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http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node138.html.
http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node138.html.
1. The AstroStat Slog Blog Archive my first AAS. VI. Normalization
... Archives . ... One realization of mine during the meeting was related to a cultural difference; therefore, there is no relation to any presentations during the 212th AAS in this post. ... I cannot cover all perspectives from both disciplines but I think there are two distinct fashions in practicing normalization. $$\frac{1}{N(\theta)}\int_{\Omega} f(x;\theta)dx=1$$ . ... This is my last posting on my first AAS . Tags: AAS , measure , measure theory , normalization , PDF , pmf . ... Chandra Blog . ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/my-first-aas-normalization/index.html -- 22.6 Кб -- 01.03.2014
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2. AGN SED/colour simulations
... Use SEDs of various AGN and normal galaxy types, spanning the whole range (from X-rays to radio-wavelengths) that the GOODS data will cover. ... Randomize the magnitude (for m(3mum) lt 19 ), the redshift (for 0.01 lt z lt 2 or 4 ) and the SED type creating a fake catalog of 1000 "observed" galaxies. ... In Figures 4 , 5 , 6 and 7 I show various colour-colour plots, using the same symbols as before for the different SED types: RL: x, RQ: squares, Sy1: triangles, Sy2: diamonds, SB-low: +, SB-high: *. ...
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Ссылки http://www.stsci.edu/ftp/science/goods.save/Internal_old/Work/AGN_sims/ -- 7.8 Кб -- 07.11.2001
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3. APOD: 2005 August 8 - Mars to Appear Normal this August
... 2005 August 8 . Mars to Appear Normal This August . ... Regardless of numerous urban legends circulating, Mars will appear relatively normal in August. October is the best month to see Mars this year. ... As Earth catches up to Mars in their respective orbits around the Sun, Mars will keep rising earlier in the night. On 2005 October 30, Earth will have caught up to Mars and the planets will be the nearest to each other in their orbits -- this time around. ... About APOD | ...
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Ссылки http://www.sai.msu.su/apod/ap050808.html -- 5.8 Кб -- 02.10.2012
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4. Pre-processing the spectra
... Observation pre-processing consists of standard bias, dark and flat-field corrections. The package provides different commands to average images, extract sub-images or normalize flat-fields. General information related to preprocessing commands is available in the section Dark, Bias and Flat-Field of SHOW/LONG and can be obtained by: . ... The command PREPARE/LONG extracts sub-images. ... The command processes a catalog by default or an image if the name is provided with the extension .bdf . ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/94NOV/vol2/node507.html -- 5.6 Кб -- 23.02.1996
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5. Atmospheric influence on the different radioengineering systems functioning.
Atmospheric influence on the different radio-engineering system functioning . ESTIMATION OF ATMOSPHERIC OPTICAL CHARACTERISTICS AND REMOTELY SANSED IMAGE CORRECTION . ... Direct transmittance estimation results for 12 channels of the spectrometer CHRIS. ... We have managed to develop a direct method of estimating the discrete Normalized Atmospheric Point Spread Function (NAPSF) from available images alone, not using any external sources of information about the atmosphere. ... IRE RAS 1996-20 11 ...
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Ссылки http://www.cplire.ru/html/atm/correction.html -- 19.8 Кб -- 18.10.2011
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6. Normal star evolution
... We consider stars with a constant (solar) initial chemical composition. Before the Roche lobe overflow, the components evolve as single stars (see for details LPP96). ... If the mass transfer onto a normal star occurs on a time-scale ten time shorter than the thermal Kelvin-Helmholz time for this star or a compact star is engulfed by a giant companion (e.g. as a result of the kick), the common envelope (CE) stage of the binary evolution is set in (Paczynski 1976). ...
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Ссылки http://xray.sai.msu.ru/~polar/sceintro/poster/be_inwww/node3.html -- 3.9 Кб -- 21.06.1996
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7. http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/multitone_phasecal.pdf
... This memo describes a new mode , called multitone mode , which introduces new capabilities, as well as incorporating most of the functionality of the 3 previous modes. mode normal manual description any single tone extracted by corr. hardware each channel 's phase is manually specified pcal phase for a single tone is extracted and applied independently for each AP advantages simplicity disadvantages poor snr due to ignored ...
