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	<id>https://vmcoolwiki.ipac.caltech.edu/index.php?action=history&amp;feed=atom&amp;title=Gliese_Catalog_Explorations</id>
	<title>Gliese Catalog Explorations - Revision history</title>
	<link rel="self" type="application/atom+xml" href="https://vmcoolwiki.ipac.caltech.edu/index.php?action=history&amp;feed=atom&amp;title=Gliese_Catalog_Explorations"/>
	<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;action=history"/>
	<updated>2026-07-13T02:42:46Z</updated>
	<subtitle>Revision history for this page on the wiki</subtitle>
	<generator>MediaWiki 1.34.2</generator>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13788&amp;oldid=prev</id>
		<title>Rebull at 21:44, 16 May 2022</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13788&amp;oldid=prev"/>
		<updated>2022-05-16T21:44:26Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 21:44, 16 May 2022&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [https://vmcoolwiki.ipac.caltech.edu/images/1/1a/Gj.tbl.txt&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;| &lt;/del&gt;Here] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to save it, make sure it has a .tbl extension, and pass your copy through the Table Validator to be safe.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [https://vmcoolwiki.ipac.caltech.edu/images/1/1a/Gj.tbl.txt Here] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to save it, make sure it has a .tbl extension, and pass your copy through the Table Validator to be safe.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13787&amp;oldid=prev</id>
		<title>Rebull at 21:44, 16 May 2022</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13787&amp;oldid=prev"/>
		<updated>2022-05-16T21:44:11Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 21:44, 16 May 2022&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;[&lt;/del&gt;[https://vmcoolwiki.ipac.caltech.edu/images/1/1a/Gj.tbl.txt| Here&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;]&lt;/del&gt;] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to save it, make sure it has a .tbl extension, and pass your copy through the Table Validator to be safe.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [https://vmcoolwiki.ipac.caltech.edu/images/1/1a/Gj.tbl.txt| Here] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to save it, make sure it has a .tbl extension, and pass your copy through the Table Validator to be safe.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13721&amp;oldid=prev</id>
		<title>Rebull at 22:51, 13 November 2020</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13721&amp;oldid=prev"/>
		<updated>2020-11-13T22:51:04Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 22:51, 13 November 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l13&quot; &gt;Line 13:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 13:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. (Hint: phot_g_mean_mag- (5*log10(1000/parallax) - 5).) Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. (Hint: phot_g_mean_mag- (5*log10(1000/parallax) - 5).) Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;list that &lt;/del&gt;have &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;a mid-IR excess&lt;/del&gt;? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;What is &lt;/del&gt;artifacts and &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;what is &lt;/del&gt;real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Try 2MASS J-H vs. H-Ks. Why does this look the way it does? What is it telling you? (hint: &lt;/ins&gt;Are there any stars &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;subject to reddening?) Explain the structure &lt;/ins&gt;in this &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;diagram. Which features are artifacts and which are real?  Which stars &lt;/ins&gt;have &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;the most reddening&lt;/ins&gt;? &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Explore them with SIMBAD (find papers and scan them) to learn more about them to see if they are really known to be highly reddened.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Are there any stars subject to reddening? Try &lt;/del&gt;2MASS J&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;-H &lt;/del&gt;vs. H-Ks. &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Explain &lt;/del&gt;the &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;structure in &lt;/del&gt;this &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;diagram&lt;/del&gt;. What is &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;artifacts and what is real?  Which &lt;/del&gt;stars &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;have the most reddening&lt;/del&gt;? &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;Explore them with SIMBAD to learn more about them.&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;** &lt;/ins&gt;Try WISE-1 vs. WISE-1-WISE3. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Why does this look the way it does? What is it telling you? (hint: Are there any stars in this list that have a mid-IR excess?) &lt;/ins&gt;Explain the structure in this diagram. