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21. 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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22. TELEVISION CAMERA TVC
... It?s needs solution satellite?s orientation problem for defining location of sources of ionospheric emissions above Earth?s surface with necessary accuracy. There is possibility to define orientation of photometric devices by using TV images of star background. The CCD TV camera is designed for recording of images of star sky, Earth? limb and adjoining part of Earth? surface to fix the orbit point coordinates during the measurements by FAGOT and SICH-F devices. ...
[ Сохраненная копия ]  Ссылки http://space.univ.kiev.ua/projects/warning/tvc.html -- 5.0 Кб -- 15.02.2000
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23. Archeops Main Page
The Archeops experiment aimed at measuring the cosmic background emitted just after the Big Bang. The study of this radiation is essential to obtain precise information on the evolution of the Universe: density, Hubble constant, age of the Universe.. To achieve this goal, measurements have been done with devices cooled down at 100mK temperature placed at the focus of a warm telescope. ... 28960 visitors . ...
[ Сохраненная копия ]  Ссылки http://www.archeops.org/ -- 6.8 Кб -- 09.04.2016
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24. Iт??ve read about background radiation fields that fill the universe. Is the
... Cosmic Adventures . ... Iт??ve read about background radiation fields that fill the universe. Is the infrared radiation as ancient as the microwave, and are there other cosmic fields of radiation besides these two? ... ESA/Planck consortium The cosmic background radiation currently emits mainly at microwave wavelengths. ... When the universe was 1 million years old, the cosmic background was mostly infrared radiation. ... Get instant access to subscriber content on Astronomy.com! ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/magazine/ask-astro/2012/04/cosmic-backgrounds -- 63.5 Кб -- 10.04.2016
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25. Basic Properties
. Next: Spectrum Up: R Coronae Borealis Stars Previous: Historical Background . Figure 1: The light curve of RCoronae Borealis during a fading event in 1859 . RCB stars were first identified by their characteristic light curves. A part of the light curve of RCrB itself is shown in Figure 1 . Spectrum . Galactic distribution and absolute magnitudes . Numbers and distances . Simon Jeffery . 2000-03-16
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/~csj/rcrb_rev/node4.html -- 3.5 Кб -- 16.03.2000
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26. APEX/Intro
... Research . Projects . ... The name of the project APEX is a reduction from words " Active Plasma Experiments " . The core of the project are active experiments with injection of electron and (or) plasma beams from a board of the satellite with simultaneous registration of the phenomena, produced by interaction of injected beam with background plasma. ... Active experiments utilise modulated electron beam accelerator and source of modulated xenon plasma beam on the main spacecraft APEX. ...
[ Сохраненная копия ]  Ссылки http://www.izmiran.rssi.ru/projects/APEX/intro -- 9.0 Кб -- 09.04.2016
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27. Background Fluctuation Analysis from the Multiscale Entropy
Next: A New Entropy Measure Based on Multiple Resolution and Noise Modeling . ... The entropy measurement has been proposed for image restoration several years ago in astronomy. ... The multiscale entropy has the advantage to introduce a noise modeling, and the concept of information at different level of resolution. ... We show in this paper that it can also be used for background fluctuations analysis. ... Five simulated images were created by adding 400, 200, 100, 50, 0 sources to a noisy image. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass98/rgastaud/ -- 17.6 Кб -- 16.07.1999
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28. Trigonometry--what it is good for?
... Sighting the telescope, first at the tree and then at pole B, you measure the angle A of the triangle ABC, equal to the difference between the numbers you have read from the azimuth plate.. ... Why triangles? ... One large surveying project of the 1800s was the " Great Trigonometric Survey " of British India. ... Everest was the one who commisioned and first used those giant theodolites; they are now on display in the Museum of the Survey of India in Dehra Dum. ... Everest . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/magbase/REFMAN/STARGAZE/Strig1.htm -- 9.4 Кб -- 11.03.1999
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29. http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf
Microsymposium 34, MS058, 2001 ANOMALIES OF THE MOON'S THERMAL EMISSION IN THE IR SPECTRAL RANGE (10.5 - 12.5 micron). ... Sternberg State Astronomical Institute, Moscow, 119899, Russia, pugach@sai.msu.ru Summary: New satellite measurements of the lunar-surface radiation temperature were used to construct the spatial angular function of thermal radiation of the Moon in the infrared (10.5-12.5 micron) spectral range. ... These thermal anomalies are observed only in the limited range of phase angles. ...
