Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos
Supernova neutrinos are invaluable signals that offer information about the interior of supernovae. Because a nearby supernova can occur at any time, preparing for future supernova neutrino observation is an urgent task. For the prompt analysis of supernova neutrinos, we have developed a new analysi...
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| creator | Harada, Akira Suwa, Yudai Harada, Masayuki Koshio, Yusuke Mori, Masamitsu Nakanishi, Fumi Nakazato, Ken'ichiro Sumiyoshi, Kohsuke Wendell, Roger A |
| description | Supernova neutrinos are invaluable signals that offer information about the
interior of supernovae. Because a nearby supernova can occur at any time,
preparing for future supernova neutrino observation is an urgent task. For the
prompt analysis of supernova neutrinos, we have developed a new analysis code,
``Supernova Parameter Estimation Code based on Insight on Analytic Late-time
Burst Light curve at Earth Neutrino Detector (SPECIAL BLEND)''. This code
estimates the parameters of supernova based on an analytic model of supernova
neutrinos from the proto-neutron star cooling phase. For easy availability to
the community, this code is public and easily runs on web environments. SPECIAL
BLEND can estimate the parameters better than the analysis pipeline we
developed in the previous paper. By using SPECIAL BLEND, we can estimate the
supernova parameters within $10\%$ precision up to $\sim 20\,{\rm kpc}$ and
$\sim 60\,{\rm kpc}$ (Large Magellanic Cloud contained) with Super Kamiokande
and Hyper Kamiokande, respectively. |
| doi_str_mv | 10.48550/arxiv.2304.05437 |
| format | Article |
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interior of supernovae. Because a nearby supernova can occur at any time,
preparing for future supernova neutrino observation is an urgent task. For the
prompt analysis of supernova neutrinos, we have developed a new analysis code,
``Supernova Parameter Estimation Code based on Insight on Analytic Late-time
Burst Light curve at Earth Neutrino Detector (SPECIAL BLEND)''. This code
estimates the parameters of supernova based on an analytic model of supernova
neutrinos from the proto-neutron star cooling phase. For easy availability to
the community, this code is public and easily runs on web environments. SPECIAL
BLEND can estimate the parameters better than the analysis pipeline we
developed in the previous paper. By using SPECIAL BLEND, we can estimate the
supernova parameters within $10\%$ precision up to $\sim 20\,{\rm kpc}$ and
$\sim 60\,{\rm kpc}$ (Large Magellanic Cloud contained) with Super Kamiokande
and Hyper Kamiokande, respectively.</description><identifier>DOI: 10.48550/arxiv.2304.05437</identifier><language>eng</language><subject>Physics - High Energy Astrophysical Phenomena ; Physics - Solar and Stellar Astrophysics</subject><creationdate>2023-04</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2304.05437$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2304.05437$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Harada, Akira</creatorcontrib><creatorcontrib>Suwa, Yudai</creatorcontrib><creatorcontrib>Harada, Masayuki</creatorcontrib><creatorcontrib>Koshio, Yusuke</creatorcontrib><creatorcontrib>Mori, Masamitsu</creatorcontrib><creatorcontrib>Nakanishi, Fumi</creatorcontrib><creatorcontrib>Nakazato, Ken'ichiro</creatorcontrib><creatorcontrib>Sumiyoshi, Kohsuke</creatorcontrib><creatorcontrib>Wendell, Roger A</creatorcontrib><title>Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos</title><description>Supernova neutrinos are invaluable signals that offer information about the
interior of supernovae. Because a nearby supernova can occur at any time,
preparing for future supernova neutrino observation is an urgent task. For the
prompt analysis of supernova neutrinos, we have developed a new analysis code,
``Supernova Parameter Estimation Code based on Insight on Analytic Late-time
Burst Light curve at Earth Neutrino Detector (SPECIAL BLEND)''. This code
