Astronet Поиск по астрономическим сайтам English Russian
       
        Точная форма слов   О проекте   Сайты   Справка
Поиск по:www.stecf.org/   - Поискать по всем серверам
Найдено документов: 545 (3 сайтов) ---- Время поиска: 0.07сек.   

Показаны документы, содержащие фрагменты текста из документа
http://www.stecf.org/conferences/adass/adassVII/huths.html.

1. A Software Package for Automatic Reduction of ISOPHOT Calibration Data
... Also the measured signals are affected by detector transients, altering the final results considerably. We present the design and the main features of a software package, developed in order to support the absolute calibration of the instrument. ... In case the fit is not successful, the average of the last 30% of the data is taken as the final signal. ... The two different symbols represent individual calibrations of the final background signals, using the first or the second FCS-signal. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/huths.html -- 12.7 Кб -- 12.06.2006
Похожие документы

2. http://www.stecf.org/conferences/adass/adassVII/reprints/huths.ps.gz
... Also the measured signals are a#ected by detector transients, altering the final results considerably. ... The sequence is bounded by two measurements of the FCS , to fix the responsivity for the baseline correction 0 200 400 600 800 1000 measurement time [s] 0.00 0.02 0.04 0.06 0.08 0.10 Volt/second bg source fitted baseline 2. FCS 1. FCS source initial drifting signal corrected signal bg FCS source background signal internal calibration signal source signal corrected ...
[ Текст ]  Ссылки http://www.stecf.org/conferences/adass/adassVII/reprints/huths.ps.gz -- 111.1 Кб -- 12.06.2006
Похожие документы

3. IRAF/STECF 2-D spectrum point source / background decomposition package
IRAF/STECF 2-D spectrum point source / background decomposition package . ... The general problem is one of spectral decomposition - of separating the spectra of the point sources from the background. ... The STECF IRAF layered package "specres" provides two tasks to extract point source spectra from 2-D images (either longslit, multislit or cross-dispersed) and decompose the full background over the image. ... A Point Source Function spectrum image is required as a 2-D spectrum. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/software/IRAFtools/stecf-iraf/specres/ -- 16.5 Кб -- 08.06.2006
Похожие документы


Астронет | Научная сеть | ГАИШ МГУ | Поиск по МГУ | О проекте | Авторам

Комментарии, вопросы? Пишите: info@astronet.ru или сюда

Rambler's Top100 RFBR Яндекс цитирования