Next: Transform of modulated Up: No Title Previous: Frequency/duration relation. Let us now turn to gradually more complicated signals, for which we soon lose the support of analytical expressions of the transforms. First, examine the sum of 3 cosine waves at different frequencies and phases. The Mexican hat wavelet analysis is carried out as above, yielding the wavelet map (Fig. ... Figure 11: g2 transform of a multiperiodic signal. ... Mon Nov 13 10:51:25 EST 1995 ...

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• Commentary
• ApSA courses
• Introduction

AO Home AO Astronomy Schedule Receivers CIMA AO IDL . IDL is the recommended data-reduction package for Arecibo spectral-line data. The different back-ends produce different data format. ... Mock spectrometer standard FITS format headers . Mock spectrometer PSRFITS format headers . WAPP CIMAFITS format headers . Interim Correlator IDL headers . ... Search WAPP data . ... How to fix WAPP FITS files taken with doppler tracking in order to read them with standard FITS readers . ...

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• DATA ANALYSIS
• Parties with an Interest in the Surveys, AKA ?the Stakeholders?
• NSF Senior Review of Astronomical Facilities

... Bojan Nikolic web pages (r. 329) . ... Analysis of (radio) spectra . The RNested package is a re-implementation of the main algorithms from the radiospec package into the R statistical data analysis environment. ... packages ( "RNested" , repos = c ( "http://www.mrao.cam.ac.uk/~bn204/soft/R" , "http://cran.us.r-project.org" )) . ... RNested ? Nested Sampling in R & analysis of spectra . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• Statistics for astronomy graduate course Bojan Nikolic web pages (r. 329)
• Statistics for astronomy graduate course
• XXVIIth YERAC Preface

... Latest Supernovae . ... Sorted by Name For the year 2016 , 2097 supernovae and 12 extragalactic novae were reported. 172 of these supernovae were named by CBAT, 1498 were given possible supernova designations, and 427 were not reported to CBAT. 36 supernovae were found in NGC/IC galaxies, 147 were found in named galaxies 46 objects were discovered by amateurs 0 were brighter than 13th Magnitude 19 were brighter than 16th Magnitude 198 were brighter than 18th Magnitude 145 ...

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• Bright Supernova pages - Statistics for 2004
• Bright Supernova pages - Statistics for 2002
• Bright Supernova pages - Statistics for 2003

... astro-ph . ... Statistical Characterization of the Chandra Source Catalog . ... The first release of the Chandra Source Catalog (CSC) contains ~95,000 X-ray sources in a total area of ~0.75% of the entire sky, using data from ~3,900 separate ACIS observations of a multitude of different types of X-ray sources. ... In addition to these traditional catalog elements, for each X-ray source the CSC includes an extensive set of file-based data products that can be manipulated interactively. ...

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• SAI CAS: About the SAI CAS project

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. ...

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Next: The Evolution of Stars Up: NICMOS Science Previous: A Coronagraphic Search for . ... The NICMOS Parallel program . ... The Stellar Population . ... NICMOS Camera 3 is being used in parallel mode to observe galactic fields at both high and low galactic latitudes. ... Most of the fields are at high galactic latitude; as Figure 1 shows, only 8 pointings are within |b| = 10 o , i.e. the galactic disk. Figure 1: NICMOS parallel fields distribution in galactic latitude. ... Figure 6 ). ...

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• Space Telescope-European Coordinating Facility
• STScI NICMOS Software
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

... Team . ... The main goal of observations of GRB host galaxies is accumulation of statistics of their spectroscopic and photometric properties. ... The Hubble diagram for 22 GRB host galaxies with known magnitudes and redshifts (GRB 970228, GRB 970508, GRB 970828, GRB 971214, GRB 980613, GRB 980703, GRB 990123, GRB 990510, GRB 990712, GRB 9912008, GRB 991216, GRB 000131, GRB 000210, GRB 000301C, GRB 000418, GRB 000911, GRB 000926, GRB 001109, GRB 010222, GRB 010921, GRB 011121 and GRB011211). ... 600...

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• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Magnetic stars -
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - History of
• Description of algorithm

Astronotes Armagh Planetarium's Stellar Blog! ... Our Galaxy . ... Space Flight . ... Posted on April 21, 2011 | No Comments An image from the European Southern Observatory, reveals two galaxies, NGC 3169 and NGC 3166, meeting in intergalactic space. ... Continue Reading.. ... 1 Comment NGC 2841 is a rather beautiful flocculent spiral galaxy. The Hubble Space Telescope recently imaged NGC 2841 as part of an investigation into how new stars are created. ... Posted on October 28, 2010 | ...

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• Christmas Card Competition Winners: Images of the Month | Astronotes
• physics | Astronotes - Part 3
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MAGION 5 is subsatellite of the Auroral Probe, one of the satellites of the INTERBALL program. ... Click hear for the 1999 flight situation analysis during operations scheduling . ... The satellites motion calculation during the flight situation analysis is based on the orbital elements determined by the Institute of Atmospheric Czech Academy of Sciences. ... SSC GSFC NASA Satellite Situation Centre of the NASA Goddard Space Flight Centre . ... Space Research Institute (IKI) . ... IKI RAN | ...

