{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2025,10,19]],"date-time":"2025-10-19T06:11:35Z","timestamp":1760854295375,"version":"3.37.3"},"reference-count":11,"publisher":"Springer Science and Business Media LLC","issue":"5-6","license":[{"start":{"date-parts":[[2022,9,5]],"date-time":"2022-09-05T00:00:00Z","timestamp":1662336000000},"content-version":"tdm","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0"},{"start":{"date-parts":[[2022,9,5]],"date-time":"2022-09-05T00:00:00Z","timestamp":1662336000000},"content-version":"vor","delay-in-days":0,"URL":"https:\/\/creativecommons.org\/licenses\/by\/4.0"}],"funder":[{"name":"Deutsche Forschung Gemeinschaft","award":["EXC-2094 - 390783311"],"award-info":[{"award-number":["EXC-2094 - 390783311"]}]},{"name":"Max Planck Institute for Physics"}],"content-domain":{"domain":["link.springer.com"],"crossmark-restriction":false},"short-container-title":["J Low Temp Phys"],"published-print":{"date-parts":[[2022,12]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>The experimental detection of the CE<jats:inline-formula><jats:alternatives><jats:tex-math>$$\\nu$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mi>\u03bd<\/mml:mi>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula>NS allows the investigation of neutrinos and neutrino sources with all-flavor sensitivity. Given its large content in neutrons and stability, Pb is a very appealing choice as target element. The presence of the radioisotope <jats:inline-formula><jats:alternatives><jats:tex-math>$$^{210}$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:msup>\n                    <mml:mrow\/>\n                    <mml:mn>210<\/mml:mn>\n                  <\/mml:msup>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula>Pb (T<jats:inline-formula><jats:alternatives><jats:tex-math>$$_{1\/2}\\sim$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mrow>\n                    <mml:msub>\n                      <mml:mrow\/>\n                      <mml:mrow>\n                        <mml:mn>1<\/mml:mn>\n                        <mml:mo>\/<\/mml:mo>\n                        <mml:mn>2<\/mml:mn>\n                      <\/mml:mrow>\n                    <\/mml:msub>\n                    <mml:mo>\u223c<\/mml:mo>\n                  <\/mml:mrow>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula>22 yrs) makes natural Pb unsuitable for low-background, low-energy event searches. This limitation can be overcome employing Pb of archaeological origin, where several half-lives of <jats:inline-formula><jats:alternatives><jats:tex-math>$$^{210}$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:msup>\n                    <mml:mrow\/>\n                    <mml:mn>210<\/mml:mn>\n                  <\/mml:msup>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula>Pb have gone by. We present results of a cryogenic measurement of a 15 g PbWO<jats:inline-formula><jats:alternatives><jats:tex-math>$$_4$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:msub>\n                    <mml:mrow\/>\n                    <mml:mn>4<\/mml:mn>\n                  <\/mml:msub>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula> crystal, grown with archaeological Pb (older than <jats:inline-formula><jats:alternatives><jats:tex-math>$$\\sim$$<\/jats:tex-math><mml:math xmlns:mml=\"http:\/\/www.w3.org\/1998\/Math\/MathML\">\n                  <mml:mo>\u223c<\/mml:mo>\n                <\/mml:math><\/jats:alternatives><\/jats:inline-formula>2000 yrs) that achieved a sub-keV nuclear recoil detection threshold. A ton-scale experiment employing such material, with a detection threshold for nuclear recoils of just 1 keV would probe the entire Milky Way for SuperNovae, with equal sensitivity for all neutrino flavors, allowing the study of the core of such exceptional events.<\/jats:p>","DOI":"10.1007\/s10909-022-02823-8","type":"journal-article","created":{"date-parts":[[2022,9,5]],"date-time":"2022-09-05T20:37:13Z","timestamp":1662410233000},"page":"872-878","update-policy":"https:\/\/doi.org\/10.1007\/springer_crossmark_policy","source":"Crossref","is-referenced-by-count":3,"title":["Operation of an Archaeological Lead PbWO$$_4$$ Crystal to Search for Neutrinos from Astrophysical Sources with a Transition Edge Sensor"],"prefix":"10.1007","volume":"209","author":[{"ORCID":"https:\/\/orcid.org\/0000-0001-5226-6626","authenticated-orcid":false,"given":"N.","family":"Ferreiro Iachellini","sequence":"first","affiliation":[]},{"given":"L.","family":"Pattavina","sequence":"additional","affiliation":[]},{"given":"A. 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