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Adjust discussion of multi-star selection
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bwdev01 committed Dec 23, 2024
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23 changes: 13 additions & 10 deletions help/Basic_use.htm
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Expand Up @@ -596,10 +596,10 @@ <h4><a name="Simulators"></a>Simulators</h4>
asked for a means to override guide star selection based on what they
see on the display.&nbsp; These requests have not been acted upon
because they would disrupt the underlying mathematics of the multi-star
process. More importantly, they would lead to inferior results for
algorithm. More importantly, they would lead to inferior results for
reasons described below.&nbsp; The algorithm applies the basic
principle that the accuracy of centroid calculation - the fundamental
calculation of where a star is located on the sensor - it proportional
calculation of where a star is located on the sensor - is proportional
to that star's SNR.&nbsp; It has nothing to do with the shape of the
star, its location on the sensor, its proximity to the sensor edge, or
any other visual characteristics of the star candidate. The algorithm
Expand All @@ -608,7 +608,7 @@ <h4><a name="Simulators"></a>Simulators</h4>
on a particular system.&nbsp; Two parameters, Min-HFD and Max-HFD,
define a range of star "sizes" that control whether a bright area on
the sensor can be accepted as a star candidate rather than being
rejected as sensor noise, internal reflections, or close pairs of
rejected as sensor noise, an internal reflection, or a close pair of
stars.&nbsp; The third parameter, Saturation ADU, defines an upper
limit to the peak brightness of a star candidate, usually defined as
the maximum ADU value produced by the guide camera.&nbsp; The algorithm
Expand All @@ -620,7 +620,8 @@ <h4><a name="Simulators"></a>Simulators</h4>
examining the PHD2 guide logs to see the range of star sizes that are
typical for the guiding system and its seeing conditions. Once set,
they should rarely need to be changed unless something in the
configuration or the atmospheric conditions has substantially changed.<br><br>Users
configuration or the atmospheric conditions has&nbsp;changed
substantially.<br><br>Users
are commonly fooled by what they see on the display and think they can
do a better job of guide star selection.&nbsp; This is a mistaken
impression.&nbsp; The single biggest reason is that many of the
Expand All @@ -631,13 +632,15 @@ <h4><a name="Simulators"></a>Simulators</h4>
completely eliminate these artifacts. In summary, simply squinting at
the screen and clicking on bright spots will produce inferior results
compared to the quantitative, systematic approach taken by the
auto-select star-finding mechanism.&nbsp; Of course, die-hard users can
auto-select star-finding mechanism.&nbsp; Of course, skeptical users
can
still manually choose a guide star, but they won't then be able to use
multi-star guiding. For people who are not convinced about the merits
of the auto-select process, the debug log file contains a detailed
list, for every auto-find, of the location and properties of every
single candidate object in the guide frame and how these were included
or excluded to compile the final list.<span style="font-weight: bold;"></span>
multi-star guiding. For people who question&nbsp;the auto-selection
process, the debug log file contains a detailed
list, for every auto-find, of the location and properties of
every&nbsp;candidate object in the guide frame and how these were
included
or excluded to compile the final list of usable guide stars.<span style="font-weight: bold;"></span>
<h3><a name="Automatic_Calibration"></a>Automatic
Calibration</h3>
<h4>Conventional Mounts</h4>
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