[ Текст ]  Ссылки http://selena.sai.msu.ru/Pug/Publications/ms34/MS058.pdf -- 568.0 Кб -- 06.10.2008
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30. CHIANTI atomic database
... References: %Observed energy levels (1 - 10): Edlen, 1983, Ph. ... 28, 51 % Observed energy levels (4,5): Feldman, Curdt, Landi , Wilhelm, 2000, ApJ, 544, 508 % Observed energy levels (11): from the spectrum of Acton et al 1985, ApJ, 291, 865 % Observed energy levels (12 - 16,25 - 26): Doschek et al 1973, J.Opt.Soc.Am, 63, 1463 % Observed energy levels (2s2.2p3.3d configuration): Fawcett Hayes, 1975, MNRAS, 170, 185 %theoretical energy levels : Landi , E., ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/chianti/chianti_5.1/database/ca/ca_13.html -- 5.3 Кб -- 15.09.2005
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31. Experiment COLD: Astrophysical Problems Studied in Experiment Cold
Experiment COLD . ... High-Latitude Background Emission . Only the narrow band of the Milky Way near b II = 0 o has been studied at centimeter wavelengths; even here, the most sensitive surveys of the Milky Way have gaps toward the anticenter. ... The right ascension where the band of sky studied comes closest to the Galactic Pole is indicated by the arrow labelled NP. the Milky Way: we detected background emission toward the anticen-ter for the first time, near the radio source W16. ...
[ Сохраненная копия ]  Ссылки http://mavr.sao.ru/hq/CG/cold/part8.htm -- 22.6 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://www.sao.ru/hq/CG/cold/part8.htm -- 22.6 Кб -- 24.02.2010
[ Сохраненная копия ]  Ссылки http://jet.sao.ru/hq/CG/cold/part8.htm -- 22.6 Кб -- 24.02.2010
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32. sune
The Star called the Sun. The Sun as the star . ... The visible star value . ... Spectrum class . ... 149 597 870 km . ... The Solar energy sourse is the core transformation of the Sun, where temperature is 15 000 000 K. The energy from inside is carried by irradiation and then in the external layer with 0,2 Ra of thikness - by convection. ... The Earth, situating far from the Sun (149 mil km), receives about 2.1017 W of the Solar beam energy (see item "The Solar constant" ). ...
[ Сохраненная копия ]  Ссылки http://www.space.vsi.ru/sune.htm -- 6.1 Кб -- 14.10.2000
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33. Trigonometry--what it is good for?
... Sighting the telescope, first at the tree and then at pole B, you measure the angle A of the triangle ABC, equal to the difference between the numbers you have read from the azimuth plate.. ... Why triangles? ... One large surveying project of the 1800s was the " Great Trigonometric Survey " of British India. ... Everest was the one who commisioned and first used those giant theodolites; they are now on display in the Museum of the Survey of India in Dehra Dum. ... Everest . ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/mirrors/stern/stargaze/Itrig1.htm -- 9.1 Кб -- 18.07.2004
[ Сохраненная копия ]  Ссылки http://www.cosmos.ru/mirrors/stern/stargaze/Itrig1.htm -- 9.1 Кб -- 22.12.2007
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34. MILLIMETRON
... The project assumes creation of an international space observatory - the interferometer "Earth - Space - Space" in order to perform of astronomical investigations in millimeter, submillimeter and infrared regions with extremely high sensitivity (to a few nanoJanskies units of flux density in continuum spectrum) and extremely high angular resolution (to a parts of microsecond of arc or, possibly, nanosecond). ... radio-interferometric channels of the system "Space - Space", region 0.2 - 3 mm; . ...
