https://vmcoolwiki.ipac.caltech.edu/api.php?action=feedcontributions&feedformat=atom&user=Rutherford 2026-04-08T03:59:39Z User contributions MediaWiki 1.34.2 https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Palomar_3.xlsx&diff=11755 2013-05-14T16:24:40Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=Media_Palomar_3.xlsx&diff=11754 2013-05-14T16:24:02Z

<p>Rutherford: Created page with &quot;Media:Palomar 3.xlsx&quot;</p> <hr /> <div>[[Media:Palomar 3.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Palomar_5.xlsx&diff=11753 2013-05-14T16:06:14Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=Media_Palomar_5.xlsx&diff=11752 2013-05-14T16:05:24Z

<p>Rutherford: Created page with &quot;Media:Palomar 5.xlsx&quot;</p> <hr /> <div>[[Media:Palomar 5.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Palomar_3-Wes.xlsx&diff=11751 2013-05-14T16:04:03Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Palomar_5-Wes.xlsx&diff=11750 2013-05-14T16:03:38Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_SDSS_Globular_Cluster_CM_Exercise&diff=11749 2013-05-14T16:02:52Z

<p>Rutherford: /* An Exercise in Globular Cluster Distance Measurement */</p> <hr /> <div><br /> <br /> [[Media:]]== An Exercise in Globular Cluster Distance Measurement ==<br /> <br /> Attached here is an Excel file with data from two clusters. This is not what I give the kids. I give them LESS data than what is here. I make them take the raw data and knowledge of the distance to NGC 6791 to calculate the stars' absolute values for that cluster. That then becomes the &quot;standard HR Diagram&quot; for stars which they can use to compare to the more distance PAL5 (Palomar 5) cluster for which only apparent magnitude information is given. All this data was pulled from the SDSS using their radial search tools. In this particular file, there is a plot with NGC6791 already on it using its absolute G magnitude. Also plotted is the raw PAL5 apparent G magnitude....and a shifted PAL5. There is a cell labelled &quot;SHIFT&quot; which is the delta-magnitude used for the relationship: m-M = shift = -5+5LOG(D). By entering a shift value, the PAL5 cluster plot is moved up or down relative to the known NGC6791 data. A box labeled &quot;Distance&quot; is then automatically updated to show the distance to PAL5 in parsecs. If anything this is a great way to learn Excel.... and a good way to get into discussions about distance measurements using the HR Diagram, CM diagrams as a whole, and even interstellar reddening if you want. Enjoy!<br /> <br /> &lt;br&gt; [[Media:PAL5_and_ngc6791.xlsx]]<br /> <br /> Theresa here: I simply asked my students to to the activity described the link John sent: http://skyserver.sdss3.org/public/en/proj/advanced/hr/globularcluster.asp<br /> The kids selected the stars, downloaded the data and made graphs with excel. They then copied and pasted their graphs to a google doc and shared them with me. <br /> This is what I got: <br /> &lt;br&gt; [[Media:GlobularClusterHRDiagrams.docx]]<br /> <br /> Tom here: Here are my H-R Diagrams as displayed in &quot;Logger Pro.&quot; I have pasted them into a WORD document. Its easy to see the turn-off for Palomar 5, by the one for Palomar 3 is not nearly as pronounced.<br /> &lt;br&gt; [[Media:Palomar 5 and Palomar 3.docx]]<br /> Here are the graphs of one of my students, both Palomar 3 and Palomar 5<br /> &lt;br&gt; [[Media Palomar 5.xlsx]]<br /> &lt;br&gt; [[Media Palomar 3.xlsx]]<br /> <br /> &lt;br&gt; Nicole here: These are my H-R Diagrams.<br /> [[Media:Granucci Palomar HR Diagram 2013.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_SDSS_Globular_Cluster_CM_Exercise&diff=11748 2013-05-14T16:01:11Z

