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List:       kstars-devel
Subject:    Re: KStars v3.5.0 Release Date?
From:       Eric Dejouhanet <eric.dejouhanet () gmail ! com>
Date:       2020-11-12 8:56:37
Message-ID: 1fmsudg3r0vlpq62c47k6n84.1605171397870 () gmail ! com
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style="outline:none;" dir="auto" contenteditable="false"> <div name="BB10" id="BB10_response_div_BBPPID" \
dir="auto" style="width:100%;"> I confirm, but this is probably a minor that can be addressed in \
3.5.1.</div> <div id="blackberry_signature_BBPPID" name="BB10" dir="auto">     <div \
id="_signaturePlaceholder_BBPPID" name="BB10" dir="auto"><p dir="ltr">eric.dejouhanet@gmail.com - \
https://astronomy.dejouha.net</p></div> </div></div><div id="_original_msg_header_BBPPID" dir="auto">     \
<table width="100%" style="border-spacing: 0px; display: table; outline: none;" \
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font-family: Tahoma, &quot;BB Alpha Sans&quot;, &quot;Slate Pro&quot;; font-size: 10pt;">  <div \
id="from"><b>De:</b> murveit@gmail.com</div><div id="sent"><b>Envoyé:</b> 12 novembre 2020 \
09:37</div><div id="to"><b>À:</b> eric.dejouhanet@gmail.com</div><div id="reply_to"><b>Répondre à :</b> \
hy@murveit.com</div><div id="cc"><b>Cc:</b> mutlaqja@ikarustech.com; hy@murveit.com; rlancaste@gmail.com; \
sterne-jaeger@openfuture.de; kstars-devel@kde.org</div><div id="subject"><b>Objet:</b> Re: KStars v3.5.0 \
Release Date?</div></div></td></tr></tbody></table> <br> </div><!--start of _originalContent --><div \
name="BB10" dir="auto" style="background-image: initial; line-height: initial; outline: none;" \
contenteditable="false"><div dir="ltr"><b>Eric:</b>&nbsp;I see. So, can you check to see you don't have a \
file saved that's messing things up (e.g. delete your ~/.local/share/kstars/<wbr><a \
href="http://SavedFocusProfiles.ini">SavedFocusProfiles.ini</a><wbr> file if it exists, and then make \
sure you're using the "1-Focus Default" profile). You could play with the initialKeep and keepNum values \
in the kstars/ekos/auxiliary/<wbr><a \
href="http://stellarsolverprofile.cpp">stellarsolverprofile.cpp</a><wbr> file in the Focus method. (Also \
see the note to Rob below).&nbsp;<div><br></div><div><b>Rob:</b>&nbsp;could there be a bug that if you \
have a saved .ini file, then the initialKeep parameter no longer gets set and uses a very high default? I \
wouldn't be surprised if that's what messing Eric \
up.</div><div><br></div><div>Hy</div><div></div></div><br><div class="gmail_quote"><div dir="ltr" \
class="gmail_attr">On Thu, Nov 12, 2020 at 12:24 AM Hy Murveit &lt;<a \
href="mailto:murveit@gmail.com">murveit@gmail.com</a>&gt; wrote:<br></div><blockquote class="gmail_quote" \
style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 );padding-left:1ex"><div \
dir="ltr">Also, for the record, I do agree that Rob should either expose the initialKeep parameter or \
make it a multiple of the Keep parameter.<div>As it currently stands, it effectively limits the maximum \
value of the keep parameter.</div><div>H</div></div><br><div class="gmail_quote"><div dir="ltr" \
class="gmail_attr">On Thu, Nov 12, 2020 at 12:19 AM Hy Murveit &lt;<a \
href="mailto:murveit@gmail.com">murveit@gmail.com</a>&gt; wrote:<br></div><blockquote class="gmail_quote" \
style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 );padding-left:1ex"><div \
dir="ltr"><div>Jasem: I can go either way I suppose, but in my experience, it's running reasonably \
quickly. I won't object too strongly if you want to fix it.</div><div><br></div>Eric:&nbsp; When I \
processed your images on my RPi4, they processed reasonably quickly:<div><br></div><blockquote \
