Evidence of weak circumstellar medium interaction in the Type II SN 2023axu
We present high-cadence photometric and spectroscopic observations of SN~2023axu, a classical Type II supernova with an absolute \(V\)-band peak magnitude of \(-16.5 \pm 0.1\) mag. SN~2023axu was discovered by the Distance Less Than 40 Mpc (DLT40) survey within 1 day of the last non-detection in the...
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| creator | Shrestha, Manisha Pearson, Jeniveve Wyatt, Samuel Sand, David J Griffin Hosseinzadeh Bostroem, K Azalee Andrews, Jennifer E Dong, Yize Hoang, Emily Janzen, Daryl Jencson, Jacob E Lundquist, M J Mehta, Darshana Nicolas Meza Retamal Valenti, Stefano Rastinejad, Jillian C Daly, Phil Porter, Dallan Hinz, Joannah Self, Skyler Weiner, Benjamin Williams, Grant G Hiramatsu, Daichi Howell, D Andrew McCully, Curtis Estefania Padilla Gonzalez Pellegrino, Craig Terreran, Giacomo Newsome, Megan Farah, Joseph Itagaki, Koichi Jha, Saurabh W Kwok, Lindsey Smith, Nathan Schwab, Michaela Rho, Jeonghee Yang, Yi |
| description | We present high-cadence photometric and spectroscopic observations of SN~2023axu, a classical Type II supernova with an absolute \(V\)-band peak magnitude of \(-16.5 \pm 0.1\) mag. SN~2023axu was discovered by the Distance Less Than 40 Mpc (DLT40) survey within 1 day of the last non-detection in the nearby galaxy NGC 2283 at 13.7 Mpc. We modeled the early light curve using a recently updated shock cooling model that includes the effects of line blanketing and found the explosion epoch to be MJD 59971.48 \(\pm\) 0.03 and the probable progenitor to be a red supergiant with a radius of 417 \(\pm\) 28 \(R_\odot\). The shock cooling model cannot match the rise of observed data in the \(r\) and \(i\) bands and underpredicts the overall UV data which points to possible interaction with circumstellar material. This interpretation is further supported by spectral behavior. We see a ledge feature around 4600 \AA\ in the very early spectra (+1.1 and +1.5 days after the explosion) which can be a sign of circumstellar interaction. The signs of circumstellar material are further bolstered by the presence of absorption features blueward of H\(\alpha\) and H\(\beta\) at day \(>\)40 which is also generally attributed to circumstellar interaction. Our analysis shows the need for high-cadence early photometric and spectroscopic data to decipher the mass-loss history of the progenitor. |
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| fullrecord | <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2871973146</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2871973146</sourcerecordid><originalsourceid>FETCH-proquest_journals_28719731463</originalsourceid><addsrcrecordid>eNqNiksKwjAUAIMgWLR3eOC60Cb9uZaKRXBj9xLSV0xtk5qPn9vbhQdwNQMzCxJQxpKoTCldkdDaPo5jmhc0y1hATtVTtqgEgu7ghfwOQhrhR-twGLiBEVvpR5DKoeHCSa1mB3dDaD4TQl3D5Qw0poy__YYsOz5YDH9ck-2havbHaDL64dG6a6-9UXO60rJIdgVL0pz9d30Bit47zQ</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2871973146</pqid></control><display><type>article</type><title>Evidence of weak circumstellar medium interaction in the Type II SN 2023axu</title><source>Freely Accessible Journals</source><creator>Shrestha, Manisha ; Pearson, Jeniveve ; Wyatt, Samuel ; Sand, David J ; Griffin Hosseinzadeh ; Bostroem, K Azalee ; Andrews, Jennifer E ; Dong, Yize ; Hoang, Emily ; Janzen, Daryl ; Jencson, Jacob E ; Lundquist, M