<p>Rutherford: /* An Exercise in Globular Cluster Distance Measurement */</p> <hr /> <div><br /> <br /> == An Exercise in Globular Cluster Distance Measurement ==<br /> <br /> Attached here is an Excel file with data from two clusters. This is not what I give the kids. I give them LESS data than what is here. I make them take the raw data and knowledge of the distance to NGC 6791 to calculate the stars' absolute values for that cluster. That then becomes the &quot;standard HR Diagram&quot; for stars which they can use to compare to the more distance PAL5 (Palomar 5) cluster for which only apparent magnitude information is given. All this data was pulled from the SDSS using their radial search tools. In this particular file, there is a plot with NGC6791 already on it using its absolute G magnitude. Also plotted is the raw PAL5 apparent G magnitude....and a shifted PAL5. There is a cell labelled &quot;SHIFT&quot; which is the delta-magnitude used for the relationship: m-M = shift = -5+5LOG(D). By entering a shift value, the PAL5 cluster plot is moved up or down relative to the known NGC6791 data. A box labeled &quot;Distance&quot; is then automatically updated to show the distance to PAL5 in parsecs. If anything this is a great way to learn Excel.... and a good way to get into discussions about distance measurements using the HR Diagram, CM diagrams as a whole, and even interstellar reddening if you want. Enjoy!<br /> <br /> &lt;br&gt; [[Media:PAL5_and_ngc6791.xlsx]]<br /> <br /> Theresa here: I simply asked my students to to the activity described the link John sent: http://skyserver.sdss3.org/public/en/proj/advanced/hr/globularcluster.asp<br /> The kids selected the stars, downloaded the data and made graphs with excel. They then copied and pasted their graphs to a google doc and shared them with me. <br /> This is what I got: <br /> &lt;br&gt; [[Media:GlobularClusterHRDiagrams.docx]]<br /> <br /> Tom here: Here are my H-R Diagrams as displayed in &quot;Logger Pro.&quot; I have pasted them into a WORD document. Its easy to see the turn-off for Palomar 5, by the one for Palomar 3 is not nearly as pronounced.<br /> &lt;br&gt; [[Media:Palomar 5 and Palomar 3.docx]]<br /> Here are the graphs of one of my students, both Palomar 3 and Palomar 5<br /> &lt;br&gt; [[Media Palomar 5.xlsx]]<br /> &lt;br&gt; [[Media Palomar 3.xlsx]]<br /> <br /> &lt;br&gt; Nicole here: These are my H-R Diagrams.<br /> [[Media:Granucci Palomar HR Diagram 2013.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_SDSS_Globular_Cluster_CM_Exercise&diff=11744 2013-05-13T16:23:08Z

<p>Rutherford: </p> <hr /> <div><br /> <br /> == An Exercise in Globular Cluster Distance Measurement ==<br /> <br /> Attached here is an Excel file with data from two clusters. This is not what I give the kids. I give them LESS data than what is here. I make them take the raw data and knowledge of the distance to NGC 6791 to calculate the stars' absolute values for that cluster. That then becomes the &quot;standard HR Diagram&quot; for stars which they can use to compare to the more distance PAL5 (Palomar 5) cluster for which only apparent magnitude information is given. All this data was pulled from the SDSS using their radial search tools. In this particular file, there is a plot with NGC6791 already on it using its absolute G magnitude. Also plotted is the raw PAL5 apparent G magnitude....and a shifted PAL5. There is a cell labelled &quot;SHIFT&quot; which is the delta-magnitude used for the relationship: m-M = shift = -5+5LOG(D). By entering a shift value, the PAL5 cluster plot is moved up or down relative to the known NGC6791 data. A box labeled &quot;Distance&quot; is then automatically updated to show the distance to PAL5 in parsecs. If anything this is a great way to learn Excel.... and a good way to get into discussions about distance measurements using the HR Diagram, CM diagrams as a whole, and even interstellar reddening if you want. Enjoy!<br /> <br /> &lt;br&gt; [[Media:PAL5_and_ngc6791.xlsx]]<br /> <br /> Theresa here: I simply asked my students to to the activity described the link John sent: http://skyserver.sdss3.org/public/en/proj/advanced/hr/globularcluster.asp<br /> The kids selected the stars, downloaded the data and made graphs with excel. They then copied and pasted their graphs to a google doc and shared them with me. <br /> This is what I got: <br /> &lt;br&gt; [[Media:GlobularClusterHRDiagrams.docx]]<br /> <br /> Tom here: Here are my H-R Diagrams as displayed in &quot;Logger Pro.&quot; I have pasted them into a WORD document. Its easy to see the turn-off for Palomar 5, by the one for Palomar 3 is not nearly as pronounced.<br /> &lt;br&gt; [[Media:Palomar 5 and Palomar 3.docx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_SDSS_Globular_Cluster_CM_Exercise&diff=11743 2013-05-13T16:21:12Z

