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1. XMM-Newton Extended Source Analysis Software
... News Latest News News Archive Newsletter Quarterly Status Report . ... Data Analysis SAS News What is SAS? ... Calibration & Background Calibration Background Analysis . ... Back to Background Analysis Page . The XMM-Newton Extended Source Analysis Software package (XMM-ESAS) is developed at the NASA/GSFC XMM-Newton Guest Observer Facility (GOF) in cooperation with the XMM-Newton SOC and the Background Working Group. ... http://xmm.esac.esa.int/sas/current/doc/esas/index.html . ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/external/xmm_sw_cal/background/epic_esas.shtml -- 13.8 Кб -- 11.04.2016
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2. OptInt PmWiki : Wiki Style Examples
OptInt PmWiki . Pm Wiki / . ... Wiki Style Examples . Wiki styles | ... PmWiki uses WikiStyles for styling text with color and other attributes. PmWiki 2.0 introduced the ability to control the styling further and to even place styles on blocks. ... In addition, an author can define a style "shortcut" by using the define= property. For example, to define a style of %red% , one can use: . define=mystyle color=red% Here is some %mystyle% red text created using a style shortcut. ...
[ Сохраненная копия ]  Ссылки http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/PmWiki/WikiStyleExamples -- 32.2 Кб -- 28.02.2014
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3. QPSIM: An IRAF/PROS Tool for Source Simulation
... The generation of simulated sources whose physical properties are well understood is useful in assessing the functionality of point source analysis software. Qpsim is an IRAF/PROS task which will generate events from sources of given intensity, shape, and position and either overlay them on a flat background in a new QPOE file or inject them into an existing QPOE file. ... The simulated data can be a useful tool in calibrating point source analysis software. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/manningk.html -- 11.9 Кб -- 03.11.2000
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4. Spectral Extraction of Extended Sources
. Next: Charged Particle Subtraction Up: *qpspec* - Extraction of Previous: Spectral Extraction of Point . When analyzing extended sources the background must be obtained from a region well separated from the source. To correct the background for the differential vignetting (i.e., the difference between source and background vignetting) of the ROSAT mirror, set the vign_corr flag in qpspec to yes. For example: . xs > qpspec vign_corr=yes . rsdc@cfa.harvard.edu . 1998-06-10
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node143.html -- 3.4 Кб -- 01.10.2012
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5. NICMOS Background
... HST Overview . ... Important updates, discoveries and developments that could potentially affect NICMOS observations, calibration, or data analysis. ... The HST Data Handbook is the primary guide for calibration, reduction and analysis of NICMOS data. ... NICMOS ISR 2003-007:Analysis of the HST Thermal Background as Seen by NICMOS and NCS . ... This ISR presents the results of the analysis of NICMOS parallel thermal background data obtained as part of both SMOV and the cycle 7 calibration plan. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/nicmos/performance/background -- 23.5 Кб -- 10.04.2016
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6. World Coordinate Systems (WCS) in FITS
The FITS "World Coordinate System" (WCS) standard defines keywords and usage that provide for the description of astronomical coordinate systems in a FITS image header. ... I: "Representations of world coordinates in FITS" , Greisen, E.W. & Calabretta, M.R. (2002), Astronomy & Astrophysics , 395 , 1061-1075. ... This diagram illustrating Bonne's projection with conformal latitude +35 was produced by WCSLIB , a C implementation of the coordinate transformations defined in the FITS WCS papers. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Mark.Calabretta/WCS/index.html -- 14.0 Кб -- 10.04.2016
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7. ST-ECF Grism Spectrum Software for NICMOS Grism Data
