. Album : asv-album :: Reports from various events :: 2003/02 Встреча курса, 10 лет :: Снимки Ю.В.Липатова :: Пленка 1 (Исторический музей, Красная площадь, регистрация) . Up . << Prev . 001-07 . Next >> . Photo album generated by album a tool by David on Wed Aug 26 20:43:59 2015 .

... Тип: набор, . ... Цвет: серебряный, . Материал: нержавеющая сталь, . Набор: есть . ... Цвет: разноцветный . Коллекция: Весна-лето 2016 . ... Футболка Z Generation. Цвет: мультиколор. Сезон: Весна-лето 2016. ... Цвет: серый . ... Материал верха: текстиль . ... Материал подошвы: резина . ... Материал: текстиль. ... Package weight : 0.510 kg . ... Package size (L x W x H) : 60 x 10 x 10 cm / 23.58 x 3.93 x 3.93 inches . ... Package Contents: 1 x Infant Tummy Time Mat . ...

... user-defined data file formats . ... better integration with a user's analysis routines To add such functionality to SAOimage, we developed the XPA Messaging System that allows X programs to define points of public access through which data and commands can be exchanged with external programs. ... We have utilized XPA to develop "SAOimage: The Next Generation" (SAOtng), an extensible image display service that can cooperate with other processes and programs. ... SAOtng help pages . ...

... Астронет | ... Переменные Звезды | ... Превосходная" . ... Перевод: Д.Ю.Цветков Пояснение: Y Гончих Псов (Y CVn) очень редкая звезда на ночном небе планеты Земля. Она окрашена в красный цвет, а ее спектр настолько необычен, что астроном 19-го века Анджело Секки назвал ее La Superba (Превосходная). ... Публикации с ключевыми словами: carbon star - variable star - углеродная звезда - Переменные звезды . Публикации со словами: carbon star - variable star - углеродная звезда - Переменные звезды . ...

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

Next: PSF1DRB Up: PIXTOPIXSENS Previous: Generation from Ground Calibration Contents . Ideally the in-orbit PixToPixSens file will be generated from internal calibration measurements using the fullframe high resolution engineering mode. However due to their large data volume the fullframe high resolution data won't be available frequently enough to base the in-flight generation of the PixToPixSens file on the high resolution data. ... i.e. the average counts per pixel per CCD-frame . ...

Next: HST Paper Products: A New Way to Look at HST Data . ... After providing on-the-fly re-calibration of HST data to archive users, ST-ECF has embarked on a new project aiming at grouping, cosmic ray cleaning and drizzling images taken by most HST instruments. ... The production of the missing jitter files combined with the extraction of additional engineering parameters will greatly enhance the homogeneity and the scientific value of the entire archive. ... 1995, HST Data Handbook, STScI, 107 . ...

Next: Flagging, Manipulating and Examining Up: Generating Dummy Visibility Data Previous: Making a Fake Observation . If you just want to generate visibilities corresponding to a particular model image, and do not care whether they follow realistic tracks in the uv plane, then im2uv may suit you. Task im2uv simply Fourier transforms an image (whose units should be Jy/pixel) and writes this transform into a visibility dataset. ... IM2UV . ... Normal visibility selection. Only visibilities . ...

WEEKLY ( $ SET DEF [LRP.WEEKLY] ) . The first thing to do is to generate a diff report between the last baselined LRP and the LRP which is to be baselined: . ... This command automatically sets its defaults as described below to generate baseline analysis reports for the most r