<p>Rutherford: /* An Exercise in Globular Cluster Distance Measurement */</p> <hr /> <div><br /> <br /> == An Exercise in Globular Cluster Distance Measurement ==<br /> <br /> Attached here is an Excel file with data from two clusters. This is not what I give the kids. I give them LESS data than what is here. I make them take the raw data and knowledge of the distance to NGC 6791 to calculate the stars' absolute values for that cluster. That then becomes the &quot;standard HR Diagram&quot; for stars which they can use to compare to the more distance PAL5 (Palomar 5) cluster for which only apparent magnitude information is given. All this data was pulled from the SDSS using their radial search tools. In this particular file, there is a plot with NGC6791 already on it using its absolute G magnitude. Also plotted is the raw PAL5 apparent G magnitude....and a shifted PAL5. There is a cell labelled &quot;SHIFT&quot; which is the delta-magnitude used for the relationship: m-M = shift = -5+5LOG(D). By entering a shift value, the PAL5 cluster plot is moved up or down relative to the known NGC6791 data. A box labeled &quot;Distance&quot; is then automatically updated to show the distance to PAL5 in parsecs. If anything this is a great way to learn Excel.... and a good way to get into discussions about distance measurements using the HR Diagram, CM diagrams as a whole, and even interstellar reddening if you want. Enjoy!<br /> <br /> &lt;br&gt; [[Media:PAL5_and_ngc6791.xlsx]]<br /> <br /> Theresa here: I simply asked my students to to the activity described the link John sent: http://skyserver.sdss3.org/public/en/proj/advanced/hr/globularcluster.asp<br /> The kids selected the stars, downloaded the data and made graphs with excel. They then copied and pasted their graphs to a google doc and shared them with me. <br /> This is what I got: <br /> &lt;br&gt; [[Media:GlobularClusterHRDiagrams.docx]]<br /> <br /> Tom here: Here are my H-R Diagrams as displayed in &quot;Logger Pro.&quot; I have pasted them into a WORD document.<br /> &lt;br&gt; [[Media:Palomar 5 and Palomar 3.docx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:--Media-Palomar_5_and_Palomar_3--.docx&diff=11742 2013-05-13T16:11:06Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Palomar_5_and_Palomar_3.docx&diff=11741 2013-05-13T16:07:09Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_SDSS_Globular_Cluster_CM_Exercise&diff=11740 2013-05-13T16:06:38Z