Next: Imaging Polarimetry with NICMOS Up: NICMOS Data Calibration and Previous: The Photometric Performance of . ... NICMOSlook and Calnic C . ... Extracting spectra from a large number of NICMOS grism images requires a convenient interactive tool which allows a user to manipulate direct/grism image pairs. ... NICMOSlook and Calnic-C are two programs that were designed to take advantage of the fact that the NICMOS grism mode typically consists of taking both a direct and a grism image. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node13.html -- 16.5 Кб -- 12.06.2006
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8. Tail Probe | Software
... Matrix of Transformation | ... Software | ... The software includes: . attidf.for - a FORTRAN subroutine to get a matrix M (named PA in the subroutine text) to transform any vector from the S/C coordinate system to the GSE coordinate system: . V GSE = M * V S/C . To transform a vector from the GSE coordinate system to the S/C coordinate system transpose the matrix M: . ... We want to know the direction of this vector in the GSE frame for date: 30.05.1997, time 1h.0min.0sec. ut. ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/interball/attitude/tail/ch4.php -- 5.1 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/interball/attitude/tail/ch4.php -- 5.1 Кб -- 02.10.2012
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9. Index of /software/archive/colorspec/colorspec-1.0/examples
Name Last modified Size Description . Parent Directory - ppm/ 2009-02-10 15:26 - tif/ 2009-02-10 15:26 - . Apache/2.4.6 (Linux/SUSE) Server at www.astro.louisville.edu Port 80
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/archive/colorspec/colorspec-1.0/examples/ -- 2.0 Кб -- 10.04.2016
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10. coordConv
... CoordConv is written in C++ and Python, using SWIG as the C++ wrapper. ... In Python the following will convert an FK5 J2000 position to apparent topocentric coordinates at a specified TAI date: import coordConv taiDate = 4916391905 # TAI date in MJD, seconds site = coordConv . Site (-105.822616, 32.780988, 2788) # Apache Point Observatory 3.5m telescope # For better accuracy you may also specify UT1- TAI and pole wander in site ; # these may be obtained from IERS Bulletin B fk5Sys = ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/coordConv/ -- 5.1 Кб -- 14.01.2015
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11. mod_authn_alias - Apache HTTP Server
... Apache HTTP Server Version 2.2 . ... Provides the ability to create extended authentication providers based on actual providers . ... The example below creates two different ldap authentication provider aliases based on the ldap provider. ... AuthnProviderAlias ldap ldap-other-alias> . ... AuthnProviderAlias> and </AuthnProviderAlias> are used to enclose a group of authentication directives that can be referenced by the alias name using one of the directives AuthBasicProvider or AuthDigestProvider ....
[ Сохраненная копия ]  Ссылки http://www.sao.ru/ztcs/manual/de/mod/mod_authn_alias.html -- 8.0 Кб -- 25.02.2008
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12. http://site2010.sai.msu.ru/static/doc/TTravouillon_TMT_site_testing_site2010.pdf
Lessons learned from the Thirty Meter Telescope site testing Tony Travouillon Sebastian Els, Angel Otarola, Reed Riddle, Matthias Schoeck, Warren Skidmore TMT.XXX.PRE.05.0XX.DRF01 1 Introduction TMT and its Site testing. Important choice before going on site. ... Considerations during analysis of the data. TMT.XXX.PRE.05.0XX.DRF01 2 Some Background about the TMT Site Testing TMT is a 30m, segmented, RitcheyChretien telescope design. ... ASCA Cloud Cover Analysis So how do we do it in practice? ...
[ Текст ]  Ссылки http://site2010.sai.msu.ru/static/doc/TTravouillon_TMT_site_testing_site2010.pdf -- 2354.3 Кб -- 18.10.2010
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13. Long description of example illustrating background calculation
. This diagram shows a small table with three transparent cells and illustrates how their final background is determined. The table consists of two rows. Four (labeled) cells lie in the first row, but the second cell spans the first and second row. The first, third, and fourth cells of the second row are "empty". Each non-empty cell has a red background and a double black border. Each empty cell has the table's background color (specified as #ff0) as its own. Return to image.
