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21. RR LYRAE VARIABLES SUBSYSTEMS IN THE GALAXY, figures
... The vertical and slanted dashed lines in the first panel mark the separation distinguishing are as occupied by thick-disk objects according to Hanson et al. (1998) and Martin, Morrison (1998) , respectively. An abrupt change in the dispersion near V res 290 km/s (the vertical dashed lines) is apparent in all panels except the first. discussion in the text | next figure | privious figure . ...
[ Сохраненная копия ]  Ссылки http://ip.rsu.ru/~marsakov/paper6/p6fg3_1.htm -- 2.5 Кб -- 02.02.2007
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22. http://zebu.uoregon.edu/~uochep/talks/talks04/et-l1-12-04.pdf
L1 Simulation Upgrade December 6th, 2004 BaBar Collaboration Meeting SLAC Eric Torrence University of Oregon Eric Torrence 1/15 December 2004 Phase 0 (Now) DchDigis EmcDigis EmtSim trgDC L1Accept This IS the current SP6 (14.4.X) Base simulation code unchanged, but interface elements are updated (Digis, TsfLUT) Remaining changes are inside black blob Eric Torrence 2/15 December ... Done · L1DZpdTrackDigi - cellLocation and cellPhi are not currently being simulated. ...
[ Текст ]  Ссылки http://zebu.uoregon.edu/~uochep/talks/talks04/et-l1-12-04.pdf -- 404.0 Кб -- 21.12.2004
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23. INTERBALL-TAIL KP changes
... New version of magnetic field data (descriptor "itm") is now available with small corrections in offsets and attitude coverage. ... Full set of INTERBALL-TAIL AKR radiointensity KP for AKR instrument is now available (descriptor "ita"). ... KP data availability plots are created. ... Magnetic field data (descriptor "itm") after 1st January, 1998 are recomputed with corrected Bx_GSE offset (this was just 0.5 nT correction). ... CDF files for plasma wave KP are now available (descriptor "itw"). ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/apetruko/kppnews.html -- 3.2 Кб -- 27.10.2003
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24. The Sparkle Plug-In: The Sparkle Dialog Box
... There are number of features that can be set by the user in the Sparkle Dialog box. ... The Sparkle plug-in computes the luminosity (level of whiteness) of each pixel in the image (the user can see this when the progress window labeled Generating luminosity array... is displayed). ... The threshold value is currently a slider/text field pair which have a precision of .0001. ... Like the Threshold value, the Flare Intensity has both a slider and a text input field for specifying its value. ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/~megera/gimp/mjhammel/gdp/plug-ins/sparkle-3.html -- 7.9 Кб -- 22.12.2007
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25. http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/xpa-2.1.14/man/mann/xpaacl.n
... C+ will give a nicer C++. ... IX Title "xpaacl n" .TH xpaacl n "June 7, 2012" "version 2.1.14" "SAORD Documentation" .SH "NAME" \&\fBXPAAcl: Access Control for XPA Messaging\fR .SH "SYNOPSIS" .IX Header "SYNOPSIS" \&\s-1XPA\s0 supports host-based access control for each \s-1XPA\s0 access point. ... PP Assuming that access control is turned on, the \s-1ACL\s0 for an individual \&\s-1XPA\s0 access point is set up when that access point is registered (although it can be changed later on; see below). ...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/sbig/archive/xmccd-4.1/xmccd-4.1e/xpa-2.1.14/man/mann/xpaacl.n -- 9.3 Кб -- 08.06.2012
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26. StelTextureMgr Class Reference
... Home All Namespaces All Classes Functions Coding Style Scripting Plugins File Structure . ... Manage textures loading. ... createTexture (const QString &filename, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams ()) . Load an image from a file and create a new texture from it. ... createTextureThread (const QString &url, const StelTexture::StelTextureParams &params= StelTexture::StelTextureParams (), const QString &fileExtension=QString(), bool lazyLoading=true) . ...
