... Submitted by Paul Cicchetti on 01/29/2012 18:21:17 . M42 using ST-8300 . Another test with the ST-8300 and filters (LRGB). Combined image from L is 15 of 2min, R is 10 images at 3 min, G 10 at 2 in, and B is 10 images at 2 min. ... Processed through CCDStack and then further processed in Photoshop CS5. ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

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... Apache HTTP Server Version 2.2 . ... This document describes the use of filters in Apache. ... The Filter Chain is available in Apache 2.0 and higher, and enables applications to process incoming and outgoing data in a highly flexible and configurable manner, regardless of where the data comes from. ... A wider range of applications are implemented by third-party filter modules available from modules.apache.org and elsewhere. ... There are two ways to use filtering: Simple and Dynamic. ...

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• mod_sed - Apache HTTP Server
• mod_xml2enc - Apache HTTP Server
• mod_reflector - Apache HTTP Server

... Posts tagged ?particle filter? ... Astronomers have developed their ways of processing signals almost independent to but sometimes collaboratively with engineers, although the fundamental of signal processing is same: extracting information. ... This particular issue of IEEE signal processing magazine may shed lights for astronomers interested in signal processing and statistics outside the astronomical society. IEEE Signal Processing Magazine Jul. ... ArXiv] 3rd week, Dec. ... Entries RSS . ...

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• The AstroStat Slog Blog Archive [MADS] Adaptive filter
• The AstroStat Slog Blog Archive [MADS] Kalman Filter
• The AstroStat Slog spatial statistics

... omichain (omichain-1.50) [xmmsas_20070708_1801-7.1.0] . ... The omichain then cycles through each filter in the filter list and processes each exposures in the exposure list for that filter. ... First it checks to see if the exposure is a full-frame low resolution mode, and if so it runs omcomb to combine the four separate image segments into a single full-frame image, which is then processed instead of the individual image segments. ...

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• Comments
• Stage Three: ``filter''

Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Telescopes and Observatories . ... The majestic star-forming region in the Lagoon Nebula. The pale ring to the right is an internal reflection in the telescope.€а (Image credit: ESO/ VPHAS+/ V. Kalari and J. Vink (Armagh Observatory) . ... The 18 component images were further processed twice. ... Venu and his colleagues use images like this to identify individual young forming stars in the Lagoon Nebula and determine their ages. ...

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... ESO is building what will be the World's largest optical telescope array, The Very Large Telescope (VLT). The VLT Project organisation is responsible for the design and construction of the Unit Telescopes, including enclosures, optics, adapter-rotators and coating unit. ... Unit Telescopes Overview - This page is outdated, an update is in process. ... Secondary mirror (M2 Unit) - This page is outdated, an update is in process. ... Coating Unit - This page is outdated, an update is in process. ...

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• Operations with DFOS: daily workflow, the simple model
• Basic CCD image processing
• ESO - A number of OmegaCAM filters show vignetting in their central regions.

WFC3 Instrument Handbook for Cycle 24 . ... Wide Field Camera 3 Instrument Handbook for Cycle 24 > Chapter 2: WFC3 Instrument Description > 2.3 Spectral Elements . ... 2.3.1 The Filter Selection Process . ... Both WFC3 channels are equipped with a broad selection of spectral elements. ... The UVIS channel has a selectable optical filter assembly (SOFA) that contains a stack of 12 filter wheels housing a total of 48 elements: 42 full-frame filters, 5 quad filters, and 1 UV grism. ...

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• Flat Fields
• WFPC-2 ETC Help
• ramp_optimal_filter.pro (JWST Pipeline routines in IDL)

For the calibration of RATAN-600 data you will need to Download Nobeyama Fluxes (1, 2, 3.75, 9.4, 17 GHz): year 1999 2000 2001 2002 2003 . Brief description of Work Scan . Main functions of processing, realized in the program are: . ... Correction of various (not fatal) defects of data; . ... Calculating of the lower enveloping curve or an average scan from observations data for a few days; . ... COMMENT This table contains the set (TFIELDS) of 1-dimensional (TFORM# . ... AZIMUTH = 'float' / . ...

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• Приложение B. Requests for Comments (RFC), связанные с информацией приведенной

... Apache HTTP Server Version 2.2 . ... This document describes the use of filters in Apache. ... The Filter Chain is available in Apache 2.0 and higher, and enables applications to process incoming and outgoing data in a highly flexible and configurable manner, regardless of where the data comes from. ... A wider range of applications are implemented by third-party filter modules available from modules.apache.org and elsewhere. ... There are two ways to use filtering: Simple and Dynamic. ...

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• The Wiener-like filtering in the wavelet space
• Hierarchical Wiener filtering
• Artifacts

. unfiltered . GGM02C model . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 . PC 1 . PC 2+3 . PC 2 . PC 3 . PC 4 . PC 5 . Sum of nine first PCs 2-10 . Difference between the initial signal and ten first PCs 1-10 .

