... GPI Data Pipeline 1.0 documentation . ... Thermal/Sky Backgrounds . ... Using Thermal/Sky Backgrounds in GPI Data Reduction: . Creating Calibrations: . ... Thermal emission (from sky or telescope) becomes an important background source for wavelengths longer than 2 microns. ... The pipeline treats thermal/sky backgrounds similar to dark frames and is designed to subtract a thermal/sky background, scaled to the integration time of the science image, from K-band observations. ...

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• COS Background Performance
• Standard Patterns for Substepping and Background Measurement
• Zodical Background and Earthshine

... Posts tagged ?background? ... Probability density functions are another way of summarizing the consequences of assuming a Gaussian error distribution when the true distribution is Poisson. We can compute the posterior probability of the intensity of a source , when some number of counts are observed in a source region, and the background is estimated using counts observed in a different region. ... In both cases a background of 200 counts collected in an area 40x the source area is used. ...

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• The AstroStat Slog background marginalization
• The AstroStat Slog background subtraction
• The AstroStat Slog Blog Archive Background Subtraction, the Sequel [Eqn]

... If requested ( runbackground =Y), the task creates a background lightcurve, as well as a background spectrum for the imaging modes (FF, eFF, LW, SW) using background masks. ... The background masks are created by task badpixfind using threshold parameters, appropriate for the detection of real X-ray sources. ... As the GTIs strongly depend on the intended science this screening is not performed and only background masks, the lightcurve, and a GTI file are created by epchain . ...

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• Background correction

Next: Bivariate polynomial interpolation Up: Echelle Spectra Previous: Removal of particle . The estimation of the background is one of the critical points in the reduction of echelle spectra for two reasons. ... diffuse light in the interorder space coming from adjacent orders. sky background spectrum . ... These locations are defined when performing the order definition (command DEFINE/ECHELLE or DEFINE/HOUGH ) and can be displayed by command LOAD/ECHELLE . ... Sky background definition . ...

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• Background Estimates
• Background Correction
• Sky background definition

... This paper describes the main algorithms used by the Einstein Level One processing to create the exposure masks and the background maps for Einstein IPC images, and how these algorithms were recreated in the IRAF environment. Our goal was to recreate the algorithms used by the Level One Processing to create exposure masks and background maps for Einstein Image Proportional Counter (IPC) data (cf. sections 2.5 and 2.7 of Harnden et al. ...

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• A Method for Minimizing Background Offset Errors When Creating Mosaics
• Background Fluctuation Analysis from the Multiscale Entropy
• Towards Optimal Analysis of HST Crowded Stellar Fields

Next: Gravitational Wave Background from Previous: Galactic Gravitational Wave Background . ... It is intuitively clear that at frequencies above the critical ones for our Galaxy, one will detect rare bright jerks produced by coalescing white dwarfs   (at a rate of 1 per 100 year) and NS (at a rate of 1 per - year) in our Galaxy, against a background of the extragalactic stochastic GW. ... Firstly we consider GWB from close individual galaxies, and then will discuss overall extragalactic GWB. ...

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• Transparency of the Stochastic Background
• Galactic Gravitational Wave Background
• Gravitational wave background from nearby galaxies

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 . ...

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• Placing a foreground process in the background
• Managing background jobs

Next: Reduce point data Up: Quick Guide Previous: Print form sheets Contents . You should reduce this data of type ``scan'' before anything else. ... Plot the background rate (four channels at a time) versus time. ... Use P ROCESS BG if you want to replace edited scans with an average value from other valid scans in the same channel. ... The reason for reducing the background data first is that average will not average the point data of a scan for which no background data exists. ...

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• ESO - Thesis Topic: Foreground emission and Cosmic Microwave background
• Vegetation on the ALMA site with Licancabur in the background
• An Ancient Cluster of Stars Against a Stunning Background

... A Year of Resolving Backgrounds . ... In X-ray light the recently launched spacecraft Chandra and XMM resolved much of the seemingly uniform X-ray background into many discrete sources, many of which appear to be black holes at the centers of galaxies accreting matter. In microwave light , the BOOMERANG and MAXIMA-1 missions resolved with new clarity the seemingly uniform microwave background . ... Publications with keywords: cosmic microwave background radiation . ... Our Dusty Universe . ...

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• The Cosmic X-Ray Background
• Астронет > The Cosmic X-Ray Background
• Chandra Resolves the Hard X Ray Background

... Gallery . ... The repainted Farnham dome with the AITC in tтАж . Sidebar Left . Sidebar Top . ... Title: The repainted Farnham dome with the AITC in the background . Description: NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ... The repainted Farnham dome with the AITC in the background NOTE: All images and movies are copyright and must not be reproduced or mirrored in any form without written permission. ...

