Next: Rebin to wavelength Up: Getting Started Previous: Identify the lines . After having identified a few lines with the Identify window, click the button in the Main window. The Wavelength Calibration window appears. ... Results can be checked with the buttons located at the bottom of the Wavelength Calibration window. plots the dispersion relation, plots the residuals, plots the lines identified during the calibration process. ... Figure: Wavelength Calibration window . ...

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... DPERSC-CP34SE: ...and 0 packets were found to have segments without Reed Solomon corrections CPEEND- DATA EDITING ENDED 26-APR-95 18:05:56 FOR W1DR0806T . CPE0EN--------------------------------------------- DATA EDITING COMPLETED ----------------------------------------------------- CPG0VS--------------------------------------------- DATA EVALUATION STARTED ----------------------------------------------- DPVSTR- DATA EVALUATION STARTED 26-APR-95 18:16:57 FOR ...

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• http://www.stsci.edu/instrument-news/handbooks/nicmos/c10_backgrounds.doc7.html
• Obsolescent Acquisition Parameters

... An Association Block (AB) contains for a set of raw frames all information about associated other files. ... associated calibration products . It also hosts information about pipeline reduction (recipe name, parameters for execution). ... set of specific keys (name=value) used to group the raw input files . ... column 5: associated AB of that product (pointing to the associated calib raw files) . ... further associated information: . ... name(s) of associated further information (e.g. QC1 plots) . ...

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• Sample Properties
• A More Complete Picture of the Blazar Class
• FSRQs

... This paper describes distortion calibration procedures for the SOHO /LASCO-C2 Coronagraph, based on in-orbit data and extensive image processing methods. ... C2 suffers from moderate optical distortion, which must be corrected in order to properly locate the stars crossing its field-of-view (which are subsequently used for photometric calibrations), to retrieve critical attitude parameters, and to insure a correct overlapping of the region common to the C2 and C3 instruments. ...

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• Pipeline Processing and Quality Control for Echelle Data
• The SuperCOSMOS Sky Surveys
• Robust Data Analysis Methods for Spectroscopy

Next: Setup Files Up: Frequency Catalog Previous: Frequency Catalog Contents . The parameters of the frequency file tell SCHED over what frequency range the group if usable and on which stations. Most of the parameters are the same as parameters in the setup file since they are meant for direct substitution once the correct frequency group has been identified. ... This will be matched against the station name in the setup file. The name VLBA will be a default for all VLBA stations. ...

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• Selavy and the ASKAP Source-finding Service
• User Parameters - Continuum Source-finding CentralProcessor 0.11 documentation
• Package: mt

... boolean . ... integer . ... Quadrant wait states [F1294], defines the length of the Extended Full Frame Mode frame time, typical values are 0, 3, or 5 (will be removed once complete PAH and PMH files in ODF available) . ... HK value of DTIMAUTRSTPREVAL [F1052], (will be removed once complete PAH and PMH files in ODF available) . ... CCD fine temperature [ C]: H_CE_TTMPFPFE [F1128], only active in absence of real PMH files (will be removed once complete PAH and PMH files in ODF available) . ...

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• Input

Next: Algorithm Up: Description of program searchdup Previous: Program parameters . Program is started by the command searchdup with no parameters. The graphic user interface appears, with all parameters to their default value. After parameter entry, the button START starts data processing. ... It is possible to stop the program clicking button BREAK! ... It is then possible to change some parameters, or to exit the program, by clicking on the EXIT button. ... 2000-06-30 ...

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• mod_session_crypto - Apache HTTP Server
• Determination of the Detector Parameters
• mod_macro - Apache HTTP Server

... Первая страница Назад Продолжить Последняя страница Обзор Изображения . Публикации с ключевыми словами: Галактика - звездная астрономия . Публикации со словами: Галактика - звездная астрономия . ... Дальний рукав в 3 кпк от центра . Лекции по Галактической Астрономии. ... Стрелец A*: быстрые звезды вблизи центра Галактики . ... KINO.RU - фильмы, кино театры, кино, расписание кино в г. Москва | ... Дизайн квартир и дизайн интерьера . ... Нужно рекламное агентство? ...

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• XWare > APOD

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

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• Absorption bands identified with DIBs
• harak_e
• Determination of atmospheric parameters and calculation of chemical composition

... Posts tagged ?parameter estimation? ... Leccardi & Molendi (2007) have a paper in A&A ( astro-ph/0705.4199 ) discussing the biases in parameter estimation when spectral fitting is confronted with low counts data. Not surprisingly, they find that the bias is higher for lower counts, for standard chisq compared to C-stat, for grouped data compared to ungrouped. ... Tags: bias , C-stat , chi-square , chisq , Cstat , Fitting , parameter estimation , Peter Freeman , spectra . ... 1 Comment . ...

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• Completeness
• HST/FOS Atlas of AGN and Quasars
• The AstroStat Slog Blog Archive [SPS] Testing Completeness

... Fortran . Storage rules Dummy argument is a quantity in the specification of a procedure, function or subroutine. Actual argument is a quantity in the call of a procedure, function or subroutine. ... Becomes 101 END PROGRAM EXAMPLE SUBROUTINE SUB(X, Y, Z) IMPLICIT NONE REAL, INTENT(IN) :: X REAL, INTENT(INOUT) :: Y REAL, INTENT(OUT) :: Z Y = Y**2 Z = X + Y END SUBROUTINE SUB In Fortran there is really only one kind of argument usage, called argument association. ...

