Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date
We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong AGN activity over the past decade. With a redshift of \(z = 0.01107\) and a peak UV/optical luminosity of \((5.4\pm0.4)\...
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creator | Hoogendam, W B Hinkle, J T Shappee, B J Auchettl, K Kochanek, C S Stanek, K Z Maksym, W P Tucker, M A Huber, M E Morrell, N Burns, C R Hey, D Holoien, T W -S Prieto, J L Stritzinger, M A Do Polin, A Ashall, C Brown, P J DerKacy, J M Ferrari, L Galbany, L Hsiao, E Y Kumar, S J Lu Stevens, C P |
description | We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong AGN activity over the past decade. With a redshift of \(z = 0.01107\) and a peak UV/optical luminosity of \((5.4\pm0.4)\times10^{42}\) erg s\(^{-1}\), ASASSN-23bd is the lowest-redshift and least-luminous TDE discovered to date. Spectroscopically, ASASSN-23bd shows H\(\alpha\) and He I emission throughout its spectral time series, and the UV spectrum shows nitrogen lines without the strong carbon and magnesium lines typically seen for AGN. Fits to the rising ASAS-SN light curve show that ASASSN-23bd started to brighten on MJD 59988\(^{+1}_{-1}\), \(\sim\)9 days before discovery, with a nearly linear rise in flux, peaking in the \(g\) band on MJD \(60000^{+3}_{-3}\). Scaling relations and TDE light curve modelling find a black hole mass of \(\sim\)10\(^6\) \(M_\odot\), which is on the lower end of supermassive black hole masses. ASASSN-23bd is a dim X-ray source, with an upper limit of \(L_{0.3-10\,\mathrm{keV}} < 1.0\times10^{40}\) erg s\(^{-1}\) from stacking all \emph{Swift} observations prior to MJD 60061, but with soft (\(\sim 0.1\) keV) thermal emission with a luminosity of \(L_{0.3-2 \,\mathrm{keV}}\sim4\times10^{39}\) erg s\(^{-1}\) in \emph{XMM-Newton} observations on MJD 60095. The rapid \((t < 15\) days) light curve rise, low UV/optical luminosity, and a luminosity decline over 40 days of \(\Delta L_{40}\approx-0.7\) make ASASSN-23bd one of the dimmest TDEs to date and a member of the growing ``Low Luminosity and Fast'' class of TDEs. |
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With a redshift of \(z = 0.01107\) and a peak UV/optical luminosity of \((5.4\pm0.4)\times10^{42}\) erg s\(^{-1}\), ASASSN-23bd is the lowest-redshift and least-luminous TDE discovered to date. Spectroscopically, ASASSN-23bd shows H\(\alpha\) and He I emission throughout its spectral time series, and the UV spectrum shows nitrogen lines without the strong carbon and magnesium lines typically seen for AGN. Fits to the rising ASAS-SN light curve show that ASASSN-23bd started to brighten on MJD 59988\(^{+1}_{-1}\), \(\sim\)9 days before discovery, with a nearly linear rise in flux, peaking in the \(g\) band on MJD \(60000^{+3}_{-3}\). Scaling relations and TDE light curve modelling find a black hole mass of \(\sim\)10\(^6\) \(M_\odot\), which is on the lower end of supermassive black hole masses. ASASSN-23bd is a dim X-ray source, with an upper limit of \(L_{0.3-10\,\mathrm{keV}} < 1.0\times10^{40}\) erg s\(^{-1}\) from stacking all \emph{Swift} observations prior to MJD 60061, but with soft (\(\sim 0.1\) keV) thermal emission with a luminosity of \(L_{0.3-2 \,\mathrm{keV}}\sim4\times10^{39}\) erg s\(^{-1}\) in \emph{XMM-Newton} observations on MJD 60095. The rapid \((t < 15\) days) light curve rise, low UV/optical luminosity, and a luminosity decline over 40 days of \(\Delta L_{40}\approx-0.7\) make ASASSN-23bd one of the dimmest TDEs to date and a member of the growing ``Low Luminosity and Fast'' class of TDEs.