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Which features are &lt;/ins&gt;artifacts and &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;which are &lt;/ins&gt;real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Advanced: try &lt;/ins&gt;2MASS J vs. H-Ks. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;Use &lt;/ins&gt;the &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;parallax as above to make absolute J vs. H-K. Why does &lt;/ins&gt;this &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;look the way it does, e.g&lt;/ins&gt;.&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;, different than the optical CMD? &lt;/ins&gt;What is &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;it telling you about these &lt;/ins&gt;stars?  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13720&amp;oldid=prev</id>
		<title>Rebull at 22:46, 13 November 2020</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13720&amp;oldid=prev"/>
		<updated>2020-11-13T22:46:27Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
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				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 22:46, 13 November 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l10&quot; &gt;Line 10:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 10:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Use this source list and IRSA's [https://irsa.ipac.caltech.edu/applications/Gator/ Catalog Search Tool] to find 1-to-1 matches for these stars in 2MASS, WISE/AllWISE, and Gaia DR2. There's no way to easily merge these lists within IRSA. You can work with each catalog independently or merge them yourself - if you use 1-to-1 matching, each output merged list will have one line per source, so matching up sources across catalogs is trivial. Create an IPAC table (and pass it through the Table Validator to be sure it's compliant).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Use this source list and IRSA's [https://irsa.ipac.caltech.edu/applications/Gator/ Catalog Search Tool] to find 1-to-1 matches for these stars in 2MASS, WISE/AllWISE, and Gaia DR2. There's &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;currently &lt;/ins&gt;no way to easily merge these lists within IRSA. You can work with each catalog independently or merge them yourself - if you use 1-to-1 matching &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;in the Catalog Search Tool&lt;/ins&gt;, each output merged list will have one line per source, so matching up sources across catalogs is trivial. Create an IPAC table (and pass it through the Table Validator to be sure it's compliant).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. (Hint: phot_g_mean_mag- (5*log10(1000/parallax) - 5).) Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. (Hint: phot_g_mean_mag- (5*log10(1000/parallax) - 5).) Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13712&amp;oldid=prev</id>
		<title>Rebull at 15:54, 30 September 2020</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13712&amp;oldid=prev"/>
		<updated>2020-09-30T15:54:27Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 15:54, 30 September 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [[&lt;del class=&quot;diffchange diffchange-inline&quot;&gt;gj&lt;/del&gt;.tbl| Here]] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to pass your copy through the Table Validator &lt;del class=&quot;diffchange diffchange-inline&quot;&gt;tot &lt;/del&gt;be safe.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [[&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;https://vmcoolwiki.ipac.caltech.edu/images/1/1a/Gj&lt;/ins&gt;.tbl&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;.txt&lt;/ins&gt;| Here]] is the IPAC table I constructed from these sources. I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;save it, make sure it has a .tbl extension, and &lt;/ins&gt;pass your copy through the Table Validator &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;to &lt;/ins&gt;be safe.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Explore these stars=&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13710&amp;oldid=prev</id>
		<title>Rebull: /* Explore these stars */</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13710&amp;oldid=prev"/>
		<updated>2020-09-30T15:51:51Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explore these stars&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 15:51, 30 September 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 14:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars appear to have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;(Hint: phot_g_mean_mag- (5*log10(1000/parallax) - 5).) &lt;/ins&gt;Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13709&amp;oldid=prev</id>
		<title>Rebull: /* Explore these stars */</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13709&amp;oldid=prev"/>
		<updated>2020-09-30T15:50:58Z</updated>