<p>Rutherford: /* An Exercise in Globular Cluster Distance Measurement */</p> <hr /> <div><br /> <br /> == An Exercise in Globular Cluster Distance Measurement ==<br /> <br /> Attached here is an Excel file with data from two clusters. This is not what I give the kids. I give them LESS data than what is here. I make them take the raw data and knowledge of the distance to NGC 6791 to calculate the stars' absolute values for that cluster. That then becomes the &quot;standard HR Diagram&quot; for stars which they can use to compare to the more distance PAL5 (Palomar 5) cluster for which only apparent magnitude information is given. All this data was pulled from the SDSS using their radial search tools. In this particular file, there is a plot with NGC6791 already on it using its absolute G magnitude. Also plotted is the raw PAL5 apparent G magnitude....and a shifted PAL5. There is a cell labelled &quot;SHIFT&quot; which is the delta-magnitude used for the relationship: m-M = shift = -5+5LOG(D). By entering a shift value, the PAL5 cluster plot is moved up or down relative to the known NGC6791 data. A box labeled &quot;Distance&quot; is then automatically updated to show the distance to PAL5 in parsecs. If anything this is a great way to learn Excel.... and a good way to get into discussions about distance measurements using the HR Diagram, CM diagrams as a whole, and even interstellar reddening if you want. Enjoy!<br /> <br /> &lt;br&gt; [[Media:PAL5_and_ngc6791.xlsx]]<br /> <br /> Theresa here: I simply asked my students to to the activity described the link John sent: http://skyserver.sdss3.org/public/en/proj/advanced/hr/globularcluster.asp<br /> The kids selected the stars, downloaded the data and made graphs with excel. They then copied and pasted their graphs to a google doc and shared them with me. <br /> This is what I got: <br /> &lt;br&gt; [[Media:GlobularClusterHRDiagrams.docx]]<br /> <br /> Tom here: Here are my H-R Diagrams as displayed in &quot;Logger Pro.&quot;<br /> &lt;br&gt; [[Media:Palomar 5 and Palomar 3]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:CM4SyProposal-Revision2-tp-vg-jb-vg2-jb2-ng-tp2-jb3-tr3.docx&diff=11579 2013-04-06T18:45:12Z

<p>Rutherford: uploaded a new version of &amp;quot;File:CM4SyProposal-Revision2-tp-vg-jb-vg2-jb2-ng-tp2-jb3-tr3.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:CM4SyProposal-Revision2-tp-vg-jb-vg2-jb2-ng-tp2-jb3-tr3.docx&diff=11578 2013-04-06T18:43:11Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11280 2013-02-24T01:30:08Z

<p>Rutherford: uploaded a new version of &amp;quot;File:Proposal Color-Magnitude Diagram of Seyfert Galaxies TRutherford.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11278 2013-02-24T01:24:22Z

<p>Rutherford: uploaded a new version of &amp;quot;File:Proposal Color-Magnitude Diagram of Seyfert Galaxies TRutherford.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11276 2013-02-23T22:17:17Z

<p>Rutherford: uploaded a new version of &amp;quot;File:Proposal Color-Magnitude Diagram of Seyfert Galaxies TRutherford.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11275 2013-02-23T22:16:17Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal-_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TR.docx&diff=11273 2013-02-23T22:07:28Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal-_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11270 2013-02-23T22:03:03Z

<p>Rutherford: </p> <hr /> <div>[[Media:Proposal:Color-Magnitude Diagram of Seyfert Galaxies_TRutherford]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:Proposal-_Color-Magnitude_Diagram_of_Seyfert_Galaxies_TRutherford.docx&diff=11269 2013-02-23T22:02:00Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:CM4SY_Proposal.docx&diff=11268 2013-02-23T21:58:24Z

<p>Rutherford: uploaded a new version of &amp;quot;File:CM4SY Proposal.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:CM4SY_Proposal.docx&diff=11267 2013-02-23T21:53:38Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:TRutherford_2013_CM4SY_Proposal.docx&diff=11264 2013-02-23T00:13:49Z

<p>Rutherford: uploaded a new version of &amp;quot;File:TRutherford 2013 CM4SY Proposal.docx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:TRutherford_2013_CM4SY_Proposal.docx&diff=11263 2013-02-23T00:11:15Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page01-06-Final-tr.xlsx&diff=11192 2013-02-18T21:15:11Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11191 2013-02-18T21:14:46Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> &lt;br&gt;[[Media:SDSS-Page01-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page02-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page03-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page04-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page05-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page06-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page01-06-Final-tr.xlsx]]<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page01-Final-tr.xlsx&diff=11190 2013-02-18T21:13:57Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page06-Final-tr.xlsx&diff=11189 2013-02-18T21:13:23Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page05-Final-tr.xlsx&diff=11188 2013-02-18T21:12:56Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page04-Final-tr.xlsx&diff=11187 2013-02-18T21:12:28Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page03-Final-tr.xlsx&diff=11186 2013-02-18T21:11:48Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page02-Final-tr.xlsx&diff=11185 2013-02-18T21:11:04Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11184 2013-02-18T20:51:54Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> &lt;br&gt;[[Media:SDSS-Page01-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page02-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page03-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page04-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page05-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page06-Final-tr.xlsx]]<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_03-Final.xlsx&diff=11183 2013-02-18T20:44:15Z

