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http://xmm.vilspa.esa.es/sas/6.5.0/doc/epatplot/node2.html.
http://xmm.vilspa.esa.es/sas/6.5.0/doc/epatplot/node2.html.
1. Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
... Up: Data Analysis and Processing Techniques . ... Also, a method for quality control of CCD observations is suggested. ... Everyone who observes a celestial object using a CCD detects moving celestial objects as a ``by product''. ... We hope that our investigations may be useful for near-Earth space control and also for searches of the moving celestial objects through analysis of old and new CCD frames obtained at any amateur or professional astronomical observatory. ...
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Ссылки http://www.adass.org/adass/proceedings/adass98/bykovo/ -- 12.3 Кб -- 16.07.1999
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2. Use
XMM-Newton Science Analysis System . epatplot (epatplot-1.13.5) [xmmsas_20041122_1834-6.1.0] . ... interactive analysis . ... Figure 1: Example of epatplot output using a weak source from the Lockman Hole (Rev.70) observation . Figure 2: Example of epatplot output using a bright source (PKS2155), the pile-up is obvious in the keV range. Figure 3: Example of epatplot output using a bright source (PKS2155) where the central 20 arcsec radius has been excluded, the pile-up is gone. ...
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Ссылки http://xmm.vilspa.esa.es/sas/6.1.0/doc/epatplot/node2.html -- 4.7 Кб -- 22.11.2004
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3. HyperLeda: example of online pipeline processing
Examples of pipeline processing . ... This page presents examples of "on the fly" processing of FITS astronomical data available on the WEB using the HyperLeda pipeline tools. ... In many cases, raw data are archived and a consisten description of the file (FITS header) allows to process them on the fly. ... This first command makes a "pre-view" display of the image. o=fa:L93111HP1/00147&z=vg . ... The result of a pipeline processing is a FITS file that you can read as a normal disk file. ...
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Ссылки http://www.sao.ru/fetch/HL/11/examples.html -- 11.1 Кб -- 23.12.2013
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4. Pulkovo NEO Page: Estimation of Observational Accuracy
Pulkovo NEO Page . Central Astronomical Observatory at Pulkovo . ... NEA Accuracy Estimation . Positions of the asteroids that have been sent by observers to the Minor Planet Center are automatically processed by means of calculation of (O-C) values with the help of the EPOS software package created at Pulkovo Observatory. ... Here attention is paid to observations of the near-Earth asteroids. This work was initiated by Dr. O.Bykov at Pulkovo Astronomical Observatory. ...
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Ссылки http://www.gao.spb.ru/personal/neo/eng/accuracy/main.htm -- 9.2 Кб -- 25.11.2013
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5. Central Processor Manager CentralProcessor 0.11 documentation
... CentralProcessor 0.11 documentation . ... The Central Processor Manager is the local monitoring and control agent for the Central Processor sub-system. ... At the moment the Central Processor Manager only controls the acquisition phase; that is, it only controls the ingest pipeline. ... In addition to the CP manager specific parameters, any parameters that begin with ice_properties are passed directly to the ICE Communicator during initialisation. ... string . ... Central Processor Manager . ...
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Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/services/manager/index.html -- 16.3 Кб -- 12.04.2016
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6. Fine Guidance Sensor Instrument Handbook
FGS Instrument Handbook for Cycle 24 . ... Fine Guidance Sensor Instrument Handbook for Cycle 24 > Chapter 7: FGS AstrometryData Processing > 7.2 Exposure-Level Processing . ... 7.2.2 Observing Mode Dependent Processing . ... After pipeline initialization and data quality assessments, successful observations (i.e., those that acquired the target), are processed according to the FGS observation mode: Position or Transfer. ... The corrections applied to the FGS data are as follows: . ... Transfer mode . ...
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Ссылки http://www.stsci.edu/hst/fgs/design/documents/instrumenthandbook/c07_dataproc3.html -- 15.6 Кб -- 12.04.2016
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7. An example of a typical timing analysis
Next: *timsort* Up: Timing Analysis Previous: Summary of tasks in . ... Events will be time ordered in the output file. xt> timsort xdata$snr psr ``c 503 513 24'' none A light curve is then generated and plotted so we can inspect the gross properties of the sample (the sequence of good-data intervals and gaps) and any source variability. xt> ltcurv psr none psr 500 xt> ltcplot psr_ltc Finding this sample satisfactory, we search for periodicity with a fast Fourier transform. ...
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Ссылки http://hea-www.harvard.edu/PROS/PUG/node165.html -- 6.5 Кб -- 01.10.2012
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8. Example of suspending a foreground process
To suspend a foreground process: find / -name *.c -print find: cannot read /dev/diag .. Z [1]+ Stopped find / -name *.c -print ps 22926 p9 S 0:03 -Tcsh (Tcsh) 29857 p9 T 0:00 find / -name *.xdh -print 29859 p9 R 0:00 ps mail tony < memo.txt . ... Realising that this process will take a long time to run they stop it while they do something else. They check to see that the process still exists: it does. ... Now they can restart the process again in the foreground or run it as a background job . ...
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Ссылки http://comet.sai.msu.ru/UNIXhelp/shell/jobz1.2.1.html -- 2.5 Кб -- 17.01.1997
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9. Actor Prolog User Guide. Residents.
In Actor Prolog a resident is a special mechanism that helps processes to inspect state of other processes. A resident observes the state of a specified (target) process and if the state of the process changes (for instance, after message handling) it proves a specified predicate of the process. ... Work of the resident. ... Any change of the list of target processes or arguments of resident function results in activation of the resident and repeated collection of information in the target worlds. ...