style="margin:0px 0px 0px 40px;border:none;padding:0px"><div><i>Looking at the 1x1 \
image:</i></div><div><div><i>Computing the HFR took 1-2s, but that's using my "quick HFR" which only \
looks at stars in the middle 25% of the image.</i></div></div><div><div><i>Turning off the quick HFR \
option slowed it down to 4-5 seconds (again possibly alongside guiding).</i></div></div><div><div><i>Are \
you using something slower than a RPi4? Could there be something else slowing down the \
computations?</i></div></div><div><div><i><br></i></div></div><div><div><i>Looking at the 2x2 \
image:</i></div></div><div><div><i>Seemed to take 1-2s without quickhfr, and 1s or less with \
quickhfr.</i></div></div><div><div><i>FWIW, I run my focus with 2x2 binning of a ZWO ASI \
1600.</i></div></div></blockquote><div><div></div></div><div><br></div><div>We should figure out what the \
issue is.&nbsp;</div><div>Hy</div><div><br></div><div><br></div></div><br><div class="gmail_quote"><div \
dir="ltr" class="gmail_attr">On Wed, Nov 11, 2020 at 11:50 PM Eric Dejouhanet &lt;<a \
href="mailto:eric.dejouhanet@gmail.com">eric.dejouhanet@gmail.com</a>&gt; wrote:<br></div><blockquote \
class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 \
);padding-left:1ex"><div style="background-color:rgb( 255 , 255 , 255 )"><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733response_container_BBPPID" \
style="outline:none" dir="auto"> <div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733BB10_response_div_BBPPID" \
dir="auto" style="width:100%"> Which is my case right now. But in the particular subject of 3.5, I agree. \
I would like to know if the profiles are editable by the end-user when they are saved locally, I mean, \
are all parameters from the file loaded back properly?&nbsp;</div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733BB10_response_div_BBPPID" \
dir="auto" style="width:100%"><br></div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733BB10_response_div_BBPPID" \
dir="auto" style="width:100%">You know what I also mean here. Are there any tests validating that \
part?&nbsp;</div>                                                                                         \
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dir="auto"><p dir="ltr"><a href="mailto:eric.dejouhanet@gmail.com">eric.dejouhanet@gmail.com</a> - <a \
href="https://astronomy.dejouha.net">https://astronomy.dejouha.net</a></p></div> </div></div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733_original_msg_header_BBPPID" \
dir="auto">                                                                                               \
<table width="100%" style="border-spacing:0px;display:table;outline:none"><tbody><tr><td colspan="2">     \
<div style="border-right:none;border-bottom:none;border-left:none;border-top:1pt solid rgb( 181 , 196 , \
223 );padding:3pt 0in 0in;font-family:'tahoma' , 'bb alpha sans' , 'slate pro';font-size:10pt">  <div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733from"><b>De:</b> \
<a href="mailto:mutlaqja@ikarustech.com">mutlaqja@ikarustech.com</a></div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733sent"><b>Envoyé:</b> \
12 novembre 2020 08:46</div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733to"><b>À:</b> \
<a href="mailto:hy@murveit.com">hy@murveit.com</a></div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733cc"><b>Cc:</b> \
<a href="mailto:rlancaste@gmail.com">rlancaste@gmail.com</a>; <a \
href="mailto:eric.dejouhanet@gmail.com">eric.dejouhanet@gmail.com</a>; <a \
href="mailto:sterne-jaeger@openfuture.de">sterne-jaeger@openfuture.de</a>; <a \
