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1. ESO-MIDAS Requirements
... System . By using software standards provided by most computer manufactures, ESO-MIDAS runs on VMS and OpenVMS systems (Trademarks of Digital Equipment Corporation) =, a large variety of UNIX (Trademark of AT ) platform, as well as one personal computers (386, 486, Pentium) running Linux. ... IBM/AIX RS/6000 systems; . ... The full MIDAS system requires of the order of 20 Mbyte of disk storage if shared libraries ( e.g. SUN, PC/Linux) are available, otherwise up to 100 Mbyte may be needed. ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/precise/Midas_doc/midas-require.html -- 6.5 Кб -- 23.02.1996
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2. Target Identification
... Chapter 4: Solar System Targets > 4.2 Target Identification . ... The following information is required to identify and classify each target. ... For example, separate targets should be defined if you plan to take spectra of several different surface features on a planet, or if you plan to observe the same feature with different timing constraints. ... Description . PLANET . If the target is the center of a planet, enter PLANET followed by its name (e.g., PLANET JUPITER , PLANET SATURN ). ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/documents/p2pi/HTMLjavahelp21/ch04_targ_ss03.html -- 99.2 Кб -- 24.05.2013
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3. 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. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/textbook/se.html -- 4.8 Кб -- 16.12.1997
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4. Automated Photometric Calibration Software For IRAF
... New IRAF tools for the photometric calibration of optical/IR images are presented. The new tools are standard star catalog and world coordinate driven, requiring both accurate standard star catalog coordinate and accurate image coordinate data. Network access to standard star catalog servers is supported. ... The photometric calibration software will automatically convert the standard star coordinates from the standard star coordinate system to the image coordinate system. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass00/P3-02/ -- 11.6 Кб -- 29.05.2001
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5. http://www.naic.edu/general_int/jobspost/OpenPositions-Electronics,Computer&VisitorCenter.pdf
... Required qualifications: BS in Electronics Engineering. ... Required qualifications: BS in Electronics Engineering or Electronics Technology field with three to five years experience in operation, calibration and maintenance of high-voltage equipment or equivalent combination. Supervisory experience required. ... Required qualifications: Bachelor's degree in Computer Science or related field, with more than five but less than seven years experience or equivalent combination. ...
[ Текст ]  Ссылки http://www.naic.edu/general_int/jobspost/OpenPositions-Electronics,Computer&VisitorCenter.pdf -- 25.9 Кб -- 29.06.2009
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6. http://www.arcetri.astro.it/irlab/doc/library/javascript/clientguide/glossary.htm
... Binary large object. ... CGI is a popular interface used to create server-based web applications with languages such as Perl or C. A web browser, such as Netscape Navigator. ... Core JavaScript contains a core set of objects, such as Array , Date , and Math , and a core set of language elements such as operators, control structures, and statements. ... A JavaScript primitive value is a member of one of the following types: undefined , null , Boolean , number , or string . ... World Wide Web . ...
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/doc/library/javascript/clientguide/glossary.htm -- 8.8 Кб -- 07.10.1999
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7. MILT Description
... This is possible at modest cost due to the low moments of inertia of the telescope and enclosure. ... This same performance will be achieved in higher winds when the telescope enclosure is facing away from the wind, or by using wind screens. ... The telescope system (MILT) will be remotely operable with an on-site operator's assistance by an astronomer located at one of the ARC member institutions. ... Mean Wind Speed . ... Offsets > 10 deg: 1 arc sec rms max . ... 5 sec max, tracking to tracking . ...
[ Сохраненная копия ]  Ссылки http://www.apo.nmsu.edu/Telescopes/eng.papers/milt/description.html -- 8.3 Кб -- 13.12.1993
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8. SMIS IKI RAN (Equipment)
... SMIS ] . noise temperature of the low noise amplifier less than 100 K . automatic frequency and polarization adjustment of the received signal . double transform of frequency . power supply: single phase, 220 V, 50 Hz . power consumption: less than 30 Wt . the unit measures: 470 x 300 x 130 mm . weight: less than 10 kg . ... Back to SMIS Home Page . ...
[ Сохраненная копия ]  Ссылки http://smis.iki.rssi.ru/inform/engl/scanorr.htm -- 2.9 Кб -- 13.03.1997
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9. Standard Setup Files
Next: Examples of Setup Files Up: Setup Files Previous: Setup Files Contents . Over 200 standard setup files have been created, covering many of the normal modes of observing. ... These especially include precisely defined, and somewhat complex cases like the Mark III standard modes (although MarkIII went the way of the dinosaur long ago. ... v '' files: . These are setup files for VLBI observations using VLBA recording formats. ... These are setup files for Mark III observations. ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/people/Tasso.Tzioumis/sched/Standard_Setup_Files.html -- 9.1 Кб -- 10.04.2016
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10. The AstroStat Slog standard processing
... Posts tagged ?standard processing? ... Tags: ADC , astro catalogs , Cast , CDF-S , Chandra , datasets , HEASARC , Penn State , reduced , standard processing , W3Browse . Category: Astro , Data Processing , Misc | ... Algorithms arXiv Astro Bad AstroStat Bayesian CHASC Cross-Cultural Data Processing Fitting Frequentist Galaxies gamma-ray High-Energy Imaging Jargon Job Languages MC MCMC Meta Methods Misc News Nuggets Objects Optical Physics Quotes Spectral Stars Stat Timing Uncertainty X-ray . ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/tag/standard-processing/index.html -- 19.7 Кб -- 01.03.2014
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11. Standard (Johnson) Magnitudes and Colours
... Standard magnitudes can only be computed for the U, B and V filters and hence the only standard colours that can be calculated are U-B, B-V and U-V. An important point to note, is that these standard colours can be computed using the following instrumental colours - U-B, B-V, U-V, (UVW1-U), (UVW1-B), (UVW1-V), (UVW2-B) and (UVW2-V). ... The program loops through these colours and if the relevant instrumental magnitudes are present computes the standard magnitudes and standard colour. ...
[ Сохраненная копия ]  Ссылки http://xmm.vilspa.esa.es/sas/8.0.0/doc/omsrclistcomb/node5.html -- 4.7 Кб -- 02.07.2008
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