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Active galactic nuclei ; Disruption ; Light curve ; Luminosity ; Magnesium ; Red shift ; Sky surveys (astronomy) ; Supermassive black holes ; Supernovae ; Thermal emission ; Ultraviolet spectra ; X ray sources ; XMM (spacecraft)</subject><ispartof>arXiv.org, 2024-01</ispartof><rights>2024. This work is published under http://creativecommons.org/licenses/by-nc-sa/4.0/ (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>776,780</link.rule.ids></links><search><creatorcontrib>Hoogendam, W B</creatorcontrib><creatorcontrib>Hinkle, J T</creatorcontrib><creatorcontrib>Shappee, B J</creatorcontrib><creatorcontrib>Auchettl, K</creatorcontrib><creatorcontrib>Kochanek, C S</creatorcontrib><creatorcontrib>Stanek, K Z</creatorcontrib><creatorcontrib>Maksym, W P</creatorcontrib><creatorcontrib>Tucker, M A</creatorcontrib><creatorcontrib>Huber, M E</creatorcontrib><creatorcontrib>Morrell, N</creatorcontrib><creatorcontrib>Burns, C R</creatorcontrib><creatorcontrib>Hey, D</creatorcontrib><creatorcontrib>Holoien, T W -S</creatorcontrib><creatorcontrib>Prieto, J L</creatorcontrib><creatorcontrib>Stritzinger, M</creatorcontrib><creatorcontrib>A Do</creatorcontrib><creatorcontrib>Polin, A</creatorcontrib><creatorcontrib>Ashall, C</creatorcontrib><creatorcontrib>Brown, P J</creatorcontrib><creatorcontrib>DerKacy, J M</creatorcontrib><creatorcontrib>Ferrari, L</creatorcontrib><creatorcontrib>Galbany, L</creatorcontrib><creatorcontrib>Hsiao, E Y</creatorcontrib><creatorcontrib>Kumar, S</creatorcontrib><creatorcontrib>J Lu</creatorcontrib><creatorcontrib>Stevens, C P</creatorcontrib><title>Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date</title><title>arXiv.org</title><description>We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong AGN activity over the past decade. With a redshift of \(z = 0.01107\) and a peak UV/optical luminosity of \((5.4\pm0.4)\times10^{42}\) erg s\(^{-1}\), ASASSN-23bd is the lowest-redshift and least-luminous TDE discovered to date. Spectroscopically, ASASSN-23bd shows H\(\alpha\) and He I emission throughout its spectral time series, and the UV spectrum shows nitrogen lines without the strong carbon and magnesium lines typically seen for AGN. Fits to the rising ASAS-SN light curve show that ASASSN-23bd started to brighten on MJD 59988\(^{+1}_{-1}\), \(\sim\)9 days before discovery, with a nearly linear rise in flux, peaking in the \(g\) band on MJD \(60000^{+3}_{-3}\). Scaling relations and TDE light curve modelling find a black hole mass of \(\sim\)10\(^6\) \(M_\odot\), which is on the lower end of supermassive black hole masses. ASASSN-23bd is a dim X-ray source, with an upper limit of \(L_{0.3-10\,\mathrm{keV}} < 1.0\times10^{40}\) erg s\(^{-1}\) from stacking all \emph{Swift} observations prior to MJD 60061, but with soft (\(\sim 0.1\) keV) thermal emission with a luminosity of \(L_{0.3-2 \,\mathrm{keV}}\sim4\times10^{39}\) erg s\(^{-1}\) in \emph{XMM-Newton} observations on MJD 60095. The rapid \((t < 15\) days) light curve rise, low UV/optical luminosity, and a luminosity decline over 40 days of \(\Delta L_{40}\approx-0.7\) make ASASSN-23bd one of the dimmest TDEs to date and a member of the growing ``Low Luminosity and Fast'' class of TDEs.