function chanarf, rmfstr , effar , spec = spec , chnrg = chnrg ,verbose=verbose, _extra=e ;+ ;function chanarf ; compute the average effective area over each channel, as a ; weighted average of ... difference mainly for low and medium spectral ; resolution data. for high-res grating data, not so much. ; ;syntax ; carf=chanarf( rmfstr , effar , spec = spec ) ; ;parameters ; ...

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• The AstroStat Slog Blog Archive Quintessential Contributions
• Microsoft "Innovation"
• The AstroStat Slog 2008 November

... Despite the wide spread use of the terms MTF, CTF, limiting resolution, minimum resolvable target, and contrast to describe CCD image system quality, the terms are often misused and their relations are little understood. ... The modulation transfer function (MTF) is a Fourier transform of the line spread function i.e. its equivalent as an integral sum of sine waves taken over the whole range of spatial frequencies. MTF by its Fourier nature can only be used to operate on sinusoidal frequencies. ...

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• Russian-Finnish Symposium, Program

... Thomson's multiple window method of spectral estimationthomson provides a very good estimate of the power spectrum by measuring the energy contained within a collection of rectangular shaped frequency intervals. ... Often, much of the fine structure of a spectral estimate is due to noise. It should be stressed that while other methods of spectral estimation (such as the Welchoppenheim method) exist, the Thomson method is particularly noteworthy for its precisely defined rectangular frequency bins. ...

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... New hand rails, display boards and access paths were all prepared for the re-opening on 12th August. ... This ambitious pulsar timing project is being tackled jointly by the Swinburne Centre for Astrophysics and Supercomputing, and the staff at Parkes Observatory (principally John Sarkissian). ... John Sarkissian has developed software called "INTER_HPF" that has allowed Mal Smith to process the archived HIPASS raw data files for interference analysis and detection. ...

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• Australia Telescope National Facility
• Contributions to the project by the Consortium and DRAO
• Contribution of Low Surface Brightness Galaxies

The oral sessions will consist of a mixture of 1 hour invited reviews and contributed talks of 30 and 15 min. ... Participants who will not be able to give an oral presentation due to time limitations, will be asked to contribute to the poster session, to stimulate further debate with their results. Please send the *Title* and *Abstract* of your contribution using the form below. ... Contributions received after June 15, 1999 will not be considered in the selection for the oral talks. ... poster . ...

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• Decadal Survey ASTRO 2010 - Requests for Information responses submitted to the
• CVZ Subscription Monitoring.
• FGS Interferometric Response

... Default . ... The descriptions below focus on the meaning of each filename parameter, leaving the exact details of the inferred default value to be explained in the algorithm section. evlist . ... file . The response matrix file (OGIP-compliant format). ... If a spectrum file is not provided ( withspectrum =no) this parameter specifies the INDEX number of a source in the source description list (parameter srclist ), and thereby the incidence angle and selection regions for the response matrix. ...

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• Developer's notes
• XMM-Newton EPIC Response Files Page
• Description

... Space Research Institute . ... Main research and development work completed in 2009 and ready for implementation . ... Development of the Northern Eurasia land cover map based on medium spatial resolution satellite data. ... The research and development has been completed of the first in Russia and in the whole world high-speed digital streams decoder for space and satellite channels with extremely high noise levels. ... Main research and development work completed in 2008 and ready for...

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• Main research and development work completed in 2012 and ready for
• Main results of the experimental and theoretical research completed in 2011
• HYPERBOLOID Results Page

. Note: This material is from a 1994(!) Talk about CCDs - the physics remains the same, only the detector size has increased since then. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• Nuclear Power I.
• Digital Stellar Spectra

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• FITS BoF Session
• Colophon
• Towards a General Definition for Spectroscopic Resolution

... public class TiffDecoder . ... static int . ... Field Detail public static final int NEW_SUBFILE_TYPE . ... public static final int IMAGE_WIDTH . ... public static final int IMAGE_LENGTH . ... public static final int BITS_PER_SAMPLE . ... public static final int COMPRESSION . ... public static final int PHOTO_INTERP . ... public static final int IMAGE_DESCRIPTION . ... public static final int STRIP_OFFSETS . ... public static final int ORIENTATION . ... public static final int SAMPLES_PER_PIXEL . ...

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... Avg: the average value of the spectra (maybe throwing out some channels at the edges). <>:average over the spectra (throwing out points at the edges if you want). gCal(f) :- frequency dependence of the tabulated cal values. ... calInK(Avg): Scaler cal value averaged over the band. calOffSpc(Avg): cal off value averaged over the band (in spectrometer counts) . ... cntsToK(avg) = calInK(Avg) / (calDif_cnts(Avg)) . To convert a spectrum b_cnts in spectrometer counts to b_K in Kelvins using cntsToK: . ...

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• lbw_crosshead_rfi_may09
• Spectral-Line Observing
• Arecibo Observatory 430-MHz Gregorian Receiver

... Get lid on trolley . ... DONE - Re-align metrology . ... Get drive motor amp status indicators working (not vital for FDR) . Get I^2C interface working (not vital for FDR) . ... DONE - opdgui: Add constant acceleration trajectory . ... DONE - opdgui: tooltips . ... Complete the 2D detail and 2D assembly drawings of the pipe support, anchor and their interfaces with pipe for NMT's test rig. ... Printable View of http://www.mrao.cam.ac.uk/projects/OAS/pmwiki/pmwiki.php/MROIDelayLine/FDRTodoLists) ...

