View a Light Curve

The light curve viewer can be opened as follows:
  • From the Asteroid Observations tab, click View light curves
  • From the Lunar observations tab, click View a light curve
  • From the Asteroid Observations editor, click List... Display Star Light curve (if any are available)
  • From the Asteroid Observations editor, if a plot of light curves is displayed when an event is opened, by clicking Open Light curve viewer from the top of that display
  • From Lunar occultation predictions. 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. See example below

    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.

     

    Light curve files 'behind the scenes'

    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

     

    Light curve plot

    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.

    Copying the light curve graphic

    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.

     

    Viewing the displayed light curve in AOTA

     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.

     

    Viewing light curves

     There are two means of selecting a light curve to view:

    Using the options at the bottom right of the form


    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.

    Selecting by observer name

    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.

    Plotting multiple light curves

    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.

    Using the View... menu item

    The View...   menu item provides functionality for a more-direct access to light curves. The 4 options provided are:

    A light curve, by record number

    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

    A light curve, selected by asteroid number

    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

    My xxx unsubmitted light curves

    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

    My yyyy reported light curves

    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

     

    Viewing light curves from Lunar predictions

    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.

    Publication and related tools

    The Menu item With displayed light curve... provides several tools to enhance aspects of the plot for publication purposes. Thay are:

  • Add this text to the plot header. Specify text to include in the plot header.
  • Add this marker for a UT time (two instances)  Specify a time, and an arrow will be placed on the horizontal axis, in the color of the menu item. This is useful for indicating where an event would be. For example, the location corresponding to an event in a different observer's light curve
  • Draw curves with thick lines
  • Indicate missed images
  • Open Fresnel controls This control panel is required for locating a Fresnel diffraction pattern light curve against the observed light curve. If the Fresnel tool has created relevant light curve files for the event, open this panel to select the relevant light curve. The panel provides controls to:
  • Select the relevant light curve
  • Re-read a light curve file. [This is relevant when using the Fresnel tool to get the best fit. It has no relevance when called using existing light curve files
  • Adjust the vertical scale to match the full light level. Beneath the slider there is a check box 'Use average of all (no filtering'. When the Fresnel file is added, a calculation of the approximate full light level is undertaken. However this will not work properly when the light curve has a large noise signal, or the light drop is small. If there is a significant miss-match between the full light of the Fresnel light curve and the plotted light curve, check this box. It will set the full light level on the basis of all points in the light curve.
  • Time offset Adjust the horizontal position of the Fresnel light curve. Note that you cannot adjust the relative time scales. They are set to be exactly the same.
  • Write .csv file for this light curve
  • Display light curve in AOTA  This will take the displayed light curve into AOTA where it can be analysed using all the AOTA functionality
  • Copy image  This will be of the entire light curve, and not just that displayed in the viewing window.
  • Save image  This will be of the entire light curve, and not just that displayed in the viewing window.


    Admin functions

    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:

    Processing submitted light curves

    The process for dealing with submitted light curves is:

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    Light curve distribution

    The light curve data is distributed in 2 ways:

    Taking on the role of managing the light curves

    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.