Saving SED Data in Iris

The X and Y (spectral and flux) data values comprising the currently displayed SED data segment(s), along with associated metadata, may be saved to a file in one of the following formats:

• VOTable (.vot) / XML (.xml) - XML standard for the interchange of data represented as a set of tables. Consists of an unordered set of rows, each of a uniform structure, as specified in the table metadata. Each row in a table is a sequence of table cells, and each of these contains either a primitive data type, or an array of such primitives.
• FITS (.fits) - consists of a series of Header Data Units (HDUs), each containing two components: an ASCII text header and the binary data. The header contains a series of header keywords that describe the data in a particular HDU and the data component immediately follows the header.

In order to write your SED data to file in XML, VOT, or FITS format, simply select the "File->Save as" menu option and enter a filename with extension ".xml", ".vot", or ".fits".

Iris copies the metadata from the input SED file to the saved output file. When multiple input files are plotted together in the main display, the output file contains the merged metadata from all input files together. The goal is to allow the SED builder to gather separate SED data segments from various places and save them together as an aggregate SED which complies with the IVOA Spectrum V1.03 model.

Saved SED data may be opened in a future session of Iris simply by selecting the File->Read from File option.

Saving Data Images

The SED data currently displayed in Iris may be printed to a hardcopy image in either JPG (.jpg), PNG (.png), GIF (.gif), BITMAP (.bmp), WBITMAP(.wbmp) format, by selecting File->Print to image file, and making the desired image format selection.

There is also the option to generate a printed hardcopy of the Iris main plot area via the "Print main display" option in the File menu, which is available for both imported data and data read from file.

Saving Fitted Model Data

After fitting a model to SED data in Iris, the model X and Y data arrays may be saved separately from the source data by selecting the "Save" option in the Iris Fit window after finalizing a fit, and prior to exiting the fitting session with the "Dismiss" button (see the "Modeling and Fitting SED Data" section of the Iris How-to Guide for details). Saved custom fit parameters may be restored in a future Iris session by opening the saved CDB-format file from within the Iris Fit window, using the File->Read from File menu option.

Selecting File -> Write to text file, instead, saves the model data to a human-readable text file. The saved model values contained in such a text file would appear in the format shown below.

% more bpl_active_comps.txt

Tue Aug 8 13:30:54 EDT 2011  Iris Beta 2.5

TARGNAME: 3C 273

Component 1: brokenpowerlaw
   F   refer  = 5000.0                                     angstroms      
       ampl   = 0.008195945 (1.0992086E-4 -6.804952E-5)    angstroms      
       index1 = -1.2218841  (0.53747505   -0.0011722799)                  
       index2 = -0.42091045 (0.004602734  -0.005547297)