<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-19T21:38:04Z</responseDate><request verb="GetRecord" identifier="oai:dspace.mit.edu:1721.1/114124" metadataPrefix="dim">https://dspace.mit.edu/server/oai/request</request><GetRecord><record><header><identifier>oai:dspace.mit.edu:1721.1/114124</identifier><datestamp>2022-01-13T07:53:59Z</datestamp><setSpec>com_1721.1_7582</setSpec><setSpec>com_1721.1_7581</setSpec><setSpec>col_1721.1_131024</setSpec></header><metadata><dim:dim xmlns:dim="http://www.dspace.org/xmlns/dspace/dim" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.dspace.org/xmlns/dspace/dim http://www.dspace.org/schema/dim.xsd">
   <dim:field mdschema="dc" element="contributor" qualifier="advisor" lang="en_US">Richard Binzel and Michael Person.</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="author" lang="en_US">Kosiarek, Molly (Molly R.)</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="other" lang="en_US">Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences.</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="department">Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="accessioned">2018-03-12T19:30:54Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="available">2018-03-12T19:30:54Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="copyright" lang="en_US">2015</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="issued" lang="en_US">2015</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="uri">http://hdl.handle.net/1721.1/114124</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="oclc" lang="en_US">1027722746</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">Thesis: S.B., Massachusetts Institute of Technology, Department of Earth, Atmospheric, and Planetary Sciences, 2015.</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">Cataloged from PDF version of thesis.</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">Includes bibliographical references (pages 75-76).</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="abstract" lang="en_US">The construction and characterization of an autonomous telescope began in Fall 2014 at the MIT George R. Wallace, Jr. Astrophysical Observatory. An 11-inch Cassegrain Telescope was assembled in a 10-foot Technical Innovations ProDome. This telescope, the Small AUtonomous Robotic Optical Nightwatcher (SAURON), has the potential to autonomously collect photometric images. Data were taken on T-And0-15785, an eclipsing binary star, in order to test and characterize the system. The out-of-ecliptic R magnitude of T-AndO-15785 was found to be 13.487 ± 0.016. The magnitude changes for the primary and secondary eclipses were found to be 0.72 ± 0.036 and 0.62 ± 0.031 R magnitudes respectively. The telescope, SAURON, is currently able to locate targets and collect data robotically with an observer monitoring from afar.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="statementofresponsibility" lang="en_US">by Molly Kosiarek.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="degree" lang="en_US">S.B.</dim:field>
   <dim:field mdschema="dc" element="format" qualifier="extent" lang="en_US">76 pages</dim:field>
   <dim:field mdschema="dc" element="language" qualifier="iso" lang="en_US">eng</dim:field>
   <dim:field mdschema="dc" element="publisher" lang="en_US">Massachusetts Institute of Technology</dim:field>
   <dim:field mdschema="dc" element="rights" lang="en_US">MIT theses are protected by copyright. They may be viewed, downloaded, or printed from this source but further reproduction or distribution in any format is prohibited without written permission.</dim:field>
   <dim:field mdschema="dc" element="rights" qualifier="uri" lang="en_US">http://dspace.mit.edu/handle/1721.1/7582</dim:field>
   <dim:field mdschema="dc" element="subject" lang="en_US">Earth, Atmospheric, and Planetary Sciences.</dim:field>
   <dim:field mdschema="dc" element="title" lang="en_US">First autonomous telescope at Wallace Observatory : impact and preliminary results</dim:field>
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   	&lt;Title>First autonomous telescope at Wallace Observatory : impact and preliminary results&lt;/Title>
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   	&lt;PublicationDate>2015&lt;/PublicationDate>
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        	&lt;DisplayName>Kosiarek, Molly (Molly R.)&lt;/DisplayName>
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    &lt;Keyword>Earth, Atmospheric, and Planetary Sciences.&lt;/Keyword>
   	&lt;Abstract>The construction and characterization of an autonomous telescope began in Fall 2014 at the MIT George R. Wallace, Jr. Astrophysical Observatory. An 11-inch Cassegrain Telescope was assembled in a 10-foot Technical Innovations ProDome. This telescope, the Small AUtonomous Robotic Optical Nightwatcher (SAURON), has the potential to autonomously collect photometric images. Data were taken on T-And0-15785, an eclipsing binary star, in order to test and characterize the system. The out-of-ecliptic R magnitude of T-AndO-15785 was found to be 13.487 ± 0.016. The magnitude changes for the primary and secondary eclipses were found to be 0.72 ± 0.036 and 0.62 ± 0.031 R magnitudes respectively. The telescope, SAURON, is currently able to locate targets and collect data robotically with an observer monitoring from afar.&lt;/Abstract>
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