Next: INTRODUCTION . ... This article presents the Quality Control system of the Very Large Telescope. ... After a presentation of the QC levels and their implementation for the VLT, the paper discusses the usage of instrument models. ... On the other hand the observatory can control the instrumental configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. ... Quality Control . ... Instrument models for calibration and quality control . ...
Russian Version ( KOI-8 , Win ) . Institute of Astronomy of the RAS . ... Self-consistent simulation of chemical and dynamical evolution of protostellar clouds . Chemical evolution of galaxies . ... Soon after my birth I was moved (I was not able to move on my own in those times, you know) in Novouljanovsk, small town to the south of Uljanovsk. ... Since that time my life and work is bound to the Institute of Astronomy of the Russian Academy of Sciences. ... Back to the INASAN home page . ...
Emily Curtis eic22@mrao.cam.ac.uk Script for working with ATM dispersive phase for Memo 590 import os import string import numpy from atmtools import * System variable parameters ... #Users' output directory dcval = 0.01 #Change in water vapour to compute change in path /mm fmin = 0 #Minimum frequency to compute phase /GHz fmax = 1000 #Maximum frequency to compute ...
... Module name: parse_list_mod . ... SUBROUTINE parse_list(in_str, out_array, in_delim) CHARACTER(LEN=*), DIMENSION(:), POINTER :: out_array CHARACTER(LEN=*), :: in_str CHARACTER(LEN=1), OPTIONAL, INTENT(IN) :: in_delim . where in_str is the string to be parsed, out_array is returned array of strings, and in_delim is the delimeter seperating the list items. in_delim is an optional parameter, and if not given defaults to a space. Note that in any case list items may not contain spaces. ...
... OBJECT имя объекта MODEL тип модели спектров (пока 2 значения: PEGASE1 и GISSEL98) G_TYPE тип галактики (E, S0, Sa, Sb, Sc или Sd) FILT_MAG_STR список данных по фильтрам с ошибками, формируется как строка из заданных фильтров, например: FILT_MAG_STR="B=23.73+0.21 V=23.57+0.2 R=22.36 I=20.81" Z_FIXED заданное красное смещение z Z_LIMITS пределы поиска z, когда красное смещение неизвестно AGE_LIMITS пределы поиска возраста EXTINCTION ключ задания вычисления экстинкции в заданных фильтрах RA | ...
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... The improvement will be more pronounced in our crowded Wide Field Camera (WFC) images, and may be increased further through use of a more sophisticated method of combining the individual dithered images. Our analysis allows us to check for point spread function shape variations in the HST Planetary Camera (PC) field. ... In crowded field images, we are deriving information about the faint end of the luminosity function (LF) from the texture of the image background. ...
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Zu der Zeit, als Gau das erdmagnetische Feld studierte, suchte anderswo in Deutschland ein gewissenhafter Amateurastronom namens Heinrich Schwabe , von Beruf Apotheker, nach einem neuen unbekannten Planeten. ... Sonnenflecken" . ... Offensichtlich bremste das magnetische Feld den W rmeflu aus dem Sonneninneren und dunkelte damit die Sonnenflecken gegen ber der ungest rten restlichen Sonnenoberfl che ab. Der Beweis f r den Magnetismus der Sonnenflecken war das von ihnen abgestrahlte Licht . ...
Michael Mazo Independent Unversity of Mosco w Advisor: Michael Ts fasman Sivashskaya Str. 6 -1, Apt .187 Mosco w 117638, Russia Phone: +7 926 213 8084 mazo @mccme.ru FIELDS of I NTEREST Algebraic geometry, numb er theory (global fields , zeta-functions, infinite global fields and asymptotic theory) EDUCATION Independent University of Mos co w, Russia , Independent University of Mos co w, Russia , Ph.D. programme in Mathematics M.V. Lo mo nosov Mosco w Sta te University , ...
... Almudena Alonso-Herrero , University of Arizona, Steward Observatory, 933 N. Cherry Avenue, Tucson, AZ 85721, USA (aalonso@as.arizona.edu) . ... 2, D-85748 Garching, Germany (pbenvenu@eso.org) . ... Howard Bushouse , Space Telescope Science Institute, Science Software Group, 3700 San Martin Drive, Baltimore, MD 21218, USA (bushouse@stsci.edu) . Luis Colina , Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA (colina@stsci.edu) . ...
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Ссылки http://vega.inp.nsk.su/~inest/book/LS/Quotation%20Nesterenko.doc -- 34.0 Кб -- 19.09.2008 Похожие документы
High Energy Astrophysics Solutions to Exercises 5. (a) The beam is defined by x2 y2 B x y = exp -------- + -------- 2 2 2 2 x y The FWHM contour is defined by: 1 x2 y2 B x y = -- -------- + -------- = ln 2 2 2 2 2 x 2 y The axes of this ellipse are therefore: x y = 8 ln 2 x 8 ln 2 y (b) The flux per beam is B F x y = I x y B x x y y dx dy Now, if I x y varies slowly within the extent of the ...