Next: Determination of the Up: Getting the Dispersion Previous: Line Detection in . In order to compute the dispersion relation, lines stored in table line.tbl have to be cross-identified with a reference catalogue . For the first few spectral lines in the central row, this has to be done interactively, the rest is automatic. ... Midas.. ... IDENTIFY/LONG . ... which plots the central row of the comparison spectrum and the interactive line identifications. ...

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... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...

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• Automatic Detection of Linear Features in Astronomical Images
• Identification and Analysis of Binary Star Systems using Probability Theory
• CDS GLU, a Tool for Managing Heterogeneous Distributed Web Services

... Each DFS Department official document has to be issued according to the following internal procedure. Documents to be distributed outside DMD division must also be issued according to the Technical Archive procedure . ... Several documents are also available as complete templates defined internally for DFS Department documentation (e.g. template for Test Plan, for Test Report, .. ... Define the internal document number as: dfs-volxx-yyy-zzzz . ... Document title, . ... Issue number (e.g. 1). ...

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• the Technical Archive procedure for issue of documentation
• Redshift Distribution
• ESO - Data Reduction Pipelines Distributed as RPM Packages

... Radio Catalog . The corrections in NVSS fluxes leading to the corrected Version 1.1 also result in changes to some of the figures and tables in Kimball Ivezi? ... The results are qualitatively the same. ... The new versions of the figures, along with the original versions (in high resolution), are available here . ... These figures, along with Table 4, continue to motivate t = 0.35 as the optimal separator between "simple" and "complex" sources). ... Complex Sources . ... t NVSS . ... galaxy . ...

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• The ATNF Electronics Group : AT Distributed Clock
• The ATNF Electronics Group : AT Distributed Clock Display
• Distributed Archives Interoperability

... Institute of Physics Publishing, Dirac House, Temple Back, Bristol, UK, e-mail: anne.dixon@ioppublishing.co.uk . ... I shall describe Institute of Physics Publishing's efforts in this area, including our HyperCite technology, which allows users to roam the literature, backwards and forwards in time, and to experience fascinating information trails. ... Finally I should explain that STACKS(tm) has many other uses beyond linking from existing Institute of Physics Publishing customers. ...

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• Stellar Photometry
• H 2O- and OH-bearing minerals in the martian regolith: . analysis of 1997
• Technique

... The package AMPLE (Adaptable Minor Planet Ephemerides) is dedicated to solving a number of problems concerning minor planets with the aid of IBM-type personal computer. ... Obtaining selection of orbital elements and/ or photometric parameters of minor planets in conformity with imposed restrictions. ... The orbital elements of all minor planets used in AMPLE for 2015 have been determined in IAA on the ground of available observations in the catalogue of observations of the Minor Planet Center. ...

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The summary plot shows the monthly time distribution of all predicted magnetic conjugations between four spacecraft considered. ... To show the time of conjugation, in frame of the corresponding day for each SC the corresponding colour and line are used: . for the first SC the red color and the first line are used, . ... On the plot the SC names are shown by the corresponding colours. The summary plot permit to find the simultaneous magnetic conjugations of 3 and even 4 satellites. ...

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• The plot of the magnetic conjugation's time distribution
• Earth Research

Next: Structure of the Galaxy Up: Model of the Galaxy Previous: Model of the Galaxy . As discussed above (Section  6 ), galactic binary systems are assumed to be distributed logarithmically along their semi-major axis A (Abt and Levy, 1976[ 2 ]), . ... Figure 40: Number of binary stars per frequency decade. ... As the observed distribution of binary periods is flat (equation ( 15.3.1 )), the normalization constant is the total number of galactic binaries per frequency decade: . ...

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• Initial Distributions of Binary Parameters
• Results of calculations
• SIMBAD: Object list from refcode

... Identification and Analysis of Binary Star Systems using Probability Theory E. Grocheva and A. Kiselev Photographic Astrometry Department, Pulkovo Observatory, S.Petersburg, 196140, Russia, Email: gl@spb.iomail.lek.ru Abstract. Accurate identification of physical binary star systems has become of increasing interest in recent years. ... We chose 76 double stars from Pulkovo's observation program and calculated the probabilities of a random distribution for these pairs. ...

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• http://www.stecf.org/conferences/adass/adassVII/reprints/ferniquep.ps.gz
• The Stellar Population in the NICMOS Parallel Fields

Following are instructions to build and install the programs in this distribution. Make sure that you have all necessary tools for building executables. ... The automatic build process expects a configuration file called Config.local . ... The configuration file specifies the directory in which to install the binaries, as well as control over the generation of debugging code and reference clock support. ... Cleans out object files, programs and temporary files. make distclean . ...

