This diagram illustrates the normal flow of text between parent and sibling boxes. A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. Four lines of text are displayed, occupying line 1 through 4. In the following PRE element, each 24 pixel line is simulated by two lines, the second beginning with the appropriate number. The lines, as they appear in the image, contain: 1 Beginning of body contents. ... 3 End of outer contents. End of body 4 contents. ...

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• Property index

... Classes . ... casa::LatticeFractile< T > . ... Static functions to get median and fractiles of a lattice. ... unmaskedFractile (const Lattice < T > &lattice, Float fraction, uInt smallSize=4096 *4096) . ... unmaskedFractiles (const Lattice < T > &lattice, Float left, Float right, uInt smallSize=4096 *4096) . ... Determine the fractiles for a small masked lattice. static uInt . ... static uInt casa::LatticeFractile < T >::findBin . ... static uInt casa::LatticeFractile < T >::maskedHistogram . ...

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• Containers and Pop-up Shells
• WCSLIB: tabprm Struct Reference
• casacore: casa::BinarySearch_global_functions_binarysearch Struct Reference

... Format of the orbital elements | Estimation of the extrapolation errors | Version 1" of the orbital elements collection, determined by KIAM during flight and used for operations planning . Version 2" of the of the orbital elements collection, modified by IKI during flight and recommended for the orbital calculations during scientific data processing . ... Three kinds of the INTERBALL Auroral probe (IB_AUR) orbital elements' collections are presented here. ... IKI RAN | SSC IKI RAN | ...

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• The INTERBALL Tail PROBE orbital elements
• About modification of the INTERBALL orbital elements
• The INTERBALL Auroral PROBE orbital elements

... 1 Instruments/Modes Instrument Mode EPIC SPECTROSCOPY 2 Use pipeline processing yes interactive analysis yes 3 Description This task calculates the area of a source region used to make a spectral le. ... The nal value is: area = geometric_area - ccd_gaps - bad_pixels In normal use only pixels which lie within the CCD boundaries and not on bad pixels contribute to the total area. The units of area are detector pixels which are square pixels of side 0.05 arcseconds. ...

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• http://xmm.vilspa.esa.es/sas/6.5.0/doc/backscale.ps.gz
• http://xmm.vilspa.esa.es/sas/7.0.0/doc/backscale.ps.gz
• http://xmm.vilspa.esa.es/sas/6.0.0/doc/backscale.ps.gz

... Most imaging systems contain intrinsic geometric distortions. Although they can often be disregarded for small field corrections they must be applied when image tubes or dispersive elements (e.g. in spectrographs) are used. ... A wavelength transformation for an image tube spectrum is shown in Figure where both resulting spectra with and without flux correction are given. ... The main problem is that one has to assume a certain distribution of flux inside a pixel e.g. constant. ...

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• Artifacts
• The Button Widget
• Comparison of two stochastic processes

... The <B> element specifies that the enclosed text should be displayed in a boldface. ... The <I> element specifies that the enclosed text should be displayed, if practical, in an italic font (or slanted). ... The <SMALL> element specifies that the enclosed text should be displayed, if practical, using a small font (compared with normal text). ... The <SUB> element specifies that the enclosed text should be displayed as a subscript, and if practical, using a smaller font (compared with normal text). ...

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• Table Rows
• The IMG (Image) Element
• Fill-Out Forms

function fringevissq,c,k,n,normal=normal . ... Zero if no counts. The first index in the frames must correspond to the phase bins. Use k to select a baseline, if multiple baseline are present. ; . ... if n_elements(k) eq 0 then k=1 . ... nominator=add(abs(fringevis(c-avg(c),k))^2-s,n,r(0)-2)/n . denominator=(add(s,n,r(0)-2)/n)^2 . index=where(denominator eq 0,count) . if count gt 0 then denominator(index)=1 . ... if normal then norm_factor=4.0/sinc(float(k)/n0)^2 $ . ...

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Next: Limiting Energy Channels Input Up: *fit* - Fit Data Previous: Raymond Model . The model is a two-temperature Raymond thermal spectrum, low temperature range is 0.55 to 0.65 keV, high temperature range is 1 to 2 keV, element abundance table is cosmic, abundance of heavy elements (atomic number >2 ) is 50% of the value in the table. Note that 0.7 = log(5.0), specifies that the second component normalization will be 5 times the normalization of the first component. ...

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• The AstroStat Slog education
• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog Blog Archive my first AAS. VI. Normalization

... The effect of the normal star on the compact magnetized component is largely determined by the rate and velocity of stellar wind at infinity . ... For Be-stars (i.e. those stars at the stage ``I'' whose mass increased during the first mass exchange), the wind velocity at infinity is taken to be equal to the Keplerian velocity   at the stellar surface . Thus, the lower stellar wind velocity leads to an effective increase of the captured mass rate by a secondary companion to such Be-stars. ...