</description><subject>Active galactic nuclei</subject><subject>Disruption</subject><subject>Light curve</subject><subject>Luminosity</subject><subject>Magnesium</subject><subject>Red shift</subject><subject>Sky surveys (astronomy)</subject><subject>Supermassive black holes</subject><subject>Supernovae</subject><subject>Thermal emission</subject><subject>Ultraviolet spectra</subject><subject>X ray sources</subject><subject>XMM (spacecraft)</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqNjc1qwzAQhEWhkNDmHRZyaQ4GZ1U7bm8mP_Rgeqh1N6otExlV61qS0-Tpa0IeIKeBmW9mHtgcOV9H2SvijC2c6-I4xnSDScLn7LLTrqZRDWeQtoEDGUOnKPRALeRlXpafEfLvBl5yARgjr83f6h3EUUFBJ-U8fKnGHXXrr_VCyckqwo-2FBwI3UgD08MQeq_Jwn5U1oMg2EmvntljK41Ti5s-seVhL7YfUT_Qb5i2q47CYKeowrc1T3iWpht-H_UPrxVK2Q</recordid><startdate>20240110</startdate><enddate>20240110</enddate><creator>Hoogendam, W B</creator><creator>Hinkle, J T</creator><creator>Shappee, B J</creator><creator>Auchettl, K</creator><creator>Kochanek, C S</creator><creator>Stanek, K Z</creator><creator>Maksym, W P</creator><creator>Tucker, M A</creator><creator>Huber, M E</creator><creator>Morrell, N</creator><creator>Burns, C R</creator><creator>Hey, D</creator><creator>Holoien, T W -S</creator><creator>Prieto, J L</creator><creator>Stritzinger, M</creator><creator>A Do</creator><creator>Polin, A</creator><creator>Ashall, C</creator><creator>Brown, P J</creator><creator>DerKacy, J M</creator><creator>Ferrari, L</creator><creator>Galbany, L</creator><creator>Hsiao, E Y</creator><creator>Kumar, S</creator><creator>J Lu</creator><creator>Stevens, C P</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20240110</creationdate><title>Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date</title><author>Hoogendam, W B ; Hinkle, J T ; Shappee, B J ; Auchettl, K ; Kochanek, C S ; Stanek, K Z ; Maksym, W P ; Tucker, M A ; Huber, M E ; Morrell, N ; Burns, C R ; Hey, D ; Holoien, T W -S ; Prieto, J L ; Stritzinger, M ; A Do ; Polin, A ; Ashall, C ; Brown, P J ; DerKacy, J M ; Ferrari, L ; Galbany, L ; Hsiao, E Y ; Kumar, S ; J Lu ; Stevens, C P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_29135386673</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Active galactic nuclei</topic><topic>Disruption</topic><topic>Light curve</topic><topic>Luminosity</topic><topic>Magnesium</topic><topic>Red shift</topic><topic>Sky surveys (astronomy)</topic><topic>Supermassive black holes</topic><topic>Supernovae</topic><topic>Thermal emission</topic><topic>Ultraviolet spectra</topic><topic>X ray sources</topic><topic>XMM (spacecraft)</topic><toplevel>online_resources</toplevel><creatorcontrib>Hoogendam, W B</creatorcontrib><creatorcontrib>Hinkle, J T</creatorcontrib><creatorcontrib>Shappee, B J</creatorcontrib><creatorcontrib>Auchettl, K</creatorcontrib><creatorcontrib>Kochanek, C S</creatorcontrib><creatorcontrib>Stanek, K Z</creatorcontrib><creatorcontrib>Maksym, W P</creatorcontrib><creatorcontrib>Tucker, M A</creatorcontrib><creatorcontrib>Huber, M E</creatorcontrib><creatorcontrib>Morrell, N</creatorcontrib><creatorcontrib>Burns, C R</creatorcontrib><creatorcontrib>Hey, D</creatorcontrib><creatorcontrib>Holoien, T W -S</creatorcontrib><creatorcontrib>Prieto, J L</creatorcontrib><creatorcontrib>Stritzinger, M</creatorcontrib><creatorcontrib>A Do</creatorcontrib><creatorcontrib>Polin, A</creatorcontrib><creatorcontrib>Ashall, C</creatorcontrib><creatorcontrib>Brown, P