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Ссылки http://www.atnf.csiro.au/vlbi/dokuwiki/lib/exe/fetch.php/difx/multitone_phasecal.pdf -- 212.4 Кб -- 28.03.2011
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8. Interacting Electrons in Normal Metals
... MIPT Solid State Physics Department . ... Interacting Electrons in Normal Metals . ... The course is an introduction to interacting Fermi-particle physics and intended for future experimentalists. ... Hartree-Fock approximation. ... Linear reaction function. Calculation of density-density reaction function. Relation of density-density reaction function to compressibility of Fermi liquid and thermodynamic state density. ... Density-density reaction function of free Fermi gas in long-wave limit. ...
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Ссылки http://www.issp.ac.ru/engl/education/miptsspd/53-interactingelectronsinnormalmetals- -- 17.3 Кб -- 10.04.2016
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9. FORS1: Sky Flats and Rotator Effect
Median Twilight Image . all frames normalized by their median before averaging and corrected for 4-port structure) . Median of Normalized Twilight Images at Rotator Angle 0 . Median of Normalized Twilight Images at Random Rotator Angle . Time Frame and Rotator Angle Distribution . B_UT2_2CCD: 134 frames . ... distribution of rotator angles) . U_UT2_2CCD: 106 frames . ... uncorrected median twilight image) . B_UT2: 298 frames . ... U_UT2: 246 frames . ... B_UT3: 266 frames . ...
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Ссылки http://www.eso.org/~smoehler/FORS_ROT/FORS1_ROT.html -- 10.7 Кб -- 04.06.2009
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10. sfit help file
... SFIT is a general-purpose code designed to optimize theoretical stellar spectra to an observed spectrum. ... While the programme expects input from "stdio", it is more natural to save commands in a file (eg "sfit_input") and run the code simply by . ... If the spectra to be fitted have a filename "star_spectrum", then the best fit spectrum will be written out, together with the renormalized input spectrum, to a file called "star_spectrum.fit". ... sets up model spectrum grid (and for 2nd star) . ...
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Ссылки http://star.arm.ac.uk/~csj/software_store/guide/sfit2_help.html -- 7.6 Кб -- 18.10.2004
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11. Feature enhancement: normalizing
Next: Feature enhancement: local Up: No Title Previous: Feature enhancement: filtering . ... As a result, a common magnitude scale (contour lines on the maps above, or color scale on Fig.1) will poorly display the short-duration events in a signal. Normalizing each line of the map (fixed duration) so it has unit variance (in effect dividing the energy map by the mean energy spectrum) at each duration restores more details of small-scale activity (Fig. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Tutor.dir/node20.html -- 3.2 Кб -- 12.04.1998
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12. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/marshall-cal-2012.pdf
HETGS Update and ACIS Contamination Herman L. Marshall (MIT Kavli Inst.) ... 7, 2012 HEG-MEG Comparison 30 Blazar Observations Used NEW Version 10% correction needed consistent with MEG-LETG cross-cal H. Marshall -- Chandra 2 /26 EPIC BOC 2012 Correcting HETGS Ratio H. Marshall -- Chandra 3 /26 EPIC BOC 2012 Correcting HETGS Ratio H. Marshall -- Chandra 3 /26 EPIC BOC 2012 Correcting HETGS Ratio H. Marshall -- Chandra 3 /26 EPIC BOC ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201203/marshall-cal-2012.pdf -- 2898.0 Кб -- 13.05.2014
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13. ASP: What If the Moon Didn't Exist?
... I normally begin by asking the class what they think would be different if the Moon didn't exist, or if the Sun were closer to Earth, or if a star exploded nearby. ... The winds would be much stronger. ... In using what-if questions in the classroom, it is worth bearing in mind that students extrapolating the effects of new scenarios will encounter two different situations: direct changes to the new version of Earth and indirect changes resulting from the direct changes. ...
