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Gaia16apd - a link between fast and slowly declining type I superluminous supernovae

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dc.abstract.enWe present ultraviolet (UV), optical and infrared photometry and optical spectroscopy of the type Ic superluminous supernova (SLSN) Gaia16apd (=SN 2016eay), covering its evolution from 26 d before the g-band peak to 234.1 d after the peak. Gaia16apd was followed as a part of the NOT Unbiased Transient Survey (NUTS). It is one of the closest SLSNe known (z = 0.102 ± 0.001), with detailed optical and UV observations covering the peak. Gaia16apd is a spectroscopically typical type Ic SLSN, exhibiting the characteristic blue early spectra with O II absorption, and reaches a peak M<SUB>g</SUB> = -21.8 ± 0.1 mag. However, photometrically it exhibits an evolution intermediate between the fast and slowly declining type Ic SLSNe, with an early evolution closer to the fast-declining events. Together with LSQ12dlf, another SLSN with similar properties, it demonstrates a possible continuum between fast and slowly declining events. It is unusually UV-bright even for an SLSN, reaching a non-K-corrected M<SUB>uvm2</SUB> ≃ -23.3 mag, the only other type Ic SLSN with similar UV brightness being SN 2010gx. Assuming that Gaia16apd was powered by magnetar spin-down, we derive a period of P = 1.9 ± 0.2 ms and a magnetic field of B = 1.9 ± 0.2 × 10<SUP>14</SUP> G for the magnetar. The estimated ejecta mass is between 8 and 16 M<SUB>⊙</SUB>, and the kinetic energy between 1.3 and 2.5 × 10<SUP>52</SUP> erg, depending on opacity and assuming that the entire ejecta is swept up into a thin shell. Despite the early photometric differences, the spectra at late times are similar to slowly declining type Ic SLSNe, implying that the two subclasses originate from similar progenitors.
dc.affiliationUniwersytet Warszawski
dc.contributor.authorKangas, T.
dc.contributor.authorBlagorodnova, N.
dc.contributor.authorMattila, S.
dc.contributor.authorLundqvist, P.
dc.contributor.authorFraser, M.
dc.contributor.authorBurgaz, U.
dc.contributor.authorCappellaro, E.
dc.contributor.authorMartínez, J. M. Carrasco
dc.contributor.authorElias-Rosa, N.
dc.contributor.authorHardy, L. K.
dc.contributor.authorHarmanen, J.
dc.contributor.authorHsiao, E. Y.
dc.contributor.authorIsern, J.
dc.contributor.authorKankare, E.
dc.contributor.authorKołaczkowski, Z.
dc.contributor.authorNielsen, M. B.
dc.contributor.authorReynolds, T. M.
dc.contributor.authorRhodes, L.
dc.contributor.authorSomero, A.
dc.contributor.authorStritzinger, M. D.
dc.contributor.authorWyrzykowski, Łukasz
dc.date.accessioned2024-01-25T01:42:49Z
dc.date.available2024-01-25T01:42:49Z
dc.date.copyright2016-11-30
dc.date.issued2017
dc.description.accesstimeBEFORE_PUBLICATION
dc.description.financeNie dotyczy
dc.description.number1
dc.description.versionORIGINAL_AUTHOR
dc.description.volume469
dc.identifier.doi10.1093/MNRAS/STX833
dc.identifier.issn0035-8711
dc.identifier.urihttps://repozytorium.uw.edu.pl//handle/item/107677
dc.identifier.weblinkhttp://adsabs.harvard.edu/abs/2017MNRAS.469.1246K
dc.languageeng
dc.pbn.affiliationastronomy
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.relation.pages1246-1258
dc.rightsOther
dc.sciencecloudnosend
dc.titleGaia16apd - a link between fast and slowly declining type I superluminous supernovae
dc.typeJournalArticle
dspace.entity.typePublication