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| 題名: | The superluminous supernova PS1-11ap: Bridging the gap between low and high redshift |
| 作者: | 陳婷琬;McCrum, M.;Smartt, S. J.;Kotak, R.;Rest, A.;Jerkstrand, A.;Inserra, C.;Rodney, S. A.;Chen, T.-W.;Howell, D. A.;Huber, M. E.;Pastorello, A.;Tonry, J. L.;Bresolin, F.;Kudritzki, R.-P.;Chornock, R.;Berger, E.;Smith, K.;Botticella, M. T.;Foley, R. J.;Fraser, M.;Milisavljevic, D.;Nicholl, M.;Riess, A. G.;Stubbs, C. W.;Valenti, S.;Wood-Vasey, W. M.;Wright, D.;Young, D. R.;Drout, M.;Czekala, I.;Burgett, W. S.;Chambers, K. C.;Draper, P.;Flewelling, H.;Hodapp, K. W.;Kaiser, N.;Magnier, E. A.;Metcalfe, N.;Price, P. A.;Sweeney, W.;Wainscoat, R. J. |
| 貢獻者: | 理學院天文研究所 |
| 關鍵詞: | Astronomy;Spectrum analysis;Supernovae |
| 日期: | 2013-01-01 |
| 上傳時間: | 2026-04-21 14:18:40 (UTC+8) |
| 出版者: | Oxford University Press;London: Oxford University Press |
| 摘要: | 摘要： We present optical photometric and spectroscopic coverage of the superluminous supernova (SLSN) PS1-11ap, discovered with the Pan-STARRS1 Medium Deep Survey at z = 0.524. This intrinsically blue transient rose slowly to reach a peak magnitude of M u = −21.4 mag and bolometric luminosity of 8 × 1043 erg s−1 before settling on to a relatively shallow gradient of decline. The observed decline is significantly slower than those of the SLSNe-Ic which have been the focus of much recent attention. Spectroscopic similarities with the lower redshift SN2007bi and a decline rate similar to 56Co decay time-scale initially indicated that this transient could be a candidate for a pair instability supernova (PISN) explosion. Overall the transient appears quite similar to SN2007bi and the lower redshift object PTF12dam. The extensive data set, from 30 d before peak to 230 d after, allows a detailed and quantitative comparison with published models of PISN explosions. We find that the PS1-11ap data do not match these model explosion parameters well, supporting the recent claim that these SNe are not pair instability explosions. We show that PS1-11ap has many features in common with the faster declining SLSNe-Ic, and the light-curve evolution can also be quantitatively explained by the magnetar spin-down model. At a redshift of z = 0.524, the observer-frame optical coverage provides comprehensive rest-frame UV data and allows us to compare it with the SLSNe recently found at high redshifts between z = 2 and 4. While these high-z explosions are still plausible PISN candidates, they match the photometric evolution of PS1-11ap and hence could be counterparts to this lower redshift transient.
其他題名： Mon. Not. R. Astron. Soc
出版者： London: Oxford University Press
出版日期： 2014-01
出處： Monthly notices of the Royal Astronomical Society, 2014, Vol.437 (1), p.656-674
資源來源： Alma/SFX Local Collection
版權： 2013 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society 2013
版權： Copyright Oxford University Press, UK Jan 1, 2014
識別號： ISSN: 0035-8711
識別號： ISSN: 1365-8711
識別號： ISSN: 1365-2966
識別號： EISSN: 1365-2966
識別號： DOI: 10.1093/mnras/stt1923 |
| 顯示於類別: | [天文研究所] 期刊論文
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