estimates the parameters of supernova based on an analytic model of supernova
neutrinos from the proto-neutron star cooling phase. For easy availability to
the community, this code is public and easily runs on web environments. SPECIAL
BLEND can estimate the parameters better than the analysis pipeline we
developed in the previous paper. By using SPECIAL BLEND, we can estimate the
supernova parameters within $10\%$ precision up to $\sim 20\,{\rm kpc}$ and
$\sim 60\,{\rm kpc}$ (Large Magellanic Cloud contained) with Super Kamiokande
and Hyper Kamiokande, respectively.</description><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Solar and Stellar Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNptkM1OwkAURrtxYdAHcOV9gdZh2pm27rCgEhsggbglt9M7MLF0mukP8iC-rwFcuvo2X85Jjuc9jFkQJUKwJ3TfZgh4yKKAiSiMb72fZdGSG0y9g3XfkKvtgLCgvnOmtpCb3b6DrHcDtXA03f568j_wYOwX1iUFMP8MYEoDVbY5UN2B1bBezbL5JIeXfLaYPsMZeIRVX1RGwaTG6tSaFjJbEmjr_vG2d96Nxqql-78deZvX2SZ79_Pl2zyb5D7KOPZFlCSlxDRVJJnSjBcKC5UwyYskJo1ScJQRLxXytNSUxmOpBWqpk7HSJHg48h6v2EuXbePMAd1pe-6zvfQJfwH40GIK</recordid><startdate>20230411</startdate><enddate>20230411</enddate><creator>Harada, Akira</creator><creator>Suwa, Yudai</creator><creator>Harada, Masayuki</creator><creator>Koshio, Yusuke</creator><creator>Mori, Masamitsu</creator><creator>Nakanishi, Fumi</creator><creator>Nakazato, Ken'ichiro</creator><creator>Sumiyoshi, Kohsuke</creator><creator>Wendell, Roger A</creator><scope>GOX</scope></search><sort><creationdate>20230411</creationdate><title>Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos</title><author>Harada, Akira ; Suwa, Yudai ; Harada, Masayuki ; Koshio, Yusuke ; Mori, Masamitsu ; Nakanishi, Fumi ; Nakazato, Ken'ichiro ; Sumiyoshi, Kohsuke ; Wendell, Roger A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a677-5488d6a99ce60cf02bcabc8062b87efa652a642dca29dfe9716f5af6f81cfe523</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Solar and Stellar Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Harada, Akira</creatorcontrib><creatorcontrib>Suwa, Yudai</creatorcontrib><creatorcontrib>Harada, Masayuki</creatorcontrib><creatorcontrib>Koshio, Yusuke</creatorcontrib><creatorcontrib>Mori, Masamitsu</creatorcontrib><creatorcontrib>Nakanishi, Fumi</creatorcontrib><creatorcontrib>Nakazato, Ken'ichiro</creatorcontrib><creatorcontrib>Sumiyoshi, Kohsuke</creatorcontrib><creatorcontrib>Wendell, Roger A</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Harada, Akira</au><au>Suwa, Yudai</au><au>Harada, Masayuki</au><au>Koshio, Yusuke</au><au>Mori, Masamitsu</au><au>Nakanishi, Fumi</au><au>Nakazato, Ken'ichiro</au><au>Sumiyoshi, Kohsuke</au><au>Wendell, Roger A</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos</atitle><date>2023-04-11</date><risdate>2023</risdate><abstract>Supernova neutrinos are invaluable signals that offer information about the
interior of supernovae. Because a nearby supernova can occur at any time,
preparing for future supernova neutrino observation is an urgent task. For the
prompt analysis of supernova neutrinos, we have developed a new analysis code,
``Supernova Parameter Estimation Code based on Insight on Analytic Late-time
Burst Light curve at Earth Neutrino Detector (SPECIAL BLEND)''. This code
estimates the parameters of supernova based on an analytic model of supernova
neutrinos from the proto-neutron star cooling phase. For easy availability to
the community, this code is public and easily runs on web environments. SPECIAL
BLEND can estimate the parameters better than the analysis pipeline we
developed in the previous paper. By using SPECIAL BLEND, we can estimate the
supernova parameters within $10\%$ precision up to $\sim 20\,{\rm kpc}$ and
$\sim 60\,{\rm kpc}$ (Large Magellanic Cloud contained) with Super Kamiokande
and Hyper Kamiokande, respectively.</abstract><doi>10.48550/arxiv.2304.05437</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics |
| title | Observing Supernova Neutrino Light Curves with Super-Kamiokande. IV. Development of SPECIAL BLEND: a New Public Analysis Code for Supernova Neutrinos |
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