J ; Mehta, Darshana ; Nicolas Meza Retamal ; Valenti, Stefano ; Rastinejad, Jillian C ; Daly, Phil ; Porter, Dallan ; Hinz, Joannah ; Self, Skyler ; Weiner, Benjamin ; Williams, Grant G ; Hiramatsu, Daichi ; Howell, D Andrew ; McCully, Curtis ; Estefania Padilla Gonzalez ; Pellegrino, Craig ; Terreran, Giacomo ; Newsome, Megan ; Farah, Joseph ; Itagaki, Koichi ; Jha, Saurabh W ; Kwok, Lindsey ; Smith, Nathan ; Schwab, Michaela ; Rho, Jeonghee ; Yang, Yi</creator><creatorcontrib>Shrestha, Manisha ; Pearson, Jeniveve ; Wyatt, Samuel ; Sand, David J ; Griffin Hosseinzadeh ; Bostroem, K Azalee ; Andrews, Jennifer E ; Dong, Yize ; Hoang, Emily ; Janzen, Daryl ; Jencson, Jacob E ; Lundquist, M J ; Mehta, Darshana ; Nicolas Meza Retamal ; Valenti, Stefano ; Rastinejad, Jillian C ; Daly, Phil ; Porter, Dallan ; Hinz, Joannah ; Self, Skyler ; Weiner, Benjamin ; Williams, Grant G ; Hiramatsu, Daichi ; Howell, D Andrew ; McCully, Curtis ; Estefania Padilla Gonzalez ; Pellegrino, Craig ; Terreran, Giacomo ; Newsome, Megan ; Farah, Joseph ; Itagaki, Koichi ; Jha, Saurabh W ; Kwok, Lindsey ; Smith, Nathan ; Schwab, Michaela ; Rho, Jeonghee ; Yang, Yi</creatorcontrib><description>We present high-cadence photometric and spectroscopic observations of SN~2023axu, a classical Type II supernova with an absolute \(V\)-band peak magnitude of \(-16.5 \pm 0.1\) mag. SN~2023axu was discovered by the Distance Less Than 40 Mpc (DLT40) survey within 1 day of the last non-detection in the nearby galaxy NGC 2283 at 13.7 Mpc. We modeled the early light curve using a recently updated shock cooling model that includes the effects of line blanketing and found the explosion epoch to be MJD 59971.48 \(\pm\) 0.03 and the probable progenitor to be a red supergiant with a radius of 417 \(\pm\) 28 \(R_\odot\). The shock cooling model cannot match the rise of observed data in the \(r\) and \(i\) bands and underpredicts the overall UV data which points to possible interaction with circumstellar material. This interpretation is further supported by spectral behavior. We see a ledge feature around 4600 \AA\ in the very early spectra (+1.1 and +1.5 days after the explosion) which can be a sign of circumstellar interaction. The signs of circumstellar material are further bolstered by the presence of absorption features blueward of H\(\alpha\) and H\(\beta\) at day \(>\)40 which is also generally attributed to circumstellar interaction. Our analysis shows the need for high-cadence early photometric and spectroscopic data to decipher the mass-loss history of the progenitor.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Blanketing ; Light curve ; Photometry ; Red giant stars ; Shock cooling ; Supergiant stars</subject><ispartof>arXiv.org, 2023-09</ispartof><rights>2023. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</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>781,785</link.rule.ids></links><search><creatorcontrib>Shrestha, Manisha</creatorcontrib><creatorcontrib>Pearson, Jeniveve</creatorcontrib><creatorcontrib>Wyatt, Samuel</creatorcontrib><creatorcontrib>Sand, David J</creatorcontrib><creatorcontrib>Griffin Hosseinzadeh</creatorcontrib><creatorcontrib>Bostroem, K Azalee</creatorcontrib><creatorcontrib>Andrews, Jennifer E</creatorcontrib><creatorcontrib>Dong, Yize</creatorcontrib><creatorcontrib>Hoang, Emily</creatorcontrib><creatorcontrib>Janzen, Daryl</creatorcontrib><creatorcontrib>Jencson, Jacob