omgrism.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/omgrism.ps.gz

Next: Photometry Up: Regions and Source Parameters Previous: *imcnts* - Find counts . This task (developed for use with optical images, but also useful with x-ray data) will quickly compute location, size, ellipticity, and position angle of sources. ... User can generate contour plots of any portion of the image and count rates in slices through the image. The program is advertised as ``quick [optical] photometry''. input file: rp110590_im1.imh . output file: logfile . ... Photometry . ...

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• Detect
• Background Corrections
• Spatial Analysis

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• Towards Optimal Analysis of HST Crowded Stellar Fields
• ADASS 2003 Conference Proceedings
• Background Fluctuation Analysis from the Multiscale Entropy

slitless -- Extract a spectrum from a direct/GRISM image pair slitless image grism output PARAMETERS . ... A two dimensional direct image to be used to select an object. grism . A two dimensional GRISM image containing slitless spectra of objects present in the direct image. output . ... Toggle whether or not a background estimate is subtracted from the extracted object spectrum. mingood = INDEF . Pixels of the grism image with values smaller than this are ignored. maxgood = INDEF . ...

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• NICMOS Data Calibration and Analysis
• ST-ECF Grism Spectrum Software for NICMOS Grism Data
• The ``stecf" IRAF Layered Package

Chapter 2: Header Keyword Definitions . ... T/F- Was the observation an association? ... Looking at the ASN_MTYP and EXPNAME keywords for each extension of the n48o06020_jif.fits file, we see... n48o06020_jif.fits [1], ASN_MTYP = EXP-TARG EXPNAME = N48O06G9J n48o06020_jif.fits [2], ASN_MTYP = EXP-TARG EXPNAME = N48O06GAJ n48o06020_jif.fits [3], ASN_MTYP = EXP-BCK1 EXPNAME = N48O06GBJ n48o06020_jif.fits [4], ASN_MTYP = EXP-BCK1 EXPNAME = N48O06GCJ n48o06020_jif.fits [5], ...

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• CSPICE Routines: BODS2C_C
• NICMOS Data Handbook
• Observation Logs

Next: Pyramidal Algorithm Up: The discrete wavelet Previous: Multiresolution Analysis . ... One assumes that the sampled data are the scalar products at pixels k of the function with a scaling function which corresponds to a low pass filter. ... The signal difference contains the information between these two scales and is the discrete set associated with the wavelet transform corresponding to . ... The figure shows the wavelet associated to the scaling function. Figure: Wavelet . ...

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• Period analysis
• Radio data
• Edition of the Table Containing the Cloud Model

To proceed to drawing tracks of some objects select Tracks item in menu bar and then select Input Data in drop-down menu. Enter initial and final dates of time interval in corresponding data fields of the Input Data dialog box Input Data . ... The frame with horizontal and vertical scales corresponding to the right ascension and declination axes appears on screen. ... Depending on specifications introduced in the Input Data dialog box the picture represents tracks up to three different objects. ...

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• AY (preface)

In this chapter we will consider two very simple but useful Web agents that I have written on Actor Prolog for my own needs. ... Let us start the Web agent. Fig. ... Start of the Web agent. The Context diagram consists of three blocks: "Logic Programming Sites", "Edit", and "Check". ... Some Web sites that are linked with the logic programming and Prolog are listed in the pulldown list (these addresses are transferred to the "Edit" block from the "Logic Programming Sites" block). ...

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• Actor Prolog. Example "D:\MOROZOV\Z\DEMO\EXE\EXAMPLES\SADT\JAM-E\JAM-E.A"
• Getting Started in Actor Prolog. The idea of Logical Actors.
• Report on Cosmic Call 1999

... Plot histogram and time series. Flow Chart GUILD & LIGO Tools Local File (XML) Restore Events Import XML event data into an event container LDAS Meta Database Save Events Process events (Sort, Coincidence, Cluster) Create Histogram and/or Time Series Plot Histogram/ Time Series Event Containers Hierarchy "Chain" container - A set of List containers. ... Holds one event. ... Time Series - Make a Time Series (DMT TSeries container) of the event rate, values of specified column or event function. ...

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• http://zebu.uoregon.edu/disted/ph121/parallax.html

Next: Astrometry Up: Quick Guide Previous: Reduce point data Contents . R EDUCE A VERAGE averages all the data currently contained in the point data arrays. The corresponding scans in the scans array (it will be automatically created when non-existent) will be updated. average will print out messages as to invalid (flagged) data encountered, and non-existing background scans. ... Christian Hummel 2015-04-28 ...

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• A visual tour
• API Help
• Reduce visibility data

... User Guide ] Task: atmerge Purpose: Merge ancillary information with an AT-observed uv file. ... Key: vis The names of the input uv data sets. No default. Key: tsys Either one of two names, being the text files containing the system temperatures for the various antennas. ... Key: xyphase The name of a text file containing the XY phases. ... Key: chi The name of a text file containing the RPFITS parallactic angle data. ... Key: xyamp The name of the text file containing the XY-amplitude data. ...

