... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

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• OptInt PmWiki : MROI / Tip-tilt Systems
• Atmospheric Modelling for ALMA
• ALMA WVR phase correction algorithms and software Bojan Nikolic web pages (r.

The study of energetic particles acceleration and transport within the magnetosphere and on its boundaries is the main goal of DOK-2 experiment on Auroral Probe in a frame of INTERBALL project. ... DOK-2 uses two pairs of energetic particle telescopes . ... This information is available only during the most informative Real Time mode of DOK-2. ... Full 56-57 channel spectra accumulated during time intervals from 10 s to 1464 s depending on a particle intensity. ... For this time interval: . ...

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• Trigonometry--what it is good for?
• Vectors
• Frames of Reference: The Centrifugal force

A spherical meteorite of radius 3m enters the Earth's atmosphere at an altitude of 100km and a speed (relative to the Earth) of 30 km/s. The atmosphere slows it down, so when it hits the Earth's surface it is travelling at only 1 km/s. If half of the heat generated as it passes through the atmosphere is absorbed by the meteorite, how hot will it be when it is about to land? ... However, the number I calculated (500,000 K) is correct, as is the discussion that follows it. ...

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• Worked Example 01
• Worked Example 03

Here are a set of pictures which progress from the original through a couple intermediary images to the final, rather 60ish looking final image. This is the original image, created using some PD fonts and some mucking around with the BCG plug-in. The original logo has been extruded a bit using the displace plug-in. A web is created by using the wave plug-in, duplicating it and rotating it 180 degrees, and adding the two pieces together. The original logo is then placed over that. ...

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• GIMP animations: merge-anim example 4
• The Sparkle Plug-In: Example Images
• The Sparkle Plug-In: The Sparkle Dialog Box

... This appartus will drop a mass from different heights. When the mass strikes the ground, some percentage of its original energy will be absorbed by the ground. ... The percentage of the energy which is absorbed by the surface on each "bounce" (EAS) . ... The impact velocity of the object will also be given at each bounce. ... Start= Drop the ball after Energy, Mass and EAS have been set; resume after step or pause has been selected . ... Reset = Reset experiment to intial values . ...

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• Astronomy HyperText Book
• Historical Cosmologies
• Energy From the Wind

ENERGETIC PARTICLE EXPERIMENT DOK-2 . ... Due to much higher energy, angular and time resolution, better separation of electrons and ions it is expected that DOK-2 experiment will allow to re-examine in more details energetic particle population and related processes in magnetosphere regions covered by the spacecraft orbit. ... Thin foil in front of detector absorbes protons with energies E<400 keV so this detector measures electron spectrum in 20 - 420 keV range. ... Energy values, keV . ...

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• FAQ [AE/DST]
• Energetic Particles
• ASPI experiment

... A lot Chinese names are degenerate. For example, it is hard to identify the person by just reading S. Xu. My advisor Michael Jura at UCLA and I facilitated AAS to follow APS and allow Chinese, Japanese and Korean to display their names in their original characters. It has been an option since 2010. ... Here is an example of the LaTex file and the compiled pdf . If the Chinese characters appear garbled, make sure to set the encoding of the LaTex file to be UTF 8. ...

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• The Chandra Deep Field South
• IRAF/STECF imaging linear polarimetry simulation and reduction package
• ESO - Examples of ESO developments that have been used for other similar

... In the above example, the second region uses the global coordinate system (PHYSICAL by default). ... Supported systems include: name description ---- ----------- PHYSICAL pixel coords of original file using LTM/LTV IMAGE pixel coords of current file FK4, B1950 sky coordinate systems FK5, J2000 sky coordinate systems GALACTIC sky coordinate systems ECLIPTIC sky coordinate systems ICRS currently same as J2000 LINEAR linear wcs as defined in file In addition, two mosaic coordinate ...

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• Calculation of errors in smoothed arrays
• Comments on: Kepler and the Art of Astrophysical Inference By: vlk By: aneta
• Coordinate Systems

The code calculates the extinction, scattering and absorption efficiency factors for prolate or oblate homogeneous spheroids. ... We provide the code with a test input file and two output files. A run of the code with such an input should lead to the results given in the output files. ... Parameters: . ... Values of other parameters are specified in the input file homn.dat . ... Voshchinnikov N.V., Farafonov V.G. Optical properties of spheroidal particles, . ...

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• Silicate minerals
• Database of Optical Properties -- Level: welcome
• Polarization properties (transmitted radiation)

Next: Imaging by an Optimizing Method . ... A big advantage of this numerical integrator is its stability: the error in the semi-major axis and the eccentricity depends only on the step size and does not grow with an increasing number of time steps. ... As the integration time increases, the numerical results become more contaminated by various errors. ... A new symplectic integrator produces no secular truncation errors in the actions of a Hamiltonian system. ...

