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1. Why Spectral Energy Distributions?
... Because binary X-ray sources are strong emitters over a broad range of the electromagnetic spectrum, with each part of the spectrum contributing distinct and often time-variable information, attempts to understand these systems by concentrating on information from a limited wavelength range may lead to contradictory and misleading conclusions. ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~saku/WhySEDs.html -- 4.0 Кб -- 01.10.2012
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2. The Network Time Protocol (NTP) Distribution
... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~er/xntp/ -- 8.7 Кб -- 21.12.2007
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3. Distribution of Schedule Files
. Next: Related Programs Up: INSTALLING, AND RUNNING SCHED Previous: Running SCHED on a Contents . Once SCHED has been used to make schedules for an observation, those files need to be sent to the stations, usually by way of a distribution center at NRAO or in Europe. When time for a project is allocated, instructions for how to accomplish this will be provided. Craig Walker 2014-04-14
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Distribution_Schedule_Files.html -- 3.4 Кб -- 10.04.2016
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4. NStars1A: Photometric searches - 2MASS and optical colours
... Figure c1.1 plots the spatial distribution and colour-magnitude diagrams for the 650 sources with J . ... We have cross-referenced the sample against the SIMBAD, using a search radius of 2.0 arcminutes centred on the 2MASS position. ... Figure c1.4: Stellar ultracool sources - optical/near-infrared distributions. 138 lie within 2-3 arcseconds of stars in one of either the Henry Draper, Bonner Durchmusterung, Cape Durchmusterung, Cape Photographic Durchmusterung, Guide Star Catalogue, or PPM...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/~inr/nstarsu3.html -- 14.9 Кб -- 08.06.2007
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5. Initial Distributions of Binary Parameters
Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~mystery/articles/review/node39.html -- 14.1 Кб -- 26.02.1997
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6. Algorithm
... The following algorithm shows the rough details of these calculations. ... Similarly the energy selection region for the reflection order of the output matrix is converted to the array called banana. // analyze the exposure maps within the spatial selection regions FOREACH node FOREACH b = dispersion channel of node src.exposure[ node ,b] = EXPMAP node [b] summed over src.spans[ node ,b] bkg.exposure[ node ,b] = EXPMAP node [b] summed over bkg.spans[ node ,b] D = EXPMAP ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/6.5.0/doc/rgsrmfgen/node8.html -- 10.5 Кб -- 16.08.2005
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7. Starlink's Software Distribution System
... Up: Software Systems and Tools . ... The Starlink Software is a collection of astronomical packages and utilities comprising over 120 separate components. When built, the system needs between 500 and 650 MB disk space (without source) making it ideal for distribution on CD-ROM. Each component has been individually packaged into an easy-to-install bundle for users to obtain over the Internet via a ``point and click'' WWW interface from the Starlink Software Store. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/blymj/ -- 10.9 Кб -- 16.07.1999
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8. http://zebu.uoregon.edu/~uochep/talks/talks05/G050216-00.pdf
Searching for GRB -GWB coincidence during LIGO science runs Isabel Leonor University of Oregon LIGO-G050216-00-Z Motivation almost 40 years since GRBs were discovered past 15 years has been time of important clues isotropic and inhomogeneous distribution (BATSE); first optical, x-ray, radio counterparts; redshift measurements; association with core-collapse supernovae yet important ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks05/G050216-00.pdf -- 1848.3 Кб -- 29.03.2005
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9. weight on turret floor
The weight and positions for the objects on the rotary floor were obtained from ecastro on nov03 and used to plot the weight distribution on the rotary floor. ... The figure shows the weight distribution by turret position. ... Fig 1 top: Each object on the floor is plotted with its weight vs its turret position. Fig 1 middle: The weight is averaged by turret position quadrant to show the imbalance in weight distribution. ... The turret position is that of the receiver or read off of the drawing. ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~phil/turret/turretweight.html -- 8.2 Кб -- 20.06.2013
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