Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.stsci.edu/~mperrin/software/gpidata/_sources/gpitv/intro.txt
Дата изменения: Fri Oct 18 00:37:48 2013
Дата индексирования: Sun Mar 2 14:04:19 2014
Кодировка:

Поисковые слова: active galaxy
Purpose of GPItv
############################


GPItv is a data viewer tool that provides GPI observers with both a simple
means for cursory "quick look" data analysis, in real time at the telescope,
and a sophisticated set of tools for viewing and manipulating GPI data during
post-observing scientific analyses. GPItv includes features for spectral and
polarimetric analyses of raw 2D and/or processed 3D data from GPI. GPItv should
help you to look at GPI data in a way that enables you to get your science
done.

GPItv is a heavily customized derivative from ATV, the well-known DS9-like
display tool for astronomical images in IDL (Barth et al. 2001;
http://www.physics.uci.edu/~barth/atv/), with much new functionality
developed specifically for GPI. Anyone familiar with using ATV,
SAOimage or DS9 will get used to GPItv very quickly.

One significant enhancement relative to the original ATV program is that
GPItv's internals have been rewritten to allow multiple copies to run
simultaneously. Thus users can view for instance raw frames, reduced datacubes,
and ADI-processed subtracted images all in separate windows simultaneously


Summary of Functionality: Image Manipulation and Data Analysis
=====================================================================

GPItv is a display tool that includes features for image analysis and spectral
analysis. 2D image analysis tools are available for image manipulation,
including:

* Display of 2D/3D images with a variety options for scaling, color map, color stretch, zoom, and rotation.
* World coordinate system information (X,Y,lambda) is displayed when appropriate keywords are available in the image header.
* Viewing and editing image FITS headers
* Quick photometry and image statistics
* Image output in a variety of formats (FITS, PS, JPEG, PNG, & more)
* Labeling and overplots to annotate images
* Display of radial line plots, surface plots, and histograms of data regions
* Image blinking
* Automatic detection of new fits image in chosen directories
* High-contrast AO contrast assessments


Spectral analysis tools include:

* Multi-plane image slider for datacubes
* Extraction of 1D spectra from chosen regions
* Spectral plotting
* Display and verification of the wavelength solution
* Collapse datacube
* Simple difference Imaging

Polarimetric analysis tools include:

* Display of polarized datacubes in both Stokes IQUV and perpendicular polarization pair formats
* Overplotting of polarization vectors, with many configurable options
* Computation of total intensity, polarized intensity, & polarization fraction from IQUV datacubes.

New features can be added to GPItv easily, including linking to or calling
existing IDL programs. For example, you can easily define a keyboard shortcut
that will pass the current cursor position in data coordinates to an external
IDL routine.