There is also functionality to plot multiple light curves on a single form (hereafter referred to as the Multi-plot form), which will be referred to below. Such a plot is:
Light curves in this form are limited to just the information shown in each plot. To get a detailed view of the light curve, use the menu option View... A light curve, by record number
When the form is opened, all light curve from the main file of light curves, as well as reports prepared by you but not yet submitted. With Administrator use pending submitted light curves and light curves marked for deletion) are automatically loaded.
The light curve viewer manages the following sets of light curves
The Light curve viewer assumes your un-reported light curve files are located in the Occult 4 sub-directory Occult 4/Observations/LightCurves, and your reported light curve files are in the subdirectory Occult 4/Observations/LightCurves/Reported. The light curves will be automatically managed from these locations if you use Occult to generate and submit the light curve files. If you are using other tools, you will have to move the files to these locations in order to view them in the Viewer.
The file name of the light curve file is constructed as: AAAAA_yyyymmddhhmmss-ss.txt
The horizontal axis of the plot has tick-marks along it. They are spaced at intervals of 1, 5 or 10 seconds, depending on the duration of the light curve.
The light curve files represent the light curves over a fixed range, with the top of the light curve being at the same level irrespective of the brightness of the star.
A line of text at the top left of the plot gives the event date, star or asteroid identifier, and observer.
A line of text at the bottom of the plot provides the record number in the main file, or (for administrators) an index number of the relevant file of submitted light curves. [Note. The record number for any one light curve will change with each update of the file of light curves.] When viewing light curves you have submitted, or light curves not yet submitted, the file name is also included.
On the menu bar of the plot, there is a check box Show Time + height. If this is checked, the UT and cursor height above zero for the location of the cursor are displayed with the cursor. The check status of this setting is retained between sessions.
When multiple light curves are plotted (which are displayed on a different form), the plot format is the same. the multiple plots are drawn two to a row. The multiple pot is limited to 600 light curves. If your selection involves more than 600 light curves, you will be asked to indicate how many light curves you want to plot (maximum of 600), and the index number of the first.
By default, the plot is scaled to the form width. However for the single light curve plot you can change the plot scale at the bottom left of the form. The scale can range from 0.20 to 30.00, with specific options of 1, 5, 10 and 15.
A check box show skipped frames at the bottom left of the form, when checked, will highlight any frames that are missing from the light curve. This can occur when the camera output or recorder is unable to keep up with the exposure rate being used. It is an uncommon situation. However it is important to know whether there are any skipped frames near the event.
You can copy the light curve graphic using the menu item, With displayed light curve... Copy This will place the graphic on the Clipboard ready to be pasting into other software, such as Paint or Word.
The image that is copied is of the entire light curve, even if it extends beyond the display area on the form.
Any light curve displayed on the Light Curve Viewer can be transferred to AOTA for display and analysis, using the menu item With displayed light curve... Display in AOTA. All the usual functions of AOTA can be applied to the light curve. This can be useful for reviewing event times, and applying the Short duration event test in AOTA. HOWEVER precise event times depend on how camera corrections have been incorporated in the light curve data when it was created. And for the Short duration test there are no comparison stars - which adversely affects the numeric value of the assessment.
There are two means of selecting a light curve to view:

The options available are 6 star catalogues (Hip, SAO, Tyc2, UCAC4, XZ and ZC), asteroid number, and observer name.
When one is selected, the drop-down box below those options will list:
To display an event, simply select the relevant line in the drop-down box.
The light curve is displayed, together with details of the star; date and observer; and the asteroid number and name, or lunar occultation details.
To view light curves from an observer, the program first needs to create a list of all light curves meeting the criteria for specifying the observer. In the box headed 'Index name' at the bottom-right of the form, insert a character string to identify the observer. The character string must be at least 3 characters long. Upper and lower case are treated the same. Avoid using initials or punctuation characters unless you are confident about consistency of their use for the observer of interest. Press Enter to create the index; all events matched to the search string are listed in the drop-down box - giving star number, date (month & year) and observer name. The events are sorted by event date.
You can additionally plot all light curves associated with either the selected star number, asteroid number, or observer name, by clicking Plot all of selected star [or Plot all with selected name] They are plotted in a form two light-curve plots wide, and up to a total of 600 light curves. If there are more than 600 light curves, you will be asked to specify the range to be plotted.
The View... menu item provides functionality for a more-direct access to light curves. The 4 options provided are:
This is used when you have displayed multiple light curves in the multi-plot form. With this option, simply enter the record number that is given at the bottom left of the plot, and press enter, or click the OK button. In the illustration of the multi-plot form at the start of this Help topic, the record numbers are 3509, 8503 and 9193
This is the most convenient way to select a light curve associated with a particular asteroid. When selected, enter the asteroid number in the box provided. As you enter digits, the form will display all the available light curves for the asteroid number as presently keyed in. The list gives the asteroid number, event date, and the observer(s) - so each light curve should be uniquely identifiable. When you have specified the correct number, double-click on the relevant light curve, and it will be displayed
The menu item should indicate the number of unsubmitted light curves you have. Click this item, and the light curves are displayed on the Multi-plot form. These light curves cannot be displayed on the Light Curve Viewer
The menu item should indicate the number of light curves you have submitted. Click this item, and the light curves are displayed on the Multi-plot form. If you have submitted more than 600, you will have to specify the number of the first light curve to display. These light curves cannot be displayed on the Light Curve Viewer
When light curves are available for a star, that fact will be flagged in the lunar occultation predictions - with an asterisk immediately after the 'v' magnitude. To view the light curves, right-click on the prediction, and select 'Observed light curves'
. This is an option which is only available when a light curve is flagged as
being available.
The Light Curve viewer form lists all instances of the star in the drop-down box at the bottom right of the Light curver viewer form. Click any entry to view the light curve and its associated details.

The Menu item With displayed light curve... provides several tools to enhance aspects of the plot for publication purposes. Thay are:
These options are used to manage submitted light curves, and to edit both submitted light curve files, and light curves in the Main file.
The functions are:
The process for dealing with submitted light curves is:
* Create a combined data set of the existing and submitted files
* seek confirmation of the intention to merge
* rename the existing main file to {Occult 4}\LightCurves\LightCurves_yyyymmdd_n.txt
- as a backup.
yyyymmdd is the date of renaming. n is a
sequential number if there are more than one files created on that date.
* write the new file of light curves
{Occult 4}\LightCurves\LightCurves.txt
* in the directory {Occult 4}\LightCurveReports combine all the light curve reports that have been added to the main file into the file
{Occult 4}\LightCurveReports\Consolidations\Consolidation#nnn.txt, zips all those files into
{Occult 4}\LightCurveReports\Zipped Source Files\Consolidation#nnn.zip,
(where nnn is a sequential number), and deletes all the individual files.
The light curve data is distributed in 2 ways:
Anyone taking over the role of managing the light curves will likely not have the set of consolidation files the previous person may have created. The work-around for this is to copy the latest available version of the file {Occult 4}\LightCurves\LightCurves.txt to {Occult 4}\LightCurveReports\Consolidation#000.txt (ensuring there are no other consolidation files in the directory). This will ensure they have a full back file of light curves available, with newly submitted light curves being added by way of new consolidation files created as described above.