<p>Rutherford: uploaded a new version of &amp;quot;File:SDSS-Page 03-Final.xlsx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_03-Final.xlsx&diff=11182 2013-02-18T20:42:37Z

<p>Rutherford: uploaded a new version of &amp;quot;File:SDSS-Page 03-Final.xlsx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_02-Final.xlsx&diff=11179 2013-02-18T15:07:50Z

<p>Rutherford: uploaded a new version of &amp;quot;File:SDSS-Page 02-Final.xlsx&amp;quot;</p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_01-Final-tr.xlsx&diff=11178 2013-02-18T14:39:04Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11177 2013-02-18T13:51:59Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> &lt;br&gt;[[Media:SDSS-Page 01-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 02-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 03-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 04-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 05-Final-tr.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 06-Final-tr.xlsx]]<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11176 2013-02-18T13:50:57Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> &lt;br&gt;[[Media:SDSS-Page 01-Final.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 02-Final.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 03-Final.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 04-Final.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 05-Final.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page 06-Final.xlsx]]<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11175 2013-02-18T00:55:54Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> [[Media:SDSS-Page 01-Final.xlsx<br /> [[Media:SDSS-Page 02-Final.xlsx<br /> [[Media:SDSS-Page 03-Final.xlsx<br /> [[Media:SDSS-Page 04-Final.xlsx<br /> [[Media:SDSS-Page 05-Final.xlsx<br /> [[Media:SDSS-Page 06-Final.xlsx<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11174 2013-02-18T00:55:39Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> &lt;br&gt;[[Media:SDSS-Page 01-Final.xlsx<br /> [[Media:SDSS-Page 02-Final.xlsx<br /> [[Media:SDSS-Page 03-Final.xlsx<br /> [[Media:SDSS-Page 04-Final.xlsx<br /> [[Media:SDSS-Page 05-Final.xlsx<br /> [[Media:SDSS-Page 06-Final.xlsx<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=CM4Seyferts_data&diff=11173 2013-02-18T00:55:07Z

<p>Rutherford: </p> <hr /> <div>Data for Seyferts 1 - NED/SDSS Extraction<br /> <br /> Page 1-6<br /> [[Media:SDSS-Page 01-Final.xlsx<br /> [[Media:SDSS-Page 02-Final.xlsx<br /> [[Media:SDSS-Page 03-Final.xlsx<br /> [[Media:SDSS-Page 04-Final.xlsx<br /> [[Media:SDSS-Page 05-Final.xlsx<br /> [[Media:SDSS-Page 06-Final.xlsx<br /> <br /> Page 6-11<br /> &lt;br&gt;[[Media:SDSS-Page6-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page7-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page8-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page9-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page10-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Page11-final-tp.xlsx]]<br /> &lt;br&gt;[[Media:SDSS-Pages6-11-final-tp.xlsx]]<br /> <br /> Page 11-16<br /> &lt;br&gt;[[Media:sdss-page11-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page12-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page13-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page14-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page15-ng.xlsx]]<br /> &lt;br&gt;[[Media:sdss-page16-ng.xlsx]]<br /> <br /> Page 16-21<br /> &lt;br&gt;[[Media:sdss-page16-21-jb.xlsx]]</div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_06-Final.xlsx&diff=11163 2013-02-17T00:50:33Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_05-Final.xlsx&diff=11162 2013-02-17T00:50:15Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_04-Final.xlsx&diff=11161 2013-02-17T00:49:58Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_03-Final.xlsx&diff=11160 2013-02-17T00:49:35Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_02-Final.xlsx&diff=11159 2013-02-17T00:49:15Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford https://vmcoolwiki.ipac.caltech.edu/index.php?title=File:SDSS-Page_01-Final.xlsx&diff=11158 2013-02-17T00:41:46Z

<p>Rutherford: </p> <hr /> <div></div>

Rutherford