J</creatorcontrib><creatorcontrib>DerKacy, J M</creatorcontrib><creatorcontrib>Ferrari, L</creatorcontrib><creatorcontrib>Galbany, L</creatorcontrib><creatorcontrib>Hsiao, E Y</creatorcontrib><creatorcontrib>Kumar, S</creatorcontrib><creatorcontrib>J Lu</creatorcontrib><creatorcontrib>Stevens, C P</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest Central (New)</collection><collection>ProQuest One Academic (New)</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Middle East (New)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Applied & Life Sciences</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Hoogendam, W B</au><au>Hinkle, J T</au><au>Shappee, B J</au><au>Auchettl, K</au><au>Kochanek, C S</au><au>Stanek, K Z</au><au>Maksym, W P</au><au>Tucker, M A</au><au>Huber, M E</au><au>Morrell, N</au><au>Burns, C R</au><au>Hey, D</au><au>Holoien, T W -S</au><au>Prieto, J L</au><au>Stritzinger, M</au><au>A Do</au><au>Polin, A</au><au>Ashall, C</au><au>Brown, P J</au><au>DerKacy, J M</au><au>Ferrari, L</au><au>Galbany, L</au><au>Hsiao, E Y</au><au>Kumar, S</au><au>J Lu</au><au>Stevens, C P</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date</atitle><jtitle>arXiv.org</jtitle><date>2024-01-10</date><risdate>2024</risdate><eissn>2331-8422</eissn><abstract>We report the All-Sky Automated Survey for SuperNovae discovery of the tidal disruption event (TDE) ASASSN-23bd (AT 2023clx) in NGC 3799, a LINER galaxy with no evidence of strong AGN activity over the past decade. With a redshift of \(z = 0.01107\) and a peak UV/optical luminosity of \((5.4\pm0.4)\times10^{42}\) erg s\(^{-1}\), ASASSN-23bd is the lowest-redshift and least-luminous TDE discovered to date. Spectroscopically, ASASSN-23bd shows H\(\alpha\) and He I emission throughout its spectral time series, and the UV spectrum shows nitrogen lines without the strong carbon and magnesium lines typically seen for AGN. Fits to the rising ASAS-SN light curve show that ASASSN-23bd started to brighten on MJD 59988\(^{+1}_{-1}\), \(\sim\)9 days before discovery, with a nearly linear rise in flux, peaking in the \(g\) band on MJD \(60000^{+3}_{-3}\). Scaling relations and TDE light curve modelling find a black hole mass of \(\sim\)10\(^6\) \(M_\odot\), which is on the lower end of supermassive black hole masses. ASASSN-23bd is a dim X-ray source, with an upper limit of \(L_{0.3-10\,\mathrm{keV}} < 1.0\times10^{40}\) erg s\(^{-1}\) from stacking all \emph{Swift} observations prior to MJD 60061, but with soft (\(\sim 0.1\) keV) thermal emission with a luminosity of \(L_{0.3-2 \,\mathrm{keV}}\sim4\times10^{39}\) erg s\(^{-1}\) in \emph{XMM-Newton} observations on MJD 60095. The rapid \((t < 15\) days) light curve rise, low UV/optical luminosity, and a luminosity decline over 40 days of \(\Delta L_{40}\approx-0.7\) make ASASSN-23bd one of the dimmest TDEs to date and a member of the growing ``Low Luminosity and Fast'' class of TDEs.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
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subjects | Active galactic nuclei Disruption Light curve Luminosity Magnesium Red shift Sky surveys (astronomy) Supermassive black holes Supernovae Thermal emission Ultraviolet spectra X ray sources XMM (spacecraft) |
title | Discovery and Follow-up of ASASSN-23bd (AT 2023clx): The Lowest Redshift and Least Luminous Tidal Disruption Event To Date |
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