The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343
We present the discovery of the X-ray and optical afterglows of the short-duration GRB 150101B, pinpointing the event to an early-type host galaxy at z=0.1343 +/- 0.0030. This makes GRB 150101B the most nearby short GRB with an early-type host galaxy discovered to date. Fitting the spectral energy d...
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| creator | Wen-fai Fong Margutti, Raffaella Ryan Chornock Berger, Edo Shappee, Benjamin J Levan, Andrew J Tanvir, Nial R Smith, Nathan Milne, Peter A Laskar, Tanmoy Fox, Derek B Lunnan, Ragnhild Blanchard, Peter K Hjorth, Jens Wiersema, Klaas Alexander J van der Horst Zaritsky, Dennis |
| description | We present the discovery of the X-ray and optical afterglows of the short-duration GRB 150101B, pinpointing the event to an early-type host galaxy at z=0.1343 +/- 0.0030. This makes GRB 150101B the most nearby short GRB with an early-type host galaxy discovered to date. Fitting the spectral energy distribution of the host galaxy results in an inferred stellar mass of ~7x10^10 M_sol, stellar population age of ~2-2.5 Gyr, and star formation rate of 9 deg. Using observations extending to ~30 days, we place upper limits of |
| doi_str_mv | 10.48550/arxiv.1608.08626 |
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This makes GRB 150101B the most nearby short GRB with an early-type host galaxy discovered to date. Fitting the spectral energy distribution of the host galaxy results in an inferred stellar mass of ~7x10^10 M_sol, stellar population age of ~2-2.5 Gyr, and star formation rate of <0.4 M_sol yr^-1. The host of GRB 150101B is one of the largest and most luminous short GRB host galaxies, with a B-band luminosity of ~4.3L* and half-light radius of ~8 kpc. GRB 150101B is located at a projected distance of 7.35 +/- 0.07 kpc from its host center, and lies on a faint region of its host rest-frame optical light. Its location, combined with the lack of associated supernova, is consistent with a NS-NS/NS-BH merger progenitor. From modeling the evolution of the broad-band afterglow, we calculate isotropic-equivalent gamma-ray and kinetic energies of ~1.3x10^49 erg and ~(6-14)x10^51 erg, respectively, a circumburst density of ~(0.8-4)x10^-5 cm^-3, and a jet opening angle of >9 deg. Using observations extending to ~30 days, we place upper limits of <(2-4)x10^41 erg s^-1 on associated kilonova emission. We compare searches following previous short GRBs to existing kilonova models, and demonstrate the difficulty of performing effective kilonova searches from cosmological short GRBs using current ground-based facilities. We show that at the Advanced LIGO/VIRGO horizon distance of 200 Mpc, searches reaching depths of ~23-24 AB mag are necessary to probe a meaningful range of kilonova models.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1608.08626</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Afterglows ; Astronomical models ; Galaxies ; Galaxy distribution ; Gamma ray bursts ; Gamma rays ; Luminosity ; Physics - High Energy Astrophysical Phenomena ; Searching ; Spectral energy distribution ; Star & galaxy formation ; Star formation rate ; Stellar age ; Stellar mass</subject><ispartof>arXiv.org, 2016-08</ispartof><rights>2016. 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><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>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,784,885,27925</link.rule.ids><backlink>$$Uhttps://doi.org/10.3847/1538-4357/833/2/151$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.48550/arXiv.1608.08626$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Wen-fai Fong</creatorcontrib><creatorcontrib>Margutti, Raffaella</creatorcontrib><creatorcontrib>Ryan Chornock</creatorcontrib><creatorcontrib>Berger, Edo</creatorcontrib><creatorcontrib>Shappee, Benjamin J</creatorcontrib><creatorcontrib>Levan, Andrew J</creatorcontrib><creatorcontrib>Tanvir, Nial R</creatorcontrib><creatorcontrib>Smith, Nathan</creatorcontrib><creatorcontrib>Milne, Peter A</creatorcontrib><creatorcontrib>Laskar, Tanmoy</creatorcontrib><creatorcontrib>Fox, Derek B</creatorcontrib><creatorcontrib>Lunnan, Ragnhild</creatorcontrib><creatorcontrib>Blanchard, Peter