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• Fulbright scholar Leonid Zotov
• Leonid Zotov

... A test was done with the alfa filter bank on 07dec11 to see how well the filter bank settled. ... This centered the high freq band at 1450 MHz. The low freq band at 1300 MHz was not used for the test. ... While the mock spectrometers were taking data, the alfa filterbank was switched between the wide band filter (300 MHz) and the narrow band filter (100 MHz centered at 1440 MHz). ... The alfa filter has has trouble switching between narrow band and wide band observing for most of the alfa beams. ...

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• pdev_birdies_25jun07
• GALFA Documentation
• Notes on Low-Pass Filter Coefficients

You can also see this page in Russian with using KOI8 (X Windows) or CP1251 (MS Windows) Cyrillic coding. The Laboratory supports the space TV experiments, mainly in the planetary exploration missions. ... Image Co-registration . ... PHOBOS mission - Martian satellites investigations. Phobos on the Martian limb, the image from Phobos-2 probe from 02/28/89. ... Russian Space Bulletin. ... Last modified at June,26 1997 Alexey Kuzmin: akuzmin@mx.iki.rssi.ru . Back to IKI home page ...

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• Calvin Hamilton
• Processing the "Face on Mars" Images

... Обзор LPR фильтра. Впечатления от наблюдений с LPR фильтром. ... Характеристики цветных фильтров Baader-Planetarium . Мой перевод pdf- файла о фильтрах с сайта Baader-Planetarium (379 кб) . ...

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• Baader NEODYMIUM (Moon & Skyglow) filter

... Packages that use FloatProcessor . ... Methods in ij.plugin.filter that return FloatProcessor . ... ShortProcessor. toFloat (int channelNumber, FloatProcessor fp) . Returns a FloatProcessor with the same image, no scaling or calibration (pixel values 0 to 65535). abstract FloatProcessor . ... Returns a FloatProcessor with the image or one color channel thereof. ... FloatProcessor. toFloat (int channelNumber, FloatProcessor fp) . ... Returns a FloatProcessor with one color channel of the image. ...

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• Filters (ImageJ API)
• ij.plugin.filter (ImageJ API)
• ImageMath (ImageJ API)

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Recently Acquired Images of SL9

... The filter "Lighting Effects" is a freebie that came with this program, and in my opinion is practically worth the whole purchase price all by itself. ... You can select different light sources, and combine them with texture channels to warp your image. ... Depending on how you use it, pure white is the highest point on the image, and black the lowest. ... You can adjust the brightness and spread here, or choose other types of lighting. ... Use these if your image is turning out too dark or light. ...

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• GIMP: Tips and Tricks for Creating Images
• APOD: 2001 October 11 - VDB 142 in Cepheus
• KPT#3 Brushed Aluminum.doc

adapted from Observe: Eclipses, published in 1979 by the Astronomical League and "Safe Solar Filters," by B. Ralph Chou, Sky and Telescope, August 1981) . ... Tape TWO pieces of film together into a sandwich, and tape this over the opening in the cardboard. ... The cardboard frame will act as a shade from the bright Sun, while you safely observe through the film sandwich. ... Undeveloped film is not safe. ... tape . ... At the end of one of the tubes, tape the aluminum foil, and make a tiny pinhole. ...

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ASKAP Signal Processing Overview DIFX Users and Developers Meeting Dr. Grant Hampson | ... DIFX Users and Developers Meeting | Grant Hampson | 25 Sep 12 ASKAP Differences · BETA (Eng. ... 25 Sep 12 Frequencies? ... 25 Sep 12 Why use FPGAs for Beamforming? ... 25 Sep 12 Why use FPGAs for Correlator? ... Thank you CSIRO Astronomy and Space Science Dr. Grant Hampson ADE Team Leader t + 61 2 9372 4647 e grant.hampson@csiro.au w www.csiro.au/cass CSIRO ASTRONOMY AND SPACE SCIENCE ...

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• Package: panel
• Logging CentralProcessor 0.11 documentation
• Release of 1 Aug. 1997

... 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
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M obile A stronomical Sy stem of TE lescope- R obots MASTER-II Kislovodsk Lomonosov Moscow State University, Sternberg Astronomical Institute , Moscow Union "Optic" , Kislovodsk Solar Station Latitude = 43 o љ44'.767љN; Longitude = 42 o љ31'.417љE; Altitude = 2067љm MASTERљIIљ(8љsquareљdegress) + MASTERљVWF(VeryљWideљFieldљCameras (FOV=800 square degrees, Timeљresolutionљupљtoљ150љms, with unfiltered m_lim=14m on 5 sec. exposure, and ~10.5m with 0.15 sec) . ... 11h 38m 38.0s , -09d 59m 59s) . ...

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