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Ссылки http://www.cplire.ru/Lab144/start/e_reside.html -- 14.6 Кб -- 24.09.2007
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10. IKI IPL home page
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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11. Astronomy HyperText Book: Stellar Evolution
... 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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Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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12. SMIS IKI RAN (Sample Images)
. Russian Version [ MS-Win ] . [ News ] . [ Satellite data ] . [ SMIS ] . [ ] . Cities . Rivers . Fires . Clouds . Sea and lakes . Miscellaneous . Back to SMIS Home Page .
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Ссылки http://smis.iki.rssi.ru/images/sample_e.htm -- 2.7 Кб -- 28.04.1997
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13. FADPS - Flexible Astronomical Data Processing System
... The reduction system of observations FADPS (description in Russian) (Flexible Astronomical Data Processing System) for data of wide-band receivers of the first observation cabin of the radio telescope RATAN-600 had been created under the Unix-like operational system DEMOS for computers of the SM-1420-type (PDP/11) in 1987 for observation analysis and estimates of coordinates and flux densities of radio sources. ... FADPS: flexible astronomical data processing system at RATAN-600 in UNIX environment....
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Ссылки http://sed.sao.ru/~vo/fadps_e.html -- 15.4 Кб -- 24.02.2010
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14. Example of an OOF analysis for the GBT
... OOF . ALMA . ... OOF Index . Zernike Polys . GBT example . ... Observed data and analysis . The observed beam maps are shown in the first row of the table below. ... We show the best-fitting aperture and the best-fitting beams as the number of Zernike orders used for the fitting is increased. A sample OOF observed data set (top row) and the results of analysis with increasing number of Zernike polynomials used to parameterise the aperture. ... In-focus beam . ... Observed beams . ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/mk2/oof/gbtexample.html -- 15.2 Кб -- 25.11.2009
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15. WAPP Signal Processing Page
The Wideband Arecibo Pulsar Processor Signal Processing Page . ... Raw Correlation . ... The WAPP uses custom digital hardware to create estimates of correlation functions from sampled data. The digital hardware used to estimate correlation function uses quantization to represent input . After creating an estimate of input correlation functions, the Wiener-Khintchine Theorem is applied to create estimates of input Power spectral density (PSD) and Stokes parameters . ... 3 Level . ...
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Ссылки http://www.naic.edu/~wapp/SignalProc/SPMain.htm -- 8.9 Кб -- 20.04.2000
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16. ESO - Examples of ESO developments that have been used for other similar
... ESO for the Public > Doing Business with ESO > Technology Transfer > Examples of ESO developments that have been used for other similar projects in external institutions of firms . ... UVES (UV and Visual Echelle Spectrograph) was one of the first generation VLT instruments and was developed in-house at ESO. ... This has created pools of expertise within the ESO Member States that has allowed individual institutions to provide valuable contributions to the VLT observatory as well as other projects. ...
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Ссылки http://www.eso.org/public/industry/techtrans/DevelProjects.html -- 37.3 Кб -- 10.04.2016
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17. Keywords_107
Analysis of the Systematic Errors of CCD-observations of Asteroids Performed in 2007-2008 . ... Analysis of systematic errors based on CCD-observations taken with Normal Astrograph (D/F = 0.33 m/3.5 m, FOV = 18 16 arcmin, scale = 1 arcsec/pix) of Pulkovo observatory during 2007-2008 has been made. ... A statistical approach that used mean (O-C) values obtained for positions of reference stars within the field of view separated on square bins and magnitude ranges was applied. ...
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Ссылки http://www.ipa.nw.ru/PAGE/EDITION/transaction/tbook/107.htm -- 3.8 Кб -- 02.10.2012
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18. Accuracy of World positional CCD observations of the numbered minor planets
... During all period of our investigations Dr. N.Sumzina from the Institute of Applied Astronomy of RAS had prepared the Numbered Minor Planet positions from MPC Database for our processing with kind permission of the Director of Minor Planet Center Prof. Braian Marsden. ... Our extensive processing of the MPC data allows us to conclude that CCD observations of the Numbered and Unnumbered Minor Planets have the errors, sometimes very crude. ...
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Ссылки http://www.accuracy.puldb.ru/AUTHORS.HTM -- 3.3 Кб -- 05.12.2007
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19. SPUTNIK home page
... Schedule IKI RAN Data Acquisition, Processing and Dissemination Center . SRC "Planeta" Data Acquisition, Processing and Dissemination Center . Sea Surface Temperature Adriatic Sea . Baltic Sea . Barents Sea . Black Sea . ... Composite Image of Cloudiness Russia . ... Regional Archive (only cloudless data) . ... Operative Regional Archive (all data for last 3 days) . ... NOAA Data on other Servers (about Russia) . For more information send a mail to: info@sputnik.infospace.ru . ...
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Ссылки http://sputnik.infospace.ru/noaa/engl/noaa.htm -- 8.4 Кб -- 21.01.2002
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20. http://www.stecf.org/conferences/adass/adassVII/reprints/otts.ps.gz
Astronomical Data Analysis Software and Systems VII ASP Conference Series, Vol. ... Steps for ISOCAM Data Processing At the moment, the following steps for astronomical ISOCAM data processing are generally performed: 1. data preparation (slicing, generation of CIA prepared data structures) 2. crosstalk correction (for the shortwave detector only) 3. deglitching (removal of cosmic ray hits) 4. dark current subtraction 5. transient ... The images can be shifted and annotated. ...
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Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/otts.ps.gz -- 152.1 Кб -- 12.06.2006
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