K</creatorcontrib><creatorcontrib>Hjorth, Jens</creatorcontrib><creatorcontrib>Wiersema, Klaas</creatorcontrib><creatorcontrib>Alexander J van der Horst</creatorcontrib><creatorcontrib>Zaritsky, Dennis</creatorcontrib><title>The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343</title><title>arXiv.org</title><description>We present the discovery of the X-ray and optical afterglows of the short-duration GRB 150101B, pinpointing the event to an early-type host galaxy at z=0.1343 +/- 0.0030. This makes GRB 150101B the most nearby short GRB with an early-type host galaxy discovered to date. Fitting the spectral energy distribution of the host galaxy results in an inferred stellar mass of ~7x10^10 M_sol, stellar population age of ~2-2.5 Gyr, and star formation rate of <0.4 M_sol yr^-1. The host of GRB 150101B is one of the largest and most luminous short GRB host galaxies, with a B-band luminosity of ~4.3L* and half-light radius of ~8 kpc. GRB 150101B is located at a projected distance of 7.35 +/- 0.07 kpc from its host center, and lies on a faint region of its host rest-frame optical light. Its location, combined with the lack of associated supernova, is consistent with a NS-NS/NS-BH merger progenitor. From modeling the evolution of the broad-band afterglow, we calculate isotropic-equivalent gamma-ray and kinetic energies of ~1.3x10^49 erg and ~(6-14)x10^51 erg, respectively, a circumburst density of ~(0.8-4)x10^-5 cm^-3, and a jet opening angle of >9 deg. Using observations extending to ~30 days, we place upper limits of <(2-4)x10^41 erg s^-1 on associated kilonova emission. We compare searches following previous short GRBs to existing kilonova models, and demonstrate the difficulty of performing effective kilonova searches from cosmological short GRBs using current ground-based facilities. We show that at the Advanced LIGO/VIRGO horizon distance of 200 Mpc, searches reaching depths of ~23-24 AB mag are necessary to probe a meaningful range of kilonova models.</description><subject>Afterglows</subject><subject>Astronomical models</subject><subject>Galaxies</subject><subject>Galaxy distribution</subject><subject>Gamma ray bursts</subject><subject>Gamma rays</subject><subject>Luminosity</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Searching</subject><subject>Spectral energy distribution</subject><subject>Star & galaxy formation</subject><subject>Star formation rate</subject><subject>Stellar age</subject><subject>Stellar mass</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2016</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0FLw0AQhRdBsNT-AE8ueE6cmc0mm4OHttRWqAiae5hmN7YlNnWTauOvN7aeBh7fe8wnxA1CGBmt4Z79cfMVYgwmBBNTfCEGpBQGJiK6EqOm2QIAxQlprQbiOVs7OS5b59-r-lvyzsoZ-6oLsm7v5KJuWjnnio-drEvZ9uzbuvZ99jqRqAEBJ5Jb-fMAIapIXYvLkqvGjf7vUGSPs2y6CJYv86fpeBmwJgosoF1ZRqbCpTGZlY0cUZoykua4tMahckoDFaiYSwQLzvQlKAtWBhI1FLfn2ZNrvvebD_Zd_uecn5x74u5M7H39eXBNm2_rg9_1P-UEBnSiISL1CxKOVYU</recordid><startdate>20160830</startdate><enddate>20160830</enddate><creator>Wen-fai Fong</creator><creator>Margutti, Raffaella</creator><creator>Ryan Chornock</creator><creator>Berger, Edo</creator><creator>Shappee, Benjamin J</creator><creator>Levan, Andrew J</creator><creator>Tanvir, Nial R</creator><creator>Smith, Nathan</creator><creator>Milne, Peter A</creator><creator>Laskar, Tanmoy</creator><creator>Fox, Derek B</creator><creator>Lunnan, Ragnhild</creator><creator>Blanchard, Peter K</creator><creator>Hjorth, Jens</creator><creator>Wiersema, Klaas</creator><creator>Alexander J van der Horst</creator><creator>Zaritsky, Dennis</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>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20160830</creationdate><title>The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343</title><author>Wen-fai Fong ; Margutti, Raffaella ; Ryan Chornock ; Berger, Edo ; Shappee, Benjamin J ; Levan, Andrew J ; Tanvir, Nial R ; Smith, Nathan ; Milne, Peter A ; Laskar, Tanmoy ; Fox, Derek B ; Lunnan, Ragnhild ; Blanchard, Peter K ; Hjorth, Jens ; Wiersema, Klaas ; Alexander J van der Horst ; Zaritsky, Dennis</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a522-d01dbda1a2ce9628bd4e2299a125a6fd8e13e3502c13aaf10d0e8d010fca38073</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2016</creationdate><topic>Afterglows</topic><topic>Astronomical models</topic><topic>Galaxies</topic><topic>Galaxy distribution</topic><topic>Gamma ray bursts</topic><topic>Gamma rays</topic><topic>Luminosity</topic><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Searching</topic><topic>Spectral energy distribution</topic><topic>Star & galaxy formation</topic><topic>Star formation rate</topic><topic>Stellar age</topic><topic>Stellar mass</topic><toplevel>online_resources</toplevel><creatorcontrib>Wen-fai Fong</creatorcontrib><creatorcontrib>Margutti, Raffaella</creatorcontrib><creatorcontrib>Ryan Chornock</creatorcontrib><creatorcontrib>Berger, Edo</creatorcontrib><creatorcontrib>Shappee, Benjamin J</creatorcontrib><creatorcontrib>Levan, Andrew J</creatorcontrib><creatorcontrib>Tanvir, Nial R</creatorcontrib><creatorcontrib>Smith, Nathan</creatorcontrib><creatorcontrib>Milne, Peter A</creatorcontrib><creatorcontrib>Laskar, Tanmoy</creatorcontrib><creatorcontrib>Fox, Derek B</creatorcontrib><creatorcontrib>Lunnan, Ragnhild</creatorcontrib><creatorcontrib>Blanchard, Peter K</creatorcontrib><creatorcontrib>Hjorth, Jens</creatorcontrib><creatorcontrib>Wiersema, Klaas</creatorcontrib><creatorcontrib>Alexander J van der Horst</creatorcontrib><creatorcontrib>Zaritsky, Dennis</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>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Wen-fai Fong</au><au>Margutti, Raffaella</au><au>Ryan Chornock</au><au>Berger, Edo</au><au>Shappee, Benjamin J</au><au>Levan, Andrew J</au><au>Tanvir, Nial R</au><au>Smith, Nathan</au><au>Milne, Peter A</au><au>Laskar, Tanmoy</au><au>Fox, Derek B</au><au>Lunnan, Ragnhild</au><au>Blanchard, Peter K</au><au>Hjorth, Jens</au><au>Wiersema, Klaas</au><au>Alexander J van der Horst</au><au>Zaritsky, Dennis</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343</atitle><jtitle>arXiv.org</jtitle><date>2016-08-30</date><risdate>2016</risdate><eissn>2331-8422</eissn><abstract>We present the discovery of the X-ray and optical afterglows of the short-duration GRB 150101B, pinpointing the event to an early-type host galaxy at z=0.1343 +/- 0.0030. This makes GRB 150101B the most nearby short GRB with an early-type host galaxy discovered to date. Fitting the spectral energy distribution of the host galaxy results in an inferred stellar mass of ~7x10^10 M_sol, stellar population age of ~2-2.5 Gyr, and star formation rate of <0.4 M_sol yr^-1. The host of GRB 150101B is one of the largest and most luminous short GRB host galaxies, with a B-band luminosity of ~4.3L* and half-light radius of ~8 kpc. GRB 150101B is located at a projected distance of 7.35 +/- 0.07 kpc from its host center, and lies on a faint region of its host rest-frame optical light. Its location, combined with the lack of associated supernova, is consistent with a NS-NS/NS-BH merger progenitor. From modeling the evolution of the broad-band afterglow, we calculate isotropic-equivalent gamma-ray and kinetic energies of ~1.3x10^49 erg and ~(6-14)x10^51 erg, respectively, a circumburst density of ~(0.8-4)x10^-5 cm^-3, and a jet opening angle of >9 deg. Using observations extending to ~30 days, we place upper limits of <(2-4)x10^41 erg s^-1 on associated kilonova emission. We compare searches following previous short GRBs to existing kilonova models, and demonstrate the difficulty of performing effective kilonova searches from cosmological short GRBs using current ground-based facilities. We show that at the Advanced LIGO/VIRGO horizon distance of 200 Mpc, searches reaching depths of ~23-24 AB mag are necessary to probe a meaningful range of kilonova models.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1608.08626</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Afterglows Astronomical models Galaxies Galaxy distribution Gamma ray bursts Gamma rays Luminosity Physics - High Energy Astrophysical Phenomena Searching Spectral energy distribution Star & galaxy formation Star formation rate Stellar age Stellar mass |
| title | The Afterglow and Early-Type Host Galaxy of the Short GRB 150101B at z=0.1343 |
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