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Ссылки http://www.astrosociety.org/edu/publications/tnl/33/moon3.html -- 11.2 Кб -- 02.10.2012
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14. Amateur Telescope Makers of Boston
... Submitted by Paul Cicchetti on 05/31/2013 17:03:24 . NGC 4214 . This is a combined image of 20 Luminance, 5 Red, 5 Green, and 5 Blue. ... This was at F18 (2x Powermate barlow), different from my normal F9 of the 6"APO's prime focus. Images were processed in CCDStack and combined and processed in PS CS5. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...
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Ссылки http://www.atmob.org/gallery/showimage.php?id=2394 -- 3.1 Кб -- 10.04.2016
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15. http://www.naic.edu/~astro/NSFSR/NSF-AST%20Draft%20Metrics%20for%20Facilities.pdf
... Should be broken out by telescope within a facility.) ... Should be broken out by telescope within a facility.) - # programs allocated time number of programs with non- staff PI's number of programs with observatory staff as PI's number of thesis programs number with U.S. PI's number with foreign PI's information on geographic distribution - # states, # institutions, characterization of institution (R1, PUI, etc), if information ...
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Ссылки http://www.naic.edu/~astro/NSFSR/NSF-AST%20Draft%20Metrics%20for%20Facilities.pdf -- 19.8 Кб -- 13.07.2005
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16. Bojan Nikolic -- How to make an image in PGPLOT with correctly labelled RA/Dec
... Bojan Nikolic web pages home . ... The goal here is to make a publication quality image of the sky with the coordinates labelled in the standard Right Accession/Declination units. ... Use the PGTBOX function which knows how to label the coordinate box in time units . ... тАЬINTтАЭ To draw tick marks and label them (тАЬIтАЭ so that the ticks are inverted, i.e., going outside the box) . ... Ensure that the matrix representing the coordinate system of the image is correct when calling PGIMAG . ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/blog/2012/04/01/pgplot-ra-dec-box.html -- 5.3 Кб -- 05.10.2015
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17. Кресло MESTRE - Roomble - Roomble Normal Waist тренировочные брюки
... Кресла . ... Размер: XS . ... Цвет: белый . ... Размер шлица: PZ2 ; . ... Цвет: Фиолетовый . ... Глубина: 90 . ... Цвет: черный . ... Цвет: серый . ... Размер INT: 54 . ... Глубина пропила: 90, . ... Макс. глубина пропила под углом 90њ: 90, . ... Размер площадки: 800x550, . ...
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Ссылки http://astrokuban.info/astroku7115.html -- 22.3 Кб -- 14.02.2016
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18. Mars to Appear Normal this August
... Mars to Appear Normal this August . ... October is the best month to see Mars this year. ... As Earth catches up to Mars in their respective orbits around the Sun, Mars will keep rising earlier in the night. On 2005 October 30, Earth will have caught up to Mars and the planets will be the nearest to each other in their orbits -- this time around. On October 30, Mars will be nearly opposite to the Sun, rise at sunset, set at sunrise, and appear highest and brightest around midnight. ...
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Ссылки http://www.astronet.ru/db/xware/msg/1207539 -- 14.8 Кб -- 08.08.2005
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19. East Siberian Center for the Earth's Ionosphere Research. SW radiosignal
Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... The algorithm and appropriate program for decametric radiosignal propagation conditions prediction for paths from 500 to 9000 km have been developed at ISTP SB on the basis of normal wave method (AltyntsevaB.I,Iliyin N.V., Kurkin V.I. and others //Decameters channel simulation on the base of normal wave method . ... Solar activity indices are chosen automatically from the prediction date from the database . ...
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Ссылки http://rp.iszf.irk.ru/esceir/lchmen/predicten.htm -- 8.0 Кб -- 02.06.2001
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20. Procedures for Data Reduction
The main steps in the reduction of NIR spectroscopic data are flat-field correction, subtraction of sky emission, wavelength calibration, correction for telluric absorption and correction for optical system plus detector efficency. ... Sky subtracted frames are corrected computing analitically the tilt angle from the instrumental calibration parameters or directly measuring it from the data. ... The same procedures are applied to the reference stars frames to obtain the calibration spectra. ...
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Ссылки http://www.arcetri.astro.it/irlab/instr/longsp/doc/proc_dr.html -- 4.7 Кб -- 16.02.2000
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