The computed band passes. ... The interim correlator input is filtered by 8 analog filters (50 Mhz wide at the 260 Mhz IF... one for each sub correlator). ... For bandwidths of 25 Mhz and below the real data stream is digitally down converted to complex samples I, Q streams. ... The Top figure is the halfband filter bandpass computed from the filter coefficients. ... The computed filter has aliased power, extra IQ filtering, and two applications of the filter on the resulting real bandpass. ...

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• Polyphase Filter Bank
• pdev_birdies_25jun07
• lowpass digital fitlers

Laboratory work N7 Low-pass filtering. 1) Generate the signal with two periodic components and high-frequency noise. ... 2) Perform it's filtering with Panteleev filter 0 - h(t) = e 22 0 |t| 2 0 t 0 |t| cos + sin 2 2 , where 0 is a parameter. The frequency response of the Panteleev filter is ^ h( ) = 4 0 . 4 0 + 4 Select the cut-off frequency (by varying 0 ) for filtering out high-frequency periodic component and noise. 3) Plot the initial and filtered signal. ...

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... Directives | ... Apache HTTP Server Version 2.4 . ... ext_filter_module . ... mod_ext_filter directive to define a filter # to HTML-ize text/c files using the external # program /usr/bin/enscript, with the type of # the result set to text/html ExtFilterDefine c-to-html mode= output \ intype=text/c outtype=text/html \ cmd = /usr/bin/enscript --color -W html -Ec -o - - Directory /export/home/trawick/apacheinst/htdocs/c # core directive to cause the new filter to # be run on ...

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• mod_sed - Apache HTTP Server
• The ALMA project
• mod_filter - Apache HTTP Server

... Figure 1 shows some synthetic test data u(n) to which random noise v(n) is added. ... for the above simulations % % % % % Explore the use of eigenanalysis techniques in post detection digital signal processing for noise rejection Potential application include spectroscopy and imaging Jon Bell 24 Jul 2000 clear % Make some fake raw data nspec = 120 ; ntime = 10; scale = 1.0; noisescale = 1.0; dcoff = 0.0; psi =1.0; j=1:1:nspec; k=1:1:ntime; rawdata = sin(j/3) + sin(j/5) + 1; rawdata = ( ...

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• http://www.atnf.csiro.au/management/atuc/2011oct/science_meeting/docs/trott_FT_v3.pdf
• http://www.atnf.csiro.au/research/electronics/docs/dfc/DFCHandout.pdf
• Index

We have designed the laboratory model of static Fourier spectrometer for onboard usage for spectral study of atmosphere and ionosphere. The gain of model is to simulate onboard FS which will not have any moving elements (all its optical elements will be mounted at fused quartz monolithic construction), to compare experimental results with theoretical estimations and to measure MTF of CCD array. ... This fact connected with low frequency response of CCD array due to small format of it. ...

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• A computer controlled low light photometer for nightglow observations

... Judged by their instrumental profiles, spectrometers fall into two basic classes---Lorentzian and Gaussian---with many other line profile functions (sinc functions, Voigt functions, Airy functions, etc.) falling into one of these two categories in some limit. We demonstrate that the Rayleigh, Sparrow, and Houston resolution criteria are of limited use compared to the ``equivalent width'' of the line profile. ... Rayleigh criterion. ... All of these functions have continuous higher derivatives. ...

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• Improvements in Filter Design for Removing Galactic ``Cirrus'' from IRAS Images
• ADASS 2003 Conference Proceedings
• An Extragalactic Point Source Simulator for SIRTF Pipeline Testing

Monte Carlo Methods for Including Calibration Uncertainties in Model Fitting Analyses Jeremy J. Drakea , Peter Ratzlaffa , Vinay Kashyapa , Richard Edgara , Rima Izemb , Diab Jeriusa , Herman ... University, Cambridge, MA 02138 MIT Kavli Institute for Astrophysics and Space Research, Cambridge, MA 02139 b c SUMMARY · Instrument response uncertainties almost universally ignored in astrophysical X-ray ... Limiting accuracy of Chandra ACIS reached in spectra with 10 4 counts. ...

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• Quantum Efficiency Correction (a.k.a. `flat-fielding')
• Combining Region and Table Filters
• Filtering ROSAT HRI data on the basis of background level

This library currently provides subroutines used to transform theoretical spectra to intermediate and broad-band photometric indices. ... Typical tasks are the response functions and transmission curves for various filters, mirrors and photomultiplier windows. ... The response is zero outside the given wavelength range. ... real . input . Wavelength in nanometres . PHOT_1P21 . ... PHOT_AIR . ... PHOT_ALUM . ... Inputs must be valid as for PHOT_FILTER, PHOT_AIR, PHOT_ALUM and PHOT_1P21. ...

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• Armagh Observatory
• Gary, Callum and Peter: `Stars' of the Future
• R-N Expression of Risk

... In doing so, the filter also reads all of the RTF markup that specifies the destination, paragraph and text styles of the next character. ... If the text was not SPECIAL, process the paragraph style
. ... Using the HTML paragraph" markup name, the filter (using the .PTag table) knows what tags to generate for the text. ... For each matched entry in the .TMatch table, the filter uses the HTML "text" markup name, the filter (using the .TTag table, see 5.1.2 ) knows what tags to generate for the text...