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/~aw/stellarium/api/classStelTextureMgr.html -- 10.3 Кб -- 02.10.2012
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27. ADASS 2003 Conference Proceedings
... Thus, it is now possible for users to write their own S-Lang scripts that load data into Sherpa , perform fits, and then copy the fit results out to S-Lang variables for further analysis in their scripts. ... Thus, we have added S-Lang functions that provide interfaces to Sherpa data structures. ... These scripts copy the appropriate data, errors and model values from Sherpa and send them to ChIPS; the scripts then call various S-Lang functions which are equivalent to ChIPS plotting commands. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass03/P4-10/ -- 15.6 Кб -- 13.08.2004
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28. http://hea.iki.rssi.ru/conf/hea2007/bp-0.2.97/NOTES
... Changed format option parsing routine in bp-p-options. added opt_reverseauthor to bp-refer, and added options parsing. 0.1.1 perl5/ad425.ref->ad425.bib in 25.3 seconds perl5/timetest.pl 2.31s total, 1.03, 1.01, 3.52 Added p-output.pl. ... No noticible change in running time, which means the debugging statements aren't slowing us down enough to worry about dropping them. 0.0.11 perl5/ad425.ref->ad425.bib in 22.7 seconds perl5/timetest.pl 1.98 total, 1.02, 1.01, 3.39 Added format registration. ...
[ Сохраненная копия ]  Ссылки http://hea.iki.rssi.ru/conf/hea2007/bp-0.2.97/NOTES -- 11.3 Кб -- 16.12.1996
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29. IKI SSC, INTMINS APRIL99
Modified 11 April 1999. The last modifications concerns to the new ground tracks selection on the base of the more wide list of the INSPIRE particpants. ... The range value was changed from 2 deg to 4 deg for the distance between lat/lon of the graund track and place of the INSPIRE members. Plots of predicted tracks under USA and Europe 11 April 1999 . April, 17, 1999 (USA) . April, 17, 1999 (EUR) . ... 11 April 1999 . ... place . ... Back to the IKI Satellite Situation Center (SSC) . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/vprokhor/intmins/april99.htm -- 8.0 Кб -- 11.04.1999
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30. Bookmarks of Yakiv Pavlenko changed on Jul 1, 2015
ARI USEFUL LINKS modified and/or upgraded by YP (Jul 1, 2015) . Astronomy . ... Astronomy related journals . ... Go to TOP . ADS ( UK , US or French site) . Abstracts from the major Astronomy journals. ... Astronomy Picture of the Day . ... Astronomy and Astrophysics (Bertout's site). status of a paper . ... of Stellar Spectra by R.O.Gray and VISUAL atlas (as pdf) . ... A list of Astronomy databases from the well organised canadian site. ... Astronomy jobs.../courses Go to TOP . ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/staff/yp/TOP-liv.htm -- 27.8 Кб -- 18.09.2015
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31. Journal "Peremennye Zvezdy"
Peremennye Zvezdy ( Variable Stars ) 26 , No. ... Moscow 119992, Russia . ... 84/32, Moscow 117997, Russia . ... Our CCD observations compared to times of minima derived from the archival photographic plates and from the NSVS and ASAS-3 data clearly show that the orbital period of the system is variable. ... The phased light curve for the light elements . ... CCD, Moscow . ... and for the current linear light elements (in excellent agreement with the NSVS, ASAS, and our CCD observations): . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/varstars/msg/1217495 -- 18.2 Кб -- 09.11.2006
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32. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... I think I will break from my usual format of Bad Astronomy/ Good Astronomy by saying that the way we define seasons currently is not strictly bad, but I feel (in my opinion!) that it could be better. The definition of when the seasons begin is at the moment of solstice or equinox; that is, winter (in the north) starts on December 22 nd and summer starts on June 22 nd . ... Now imagine breaking up the Sun's 46 degree up-and-down yearly swing into 1 day intervals. ...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/bad/misc/badseasons.html -- 24.7 Кб -- 09.04.2016
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33. VaST homepage