		<summary type="html">&lt;p&gt;&lt;span dir=&quot;auto&quot;&gt;&lt;span class=&quot;autocomment&quot;&gt;Explore these stars&lt;/span&gt;&lt;/span&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 15:50, 30 September 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l12&quot; &gt;Line 12:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 12:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Use this source list and IRSA's [https://irsa.ipac.caltech.edu/applications/Gator/ Catalog Search Tool] to find 1-to-1 matches for these stars in 2MASS, WISE/AllWISE, and Gaia DR2. There's no way to easily merge these lists within IRSA. You can work with each catalog independently or merge them yourself - if you use 1-to-1 matching, each output merged list will have one line per source, so matching up sources across catalogs is trivial. Create an IPAC table (and pass it through the Table Validator to be sure it's compliant).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Use this source list and IRSA's [https://irsa.ipac.caltech.edu/applications/Gator/ Catalog Search Tool] to find 1-to-1 matches for these stars in 2MASS, WISE/AllWISE, and Gaia DR2. There's no way to easily merge these lists within IRSA. You can work with each catalog independently or merge them yourself - if you use 1-to-1 matching, each output merged list will have one line per source, so matching up sources across catalogs is trivial. Create an IPAC table (and pass it through the Table Validator to be sure it's compliant).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;appear to &lt;/ins&gt;have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;del style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;&lt;/del&gt;&lt;/div&gt;&lt;/td&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Relevant topics from the rest of the wiki=&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;=Relevant topics from the rest of the wiki=&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13708&amp;oldid=prev</id>
		<title>Rebull at 15:50, 30 September 2020</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13708&amp;oldid=prev"/>
		<updated>2020-09-30T15:50:13Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 15:50, 30 September 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [[gj.tbl| Here]] is the IPAC table I constructed from these sources.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [[gj.tbl| Here]] is the IPAC table I constructed from these sources. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;I don't know if the wiki will preserve the formatting of that sufficiently, so you may wish to pass your copy through the Table Validator tot be safe.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt; &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;=Explore these stars=&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;* Use this source list and IRSA's [https://irsa.ipac.caltech.edu/applications/Gator/ Catalog Search Tool] to find 1-to-1 matches for these stars in 2MASS, WISE/AllWISE, and Gaia DR2. There's no way to easily merge these lists within IRSA. You can work with each catalog independently or merge them yourself - if you use 1-to-1 matching, each output merged list will have one line per source, so matching up sources across catalogs is trivial. Create an IPAC table (and pass it through the Table Validator to be sure it's compliant). &lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;* Within a catalog, from the Catalog Search Tool results, you can change what is plotted. Try these things:&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;** Are there any stars in this list that have a mid-IR excess? Try WISE-1 vs. WISE-1-WISE3. Explain the structure in this diagram. What is artifacts and what is real? Which stars have an excess? Use [http://simbad.u-strasbg.fr/simbad/ SIMBAD] to explore what is known about some of these apparent IR excess stars.  Use [https://irsa.ipac.caltech.edu/applications/finderchart/ Finder Chart] to decide if you believe the WISE-3 (and WISE-4) detections. Which stars have legitimate IR excesses?&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;** Are there any stars subject to reddening? Try 2MASS J-H vs. H-Ks. Explain the structure in this diagram. What is artifacts and what is real?  Which stars have the most reddening? Explore them with SIMBAD to learn more about them.&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;** Because you have Gaia data, you have distances to these stars. However, parallax is tabulated, not distance. Because the IRSA plotting can do simple mathematical manipulations including logarithms, you can use the information there to make an absolute color-magnitude diagram. Which stars are white dwarfs in your diagram? Which stars are giants in your diagram? Use SIMBAD to investigate a few of those stars and see if you have successfully identified white dwarfs, giants, and main sequence stars. Which are the intrinsically brightest and faintest stars in this sample? Make more plots (you can make histograms!) to identify the range of distances you can find in this sample. Are they all really within ~20 pc? Which is the closest/farthest?&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;** Use the SED feature within the IRSA Radar tool to explore Vizier's SEDs for a few of these targets. Do they look like what you expect? (Radar is the box on the IRSA main web page. If you put in a galaxy name, it pulls an SED from NED; if you put in a star name, it pulls an SED from Vizier. NED are vetted SEDs, but only for galaxies. Vizier just pulls all the catalog measurements within a given radius, converts the units, and displays it, so it is not vetted.)&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l14&quot; &gt;Line 14:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 22:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*[[Photometry (finding it)]]&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;*[[Photometry (finding it)]]&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td colspan=&quot;2&quot;&gt; &lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;&lt;ins style=&quot;font-weight: bold; text-decoration: none;&quot;&gt;*[[Color-color and color-magnitude diagrams]]&lt;/ins&gt;&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13706&amp;oldid=prev</id>
