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http://xmm.vilspa.esa.es/sas/6.1.0/doc/omgprep.ps.gz.
http://xmm.vilspa.esa.es/sas/6.1.0/doc/omgprep.ps.gz.
1. Change history
... new LaTeX template, approved version . ... only minor changes for task version 1.4 . ... applies to task version 1.5: . ... applies to task version 1.6: minor updates . ... applies to task version 3.0: new parameter names . ... applies to task version 3.1: parameter gain file removed . ... applies to task version 5.0: new parameter randomization_on . ... applies to task version 5.1: new optional parameter srcposition . ... Null values, high/low accuracy gain/cti correction, new errors and warnings ....
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Ссылки http://xmm.vilspa.esa.es/sas/7.1.0/doc/epevents/node2.html -- 15.6 Кб -- 26.11.2007
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2. http://scan.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . You may download the latest source code distribution and install the period search service at your own web server. ...
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3. Bad Pixel Correction
... The CCD package includes possibilities, before doing the actual calibration step(s), to correct for bad pixels in the CCD calibration frames. This correction is applied via the command FIXPIX/CCD and based on existing MODIFY commands. Except for the input and output frame the FIXPIX/CCD command accepts two more parameters in the command line: the correction method to be applied and the MIDAS containing the bad pixel(s) of bad pixel areas(s). ... method pixel (MIDAS command MODIFY/PIX ): . ...
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Ссылки http://www.sao.ru/precise/Midas_doc/doc/95NOV/vol2/node61.html -- 4.0 Кб -- 23.02.1996
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4. IPA RAN
... 13th European VLBI Network Symposium . and Users Meeting . on September 20-23, 2016. ... 13th European VLBI Network Symposium and Users Meeting on September 20-23, 2016. ... Year book "Ephemerides of Minor Planets for 2016" on-line . ...
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5. atfix
... User Guide ] Task: atfix Purpose: Apply various miscellaneous corrections to ATCA visibility data Categories: uv analysis ATFIX performs various miscellaneous offline corrections appropriate for ATCA 3mm data. ... Correct antenna table (when some antennas were off-line) NOTE: This task will usually be used very early in the data reduction process. ... Key: vis The names of the input uv data sets. ... Leave the Tsys calibration as is. constant Apply a constant Tsys between successive Tsys...
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Ссылки http://www.atnf.csiro.au/computing/software/miriad/doc/atfix.html -- 7.3 Кб -- 10.04.2016
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6. Баллистический центр Института прикладной математики им. М.В.Келдыша РАН
... Институт прикладной математики им. М.В.Келдыша . БАЛЛИСТИЧЕСКИЙ ЦЕНТР . О Центре . ... Баллистический Центр Института прикладной математики им. М.В.Келдыша РАН . Баллистический центр (БЦ) ИПМ им. М.В. Келдыша создан по предложению С.П. Королева и М.В. Келдыша в 1965 году. На него были возложены работы по баллистико-навигационному обеспечению (БНО) управления полетом пилотируемых кораблей и автоматических космических аппаратов научного и народно-хозяйственного назначения. ...
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7. Mixing IRAF and Starlink Applications - FIGARO under IRAF
... Up: Data Analysis Applications . ... The general-purpose data reduction package FIGARO is now available to be run from the IRAF CL, and more Starlink applications will follow in due course. ... A system has been developed to enable packages written for the Starlink Software Environment to be run from the IRAF CL so that an IRAF user can mix and match application tasks from the two environments as required to process data, all under the control of the IRAF CL. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/blym.html -- 11.5 Кб -- 12.06.2006
[ Сохраненная копия ] Ссылки http://www.adass.org/adass/proceedings/adass97/blym.html -- 11.5 Кб -- 15.05.1998
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[ Сохраненная копия ] Ссылки http://www.adass.org/adass/proceedings/adass97/blym.html -- 11.5 Кб -- 15.05.1998
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8. Designated Observatory Application
The Astronomical Society of Australia has been asked by STANDARDS AUSTRALIA to compile a list of "designated" optical observatories that are valuable resources for (i) research, (ii) education and (iii) community use. The ASA is the final arbiter of whether any particular observatory is so designated. ... Upon receipt of your application form, your observatory will be entered on a list of "Pending Designated Observatories" on the ASA Home Page. ... It will be emailed for you. ... Email . ...
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Ссылки http://www.mso.anu.edu.au/~bessell/DOapp.html -- 16.5 Кб -- 01.10.2012
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9. *qplintran* -- Apply linear transformation to a qp file through filter
... Transforms a qpoe file according to the specified parameters. ... Any type of filtering can be applied to the input qpoe file, including region filtering. In addition, the size of the output event record can be different from the size of the input event record. Of course, usually one makes the output record equal to or smaller than the input. If the output record size is made greater than the input record, a warning is issued and the ``extra'' part of the record is undefined.) ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node52.html -- 6.2 Кб -- 01.10.2012
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10. Correcting ETC Calculations of CCD Spectral Observations for CTE Effects
... Correcting ETC Calculations of CCD Spectral Observations for CTE Effects . ... HST Overview . Overview . ... Post-Observation . ... ETC . ... ID: CL Script for Applying CTE Loss to Output of Spectroscopic ETC . ... However, the STIS ETC calculations do not incorporate these CTE effects as yet. ... The output from this script should then be used to calculate the appropriate input flux level for a second run of the ETC, which will then yield output which is corrected for the CTE effect. ...