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• Normal star evolution
• Star Formation Rate and Normalization of Stellar Populations
• Evolutionary Scenarios of Binary Systems

Do we need various assumptions to get a good FCN? A new multiple layer spectral method Cheng-li HuangMian Zhang Shanghai Astron. ... No FCN ! ... FCN,FCN,FCN.. Multiple layer spectral method (MLSM) + Linear Operator Method (LOM) Finite Element Method (FEM) · · Traditional approach solves one order ellipsoid only. ... Main Idea of FEM Boundary Surface could be described as: Let's consider how to solve the dynamic equation: Traditional Approach: Equivalent Spherical Domain . ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/vavilov.pdf

... The normal m 1 , c 1 indices and metallicities have been calculated for 2472 F-stars from the uvby and H fotometry. ... It is shown that the metallicity distribution of F6-G0 dwarfs is not a Gaussian one, but may be considered as a sum of two normal distributions. At the centre, the distribution shows a gap which subdivides all the stars into two metallicity groups. ... По данным uvby , H - фотометрии вычислены нормальные индексы m 1 , c 1 и определена металличность 2472 F-зыезд. ...

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• RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures

... 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 | ...

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• APOD: 2002 August 20 - The Universe in Hot Gas
• APOD: 2005 August 8 - Mars to Appear Normal this August
• APOD: 2001 May 1 - Antarctica Hears Little Normal Matter in the Big Bang

... Abstract Determine the set of osculating conic orbital elements that corresponds to the state (position, velocity) of a body at some epoch. ... In general, the elements found by this routine can have two kinds of problems: - The elements are not accurate but still represent the input state accurately. ... One recommended "sanity check" on the outputs is to supply them to the CSPICE routine conics_c and compare the resulting state vector with the one supplied to this routine. ...

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• CSPICE Routines: EKNELT_C
• CSPICE Routines: WNELMD_C
• Issues Affecting Previous ETCs

... Several HTML elements, most notably the A element , may contain an attribute which takes a URL as value. URLs, Uniform Resource Locators, are addresses of Web documents. More generally, URLs can be used on the Web to refer to "objects" on the Web or in other information systems. ... http . a Web document (to be accessed using Hypertext Transfer Protocol, HTTP ) . ... file . ... In particular, the specifications say that within a URL only a limited set of characters can be used as such : . ...

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• Determination of atmospheric parameters and calculation of chemical composition
• harak_e

... We describe enhancements made to Sherpa for the CIAO 2.0 release, concentrating upon those that enable a user to: (1) analyze Chandra X-ray Observatory grating data with wavelength- or energy-space models; (2) simultaneously fit background and source datasets; and (3) estimate and visualize confidence intervals and regions. ... Sherpa is the modeling and fitting tool of the Chandra Interactive Analysis of Observations (CIAO) software package (Doe et al. 1998 and references therein). ...

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• An Approach for Obtaining Polarization Information from COBE-DMR
• Improvements in Filter Design for Removing Galactic ``Cirrus'' from IRAS Images
• Automated Spectral Classification Using Neural Networks

Electronic Catalogue of Comets "Halley" . ... In this paper we give a description of the Electronic Catalogue of Comets "Halley", which makes it possible to calculate the evolution of the orbits of comets, to visualize orbital motion, to determine the circumstances of a comet's close approach to planets within a given time interval, as well as a number of other opportunities. ...

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• (Untitled)
• ENGAMPLE
• AY2008 (preface)

... It may be added, subtracted, divided or multiplied in any way appropriate for ordinary numbers. A mathematical relationship involving known numbers (like 25 or 40) and unknown ones (like x ) is known as an equation . ... To get a solution, one must replace the given equation (or equations) with others, containing the same information but cleaner in appearance. ... If you have an equation and modify both its sides in exactly the same way , what you get is also a valid equation. ...

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• From Stargazers to Starships
• DIGITAL WDC EXCHANGE FORMAT FOR OBSERVATORY 1.0 MINUTE VALUES
• Pictures/Рисунки

... The Universe in Hot Gas . ... 20.08.2002 . ... Explanation: Where is most of the normal matter in the Universe? ... Normal matter" refers to known elements and familiar fundamental particles . ... The distribution of much more abundant dark matter likely mimics the normal matter, although the composition of the dark matter remains mysterious. ... August 2002 . ... Publications with keywords: universe - dark matter - hot gas . Publications with words: universe - dark matter - hot gas . ...

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• Астронет > The Universe in Hot Gas
• Journal "Peremennye Zvezdy"
• XWare > APOD

AO Home AO Astronomy Robert Minchin Blog Publications IDL Routines . Rotang can either be run from the command line as described here or through the alfa_ang GUI . ... To run rotang at Arecibo: . Start IDL . ... Run Rotang: . rotang, Date , RA , Dec , Time , /choice . ... Rotang also calculates the Azimuth and Zenith Angle fir every source. If the Zenith Angle is greater than 20 degrees, then the program will return that the source is down and will not calculate an optimum ALFA angle. ...

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• Details of Rotang

The types of respirators in use at APO are half-face, full face, and mask-style filter types. ... These respirators DO NOT supply oxygen. ... The observatory does not maintain Self Contained Breathing Apparatus (SCBA) for use and, consequently, materials that require them cannot be used. ... Whenever possible chose adequate ventilation over using a respirator. ... Oxygen monitors used for confined spaces may be used to monitor oxygen levels where respirators are required. ...

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