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• The Karma Homepage
• Smoothing Images
• WCSLIB: WCSLIB data structures

... PUL VLBI Analysis Center . ... Pulkovo EOP and Reference Systems Analysis Center (PERSAC) is located at the Pulkovo Observatory . ... Processing of VLBI , GPS, and optical observations aimed at analysis of the Earth rotation, station displacement, and celestial reference system. ... Celestial Pole Offset (CPO) and Free Core Nutation (FCN) . Four daily updated CPO and FCN series (models) are provided. ... File fcn1.dat contains the ZM1 FCN model with variable amplitude and phase. ...

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• General description of the database

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. ...

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... The cosmic microwave background radiation emanating from the universe could only have the above fuzzy pattern if it contained clear amounts of dark matter and dark energy . The conclusion , based on a detailed analysis of the temperature and spacing of the bumps, was a surprise to those who felt that previous evidence for such a strange universe , based on observations of distant supernovae , was somehow inaccurate. ... Publications with keywords: CMB - early universe . ... The Early Universe . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Cosmic Ripples Implicate Dark Universe
• The Cosmic X-Ray Background

... This API (Application Programming Interface) document has pages corresponding to the items in the navigation bar, described as follows. The Overview page is the front page of this API document and provides a list of all packages with a summary for each. ... Each package has a page that contains a list of its classes and interfaces, with a summary for each. ... Each of these pages has three sections consisting of a class/interface description, summary tables, and detailed member descriptions: . ...

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• Line (ImageJ API)
• OvalRoi (ImageJ API)
• BackgroundSubtracter (ImageJ API)

... Values have been scaled arbitrarily. High ratios are shown in blue, corresponding to blue colors, and low ratios are shown in red, corresponding to red colors. ... Noise combined with background subtraction difficulties in the lower left quadrant of the WISP1 data (see Fig. \ref{Fig:wisp_snr_mskd}) make colors in this area very unreliable. ... The values shown here are typically a factor of ~3 less than those calculated for the Schmidt data, shown in Figure \ref{Fig:bj_alpha}. ...

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• ALFA Diode Temperature-Explanatory Notes
• Data and Analysis
• HISA Poster for the 197th Meeting of the AAS, January, 2001

... N.A.Bobylev, Yu.M.Burman, Morse lemmas for functionals of the variational calculus, Func.Anal.Appl., ... N.A.Bobylev, Yu.M.Burman. ... N.A.Bobylev, Yu.M.Burman, A.B.Shubin, Algorithms for control with a minimal number of switchings, Automation and remote control , V.53, 5:619, 1992. ... TeX file ) . ... Quadratic Poisson brackets compatible with an algebra structure . ... Yu.M.Burman. ... Yu.M.Burman, Whitney's index formula in higher dimensions and Laplace integrals , Preprint math.DG/9801044 . ...

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• Semiclassical Microlocal Analysis (Fall 2003)

Next: The root filesystem Up: Overview of the Directory Previous: Overview of the Directory . This chapter is loosely based on the Linux filesystem standard, FSSTND, version 1.2 (see the bibliography, [ Qui95 ]), which attempts to set a standard for how the directory tree in a Linux system is organized. ... This chapter does not explain all files in detail. ... The major parts are the root, /usr љ , /var љ , and /home љ filesystems (see figure 2.1 ). ... Figure 2.1: Parts of a Unix directory tree. ...

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• The root filesystem
• The boot process in closer look
• Armagh Observatory

... We present the first results of the application of Positive Matrix Factorization (PMF) to the analysis of molecular line spectra. ... The principles of the method are discussed and some results from the analysis of -spectra from the Thumbprint Nebula are shown. ... The Positive Matrix Factorization . ... Thumbprint Nebula . ... Figure 1: a) The first 20 singular values of a matrix containing the 92 -spectra used in the analysis. b) An example of a factorization of rank one . ...

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• Leverhulme Collaboration
• PPEUC Programme - Cosmic Microwave Background Workshop
• Accessing measurement set data Bojan Nikolic web pages (r. 329)

FEATURES OF THE HYDROGEN DISTRIBUTION AROUND LUNAR CRATERS PROCLUS AND KEPLER. ... In result of analysis of the data Lawrence and Feldman constructed the hydrogen distribution on the lunar surface [1]. ... However, the authors shown, that EN flux data features may be explained by other element abundance in the lunar soils, namely: Si, Ca, Gadolinium (Gd), Samarium (Sm) and Fe. ... Using of the Feldman's interpretation of the Lunar Prospector data [8], we constructed hydrogen distribution map (Fig.1). ...

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• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf
• Родионова Жанна Федоровна