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• Literature and Catalogs in Electronic Form: Questions, Ideas and an Example:
• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Modeling Scattered Light in the HST Faint Object Spectrograph

... Epistemology is a part of the study of Philosophy dealing with how we use our senses to know something about the world. ... Yet we know that we can be deceived by our senses. ... If we cannot always trust our senses, how can we ever know anything for certain about the world? ... A branch of epistemology that has come into vogue in the last 10-15 years is the problem of consciousness. ... What relationship is there between our conscious experience and the true nature of the physical world? ...

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... Are HVCs a common feature of star forming galaxies? ... Consider the typical properties of the smallest HVCs (compact HVCs) found in HIPASS: . Distance . HI Mass . ... At 5 kpc . meager objects ~116 solar masses . ... 1.15 x 10 4 solar masses . ... Putman et al. (2003) found none to 10 7 solar masses. 2% of Sculptor to 3 x 10 6 solar masses by de Blok et al. (2001) found none. ... High velocity gas around other galaxies can be identified from maps and dynamics: . ... 2003) . ...

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• ALFA Front End Optics
• HIPASS Results and Lessons
• The CIMA Homepage

... The simulated image is shown in Fig. ... The crowded region of the true object and of the restored object are shown in Fig. ... The original point spread function (PSF), a noisy estimate of the PSF taken from the lower right region of the data, and the PSF estimate are shown in Fig. ... The PSF estimate was obtained by estimating the point-by-point phase errors due to the telescope's aberrations and using these errors to create a predicted PSF. rlw@sundog.stsci.edu . ...

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• WFIRST Tools Server
• NICMOS Proposing Example - 3
• Fixed Target Confirmation Chart FAQ

... Credit Copyright: Hubble Legacy Archive , NASA , ESA - Processing: Jos Jim nez Priego Explanation: Dwarf galaxy NGC 5195 is best known as the smaller companion of spiral M51, the Whirlpool galaxy . Seen together they seem to trace the curve and dot of a cosmic question mark , recorded in Lord Rosse's 19th century drawings as one of the original spiral nebulae. Dwarfed by enormous M51 (aka NGC 5194), NGC 5195 spans about 20,000 light-years. ... NGC 3310: A Starburst Spiral Galaxy . ...

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• XWare > APOD

... Classes . ... casa . casa::MCuvw . ... Private Types | ... Muvw conversion routines. ... MCuvw (const MCuvw &other) . ... getConvert ( MConvertBase &mc, const MRBase &inref, const MRBase &outref) . ... Routines to convert uvws from one reference frame to another. void . ... enum casa::MCuvw::Routes [private] . ... Conversion routine to cater for inheritance question. void casa::MCuvw::fromPole . ... Show the state of the conversion engine (mainly for debugging purposes). void casa::MCuvw::toPole . ...

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• Using SPC
• casacore: casa::LCStretch Class Reference
• VSOP Long-Term Schedule

Загрузить программу (~10 MB). ... Программа izmccd предназначена для высокоточной астрометрической обработки числовых изображений небесных объектов. Программа позволяет получать как измеренные, так и экваториальные координаты малых планет, комет, спутников больших планет, визуально-двойных звезд и других объектов, а также идентифицировать уже известные малые планеты и найти на числовых изображениях движущиеся объекты. ... Программа является бесплатной. ... Автоматическая обработка, один объект. ...

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SAI, graduates year 1982. ... Note: when just a 7-digit phone number is shown, it refers to a phone located in Moscow (international access 007-495). "+" in front of a number means that you must dial an international access code first (or just press "+" on your mobile phone keypad). ... 939-1672(work); . ... Ataev Sasha . 1-(703)-536-8881(home) (USA); . ... Bychkov Sergey . ... 1-(410)-740-8205(home), +1-(301)-286-2150(work) (USA); . ... 1-(412)-767-0332(home), +1-(412)-608-9339(mobile) (USA); . ...

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... region (region-7.5) [xmmsas_20050815_1803-6.5.0] . ... The region task takes a FITS-table list of source positions (which must be RA and dec in decimal degrees) as input and creates one or more FITS-format region tables as output. ... The region tables which the task creates conform to the ASC region specification [ 1 ]. ... Source selection . Specifying source region shapes and sizes . The contour method of calculating source region shape . ... Local-background region shapes and sizes . ...

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• Home Page

Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...

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• Background estimate by filtering
• Photon/Particle Counting Image Measurement System : PIAS-TI (Hamamatsu
• An example of selection criteria

... What is there beyond the edge of the universe? ... This is often illustrated by newspaper headlines: "Scientist sees face of God, confirms Big Bang model" (a reference to results from the Cosmic Background Explorer satellite), "Is the cosmos younger than some of the stars it contains? ... The Lone Universe . ... We cannot reproduce it; we cannot take another one and see what happens to it; we cannot compare it to anything else, as astronomers routinely do with planets, stars, and galaxies. ...

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• ASP: Sharing the Universe
• ASP's 2009 Annual Meeting
• ASP's 2011 Annual Meeting