{
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  "authors": [
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Kernphysik, Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster, Wilhelm-Klemm-Stra\u00dfe 9, M\u00fcnster, 48149, Germany", 
          "organization": "Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster"
        }
      ], 
      "surname": "Lozano Mariscal", 
      "email": "c.lozano@wwu.de", 
      "full_name": "Lozano Mariscal, C.", 
      "given_names": "C."
    }, 
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Kernphysik, Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster, Wilhelm-Klemm-Stra\u00dfe 9, M\u00fcnster, 48149, Germany", 
          "organization": "Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster"
        }
      ], 
      "surname": "Classen", 
      "given_names": "L.", 
      "full_name": "Classen, L."
    }, 
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Kernphysik, Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster, Wilhelm-Klemm-Stra\u00dfe 9, M\u00fcnster, 48149, Germany", 
          "organization": "Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster"
        }
      ], 
      "surname": "Unland Elorrieta", 
      "given_names": "M.", 
      "full_name": "Unland Elorrieta, M."
    }, 
    {
      "affiliations": [
        {
          "country": "Germany", 
          "value": "Institut f\u00fcr Kernphysik, Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster, Wilhelm-Klemm-Stra\u00dfe 9, M\u00fcnster, 48149, Germany", 
          "organization": "Westf\u00e4lische Wilhelms-Universit\u00e4t M\u00fcnster"
        }
      ], 
      "surname": "Kappes", 
      "given_names": "A.", 
      "full_name": "Kappes, A."
    }
  ], 
  "titles": [
    {
      "source": "Springer", 
      "title": "Sensitivity of multi-PMT optical modules in Antarctic ice to supernova neutrinos of MeV energy"
    }
  ], 
  "dois": [
    {
      "value": "10.1140/epjc/s10052-021-09809-y"
    }
  ], 
  "publication_info": [
    {
      "page_end": "11", 
      "journal_title": "European Physical Journal C", 
      "material": "article", 
      "journal_volume": "81", 
      "artid": "s10052-021-09809-y", 
      "year": 2021, 
      "page_start": "1", 
      "journal_issue": "12"
    }
  ], 
  "$schema": "http://repo.scoap3.org/schemas/hep.json", 
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    "date": "2022-08-01T15:30:09.837419", 
    "source": "Springer", 
    "method": "Springer", 
    "submission_number": "ce4eabba11ae11eda1a1661ec451a4e4"
  }, 
  "page_nr": [
    11
  ], 
  "license": [
    {
      "url": "https://creativecommons.org/licenses//by/4.0", 
      "license": "CC-BY-4.0"
    }
  ], 
  "copyright": [
    {
      "holder": "The Author(s)", 
      "year": "2021"
    }
  ], 
  "control_number": "66323", 
  "record_creation_date": "2021-12-01T21:30:22.731224", 
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  "collections": [
    {
      "primary": "European Physical Journal C"
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  "arxiv_eprints": [
    {
      "categories": [
        "astro-ph.HE", 
        "astro-ph.IM", 
        "physics.ins-det"
      ], 
      "value": "2106.14199"
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  ], 
  "abstracts": [
    {
      "source": "Springer", 
      "value": "New optical sensors with a segmented photosensitive area are being developed for the next generation of neutrino telescopes at the South Pole. In addition to increasing sensitivity to high-energy astrophysical neutrinos, we show that this will also lead to a significant improvement in sensitivity to MeV neutrinos, such as those produced in core-collapse supernovae (CCSN). These low-energy neutrinos can provide a detailed picture of the events after stellar core collapse, testing our understanding of these violent explosions. We present studies on the event-based detection of MeV neutrinos with a segmented sensor and, for the first time, the potential of a corresponding detector in the deep ice at the South Pole for the detection of extra-galactic CCSN. We find that exploiting temporal coincidences between signals in different photocathode segments, a  $$27\\ \\mathrm {M}_{\\odot }$$  <math> <mrow> <mn>27</mn> <mspace width=\"4pt\"></mspace> <msub> <mi>M</mi> <mo>\u2299</mo> </msub> </mrow> </math>   progenitor mass CCSN can be detected up to a distance of 341 kpc with a false detection rate of  $${0.01}\\,\\hbox {year}^{-1}$$  <math> <mrow> <mrow> <mn>0.01</mn> </mrow> <mspace width=\"0.166667em\"></mspace> <msup> <mtext>year</mtext> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> </mrow> </math>   with a detector consisting of 10,000 sensors. Increasing the number of sensors to 20,000 and reducing the optical background by a factor of 70 expands the range such that a CCSN detection rate of 0.1 per year is achieved, while keeping the false detection rate at  $${0.01}\\,{\\hbox {year}^{-1}}$$  <math> <mrow> <mrow> <mn>0.01</mn> </mrow> <mspace width=\"0.166667em\"></mspace> <msup> <mtext>year</mtext> <mrow> <mo>-</mo> <mn>1</mn> </mrow> </msup> </mrow> </math>  ."
    }
  ], 
  "imprints": [
    {
      "date": "2021-12-01", 
      "publisher": "Springer"
    }
  ]
}