E</creatorcontrib><creatorcontrib>Lundquist, M J</creatorcontrib><creatorcontrib>Mehta, Darshana</creatorcontrib><creatorcontrib>Nicolas Meza Retamal</creatorcontrib><creatorcontrib>Valenti, Stefano</creatorcontrib><creatorcontrib>Rastinejad, Jillian C</creatorcontrib><creatorcontrib>Daly, Phil</creatorcontrib><creatorcontrib>Porter, Dallan</creatorcontrib><creatorcontrib>Hinz, Joannah</creatorcontrib><creatorcontrib>Self, Skyler</creatorcontrib><creatorcontrib>Weiner, Benjamin</creatorcontrib><creatorcontrib>Williams, Grant G</creatorcontrib><creatorcontrib>Hiramatsu, Daichi</creatorcontrib><creatorcontrib>Howell, D Andrew</creatorcontrib><creatorcontrib>McCully, Curtis</creatorcontrib><creatorcontrib>Estefania Padilla Gonzalez</creatorcontrib><creatorcontrib>Pellegrino, Craig</creatorcontrib><creatorcontrib>Terreran, Giacomo</creatorcontrib><creatorcontrib>Newsome, Megan</creatorcontrib><creatorcontrib>Farah, Joseph</creatorcontrib><creatorcontrib>Itagaki, Koichi</creatorcontrib><creatorcontrib>Jha, Saurabh W</creatorcontrib><creatorcontrib>Kwok, Lindsey</creatorcontrib><creatorcontrib>Smith, Nathan</creatorcontrib><creatorcontrib>Schwab, Michaela</creatorcontrib><creatorcontrib>Rho, Jeonghee</creatorcontrib><creatorcontrib>Yang, Yi</creatorcontrib><title>Evidence of weak circumstellar medium interaction in the Type II SN 2023axu</title><title>arXiv.org</title><description>We present high-cadence photometric and spectroscopic observations of SN~2023axu, a classical Type II supernova with an absolute \(V\)-band peak magnitude of \(-16.5 \pm 0.1\) mag. SN~2023axu was discovered by the Distance Less Than 40 Mpc (DLT40) survey within 1 day of the last non-detection in the nearby galaxy NGC 2283 at 13.7 Mpc. We modeled the early light curve using a recently updated shock cooling model that includes the effects of line blanketing and found the explosion epoch to be MJD 59971.48 \(\pm\) 0.03 and the probable progenitor to be a red supergiant with a radius of 417 \(\pm\) 28 \(R_\odot\). The shock cooling model cannot match the rise of observed data in the \(r\) and \(i\) bands and underpredicts the overall UV data which points to possible interaction with circumstellar material. This interpretation is further supported by spectral behavior. We see a ledge feature around 4600 \AA\ in the very early spectra (+1.1 and +1.5 days after the explosion) which can be a sign of circumstellar interaction. The signs of circumstellar material are further bolstered by the presence of absorption features blueward of H\(\alpha\) and H\(\beta\) at day \(>\)40 which is also generally attributed to circumstellar interaction. Our analysis shows the need for high-cadence early photometric and spectroscopic data to decipher the mass-loss history of the progenitor.</description><subject>Blanketing</subject><subject>Light curve</subject><subject>Photometry</subject><subject>Red giant stars</subject><subject>Shock cooling</subject><subject>Supergiant stars</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNiksKwjAUAIMgWLR3eOC60Cb9uZaKRXBj9xLSV0xtk5qPn9vbhQdwNQMzCxJQxpKoTCldkdDaPo5jmhc0y1hATtVTtqgEgu7ghfwOQhrhR-twGLiBEVvpR5DKoeHCSa1mB3dDaD4TQl3D5Qw0poy__YYsOz5YDH9ck-2havbHaDL64dG6a6-9UXO60rJIdgVL0pz9d30Bit47zQ</recordid><startdate>20230929</startdate><enddate>20230929</enddate><creator>Shrestha, Manisha</creator><creator>Pearson, 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Jencson, Jacob