		<title>Rebull at 15:34, 30 September 2020</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13706&amp;oldid=prev"/>
		<updated>2020-09-30T15:34:03Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;table class=&quot;diff diff-contentalign-left&quot; data-mw=&quot;interface&quot;&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;col class=&quot;diff-marker&quot; /&gt;
				&lt;col class=&quot;diff-content&quot; /&gt;
				&lt;tr class=&quot;diff-title&quot; lang=&quot;en&quot;&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;← Older revision&lt;/td&gt;
				&lt;td colspan=&quot;2&quot; style=&quot;background-color: #fff; color: #222; text-align: center;&quot;&gt;Revision as of 15:34, 30 September 2020&lt;/td&gt;
				&lt;/tr&gt;&lt;tr&gt;&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot; id=&quot;mw-diff-left-l7&quot; &gt;Line 7:&lt;/td&gt;
&lt;td colspan=&quot;2&quot; class=&quot;diff-lineno&quot;&gt;Line 7:&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]).  &lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt;−&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [gj.tbl| Here] is the IPAC table I constructed from these sources.&lt;/div&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt;+&lt;/td&gt;&lt;td style=&quot;color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;div&gt;# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. &lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;[&lt;/ins&gt;[gj.tbl| Here&lt;ins class=&quot;diffchange diffchange-inline&quot;&gt;]&lt;/ins&gt;] is the IPAC table I constructed from these sources.&lt;/div&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;tr&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;td class='diff-marker'&gt; &lt;/td&gt;&lt;td style=&quot;background-color: #f8f9fa; color: #222; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;&quot;&gt;&lt;/td&gt;&lt;/tr&gt;
&lt;/table&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
	<entry>
		<id>https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13705&amp;oldid=prev</id>
		<title>Rebull: Created page with &quot;  =Introduction= The Gliese catalog is a catalog of nearby stars, stars within ~20 pc, or those thought to be within ~20 pc.  ([https://en.wikipedia.org/wiki/Gliese_Catalogue_...&quot;</title>
		<link rel="alternate" type="text/html" href="https://vmcoolwiki.ipac.caltech.edu/index.php?title=Gliese_Catalog_Explorations&amp;diff=13705&amp;oldid=prev"/>
		<updated>2020-09-30T15:33:48Z</updated>

		<summary type="html">&lt;p&gt;Created page with &amp;quot;  =Introduction= The Gliese catalog is a catalog of nearby stars, stars within ~20 pc, or those thought to be within ~20 pc.  ([https://en.wikipedia.org/wiki/Gliese_Catalogue_...&amp;quot;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;&lt;br /&gt;
&lt;br /&gt;
=Introduction=&lt;br /&gt;
The Gliese catalog is a catalog of nearby stars, stars within ~20 pc, or those thought to be within ~20 pc.  ([https://en.wikipedia.org/wiki/Gliese_Catalogue_of_Nearby_Stars Wikipedia entry]) It was first published in 1957, and has been updated a few times since then. [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract This is the most recent update.] Let's explore some of the properties of these stars using IRSA services.&lt;br /&gt;
&lt;br /&gt;
=Get the catalog together=&lt;br /&gt;
# Read or at least scan the [https://ui.adsabs.harvard.edu/abs/2010PASP..122..885S/abstract PASP paper]. How many stars are in this catalog?&lt;br /&gt;
# Get the updated catalog from [https://cdsarc.unistra.fr/viz-bin/cat/J/PASP/122/885 Vizier] ([https://cdsarc.unistra.fr/ftp/J/PASP/122/885/table1.dat direct link to text catalog]). &lt;br /&gt;
# In order to get this source list into IRSA tools, you need to get it into [https://irsa.ipac.caltech.edu/applications/DDGEN/Doc/ipac_tbl.html IPAC Table Format], which is just ASCII but it has to have the right formatting. If you get it &amp;quot;close enough&amp;quot; to IPAC table format, you can pass it through [https://irsa.ipac.caltech.edu/applications/TblValidator/ IRSA's IPAC Table Validator] which can make formatting corrections. [gj.tbl| Here] is the IPAC table I constructed from these sources.&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
=Relevant topics from the rest of the wiki=&lt;br /&gt;
(e.g., these are the &amp;quot;Lego bricks&amp;quot; to go investigate in order to build this &amp;quot;Lego kit.&amp;quot;)&lt;br /&gt;
&lt;br /&gt;
*[[Photometry (finding it)]]&lt;/div&gt;</summary>
		<author><name>Rebull</name></author>
		
	</entry>
</feed>