href="mailto:kstars-devel@kde.org">kstars-devel@kde.org</a></div><div \
id="gmail-m_-6303917958834978578gmail-m_7337234694170452649gmail-m_2033396795361749696gmail-m_-1918649374322300733subject"><b>Objet:</b> \
Re: KStars v3.5.0 Release Date?</div></div></td></tr></tbody></table> <br> </div><div dir="auto" \
style="outline:none"><div dir="ltr">That's fine&nbsp;with me. As long as it does end up generating too \
many stars that ends up clogging HFR calculations unnecessarily.<div><br clear="all"><div><div \
dir="ltr"><div dir="ltr"><div><div dir="ltr"><div>--</div><div>Best Regards,<br>Jasem \
Mutlaq<br></div><div><br></div></div></div></div></div></div><br></div></div><br><div \
class="gmail_quote"><div dir="ltr" class="gmail_attr">On Thu, Nov 12, 2020 at 10:35 AM Hy Murveit &lt;<a \
href="mailto:murveit@gmail.com">murveit@gmail.com</a>&gt; wrote:<br></div><blockquote class="gmail_quote" \
style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 );padding-left:1ex"><div \
dir="ltr">Jasem,<div><br></div><div>This close to the release, I'm inclined to be conservative here and \
let it be.&nbsp;</div><div>It's just something I came up with, not some reference algorithm, and it seems \
to be working as it was implemented.</div><div>I suggest that we&nbsp;can play with this in 3.5.1 if you \
want, but not mess with this now.</div><div><br></div><div>Hy</div><div><br></div></div><br><div \
class="gmail_quote"><div dir="ltr" class="gmail_attr">On Wed, Nov 11, 2020 at 11:11 PM Jasem Mutlaq \
&lt;<a href="mailto:mutlaqja@ikarustech.com">mutlaqja@ikarustech.com</a>&gt; wrote:<br></div><blockquote \
class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 \
);padding-left:1ex"><div dir="ltr">Hello Robert,<div><br></div><div>Good catch on the partition &amp; \
keep stars. I think we ought to resolve this not by simply dividing by the number of chunks as this might \
skew the results. In some images, some regions are more star-rich than others. Maybe we should do a POST \
star detection but PRE star filter step where the # of stars are then trimmed to the required initial \
keep?</div><div><br clear="all"><div><div dir="ltr"><div dir="ltr"><div><div \
dir="ltr"><div>--</div><div>Best Regards,<br>Jasem \
Mutlaq<br></div><div><br></div></div></div></div></div></div><br></div></div><br><div \
class="gmail_quote"><div dir="ltr" class="gmail_attr">On Thu, Nov 12, 2020 at 9:41 AM Robert Lancaster \
&lt;<a href="mailto:rlancaste@gmail.com">rlancaste@gmail.com</a>&gt; wrote:<br></div><blockquote \
class="gmail_quote" style="margin:0px 0px 0px 0.8ex;border-left:1px solid rgb( 204 , 204 , 204 \
);padding-left:1ex">Oh the more significant question that I asked though, I don't think we addressed it \
yet.&nbsp; Right now initial keep doesn't work the way you meant it to due to the partitions.&nbsp; Does \
that need to be changed?<br> <br>
Sent from my iPhone<br>
<br>
&gt; On Nov 12, 2020, at 1:37 AM, Robert Lancaster &lt;<a \
href="mailto:rlancaste@gmail.com">rlancaste@gmail.com</a>&gt; wrote:<br> &gt; <br>
&gt; Yep they are the same kind of thing when it comes to stars certainly.&nbsp; Your argument that \
HFR should correlate to magnitude is probably very true for stars, but not for nebulae or galaxies.&nbsp; \
They can be large but dim.&nbsp; It also might not be true for some stars with dust around them<br> &gt; \
<br> &gt; Sent from my iPhone<br>
&gt; <br>
&gt;&gt; On Nov 12, 2020, at 1:24 AM, Hy Murveit &lt;<a \
href="mailto:murveit@gmail.com">murveit@gmail.com</a>&gt; wrote:<br> &gt;&gt; <br>
</blockquote></div>
</blockquote></div>
</blockquote></div>
</div></div></blockquote></div>
</blockquote></div>
</blockquote></div>
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