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• Astrophysics Group STFC announces бе119 million contribution to The Square
• XXVIIth YERAC Contributions
• A 215 to 265 GHz spectral line survey of the Sgr B2 molecular cloud

Meade Instruments Corporation 27 HUBBLE, IRVINE, CALIFORNIA 92618 U.S.A. (949) 451-1450 FAX: (949) 451-1460 www.meade.com Windows 7(64-bit) Installation Instructions for AutoStar Updater 5.9.2 1. ... The new Autostar update file will download to your computer. ... Double click on the Au2.EXE file to begin installation of the new Autostar updater software. ... Installation of the new Autostar Updater begins. ... Select Install. This will install the LS telescope drivers for Windows 7 64-bit. ...

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• http://www.meade.com/downloads/autostar/ASSuiteInstallQuikGuide.pdf

... About NEdit . ... Download . Get NEdit . ... Available in two versions, the version distributed with NEdit v5, which searches forwards and backwards to find a match, and a modifed version which just searches backwards, but gives alternatives with repeated use. , matchStart, regex ) completedWord = substring(scanString, matchStart, matchEnd) # replace it in the window replace_range(startScan + keyStart, $ cursor , completedWord) if ($ compword_end == $ cursor ) $ compword_rep ++ else { $ ...

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• NEdit.org
• Experiment COLD: Data Reduction Methods Used in Experiment Cold
• DINACON

... Formation and Early Evolution of Intermediate Mass Stars . Talk at IAU Symposium 221: Star Formation at High Angular Resolution . Sydney, July 2003, Viewgraphs (ppt) , proceedings contribution (PDF) . ... Invited Talk at Galactic Star Formation across the Mass Spectrum . ... Invited Talk at Modes of Star Formation and the Origin of Field Populations . ... Invited Talk at JENAM99 - Joint European and National Astronomical Meeting for 1999 . ... Mantained by: Leonardo Testi ...

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• You can!
• The first ultraviolet average spectrum of z=2.4 quasars
• A local window on galaxy formation with ALMA

Static Fourier spectrometers are often used for spectral measurements of the ionosphere emissions. There are two main advantages of Fourier spectrometers (FS) - large geometric factor and high spectral resolution; these parameters are two orders better than for grating spectral instruments. ... In scanning Fourier spectrometer optical and electric modulation of signal is used to avoid this problem, for static Fourier spectrometer there are no such ways. ...

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• Laboratory static Fourier-spectrometer

... The Observatory, the cupola of which is 480 cm wide, is equipped with a Ritchey-Cretien 500 mm f/7.5 telescope, a 200 mm f/7.5 guide telescope, and a 250 mm f/13 Baker-Schmidt, a ST4 and a ST6 CCD cameras and four computers. ... Up until now we have archived about 600 images from the first observation, and 100 from the second, thanks to the automatic telescope aiming control program written by Vairo Risoldi. ... A.Nakamura, Japan, took CCD image of NGC5775. ...

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• Contributions
• Contributions by amateurs: SN1995ad.
• APOD: 2000 May 17 - The Far Infrared Sky

... Font: Text: Variable: Symbol: Times New Roman Times New Roman Italic True Type Symbol font (Type 1 fonts only) Type Size: Paper title : Author (s): Affiliation (s): Normal text: Text in tables: Symbols: Sub/super-script: 12 10 10 10 9 10 7 pt pt pt pt pt pt pt bold ( TITLE ) bold ( Author ) italic ( Affiliation ) (regular text) ( ) (x y) GENERAL SPECIFICATIONS For Latex users, a set of macros is available on the ESA Publications www-site ... Papers must be prepared in this two-column format. ...

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• http://hea.iki.rssi.ru/integral06/proceedings.doc
• Spectrum-Roentgen-Gamma - The astrophysical Project at IKI RAN

... To introduce you to the Python programming language, and its Visual module (VPython), which allows 3D simulation. The computer labs are held in room BOZO 112, not in the usual physics lab. ... This lab will use the Python programming language. ... Click on the Windows button in the bottom left, select "Programs", then the "A-Z" list of programs. ... Later in the course you will need to write your own VPython programs for assessment - this lab is your chance to make sure you can do this. ...

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• Siding Spring Survey
• The Common Room roof is completed
• Completed dome

sw@newmail.ru THE PROBE LAYER METHOD IN THE CALCULATIONS OF CONTRIBUTION AND RESPONSE FUNCTIONS S.G.Mozharovsky Ussuriysk Astrophysical Observatory of FEB RAS, Ussuriysk, Russia sw@newmail.ru The method of probe layer for the calculation of response and contribution functions is discussed. ... This allows us to turn from the response functions to the contribution functions calculated with help of the probe layer (CFPL). ... V- VMAX . ... Solar Phys., v.136, p.239-250. ... Solar Phys., v.35, p.11-29. ...

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