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http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/omg_thread.html.

1. Processing OM Fast mode data
... The SAS_ODF environment variable shall be set to the summary file produced by odfingest , or to a directory containing the data, and access to calibration files shall be set through cifbuild . ... In order to process a single exposure containing fast mode data as . ... Note that tracking data may not be good enough, in which case no plot is produced. omdrifthist set =/path_to_your_data/fast/tmp_tracking plotfile =/path_to_your_data/fast/P0125321001OMS002TSHPLT0000.PS trackradius =0.5 hardcopy =yes ....
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/7.0.0/documentation/threads/omf_stepbystep.html -- 18.1 Кб -- 21.08.2006
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2. 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 ...
[ Сохраненная копия ]  Ссылки http://www.iki.rssi.ru/IPL/ -- 4.8 Кб -- 05.08.1997
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3. http://www.stsci.edu/documents/dhb/web/c24_stiscalib.fm3.html
[Top] [Prev] [Next] [Bottom] . This section details the data flow through the calstis pipeline for each calibrated operating mode, showing the switches, the reference file inputs, the science file inputs and the output products. The next section describes the tasks corresponding to the various calibration switches. [Top] [Prev] [Next] [Bottom] . stevens@stsci.edu Copyright ї 1997, Association of Universities for Research in Astronomy. All rights reserved. Last updated: 07/01/98 10:22:14
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/documents/dhb/web/c24_stiscalib.fm3.html -- 3.0 Кб -- 01.07.1998
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4. Titan Image Processing
... Images of Titan by the Hubble Space Telescope (HST) are very small in size and have very low spatial resolution. Special methods of image processing are required to extract information from these images. ... Currently, in searching for features on Titan's disk imaged by the HST PC1 detector, we are faced with two problems: (1) Low spatial resolution (Figure 1). ... The two aforementioned problems necessitate processing Titan images by special methods to extract information for analysis. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass96/wun.html -- 12.7 Кб -- 23.06.1998
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5. 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. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/fetch/HL/11/examples.html -- 11.1 Кб -- 23.12.2013
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6. Rev0, US-Processed Data
Next: Rev0, MPE-Processed Data Up: DETAILED LIST OF ROSAT Previous: DETAILED LIST OF ROSAT . Prior to June 1994 data processed in the U.S. were supplied in the following files: . ... rp<seq#>.fits . Photon events, data quality, and good time intervals (binary table) . ... Compressed image for display -- total energy band . ... Compressed image for display -- hard energy band . ... Compressed image for display -- soft energy band . ... Selected source spectra (ascii table) . ... Aspect files . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/PROS/PUG/node192.html -- 8.3 Кб -- 01.10.2012
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7. Basic CCD image processing
... These are the typical steps through which a CCD image has to go. ... That process is repeated until all the pixels from the 1st line are read out. ... Figure 1: raw CCD image, obtained with a Tektronics 1024; refer to the bottom of the page for the technical details. ... The corresponding raw image presents all the defects and artifacts of the CCD and the telescope. ... These are the most basic steps; every image published should have received the following corrections. ... IfA Hale-Bopp page | ...
[ Сохраненная копия ]  Ссылки http://www.eso.org/~ohainaut/ccd/ -- 11.4 Кб -- 18.08.2004
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8. Extraction of Spectra, Images and Cubelets CentralProcessor 0.11 documentation
... CentralProcessor 0.11 documentation . ... This page describes the way spectral and image data products can be extracted for each detected source. ... This set of parameters allows, for each detected source, the extraction of spectra at the corresponding position in a spectral cube. ... The final form of data product extraction is to extract ?cubelets? - cutout cubes surrounding the detected object. ... Extraction of Spectra, Images and Cubelets . Spectral Extraction . ... Cubelet extraction . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/computing/software/askapsoft/sdp/docs/current/analysis/extraction.html -- 23.7 Кб -- 12.04.2016
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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. ...
[ Сохраненная копия ]  Ссылки http://www.cplire.ru/Lab144/start/e_reside.html -- 14.6 Кб -- 24.09.2007
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10. MAKEFLAT (Sep99) --- nictools --- MAKEFLAT (Sep99)
makeflat -- makes flatfields corresponding to the output image of asncombine. makeflat association flatlist . ... ASCII file with list of flatfields as used by NICMOSlook. resolution . ... The ST-ECF tool NICMOSlook performs this task by determining the appropriate factor from narrow band flatfields. ... This task takes a list of flatfields in the same format as NICMOSlook, shifts and co-adds each of the flatfields in the list, and creates a new list which can be used as input for NICMOSlook. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/nictools/makeflat.hlp.html -- 2.7 Кб -- 06.06.2006
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11. http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf
To appear in "Fourth Workshop on Robotic Autonomous Observatories (2015)"RevMexAA(SC) METEOR OBSERVATIONS WITH MINI-MEGATORTORA WIDE-FIELD MONITORING SYSTEM S. Karpov, 1, 3 N. Orekhova2 G. Beskin, 1, 3 A. Biryukov3,4 S. Bondar,2 E. Ivanov,2 E. Katkova,2 A. Perkov, and V. Sasyuk3 RESUMEN 2 Favor de prop orcionar un resumen en espanol. ... The faintest detected meteors has the peak brightness about 10 mag, while the ma jority - from 4 to 8 mag. ... 2010; Karpov et al. 2013; Beskin et al. ...
[ Текст ]  Ссылки http://vo.astronet.ru/~karpov/pdf/2015_Malaga_mmt_meteors.pdf -- 115.6 Кб -- 15.12.2015
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