spectrum1d - compute auto- [and cross- ] spectra from one [or two] timeseries. spectrum1d [ x [ y ] file ] -S segment _ size ] [ -C ] [ -D dt ] [ -N name _ stem ] [ -V ] [ -W ] [ -bi [ s ][ n ] ] [ -bo [ s ] ] spectrum1d reads X [and Y] values from the first [and second] columns on standard input [or x [ y ] file ]. ... Units same as ypower. name _ stem .npower Power spectral density of the noise output. Units same as ypower. name _ stem .gain Gain spectrum, or modulus of the transfer function. ...

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• http://xray.sai.msu.ru/~ivan/gmt/man/project.html
• http://xray.sai.msu.ru/~ivan/gmt/man/trend1d.html
• Ivan's contribution to GMT 3.2

... Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at ST­ECF M. Dolensky, A. Micol, B. Pirenne and M. Rosa Space Telescope ­ European Coordinating Facility, Karl­Schwarzschild­Str. ... The Pipeline In order to generate the missing jitter files a pipeline was set up (Figures 1 and 2). ... Both the Mission Schedule and the AEDP subset files are retrieved from the Data Archive and Distribution System (DADS) at STScI. ... 94 STScI started producing obs logs on a regular basis. ...

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• AstroAsciiData
• DER_SNR: A simple and general spectroscopic signal-to-noise measurement

... Certificate Handling Overview 1.1 Set Certificate Cache . 1.2 Add Certificate File . ... Certificate Verification Process 2.0.1 X509_NAME_oneline 3. ... 3.3 rsa . ... By default the code we are shipping uses the directory and PEM -style encoding for the certificates contained therein. ... To add a certificate: X509_add_cert_file(char *file,int type) . ... All certificates loaded via this interface must be in PEM format as this function simply calls X509_add_cert_dir() and X509_add_cert_file() . ...

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• Structure of the file system
• Fill-Out Forms
• rtftohtml Users Guide - 5 Customizing rtftohtml

If you select Select item, the Data retrieval from observatory list dialog box will appear. Click on one of two radio buttons to the left of data fields intended for observatory code or name and introduce the required data. In case of observatory name it is possible to introduce its fragment. ... If it is necessary to enter new observatory into the list, mark one of the entries with missing data and select Edit in drop-down menu. ... In this case Landscape mode should be selected. ...

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Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Stars . ... Space Flight . ... New observations with the European Southern Observatory (ESO)тАЩs Very Large Telescope of some of the most distant galaxies ever detected are revealing the mysteries of this important phase of the early Universe. ... These powerful instruments are essential for exploring this early period in cosmic history as they alone can enable the accurate observations of €аthese extremely distant and faint galaxies. ...

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• Exoplanet HAT-P-1b: weird, warm and fuzzy | Astronotes
• Patrick Moore Obituary | Astronotes
• To Space and Back with Reid Wiseman | Astronotes

3) Planets and Brown Dwarfs . ... By its nature, this method is most sensitive to massive planets orbiting close to their stars. ... That means that some of the more massive extrasolar planets could actually be brown dwarfs (although the statistics of the finds suggest that most of them are not). ... Another possible difference between brown dwarfs and massive planets is how they are born. ... They would base the fundamental definition on the mode of formation: a planet is built from planetesimals. ...

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• Astronomical Society
• ASP: Galileo Educator Network (GEN)
• ASP: Good Astronomy Activities on the WWW

Astronomy Picture of the Day . ... Above are two computer generated images highlighting how strange things would look. ... The picture is actually composed from two images recorded weeks apart by the Voyager 2 spacecraft during its visit to the Saturnian System in August of 1981. ... Most ground-based telescopes with lenses and mirrors are hindered by the Earth's nurturing, protective atmosphere that blurs images and scatters and absorbs light. ... A Dust Devil on Mars . ... The Hubble Deep Field . ...

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... Unlike clients such as Shout and IceDJ this permits the broadcast of live audio, rather than prerecorded mp3's. LiveIce was developed after the appearance of IceCast to provide the Real Time streaming functionality which makes it a viable solution for broadcasting. It is based on the guts of 2 of my previous works - Mp3Serv, the first mp3 broadcasting system & Mp3Mixer, a toy which allows the user to 'Mix' with mp3 streams. ... LiveIce XMMS sourcecode is available here . ...

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• Astrodynamics 101
• SCL Sfit Genetic Commands
• Armagh Observatory

... Информация Руководство и преподаватели Кучеров Александр Степанович . ... Публикации . ... Куренков В.И. , Кучеров А.С. Оценка массогабаритных характеристик комплексной двигательной установки космического аппарата дистанционного зондирования Земли // Вестник СГАУ. 2014. ? ... Куренков В.И. , Кучеров А.С. Метод выбора основных проектных характеристик космических аппаратов наблюдения на основе создания проблемно-ориентированных систем автоматизированного проектирования // Вестник СГАУ. ...

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• Трек Aerospace акселератора GenerationS продолжит работу в Тольятти
• Куренков Владимир Иванович. Публикации
• В Самарской области завершился трек Aerospace акселератора GenerationS

... Let G be a locally compact group and µ be a left-invariant Borel measure on G. (There are no regularity assumptions about the measure.) ... Let µp = {z C : z p = 1 for some n}, but we view it as a discrete group, which is not its usual topology as a subset of C. Prove µp Zp as topological = groups using an explicit isomorphism. ... Since the quotient topology on Qp /Zp is discrete, Qp /Zp is the correct model for µp topological group with the discrete topology. 1 n i{x} p on Qp . ...

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• http://www.mccme.ru/dubna/2007/courses/pre.pdf
• Yu.S. Ilyashenko homepage
• Registration Form

... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

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• Database of Optical Properties -- Level: database
• Database of Optical Properties -- Level: subpage
• Database of Optical Constants -- Level: welcome