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• Siding Spring Survey
• View of The Oddie and SLR facility on Stromlo with Lake Burley Griffin and
• Lesson 2: Osciloscopes

Family ASTRO Event Leaders can follow the links below to find a number of resources and more background reading to help them with their Astronomy Events and expand their knowledge on the topics covered in our series of Leader Kits for educators. ... Print and Web Resources on the Night Sky . ... If you have questions about Family ASTRO, see our Frequently Asked Questions for Educators and Astronomers page , or our Frequently Asked Questions for Families and Friends page. ...

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• ASP: Sharing the Universe
• ASP: The Universe At Your Fingertips TOC
• ASP: Project ASTRO Astronomer Application

... Astrophysics Group . Research . Cosmic Microwave Background (CMB) . ... A significant fraction of the Astrophysics Group is involved in work on the Cosmic Microwave Background, both experimental and theoretical. We are currently operating the Arcminute Microkelvin Imager , an arcminute-scale survey telescope, and developing analysis techniques for the Planck satellite. ... 2013, Astrophysics Group, Cavendish Laboratory, JJ Thomson Avenue, Cambridge, CB3 0HE . ...

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• PPEUC Programme - Cosmic Microwave Background Workshop
• OptInt PmWiki : PmWiki / Wiki Style Examples
• OptInt PmWiki : Wiki Style Examples

This diagram shows the six superimposed "layers" of the CSS table model. This diagram illustrates the algorithm for calculating a cell's final background. ... The diagram shows how, looking down on the six rectangles, one may compute the background color of each cell. ... A cell without a background color in the top layer is depicted as a "window" onto the lower layers, which give its final background color. ...

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• Long description of example illustrating background calculation
• Long description for background pattern
• Image: Lawn of the temple. Golden spear on the background is explained on the

... 2000 December 30 . A Year of Resolving Backgrounds . ... Explanation: No matter which direction you look, no matter what type of light you see, the sky glows - but why? ... In microwave light , the BOOMERANG and MAXIMA-1 missions resolved with new clarity the seemingly uniform microwave background . ... Pictured above , a map spanning ten degrees of the microwave sky resolves the microwave background into hot and cold spots, as indicated in micro kelvins . ... About APOD | ...

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• APOD: 2000 November 9 - The Cosmic X-Ray Background
• APOD: 2000 January 14 - Chandra Resolves the Hard X Ray Background
• APOD: 2013 March 25 - Planck Maps the Microwave Background

body { // background-color : #FFFFFF; background-image: url(../images/image3.jpg); //font-family: Georgia, Times New Roman , Times , serif; font-size : 16px; margin: 0px; padding: 10px; } body a:hover, # sidebar a:active { color : # CC0000 ; text-decoration : underline; } body a { color : # CC0000 ; text-decoration : none ; } #mainTable { width: 750px; ...

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• http://hea.iki.rssi.ru/conf/hea2007/styles/style_hea.css~
• http://hea.iki.rssi.ru/Z-90/style_blue.css~
• http://hea.iki.rssi.ru/conf/hea2007/styles/style1.css~

Next: Basic Properties Up: R Coronae Borealis Stars Previous: Introduction . RCB stars are named after a star just visible to the naked eye in the constellation of Corona Borealis. RCrB was discovered by Edward Pigott, an English amateur astronomer, who had been observing a star in the `Northern Crown' for over a decade. ... Since 1795, other RCB stars have been discovered and their properties have been carefully observed. ...

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• Background
• HISTORICAL BACKGROUND
• Mutual Events of the Uranian Satellites

Next: Recording Systems Control Up: Recording Systems. ... SCHED was originally written in about 1979 as the scheduling program for global VLBI observations using the Mark II recording system. That was a system capable of recording 4 Mbps on video tape recorders. ... The wide band recording system in use for VLBI for many years was the Mark III system. ... However, SCHED was capable of scheduling Mark III observations on systems that used the VLBA control files (VLBA, VLA, and Green Bank). ...

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• Background Material for the Phase Correction Project
• The UKST H Survey - Scientific Background
• Pulsar Group PmWiki/Wiki Style Examples

Astronomy Discussion Forums . Forums: . ... Discussion Forums . ... Just A Little Background On Dick . Forum List | ... Post Message | ... Posted by Harvey on November 25, 2002 21:07:26 UTC . ... He knows a lot of math, probably more than anyone on this forum. ... 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" . ...

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Disastrous earthquakes happen 100 to 200 times a year. ... There is a chance that the data of ionospheric plasma observations hold an answer to the latter question. Satellites and ground-based facilities may detect earthquake precursors in the ionosphere a few hours or days before the main shock. ... ULF "Hz"-oscillations have been recorded several hours before the main shock in a narrow magnetic field tube (40...100 km along the satellite trajectory) conjugated with epicenter of the earthquake. ...

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Общая Астрономическая Конференция > Форумы общей направленности > Любые вопросы от новичков > Supernovae - Microwave Background - Large-Scale clustering . ... Просмотр полной версии : Supernovae - Microwave Background - Large-Scale clustering . ... 03.06.2013, 16:42 . ...

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• Supernovae - Microwave Background - Large-Scale clustering - Общая
• Выбор 6mm окуляра для SW909 - Общая Астрономическая Конференция