<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>The Haystack Telescope as an Astronomical Instrument</dc:title><dc:creator>Kauffmann, Jens; Rajagopalan, Ganesh; Akiyama, Kazunori; Fish, Vincent; Lonsdale, Colin; Matthews, Lynn D.; Pillai, Thushara G.S.</dc:creator><dc:corporate_author/><dc:editor/><dc:description>The Haystack Telescope is an antenna with a diameter of 37 m and an elevation-dependent surface accuracy of ≤100μm that is capable of millimeter-wave observations. The radome-enclosed instrument serves as a radar sensor for space situational awareness, with about one-third of the time available for research by MIT Haystack Observatory. Ongoing testing with the K-band (18–26 GHz) and W-band receivers (currently 85–93 GHz) is preparing the inclusion of the telescope into the Event Horizon Telescope (EHT) array and the use as a single-dish research telescope. Given its geographic location, the addition of the Haystack Telescope to current and future versions of the EHT array would substantially improve the image quality.</dc:description><dc:publisher/><dc:date>2023-02-01</dc:date><dc:nsf_par_id>10436894</dc:nsf_par_id><dc:journal_name>Galaxies</dc:journal_name><dc:journal_volume>11</dc:journal_volume><dc:journal_issue>1</dc:journal_issue><dc:page_range_or_elocation>9</dc:page_range_or_elocation><dc:issn>2075-4434</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.3390/galaxies11010009</dc:doi><dcq:identifierAwardId>2309542; 2108989; 1935980; 2309536</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>