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• rtftohtml Users Guide - 4 Special Processing

Part II Physics May 2004 EXAMPLES CLASS ­ SYSTEMS 1. The input function u(t) of a linear system is related to its output y(t) by the differential equations. (x(t) being an internal variable.) y=u­x x = 5y + 6y ­ u Derive the transfer function of the system H(s) = Y(s) / U(s) and deduce (from a partial fraction expansion) the response of the system to (a) a unit impulse (0) and (b) a unit step [U(s)) = 1/s]. ... Find the values of K for which the system shown is stable. ...

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• http://www.mrao.cam.ac.uk/~rachael/systems/Problem%20Sheet%202004.pdf
• http://www.mrao.cam.ac.uk/~bn204/lecture/2008/bn-l8.pdf

... To overcome this limitation we propose Cryogenic Phase Locking Loop (CPLL).The CPLL has been developed for phase locking of a Flux-Flow Oscillator (FFO) in the SIR. ... The CPLL operating frequency has been increased from 400 MHz up to 4 GHz to decrease a loop filter delay to 0.5 ns. ... We have realized an integrating loop filter for the CPLL. ... Phase noise of the FFO phase-locked with: "1" ­RT PLL; "2" ­ CPLL without integrating loop filter; "3" - CPLL with integrating loop filter. ...

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• Atmospheric influence on the different radioengineering systems functioning.
• Project 5 - State Program "Condenced Matter Physics"

.

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• Comparing AO Techniques | ESO
• Comparing AO Techniques | ESO Ireland
• Comparing AO Techniques | ESO Australia

... Meade Series 4000 Nebular Filters incorporate the very latest in interference coatings technology. ... Technical Basis of the Meade Broadband Nebular Filter: As shown in the transmission graph below, the Meade Broadband Nebular Filter strongly rejects the light of sodium- and mercury-vapor lights as well as natural airglow and auroral emissions. ... Meade Series 4000 Narrowband Nebular Filters . ... Meade Series 4000 Oxygen-III Nebular Filters . ... Meade Series 4000 Photo-Visual Color Filters . ...

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• Blocking Filters - Coronado€о Solar - Products
• Coronado 5mm Blocking Filter - Blocking Filters - Coronado€о Solar - Products
• Coronado 10mm Blocking Filter - Blocking Filters - Coronado€о Solar - Products

RTT150 . ... This search system is designed for generating the necessary information on series of pointings (observations of each source consist of sets of exposures with different filters and sometimes with different exposure times) for observed sources. Search results appear at the separate page as a table with the following data: . DATE - real (not evening!) observations date (in YYYY-MM-DD format); . ... Bin - minimal CCD binning mode (may vary during the observations); . ...

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... Colorful Clouds Of Carina . ... Credit: Hubble Heritage Team ( AURA / STScI / NASA ) Explanation: Tumultuous clouds of the Carina Nebula , 8000 light-years away, glow in planet Earth's southern sky . Striking and detailed, this close-up of a portion of the famous nebula is a combination of exposures through six different filters taken with the Hubble Space Telescope 's Wide Field Planetary Camera 2 in April of 1999. ... NASA Official: Jay Norris. ... Colorful Clouds Near Rho Ophiuchi . ...

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• Journal "Peremennye Zvezdy"
• Астронет > Colorful Clouds Of Carina
• An Orion of a Different Color

XEphem Forum Message . Forums: . ... God and Science ћ SETI ћ Software ћ UFO ћ XEphem . ... Post . ... Re: Re: Filter Based On Catalogs? Forum List | ... Post Message | ... www.astronomy.net . About Astronomy Net | Advertise on Astronomy Net | ... Unless otherwise specified, web site content Copyright 1994-2016 John Huggins All Rights Reserved . Forum posts are Copyright their authors as specified in the heading above the post. "dbHTML," "AstroGuide," "ASTRONOMY.NET" & "VA.NET" . ...

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• Re:Suggestions For Light Pollution Filters Wanted - an Astronomy Net Eyepieces
• Re: Filter Based On Catalogs? - an Astronomy Net XEphem Forum Message
• Colour Filter On A CCD - an Astronomy Net CCD Equipment and Techniques Forum

S AO's New Generation Multipurpose CCD Controller . ... In the 1990?s considerable advances have been made in the world over technology of manufacturing scientific image detectors with high photoelectric characteristics, which called for the creation of new complex array controllers to operate such detectors. ... very low readout noise; . ... Quite a few teams of researchers and engineers are ingaged in the development of controllers. ... development, SPICE modelling and design of modules; . ...

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• SCORPIO-2 project: filters
• Work Scan Program + Data Viewer (IDL widget)
• LSVFO: SCORPIO filters

. In this picture, three different filters (r' i' and z') have been combined to show how the quasar (indicated by the arrow) is very red compared to stars or galaxies in the field. The intense red color is a good indicator that the object is a very distant quasar. Provided by CFHT

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B68BEC815-22B6-4200-BE17-7823AB0C3101%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC448C87-91C7-49F7-9E5F-73EDE0187D95%7D

... Information about a variety of different calendars for different cultures (e.g., Christian, Jewish, Muslim, Chinese, Hindu etc.) ... In addition, the Chinese had two different ways of interpreting and observing celestial events. One way the Chinese used astronomy was known as lifa; it was a discipline that aimed to understand the regularities and the predictable events in the celestial system through careful, observations, measurements and records. ... back to Teachers' Newsletter Main Page ...

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• ASP: Beacons in the Gloom
• ASP: Making a Rainbow
• ASP: Good Astronomy Activities on the WWW

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...

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