XmCCD ----- XmCCD has been tested most recently on Suse 10.1 and Suse 10.3 and it will probably run on most other recent Linux distributions. ... This distribution includes source code to utilize the Santa Barbara Instrument Group (SBIG) shared library libsbigudrv.so with a Motif-based graphical user interface program to control SBIG astronomical CCD cameras. ... The sources for these programs are available from the XmCCD home at http://www.astro.louisville.edu/moore/software. ...
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. Comment on J0604-3155 . No detection: the source has a relatively steep spectrum, alpha=-0.62, in the frequency range from 80 MHz to 8 GHz and the position is probably okay. Hence, the source is probably resolved. VLBApls home page . Last modified: 16 Oct 2000
If you go out tonight and look up at the full Moon, and you're like most people, you'll probably see the face of a man, or, alternatively, a rabbit superimposed on the bright disk of the Moon. ... When people look at the full Moon, they often see either a Man in the Moon (left) or a rabbit in the Moon (right). ... The Face on Mars is a naturally occurring rock outcropping that just happens to look like a face when lit from the side. ... The Face on Mars,'' Odyssey , October 1991, page 12. ...
Configuration Files | ... Options | ... This version of Apache includes changes allowing it to run on IBM's EBCDIC-based TPF (Transaction Processing Facility) operating system. ... It is passed to Apache through the ZINET XPARM field since ZINET is the only way to start the server on TPF. A third group of options apply to both the informational displays (ZFILE) and running the server (ZINET XPARM): -d, -D and -f. The rest of Apache's options are either not applicable or are not supported on TPF. ...
... Finding Stars . ... Handling Bad Pixels . ... The guide camera image controller can control one or more guide cameras. ... Each time the camera is read, the image is automatically saved to a fits file on a shared disk. ... Cameras that have bad pixels require "bad pixel maps" in order to find stars, centroid or even compute statistics for the image. ... View this image (for instance in NIH Image) and determine an upper and lower cutoff; pixels whose values are outside of this range are considered...
... Путь книги от бумажных страниц до файлов на этом сайте можно по сути разделить на несколько этапов. ... Начальный этап, и наиболее приемлемый вариант - сканированные страницы книги в формате TIFF или PCX (а точнее в любом формате, без ощутимой на вид компрессии. ... Относитесь к книгам с уважением. Страницы именуйте цыфрами, но всегда с сохранением числа знаков, например страница номер 7 будет иметь имя 007.tif, страница 12 будет иметь имя 012.tif, ну а страница 375 будет иметь имя 375.tif. ...
Estimations of dome seeng by results of optics quality tests with Shack-Hartman wavefront sensor. ... Measurements on AZT-22 Telescope diameter: 1000 mm F/7.7 Effective subaperture: 37.5 mm Exposure time: 100 ms Time between exposures: 5 s Individual image with tilts in X direction AZT-22 tower The spatial spectrum evolution (top) and wind direction in measurements processes . AZT-22. ... ZTSH dome Zeiss-1000 dome The spatial spectrum evolution (up) end wind direction through time. ...
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Ссылки http://site2010.sai.msu.ru/static/doc/SPotanin_site2010.pdf -- 522.6 Кб -- 31.10.2010 Похожие документы
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