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/~vab/html.doc/css2/images/longdesc/tbl-empty-desc.html -- 1.9 Кб -- 02.05.1998
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14. mod_authn_alias - Apache HTTP Server
... Directives | ... Apache HTTP Server Version 2.2 . Apache > HTTP Server > Documentation > Version 2.2 > Modules . ... Provides the ability to create extended authentication providers based on actual providers . ... The alias providers can then be referenced through the directives AuthBasicProvider or AuthDigestProvider in the same way as a base authentication provider. ... The example below creates two different ldap authentication provider aliases based on the ldap provider. ... server config . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/manual/de/mod/mod_authn_alias.html -- 11.1 Кб -- 21.01.2013
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15. http://scan.sai.msu.ru/lk/
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. ...
[ Сохраненная копия ]  Ссылки http://scan.sai.msu.ru/lk/ -- 6.6 Кб -- 24.12.2015
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16. ESO - Historic examples of ESO-developed technologies
... ESO for the Public > Doing Business with ESO > Technology Transfer > Historic examples of ESO-developed technologies . ... Solar System . ... Survey Telescopes . ... Technical CCD systems . ... The original TCCD systems are now obsolescent, and have been replaced by a newer version based on a commercial controller and an ESO-developed CCD head. ... Remote Observing . ... Before the VLT era, astronomers given observing time on ESO telescopes had to travel to Chile to carry out their observations. ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/public/industry/techtrans/DevelHistoric.html -- 37.2 Кб -- 10.04.2016
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17. http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/Lab6.doc
Theory of filtering and time series processing L. Zotov Laboratory work ?6 Purpose: Studying singular spectral analysis SSA. We use Matlab software (look into the Lab N1). 1) Download the program and additional module for the lab from http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/ Study the SSA package on examples. 2) Download and install program from http://www.gistatgroup.com/cat/cat33.exe Study it. Visit http://www.gistatgroup.com/gus/examples.html
[ Текст ]  Ссылки http://lnfm1.sai.msu.ru/grav/english/lecture/filtering/Lab6.doc -- 26.0 Кб -- 18.02.2009
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18. Semiclassical Microlocal Analysis (Fall 2003)
... Microlocal Analysis is a theory of Pseudo-Differential Operators and Fourier Integral Operators (PDOs and FIOs). ... Microlocal analysis comes in few flavors. ... We will consider semi-classical PDOs and FIOs: one can always get from there to standard PDOs and FIOs but semi-classical theory has more applications. Less formal description of (semi-classical) microlocal analysis is ``a semi-classical limit of quantum mechanics'' or ``high-frequency limit of electrodynamics'' (etc). ...
[ Сохраненная копия ]  Ссылки http://www.mccme.ru/ium/f03/microlocal.html -- 5.0 Кб -- 09.12.2005
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19. The Arecibo User Manual for Astronomers
... Use of This Manual . ... Spectral-Line Observing at Arecibo (3.25 Mbyte) + Spectral line Appendices (0.56 Mbyte) ( HTML page ) . ... Data Analysis . ... Continuum Observing at Arecibo (0.36 Mbyte) + Continuum Appendices (0.31 Mbyte) . ... Pulsar Observations at Arecibo (4.03 Mbyte) + Pulsar Appendices (0.70 Mbyte) ( HTML page ) . ... VLBI Observing at Arecibo (0.36 Mbyte) + VLBI Appendices (0.35 Mbyte) . ... Introduction to Computing at Arecibo (0.33 Mbyte) + Computing Appendices (0.32 Mbyte) . ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~csalter/toppage.html -- 10.8 Кб -- 20.03.2002
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20. WD Merger Movie: POV-Ray stars
... Light sources: POV-Ray works with point sources of light. ... A real star consists of a spherical light source (the photosphere where the continuum is formed) superimposed by a scattering layer (an atmosphere) responsible for phenomena such as limb darkening and absorption lines. ... For example, in order for the central light source to illuminate the surface, the star must be transparent. ... The POVRay source for creating the white dwarf binary merger movie is given for demonstration purposes. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/movies/povray_stars.html -- 4.9 Кб -- 29.03.2002
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