E ; Lundquist, M J ; Mehta, Darshana ; Nicolas Meza Retamal ; Valenti, Stefano ; Rastinejad, Jillian C ; Daly, Phil ; Porter, Dallan ; Hinz, Joannah ; Self, Skyler ; Weiner, Benjamin ; Williams, Grant G ; Hiramatsu, Daichi ; Howell, D Andrew ; McCully, Curtis ; Estefania Padilla Gonzalez ; Pellegrino, Craig ; Terreran, Giacomo ; Newsome, Megan ; Farah, Joseph ; Itagaki, Koichi ; Jha, Saurabh W ; Kwok, Lindsey ; Smith, Nathan ; Schwab, Michaela ; Rho, Jeonghee ; Yang, Yi</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_28719731463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Blanketing</topic><topic>Light curve</topic><topic>Photometry</topic><topic>Red giant stars</topic><topic>Shock cooling</topic><topic>Supergiant stars</topic><toplevel>online_resources</toplevel><creatorcontrib>Shrestha, Manisha</creatorcontrib><creatorcontrib>Pearson, 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Hosseinzadeh</au><au>Bostroem, K Azalee</au><au>Andrews, Jennifer E</au><au>Dong, Yize</au><au>Hoang, Emily</au><au>Janzen, Daryl</au><au>Jencson, Jacob E</au><au>Lundquist, M J</au><au>Mehta, Darshana</au><au>Nicolas Meza Retamal</au><au>Valenti, Stefano</au><au>Rastinejad, Jillian C</au><au>Daly, Phil</au><au>Porter, Dallan</au><au>Hinz, Joannah</au><au>Self, Skyler</au><au>Weiner, Benjamin</au><au>Williams, Grant G</au><au>Hiramatsu, Daichi</au><au>Howell, D Andrew</au><au>McCully, Curtis</au><au>Estefania Padilla Gonzalez</au><au>Pellegrino, Craig</au><au>Terreran, Giacomo</au><au>Newsome, Megan</au><au>Farah, Joseph</au><au>Itagaki, Koichi</au><au>Jha, Saurabh W</au><au>Kwok, Lindsey</au><au>Smith, Nathan</au><au>Schwab, Michaela</au><au>Rho, Jeonghee</au><au>Yang, Yi</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Evidence of weak circumstellar medium interaction in the Type II SN 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SN~2023axu was discovered by the Distance Less Than 40 Mpc (DLT40) survey within 1 day of the last non-detection in the nearby galaxy NGC 2283 at 13.7 Mpc. We modeled the early light curve using a recently updated shock cooling model that includes the effects of line blanketing and found the explosion epoch to be MJD 59971.48 \(\pm\) 0.03 and the probable progenitor to be a red supergiant with a radius of 417 \(\pm\) 28 \(R_\odot\). The shock cooling model cannot match the rise of observed data in the \(r\) and \(i\) bands and underpredicts the overall UV data which points to possible interaction with circumstellar material. This interpretation is further supported by spectral behavior. We see a ledge feature around 4600 \AA\ in the very early spectra (+1.1 and +1.5 days after the explosion) which can be a sign of circumstellar interaction. The signs of circumstellar material are further bolstered by the presence of absorption features blueward of H\(\alpha\) and H\(\beta\) at day \(>\)40 which is also generally attributed to circumstellar interaction. Our analysis shows the need for high-cadence early photometric and spectroscopic data to decipher the mass-loss history of the progenitor.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
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| subjects | Blanketing Light curve Photometry Red giant stars Shock cooling Supergiant stars |
| title | Evidence of weak circumstellar medium interaction in the Type II SN 2023axu |
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