02.12.2012 Views

class Continuum and Line Analysis Single-dish Software - IRAM

class Continuum and Line Analysis Single-dish Software - IRAM

class Continuum and Line Analysis Single-dish Software - IRAM

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Chapter 1<br />

Introduction<br />

<strong>class</strong> is a software package for reducing spectroscopic data obtained on a single-<strong>dish</strong> telescope.<br />

It also has basic functionalities to reduce continuum drifts like pointing or focus.<br />

The originality of <strong>class</strong> with respect to similar systems already in use is in the way an<br />

observation may be identified. In addition to the traditional scan number which can be used to<br />

uniquely refer to an observation, the system also enables one to use Selection Criteria as in a<br />

data base management system. This faculty, added to a powerful comm<strong>and</strong> monitor, sic, allows<br />

easy manipulation of large volumes of data; the list of observation numbers to be added to get<br />

the mean spectrum at one position need no longer be typed in, but may be found by <strong>class</strong> itself.<br />

On a st<strong>and</strong>ard installation, <strong>class</strong> is entered by just typing <strong>class</strong>. <strong>class</strong> is divided in different<br />

parts, called “Languages”, which have somewhat independent functions:<br />

• Language LAS contains all the general utility functions to h<strong>and</strong>le the data structure, plot<br />

the spectra or drifts <strong>and</strong> calibrate them.<br />

• Language ANALYSE contains functions to analyse calibrated spectra in more detail.<br />

• Language FIT gathers the spectra fitting functionalities.<br />

Those languages are described in this manual. In addition, <strong>class</strong> imports many functionalities<br />

defined <strong>and</strong> documented in other gildas packages:<br />

• The comm<strong>and</strong> line interpretor is imported through the SIC (basic), GUI (for widgets) <strong>and</strong><br />

VECTOR (miscellaneous) languages.<br />

• The plotting possibilities through the GTVL (basic graphic actions), GREG1 (curve plotting),<br />

GREG2 (image plotting) <strong>and</strong> GREG3 (data cube plotting) languages.<br />

• And the ephemerids <strong>and</strong> atmospheric contributions through the ASTRO language.<br />

In addition to this manual, the reader should thus consult the sic manual, <strong>and</strong> for further<br />

processing, the greg manual.<br />

This version of the <strong>class</strong> documentation reflects the full rewritting of <strong>class</strong> in FORTRAN90.<br />

In this process, many things have been changed, hopefully improved. If you are an experienced<br />

<strong>class</strong> user, you may first want to consult the <strong>IRAM</strong> memo which describes only the changes in<br />

this version of <strong>class</strong>.<br />

1

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!