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• The Network Time Protocol (NTP) Distribution
• Configuration Options
• SAI SN RESEARCH GROUP

... One of the most widely used tools of Fourier analysis is the Parseval theorem. It enables the experimentalist to view how the `energy' in the signal is distributed among frequencies. The Fast Fourier Transform (FFT) algorithms have made power spectra one of the obvious diagnostics tools during data acquisition, and energy maps are a versatile alternative. ... The result is an energy map (Fig. 9), showing the distribution of energy corresponding to the wavelet map (Fig. ...

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... 1 Instruments/Modes Instrument Mode EPIC MOS Imaging EPIC pn Imaging 2 Use pipeline processing yes interactive analysis no 3 Description This task takes the EPIC images in the input list of images, divides them by the images in the input list of `exposure maps', rebins the resulting images to a user-speci ed bin size and plots the corresponding intensity (count-rate) histograms (number of image bins containing a countrate within a certain interval) to a single PostScript le. ... List of input Images...

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• Null-hypothesis probability distribution for a weighted sum of Poissonian
• Description

... Apache HTTP Server Version 2.4 . Apache > HTTP Server > Documentation > Version 2.4 > Modules . ... To enable mod_dav , add the following to a container in your httpd.conf file: Dav On . ... In addition, a location for the DAV lock database must be specified in the global section of your httpd.conf file using the DavLockDB directive: DavLockDB /usr/local/apache2/var/DavLock . ... Use the Dav directive to enable the WebDAV HTTP methods for the given container: <Location /foo> Dav On </Location> . ...

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• mod_socache_memcache - Apache HTTP Server
• mod_socache_dc - Apache HTTP Server
• Relevant Standards - Apache HTTP Server

... P2589 Date Received: 2011-Jun-01 20:09:13 Technical Page Proposal Type: General Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: Regular Pulsars Galactic 40 Hours 2 hours Reinvestigation of Unidentified Sources of Dispersed Pulses Found with As- tropulse ABSTRACT: The Astropulse pro ject, a follow-on to the SETI@home distributed computing pro ject, uses the same dataset as SETI@home. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/KorpelatagP2677tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/KorpelatagP2677tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/KorpelatagP2589tp.ps

God Science Forum Message . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... God and Science | ... Distributed Unconsciousness (DU) . ... Posted by Michael Trout on May 2, 2006 09:10:07 UTC . ... Link: - h0riz0ndu - May 3, 2006 - 04:54 UTC . ... Consciousness? - imback - June 12, 2006 - 05:02 UTC . ... www.astronomy.net . About Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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USING THE CORRELATION BETWEEN ISGRI SURVEY RESULTS AND OTHER CATALOGUES TO AID SOURCE IDENTIFICATION John B. Stephen, A. Malizia and L. Bassani IASF-INAF, Via P. Gobetti 101, 40129 Bologna, ITALY, E-mail: stephen@iasfbo.inaf.it ABSTRACT In order to help in the identification of INTEGRAL/ISGRI sources, we have developed a software package which allows a rapid and detailed cross-correlation to be performed between various source catalogues. ... We show below some preliminary results from this analysis. ...

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• http://hea.iki.rssi.ru/integral06/papers/D31_Bikmaev01-05Feb07_11:12:42.pdf

Catalogue of eclipsing variables (CEV) is the world's principal database of eclipsing binary systems with available classification. CEV contains identifications, classifications, photometry, periods, eclipses data, spectral types, references and notes for 7179 systems. Format of the current CEV . CEV main table (~1.0MB) . ... List of systems, erroneously classified as eclipsing binaries in GCVS (they are not included in the CEV main table) Download all files as a single archive (~0.6MB) . ...

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Testing the Automatic Detection of Directly Imaged Exoplanets Using Wavelet Analysis Chris Merchantz Introduction · Challenges associated with direct images of planets Distinguish planets in the following way: (1) a minimum flux threshold is from speckles maxima, anddefined for the features that are identified as local (2) the "Exoplanet Recognition Using a Wavelet Analysis Technique" Fig. ... This spectrum is used as template spectrum to recognize planets in a deep image. ...

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• The AstroStat Slog Blog Archive chi-square distribution [Eqn]
• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• Comments on: chi-square distribution [Eqn] By: Alex By: vlk By: aneta By: aneta

... General Catalog of Variable Stars (GCVS database, Version 2012 Feb.) ... The cross-identification tables of the General Catalogue of Variable Stars (GCVS) contain all GCVS (including extragalactic variables from vol.V), NSV (New catalogue of Suspected Variable stars) and Supplement to the NSV stars as well as stars from the name-lists of variable stars nos. 67 - 80; it also makes it possible to find out identifications between the GCVS and the NSV catalogue. ... I-III) names are included. ...

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• General Catalogue of Variable Stars: What's new.
• GCVS Research Group: History and Persons.

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

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• Radio sources identfification
• Absorption bands identified with DIBs
• The peculiar post-AGB supergiant IRAS04296+3429: optical spectroscopy and its