In the Global list of spectra short names for each5 spectra are shown. The short names are intended to allow the quick identification of spectra and can be modified at any time by selecting the name and then typing a new name in the Short name field (remember to press <Return> to make the change happen). Initially short names are read from the TITLE or OBJECT properties of spectral data formats that support these (i.e. NDF and FITS respectively), otherwise they default to the file name.

Another important concept related to the global list, is using it to create a selected range or list of the spectra. Selection is important as this identifies which spectra you’d like to see properties for, or want to work with. There’s a quick tutorial on selecting spectra in the introductory material (§2.2).

In the properties area there are controls for changing how the currently selected spectra are displayed (a spectrum always uses the same display properties) and where they are displayed.

If more than one spectrum is selected then the properties shown are those of the first spectrum (i.e. highest in the global list). However, any changes that you then make are applied to all the selected spectra.

If you load a table into SPLAT-VO the Columns: controls will show the names of the columns selected. If these are incorrect then you can choose a different set.

The properties that you can change include the colour (press on this to get a swatch of selectable colours), the composite value (that is the transparency so you can see lines or points through other line or points), the line type (simple connected polyline or histogram, or just a point marker). If you choose to draw lines then you can set the width and style (dashed etc.). If you choose to draw points then various types are available.

If the selected spectra have errors then you can display error bars by clicking on the Error bars: control. This is greyed out if errors are not available. The colour, number of sigma drawn and frequency of the error bars can be changed using the other controls on this line.

The views of the current spectra region shows the names of the plots that are displaying the currently selected spectra (this time if a plot is showing only some of the spectra, then it is highlighted in red). To add a spectrum or list of spectra to a plot, select their names in the global list and then click on the Displayed control (normally this results in a tick appearing). If a plot is already displaying some of the selected spectra then you force it to display them all by clicking twice – the first click removes the selected spectra and the second puts them all back, plus the ones not already shown.

To make a plot visible double click on its name. This should raise and deiconify it.

The toolbar region has a series of buttons that act as short-cuts to many of the functions found in the main menus. Here’s a quick break down of what they do:

• Create an open file dialogue. You can use this to browse any local files and select a list of them for opening. When opened they are added to the global list and displayed in a new plot (unless you untick the Display control). You may open files that are already in the global list, this just creates a new entry. Normally the type of a spectrum is determined using the file extension, but using this dialogue you can select a type, or ask that it be guessed.
• Download and display a spectrum from the Internet. If you have a URL for a spectrum to view then use this simple dialog.
• Query any known Simple Spectral Access Protocol (SSAP) servers about spectra that they hold on a region of the sky and download these to SPLAT-VO. This tool provides access to the Virtual Observatory.
• Query any known Observation Data Model Core (ObsCore) spectral services using the Table Access Protocoll (TAP) and download these to SPLAT-VO. This tool provides access to the Virtual Observatory.
• Browse a hierarchy of files. This dialogue can be used like the open file dialogue to choose a file containing a spectrum, but, it also allows you to look inside a file for any displayable components. This is useful for FITS files that contain extensions (spectral or table extensions can be opened), or HDS files that contain more than one NDF. The file type guessing used here is the same as that used when you set a type of guess (either on the command-line or by using the open file dialogue).

  

• Re-open the selected spectra. If the files containing your spectra change on disk you can select them in the global list get them opened. Note that not all spectra are backed by a suitable disk-file, these types will be ignored.
• Create a save file dialogue. Using this you can save a spectrum to disk-file. There are no restrictions on which file format you can save to, but information may be lost for certain types (i.e. TEXT format).
• Remove the currently selected spectra from the global list. This does not modify disk files. Spectra that are only resident in memory will be lost, without warning.
• Display the currently selected spectra in plots. Each of the selected spectra is displayed in a plot of its own. A similar effect is obtained by double-clicking a spectrum in the global list.
• Display all the currently selected spectra in a single plot. Use this when you want to compare spectra.
• Open a window to control the animation of some of the spectra. Using this window you can also create a JPEG or PNG sequence of the animation.
• View and possibly modify the coordinates and data values of the selected spectra. This shows an editable table of values. It is also possible to make global changes using algebraic expressions to convert or create new values.
• Open a window to set or remap the coordinate systems of any of the spectra. A variety of systems can be used covering wavelength, frequency, energy and velocity. Unit information can be used to align spectra in a plot (so you can trivially compare spectra in say angstroms and nanometres, energy and frequency or even heliocentric and topocentric rest frames etc.).
• Open a window to set the data units of any spectra. This can be useful when just setting the units displayed in a plot, but can also be used to convert spectra between flux systems when they are drawn (making them correctly aligned).
• View the FITS headers of any selected spectra. A window displaying the headers will be opened for each of the selected spectra. Note that only 1D FITS and NDFs will generally have FITS headers other types, including FITS tables, will not.
• Change the colour of all the spectra in the global list. Each time you press this button a new random seed is used to generate a different sequence of colours, so keep pressing until you see a sequence you like.
• Perform simple maths (add, subtract, divide and multiply) between pairs of spectra.
• Perform simple maths using a spectrum and a constant (add, subtract, divide and multiply).
• Access the on-line help system.

Interesting menu items not found in the toolbar are a list of standard line position catalogues (for optical and some IR and submillimeter lines), these are found in Options->Line identifiers. Others are to do with controlling the selection of the spectra and plots (see the Edit menu, just like deleting spectra from the global list you can delete all the selected plots) and changing the ‘look and feel’ of SPLAT-VO. These options are found in the Options->Look and Feel and Options->Colour Theme sub-menus. Note that if you select the CDE/Motif look and feel you cannot change the colour and fonts used.

You can also save and restore the global stack of spectra to and from diskfile using a special data format that is only recognised by SPLAT-VO. Using this method allows you to save a working set of spectra and restart an analysis later. Properties such as the line colours are restored, but any relationship between disk files and the spectra in the global list is lost. Data saved in a stack are compressed.

The Interop menu contains items for communicating with other SAMP-aware desktop applications. This is described in the Tool interoperability section (§6).

Finer control of the initial coordinate system picked by SPLAT-VO is given by the Options->Find spectral coordinates menu item. When this is selected (the default), SPLAT-VO will check for any spectral coordinate system in the input spectra and use that, if the default coordinate system isn’t spectral. It will also use any units it can locate to attempt a guess if all else fails. Unfortunately this means that if you intend to view another coordinate system (like GRID to see the channel numbers), it might fail, so switching this off gives you complete control. This option can also be enabled using the -k,--keepcoords switches on the command-line.