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• Historical Notes
• Keyword arguments and default arguments
• NAG's Fortran 90

... 09.03.2001 . ... March 09 2001 09:00 (Moscow time) . The operations scheduled on OC "Mir" for March 8 are complete. The recent telemetry data confirmed that the complex remains pressurised, the thermal mode is normal, the onboard systems perform norminal. Enough electricity is generated to maintain the onboard systems operation and measure orbit parameters. The OC "Mir" onboard systems were checked out, orbit radio monitoring performed. Currently, the OC "Mir" is in free drift. ...

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• Информация для прессы

Filename completion is only available if the the environment variables EDITOR and/or VISUAL are set to either emacs , gmacs or vi . For example: EDITOR=emacs . ... To complete a file or directory name with emacs or gmacs set press the ESC key twice. ls -l on<ESC><ESC> line_help . If the filename is not completed enter more characters until the filename can be uniquely identified. ... To complete a file or directory name with vi set press the \ (backward slash) key. ls -l on\ line_help . ...

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• Filename completion with the C shell
• Filename completion with the Bourne Again SHell
• Filename completion with the TC shell

Welcome to the 10C Survey website! ... The first 10C Survey results from an area of 27 sq. degrees complete to 1 mJy and 12 sq. degrees complete to 0.5 mJy have now been released. ... The first results from the survey, which is the deepest extragalactic radio source survey of any significant extent (> 0.2 sq. degrees) above 1.4 GHz, including the deep 15.7-GHz source count are contained in AMI Consortium: Davies et al. ... For each field, deep and shallow areas have been defined. ...

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• Simple logging of scripts and their parameters Bojan Nikolic web pages (r. 329)
• Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
• NVSS Source Search (10-July-1998) Help for NVSS Source Catalog Search

... In the framework of a collaboration between ESO and OAT concerning the development of a data reduction pipeline and the related quality control subsystems software for UVES/VLT, a detailed feasibil­ ity study is being performed on the basis of data extracted from the EMMI/NTT archive. ... Overview It is ESO policy to perform data reduction for VLT instruments in ``pipeline'' mode, either at the observing premises or at headquarters. ... The work has been carried out under ESO Contract No. ...

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• ASNPHOT (Nov98) --- nictools --- ASNPHOT (Nov98)
• The STScI NICMOS Calibration Pipeline
• ASNCOMBINE (Nov98) --- nictools --- ASNCOMBINE (Nov98)

last updated 03dec01 gain,tsys,sefd,pntErrs,beamwidth,coma,beam efficiency . Coma versus pitch and roll errors. ... Figure 1 is the gain (K/Jy) versus zenith angle (top plot) and versus azimuth angle (bottom). ... Their gains . Figure 2 plots the gain versus azimuth and zenith angle. ... The bottom plot is the pointing error (az,za error added in quadrature) versus zenith angle. ... Figure 2 bottom plots the pitch +roll errors (combined in quadrature) versus the coma parameter. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/HyselltagT2832tp.pdf
• Arecibo Observatory 430-MHz Gregorian Receiver
• Arecibo Observatory 327-MHz Gregorian Receiver

... spectrum . ... sfit . ... define >macro_name< : define a macro . ... meth_range <w1> <w2>: Set wavelength range for fit . data_spectrum <name> : data in "spectrum" format . ... data_sigma <sigma> : define mean standard error in data . ... data_line_set | ... NB: synth uses multiple calls to spectrum , so various Spectrum commands may also be required. synth : find optimum fit by adjusting abundances, v turb , v sin i , and v rad . ... save <fit> : Save the spectrum and best fit from synth . ...

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• Observations and Data Reduction
• Restoration of Three Telescopes and Associated Domes
• lte-codes: sterne model atmospheres

... Observing . ... Solar Observing . ... April 3 (SUN) - Solar Observing, Central Park , Manhattan . ... APRIL'S SKY . ... Lecture Series at the American Museum of Natural History The Amateur Astronomers Association is proud to present an astronomy lecture series from October through May each year for our members and the .. ... The€аAmateur Astronomers Association of New York€аwas organized in 1927 to promote the study of Astronomy, emphasizing its cultural and inspirational value. ...

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• Lecture Series 2015-2016 ? Amateur Astronomers Association of New York

... Radio astronomical tests of the engineering model of the space radio telescope (SRT) were completed in Pushchino - see Results . ... Monitoring of the development of the upgrade on-board 1.35-cm receiver (R-SRT-1.35 cm): . ... EM Engineering Model . ... OHCFS-SRT Space Radio Telescope On-board Heterodyne and Clock Frequency Synthesizer set . OHFS-SRT Space Radio Telescope On-board Hydrogen Frequency Standard . ORFS-SRT Space Radio Telescope On-board Rubidium Frequency Standard . ...

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• Results of measurements of SRT antenna parameters in Pushchino
• RadioAstron Monthly Notices
• Parameters of the Moon-perturbed orbit

Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

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• Dependence on the Scenario Parameters and Initial Distributions
• The Effect of Relativistic Wind on Accretion Flow Parameters
• Parameters of the starburst