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Ссылки http://www.stsci.edu/hst/stis/software/analyzing/scripts/cteloss_descrip.html -- 23.4 Кб -- 12.04.2016
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11. http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
... Basic Observables: Zero-differenced phase and code ionosphere-free combinations of global GNSS network stations, corrected by P1-C1 satellite code biases (cc2noncc), daily observations with 30 seconds sampling rate Sites coordinates : IGb08 reference frame coordinates and velocities Displacements: solid tides, ocean loading, pole tide loading (IERS 2010) Geometric model : Receivers antennas eccentricities, absolute receiver and ...
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Ссылки http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf -- 2427.5 Кб -- 30.11.2014
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12. Notation
... The operators will be explained as they are used. The general notion to keep in mind is that any combination of these operators results in a 2- D affine coordinate transformation in the TF plane, which may be represented using the homogeneous coordinates often used in computer graphicsfoley. ... S _t_c,f_c = g_t_c,f_c,(_t) | ... We denote a time shift to the position , with an operator that has a multiplicative law of composition : (Table 1). ... Note that these two operators do not commute. ...
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Ссылки http://crydee.sai.msu.ru/~vab/Wavelet.rsc/Chirplet.dir/node7.html -- 9.2 Кб -- 15.04.1998
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13. http://vast.sai.msu.ru/lk/
Please enter the lightcurve file name and period search parameters: . Lightcurve file: . ... Apply the Heliocentric correction and convert all dates to Terrestrial Time (TT)? ... Phase range for plots: -0.5 to 1.0 0.0 to 2.0 0.0 to 1.0 . ... Also, the Heliocentric correction cannot be applied to such lightcurves. ... Two period search methods are currently implemented. ... This period search service is also available at the mirror sites: Mirror 1 , Mirror 2 , Mirror 3 , Mirror 4 . ...
14. CIMA Configuration Files
CIMA configuration files offer You a conveniant way of saving CIMA set-ups to files. ... Then instead of making this selections interactively when You are observing, You can just load and apply the configuration files. ... Any other set-up will be ignored! ... In that case, You are forced to use the 'Load only' option to load the configuration file, inspect the selected set-up carefully, apply the set-up (with the 'Accept' or 'Apply' buttons) and then save a new version of the configuration file. ...
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Ссылки http://www.naic.edu/~cima/cima_config_files.html -- 8.0 Кб -- 01.03.2012
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15. http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/jg_mksp.pdf
Applying Bayesian analysis to polarisation data J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR MKSP Workshop 1 / 15 Outline 1 2 3 4 Polarisation simulations @ radio wavebands Bayesian analysis Analysis of polarisation data Conclusions J. Geisbuesch ( Cambridge ) Bayesian analysis of polarisation data LOFAR ...
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Ссылки http://www.mrao.cam.ac.uk/projects/skads/lofar/talks/jg_mksp.pdf -- 784.2 Кб -- 09.04.2009
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16. http://www.stecf.org/conferences/adass/adassVII/reprints/teubenp.ps.gz
... GUIfying and Documenting your Shell Script Peter. ... We describe a simple method to annotate shell scripts and have a preprocessor extract a set of variables, present them to the user in a GUI (using Tcl/Tk) with context sensitive help, and run the script. ... Tcl/Tk: TkRun The GUI that is created will provide a simple interface to a program that is spawned by the GUI. ... Sample Script: testscript Here is an example header from a Cshell script with which Figure 1 was made. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/teubenp.ps.gz -- 105.9 Кб -- 12.06.2006
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17. Astigmatism II
... The SDSS 2.5-m primary mirror is supported in a manner similar to the Apache Point Observatory 3.5-m telescope primary. ... The axial support is provided by 48 air pistons. The pistons have the same diameter thereby applying equal forces with the same air pressure. ... Each group supports a 120њ sector of the mirror. ... Figure 1: CAD drawing showing the 2.5-m primary mirror and the locations of actuators (green circles) These actuators apply forces (10*cos2 N) to correct astigmatism. ...
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Ссылки http://www.apo.nmsu.edu/Telescopes/SDSS/eng.papers/19980823_1ryAstigII/19980823.html -- 10.1 Кб -- 25.08.1998
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18. The Model
Next: Initial binary parameters Up: Population synthesis of Previous: Introduction . Monte-Carlo method for statistical simulation of binary evolution was originally proposed by Kornilov & Lipunov (1983a,b) for massive binaries and developed later by Lipunov & Postnov (1987) for low-massive binaries. ... Recently Leitherer & Heckman (1995) have modelled star formation for elliptical and spiral galaxies, taking into consideration only the single stars. ... Initial binary parameters . ...
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Ссылки http://xray.sai.msu.ru/~polar/html/publications/apj/node2.html -- 5.7 Кб -- 21.06.1996
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19. Research Activities of InformChaos Lab.
Analysis of general features of the chaotic system behavior and investigation of the properties of concrete chaotic sources. ... Analysis of information properties of chaotic systems and chaotic oscillations as concrete objects for information processing and comunications. ... This hypothesis gives a possibility of designing simple mathematical structures accomplishing various processes of information processing using chaos. ... Activities | ... E-mail: chaos@mail.cplire.ru ...
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Ссылки http://www.cplire.ru/html/InformChaosLab/investigations.html -- 5.7 Кб -- 21.03.2007
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20. Department of Solid State Physics MIPT
Chair of solid state physics . ... Laboratory practical training on the structural analysis for 3rd year students of the Solid State Physics Chair of MIPT . ... X-ray diffraction methods in materials research . Debye method: determination of lattice parameters, identification of crystal phases . ... X-ray phase analysis: computer processing of X-ray diffraction spectra, identification of crystal phases using ICDD database . ... X-ray powder diffraction: qualitative phase analysis. ...
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Ссылки http://www.issp.ac.ru/kafedra/en/courses/khasanov.html -- 9.4 Кб -- 28.02.2014
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Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам
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