[ Сохраненная копия ]  Ссылки http://www.asc.rssi.ru/submillimetron/mm/default.htm -- 10.5 Кб -- 05.04.1999
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35. Cool Ideas Krill - an Astronomy Net Blackholes2 Forum Message
Blackholes2 Forum Message . Forums: . ... Discussion Forums | ... Cool Ideas Krill . Forum List | ... Post Message | ... But we see it with a narrower diameter, due to bending of light at great distances by mass (like Einstein's idea of large mass bends light). ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.net/forums/blackholes2/messages/4924.shtml -- 20.5 Кб -- 09.04.2016
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36. Phil Plait's Bad Astronomy: Misconceptions
... Bad Astronomy . ... Bad Astronomy : The seasons are caused by the change in the distance of the Earth to the Sun. ... The change in distance of the Earth to the Sun is a very minor player. ... Well, not completely wrong; certainly the Earth's distance from the Sun has something to do with the temperature, but it is a relatively minor effect. ... Basically, the temperature depends only weakly on distance changes; the temperature goes as the inverse square root of the distance of the planet to the Sun...
[ Сохраненная копия ]  Ссылки http://www.badastronomy.com/bad/misc/seasons.html -- 28.4 Кб -- 09.04.2016
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37. http://xray.sai.msu.ru/~polar/sci_rev/0910.html
... Authors: The LIGO Scientific Collaboration, the Virgo Collaboration . arxiv:0910.5253 Первое точное определение параллактического расстояния до черной дыры (The first accurate parallax distance to a black hole) . ... SDSS 1257+5428: близкий массивный двойной белый карлик с нейтронной звездой или черной дырой в качестве компаньона (First Results from the Swarms Survey. SDSS 1257+5428: A Nearby, Massive White Dwarf Binary with a Likely Neutron Star or Black Hole Companion) . ...
[ Сохраненная копия ]  Ссылки http://xray.sai.msu.ru/~polar/sci_rev/0910.html -- 3.9 Кб -- 02.11.2009
[ Сохраненная копия ]  Ссылки http://astro.uni-altai.ru/astro-ph/0910.html -- 3.9 Кб -- 27.02.2014
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38. Running processes as background jobs
To run a process in the background as a job and carry on working add an (ampersand) at the end of the command line. ... The shell forks a child process to run the command and displays the job number ( [ n ] ) and the PID (Process IDentifier) number. ... If the command is likely to produce error messages you will need to redirect standard error. ... Do not run an interactive command that requires you to type something at the terminal as a background job. ... You will then have to kill its process . ...
[ Сохраненная копия ]  Ссылки http://comet.sai.msu.ru/UNIXhelp/shell/jobz2.html -- 2.7 Кб -- 17.01.1997
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39. EDM (ImageJ API)
... public class EDM . ... Euclidean Distance Map: The value of each pixel is the distance to the nearest background pixel (for background pixels, the EDM is 0) - Ultimate Eroded Points (UEPs) are maxima of the EDM. ... static int . ... Unit in old make16bitEDM: this pixel value corresponds to a distance of one pixel. static int . ... int . ... For compatibility with previous versions of ImageJ only. public FloatProcessor makeFloatEDM ( ImageProcessor ip, int backgroundValue, boolean edgesAreBackground)...
[ Сохраненная копия ]  Ссылки http://www.astro.louisville.edu/software/astroimagej/imagej/api/ij/plugin/filter/EDM.html -- 31.4 Кб -- 02.12.2010
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40. On current distance scales for open clusters
... In 1930, Trumpler noticed that linear diameters (LD) of open clusters increase with distance (D) from the Sun. ... Since that time, the interstellar absorption has become one of the best studied factor in astrophysics, and we may hope that current OCL distance scales are free from this LD-D correlation. To verify if this is the case we have chosen several modern OCL distance scales and test them with the same clusters and the same angular diameters that Trumpler had used back in 1930. ...
[ Сохраненная копия ]  Ссылки http://www.inasan.rssi.ru/~dwiebe/abstracts/dist.html -- 4.2 Кб -- 27.09.2012
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