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• INTERBALL TAIL PROBE SITUATION ANALYSIS
• INTERBALL AURORAL PROBE SITUATION ANALYSIS
• Trigonometry beyond 90 degrees

Stellarium 0.12.3 . ... Renderer . FileљStructure . FileљList . FileљMembers . core . renderer . StelQGL1Renderer.hpp . ... 63 љ // Can't check the invariant here, as the renderer will be destroyed even . ... 81 љ return false ; . ... 85 љ invariant (); . 86 љ return true ; . ... 95 љ // GL1 doesn't support shaders. 96 љ return NULL; . ... 112 љ StelProjector * projector = NULL, . ... NULL) . ... 164 љ (NULL != projector ? ... 167 љ projector = (NULL != projector ? ...

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• Stellarium: StelRendererStatistics Class Reference
• Stellarium: TuiNodeEditable Class Reference
• Stellarium: core/renderer/StelQGL2Renderer.hpp Source File

... Pluto's orbit is also highly inclined -- tilted 17 degrees to the orbital plane of the other planets. ... Ground-based observations indicate that Pluto's surface is covered with methane ice and that there is a thin atmosphere that might freeze and fall to the surface as the planet moves away from the Sun. ... This is the first image-based surface map of the solar system's most remote planet, Pluto. ... This is the first surface map of Charon, the moon of the solar system's most remote planet, Pluto....

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• Dr. Victoria I. Prokhorenko
• Coordinate systems [Oulu]
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... Центральное место в курсе занимает комплекс асимптотических результатов теории вероятностей, включающий, наряду с законом больших чисел и классической центральной предельной теоремой, обобщение последней для устойчивых законов и теоремы о предельных распределениях экстремальных значений и больших уклонений. ... Теория распределений . ... Причина нарушения закона больших чисел для распределений с тяжелыми хвостами , статистика экстремальных значений, предельная теорема Фишера-Типпета-Гнеденко. ...

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• Mathematical statistics: an introduction (Fall 2011)
• Semiclassical Microlocal Analysis (Fall 2003)
• Workshop on geometric analysis and spectral theory. Abstracts

... ursa in Unknown (configure /etc/snmp/snmpd.local.conf) . ... Max Speed: . ... at which time 'ursa' had been up for 233 days, 1:27:12 . Max . Average . Current . ... 90.0 kB/s (0.4%) . ... 152.0 kB/s (0.6%) . ... 144.0 kB/s (0.6%) . ... Incoming Traffic in Bytes per Second . ... Outgoing Traffic in Bytes per Second . ...

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• Traffic Analysis for ursa (UARNET)
• MAO NASU :: Forum Statistics
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TUI supports the following offsets: . Object Arc offset by a given amount on the sky (i.e. along the arc of a great circle). ... Arc offsets are useful for moving a different portion of your object or a different nearby object onto the boresight . ... Object Arc XY this is identical to an Object offset except that it has been rotated to align along the instrument x-y axes. ... This is just like the Calibration XY offset, except that it is typically cleared when you slew to a new object. ...

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• Primary mirror support
• Deforming Plug-plates
• APO Job Announcements

... During the analysis of the surveys carried out on RATAN-600, it was found that almost one fifth of the detected sources shows significant radio flux variations. ... We used the data from "Cold" radio surveys carried out with RATAN-600 in 1980-1994 to search for radio sources with significant flux variability. ... On possibility of detection of variable sources using the data of Cold surveys carried out on RATAN-600. ... Detection of Variable Sources Using the Data of "Cold" Surveys. ...

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... 2.06.2001 . In the Summer of 1054 A.D. Chinese astronomers reported that a star in the constellation of Taurus suddenly became as bright as the full Moon. ... From September 2000 through March 2001, astronomer Tunc Tezel patiently photographed the planet Venus on 25 different dates as it wandered through the evening twilight. ... Arcing toward southern skies in late March, this faint comet LINEAR - the one officially designated C/2001 A2 (LINEAR) - brightened unexpectedly. ... March . ...

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• Supernova Remnant E0102 72 from Radio to X-Ray

The AstroGuide . ... AstroGuide | ... AstroGuide Listing . ... See many more Astronomy Listings by: Category or Alphabet . ... The software run under Windows 95, 98 NT, including Paraxial and Seidel . ... and Energy Distribution, Optical Layout, Optimization, Tolerancing etc. ... Listed Since August 20, 2005 . ... Web Site . ... Web . ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• There Are Two Different Situations Here! - an Astronomy Net Blackholes Forum
• Everyone Will Give You A Different Answer - an Astronomy Net Bigbang Forum
• A Different Time Subject When I Was A Child. - an Astronomy Net General Forum

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? ...

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• Methods and instruments to measure/monitor major site properties

Chair of solid state physics . ... The Physics of Phonons . ... In the first part of the course “The Physics of Phonons” the dynamics of atoms in one- and three- dimensional crystalline lattices is considered in detail. The quasiparticle conception in solids, taking phonons as an example, is discussed; creation and annihilation operators of phonons, main properties of acoustic and optical phonons dispersion laws, density of phonon states. ... Crystalline state. ... Acoustic and optical phonons. ...

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• IX International Astronomy Olympiad
• Laboratory of spectroscopy of defect structures ISSP RAS
• X-Ray Structural Analysis