Using this window you can get simple constantly updated statistics on regions of the current spectrum, or fuller statistics for the whole spectrum, or collections of regions.
Constantly updated statistics for regions are:
The integrated flux is a numerical estimate and does not require even coordinate spacing. It can be removed from this list by deselecting the Options->Show flux integral item. This can be used to quickly estimate the flux in a line, providing your spectra are background subtracted.
The TSYS value is a system temperature estimate and requires data from the JCMT, or you can set the necessary parameters by enabling the Options->Set TSYS parameters item, which reveals a set of controls not seen by default. Note that the effective exposure time is:
where and are the integration times spent on and off the source. The backend degradation factor is instrument specific.
When you use the buttons along the bottom of the window these statistics are extended to also include:
Note that the Mode is determined as , not from a distribution, so will not be correct for highly skewed distributions.
If you select the Options->Show extra stats menu item you can also see:
and if you select Error stats->you can get basic statistics on the values that are being used as the spectrum errors (or variances).
To get statistics for the whole of the current spectrum just press the Whole stats button. If you want statistics for parts of the spectrum you will need to define the coordinate ranges you want to use (see the next part), and then press the Selected stats button to get statistics for the selected regions combined together (if none are selected then all regions are used), or All stats to get statistics for all the regions combined together.
This part of the window is used to define the regions of the spectra that you want to see statistics for. Once defined you will see simple, continuously updated, statistics. You can also get fuller statistics using the Selected stats and All stats buttons.
To add a region press the Add button and then drag out a region in the display area of the plot window. This should result in the creation of a green rectangular figure.
You can interact with the figure, moving it side-to-side and resizing it. To do this
point at the figure and press the left mouse button. This ‘selects’ the figure and adds
grips to its exterior. Note that it also becomes the selected row in the Coordinate
ranges: table. To move the figure just drag it and to resize it drag a grip (the little
black squares). The associated coordinate range in the table updates with these
To add a second range just press Add and repeat. The ranges can be overlapped or not.
To fine tune the ranges you can edit the values in the ranges table, just point at
the coordinate you want to change and double click the left mouse button. This
should enable the text editing cursor. Just make the modifications you want and
<Return> to make the changes permanent. (Note: if your spectra have sky
coordinates shown for the X axis, then you should use the same format for your
To read a set of ranges from a disk file choose the File->Read ranges menu item.
The format of the input file is simple. It should have at least two fields separated
by whitespace or commas. Comments are indicated by lines starting with a hash (#)
and are ignored. You can also save the ranges and simple statistics to disk file using
(File->Save ranges). It is also possible to append the contents of the Full stats log:
region to the file
SPLATStats.log by pressing the Save to log file button.