... VaST is a software tool for finding variable objects on a series of astronomical images. ... VaST performs object detection and aperture photometry using SExtractor on each image, cross-matches lists of detected stars, performs magnitude calibration with respect to the first (reference) image and constructs a lightcurve for each object. ... VaST FITS image viewer ./pgfv . ... Part I" PZP, vol. ... K. V. Sokolovsky, S. A. Korotkiy; "New Variable Stars Discovered by the NMW Survey" PZP, vol. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/vast/ -- 122.2 Кб -- 21.02.2016
[ Сохраненная копия ]  Ссылки http://saistud.sai.msu.ru/poisk/ -- 122.2 Кб -- 21.02.2016
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34. Cepheid Variables
... CEPHEID VARIABLE STARS: A Cepheid variable or Cepheid is a member of a particular class of very luminous, massive variable stars with pulsation periods of 1-70 days. ... The relationship is calibrated using data collected from Cepheids whose distances are determined by other means. ... Browse through the 68 CCD fits images he sent you, using ds9 and locate the Cepheid variable. ... Image credits: ESA - "http://sci.esa.int/science-e-media/img/20/cepheid-variables.jpg" . ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/researchprojects/cepheids/cepheids.html -- 8.3 Кб -- 02.10.2012
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35. ASP Technical Member Change of Email Address or Sign up for PASP Online Access
... SEARCH ASP SITE: Match ALL words Match ANY word . General/ Technical Membership Form for new members . Renewal General/ Technical Membership Form . ... Member Change of Contact Info . ... ASP E-mail Newsletters . ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/membership/paspchange.html -- 14.6 Кб -- 01.08.2012
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36. Linear polarization: wavelength dependence
... Fitting the observed dependence includes calculations of the polarization cross-sections averaged over particles orientation and size distribution, their normalization and the comparison of obtained dependencies with Serkowski's curve representing observational data for a chosen star. ... Variations of the polarization factors with wavelength are shown in Fig. 16 for homogeneous spheroidal particles with PF orientation. ... The distinction between prolate and oblate spheroids is also clearly seen. ...
[ Сохраненная копия ]  Ссылки http://www.astro.spbu.ru/DOP/8-GLIB/ASTNOTES/node7.html -- 18.9 Кб -- 19.11.2010
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37. The NMW survey homepage
NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/nmw/ -- 10.7 Кб -- 18.02.2015
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38. Spherical and Practical Astronomy
... Subject of Astronomy. ... Basis of Spherical and Practical Astronomy. ... Celestial Sphere. ... Changes of Star's Coordinates as a Result of Daily Rotation of Celestial Sphere. ... Time Measuring. ... Changes of Solar Equatorial Coordinates. ... Stellar Day, Stellar Time. ... Real Solar Time. ... Mean Solar Time. ... Connections between Stellar and Mean Time. ... Apparent Path and Configuration of Planets. ... Ways of Energy Transportation to Stellar Surface.Basis of Spectral Analysis. ... Solar...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/courses/zag_astr_e.html -- 7.0 Кб -- 23.02.2005
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39. (Untitled)
To construct frequency distribution (histogram) of minor planets according to value of some element/ parameter/ function user should first select Elements item in menu bar and then Histogram in drop-down menu. ... User has possibility to save histogram or to print it using standard means. To save the file select File item in menu bar and then Save As... in drop-down menu. ... To print histogram select File item in menu bar and then take advantage of options Print Preview , Print Setup , Print . ...
[ Сохраненная копия ]  Ссылки http://www.ipa.nw.ru/PAGE/FUNDAMENTAL/LSBSS/winample_guide/user4oqb.htm -- 4.2 Кб -- 10.04.2016
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40. ALIGNASN (Nov98) --- nictools --- ALIGNASN (Nov98)
alignasn -- Change the relative shifts in association file alignasn association . ... calnicb style association file with list of images to be aligned. ... Interactive program to compute relative shifts of images in an association file. ... After computing the relative shifts of the direct images, alignasn searches for corresponding grism images for each of the direct images. ... The grism association is then updated with the same relative shift measurements as determined from the direct images. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/alignasn.hlp.html -- 2.5 Кб -- 06.06.2006
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