... Columns can be re-named, added, or deleted; various operations can be performed on column contents, and the results stored in a new column; and so on. ... When you create a table from an ASCII file, the width of the table column is (by default) the width of the field in the original *.dat file. ... You can avoid this problem by specifying a width wider than the original ASCII field by using (say) C*32 instead of just C for the column in the format file, when you create the table. ...

. ОГЛАВЛЕНИЕ . Предисловие к четвертому изданию . Введение . § 1. Предмет и задачи астрономии . § 2. Подразделение астрономии . § 3. Возникновение и основные этапы развития астрономии . § 4. Практическое и идеологическое значение астрономии . § 5. Основа и источник астрономических исследований . § 6. Краткий очерк строения Вселенной . Глава I . Основные сведения из сферической астрономии . § 7. Видимые положения светил. Созвездия . § 8. Видимые движения звезд, Солнца, Луны и планет . § 9. Географические

XMM-Newton Science Analysis System Page: 1 tabcalc July 2, 2008 Abstract Perform arbitrary math with columns in a table. ... If the result column exists, it will be overwritten. 3.1 Examples  tabcalc -- tables =set.ds: table -- expression = time + 43 -- column =time43 Create the column time43 by adding row by row 43 to the values read from the column time in the table table in the dataset set.ds.  tabcalc -- tables =set.ds: table -- expression = time + 43 -- ...

... Instrument Status . Science Verification . ... CRIRES . ... SV observer shall submit their proposals using the Science Verification proposal template Proposers are asked to provide at least a short summary of the science goal, coordinates and magnitudes of GS and science target, a finding chart , the observing wavelength ID, as specified in appendix A of the UM and DIT, NDIT settings of science detectors as computed with the exposure time calculator (see below). ... with a 0.2 arcsec slit. ...

... List of Tables . ... 1.3.1 Target Acquisitions . ... Chapter 2: COS Data Files . ... 2.2 COS File Names . 2.3 COS File Structures . 2.3.1 COS FITS Table Extension Files . 2.3.2 COS FITS Image Extension Files . ... 2.4.1 Uncalibrated Science Data Files . 2.4.2 Intermediate Science Data Files . 2.4.3 Final Science Data Files (and Product Files) . 2.4.4 Auxiliary Data Files . ... 3.4.15 DQICORR: Initialize Data Quality File . ... 3.6 Customizing COS Data Calibration . ...

General Information . ... The conference is organized by the Sternberg Astronomical Institute (SAI) of Moscow University and the IAU Working group "Site-testing Instruments" . ... Use of site data in telescope operation and adaptive optics. ... Recent conferences on this subject (2007, 2008) demonstrated great interest of the community, hence the need for a new meeting. ... Unlike previous recent conferences, this meeting will cover all aspects of site monitoring for optical/IR astronomy. ...

... NICS will be the only infrared instrument for the first light of the TNG; as a consequence, we decided to incorporate a sufficient degree of operation flexibility by providing the instrument with six different observing modes, three aimed at imaging and three at spectroscopy: . ... It will be possible to use the narrow band filters as order sorters; this will allow to perform high resolution long-slit spectroscopy in the wavelength ranges covered by the available narrow band filters. ...

... Galileo Probe . The Galileo spacecraft was designed to study Jupiter's atmosphere, satellites, and surrounding magnetosphere for two years. ... From there, Galileo will spend more than five years traveling to Jupiter, where it will become the first spacecraft to make direct measurements from an instrumented probe within Jupiter's atmosphere. ... This image, taken by the Hubble Space Telescope, shows the predicted site at which the Galileo Probe will enter Jupiter's atmosphere on December 7, 1995. ...