Git commit 3d541e3f9300b8f3af29fb0506d15c250666d200 by Yuri Chornoivan.
Committed on 22/01/2019 at 12:57.
Pushed by yurchor into branch 'master'.

Docs enhancements and updates

M  +5    -5    doc/ekos-scheduler.docbook

https://commits.kde.org/kstars/3d541e3f9300b8f3af29fb0506d15c250666d200

diff --git a/doc/ekos-scheduler.docbook b/doc/ekos-scheduler.docbook
index 4c916aec3..7337ad002 100644
--- a/doc/ekos-scheduler.docbook
+++ b/doc/ekos-scheduler.docbook
@@ -21,7 +21,7 @@
     <sect3 id="ekos-scheduler-introduction">
         <title>Introduction</title>
         <para>
-            Ekos Scheduler is an indispensable arsenal in building your 
robotic observatory. A Robotic observatory is an observatory composed of 
several subsystems that are orchestrated together to achieve a set of 
scientific objectives without human intervention. It is the only Ekos module 
that does not require Ekos to be started as it is utilized to 
<emphasis>start</emphasis> and <emphasis>stop</emphasis> Ekos. It is designed 
to be straightforward and intuitive. However, the scheduler should only be used 
after you mastered Ekos and knows all the quirks of your equipment. Since the 
complete process is automated, including focus, guiding, and meridian flip. All 
equipment should be thoroughly used with Ekos and all their parameters and 
settings adjusted to achieve the best result.
+            Ekos Scheduler is an indispensable arsenal in building your 
robotic observatory. A Robotic observatory is an observatory composed of 
several subsystems that are orchestrated together to achieve a set of 
scientific objectives without human intervention. It is the only Ekos module 
that does not require Ekos to be started as it is utilized to 
<emphasis>start</emphasis> and <emphasis>stop</emphasis> Ekos. It is designed 
to be straightforward and intuitive. However, the scheduler should only be used 
after you mastered Ekos and knows all the quirks of your equipment. Since the 
complete process is automated, including focus, guiding, and meridian flip, all 
equipment should be thoroughly used with Ekos and all their parameters and 
settings adjusted to achieve the best result.
         </para>
         <para>
             With Ekos, the user can utilize the powerful sequence queue to 
image batches of images for a particular target. In simple setups, the user is 
expected to focus the CCD, align the mount, frame the target, and start guiding 
before initiating the capture process. For more complex observatory 
environments, there are usually predefined custom procedures to be executed to 
prepare the observatory for imaging, and another set of procedures on shutdown. 
The user may plan to image one or more targets during the night and expects 
data to be ready by morning. In &kstars;, tools such as the <link 
linkend="tool-obsplanner">Observation Planner</link> and <link 
linkend="tool-whatsup">What's up Tonight</link> help the user in selecting 
candidates for imaging. After selecting the desired candidates, the user can 
add them to the Ekos Scheduler list for evaluation. The user may also add the 
targets directly in Ekos scheduler or select a FITS file of a previous image.
@@ -36,17 +36,17 @@
         <itemizedlist>
             <listitem>
                 <para>
-                    <guilabel>Target name and coordinates</guilabel>: Select 
target from the Find Dialog or Add it from Observation Planner. You can also 
enter a custom name.
+                    <guilabel>Target name and coordinates</guilabel>: Select 
target from the <link linkend="findobjects">Find Dialog</link> or 
<guibutton>Add</guibutton> it from <link linkend="tool-obsplanner">Observation 
Planner</link>. You can also enter a custom name.
                 </para>
             </listitem>
             <listitem>
                 <para>
-                    <guilabel>Optional FITS file</guilabel>: If a FITS file is 
specified, the astrometry solver shall solve the file and use the central 
RA/DEC as the target coordinates.
+                    Optional <guilabel>FITS File</guilabel>: If a FITS file is 
specified, the astrometry solver shall solve the file and use the central 
RA/DEC as the target coordinates.
                 </para>
             </listitem>
             <listitem>
                 <para>
-                    <guilabel>Sequence File</guilabel>: The sequence file is 
constructed in the Ekos <link linkend="ekos-capture">Capture Module</link>. It 
contains the number of images to capture, filters, temperature settings, 
prefixes, download directory, &etc;
+                    <guilabel>Sequence</guilabel> file: The sequence file is 
constructed in the Ekos <link linkend="ekos-capture">Capture Module</link>. It 
contains the number of images to capture, filters, temperature settings, 
prefixes, download directory, &etc;
                 </para>
             </listitem>
             <listitem>
@@ -66,7 +66,7 @@
             </listitem>
             <listitem>
                 <para>
-                    <guilabel>Startup Conditions</guilabel>: Conditions that 
must be met <emphasis role="bold">before</emphasis> the observation job is 
started. Currently, the user may select to start as soon as possible 
<guimenuitem>Now</guimenuitem>, or when the target is near or past culmination, 
or at a specific time.
+                    <guilabel>Startup Conditions</guilabel>: Conditions that 
must be met <emphasis role="bold">before</emphasis> the observation job is 
started. Currently, the user may select to start as soon as possible, 
<guimenuitem>ASAP</guimenuitem>, or when the target is near or past 
culmination, or at a specific time.
                 </para>
             </listitem>
             <listitem>

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