Abstract
Superluminous supernovae are hydrogen-rich (SLSNe-II), or hydrogen-poor (SLSNe-I), explosions so bright that they require a power source beyond that of traditional supernovae. SLSNe-I rise to a peak over 20–90 days and then decline over a timescale roughly twice as long. At early times they have a blue continuum, peaking in the ultraviolet, have temperatures in excess of 14,000 K, and show ionized lines of carbon and oxygen out of thermodynamic equilibrium. As the supernovae cool, their spectra start to resemble SNe Ic, though with a time delay. They also favor environments with metallicities half solar or lower. Modeling indicates that they are explosions of stripped carbon-oxygen stellar cores, similar to but sometimes more massive than the progenitors of SNe Ic. SLSNe-I similar to SN 2007bi have broader light curves and seemingly more massive progenitors. Some have proposed that these are pair-instability supernovae, but in general the supernovae rise too quickly for this model. Most SLSNe-I show no signs of interaction and instead seem to be powered by a central engine. The magnetar spin-down model has been the most successful at reproducing the light curves and peak luminosity of SLSNe, though it may not be unique. Most SLSNe-II seem to be powered by interaction of these SNe with circumstellar material, as in SNe IIn. However, there are a handful of hybrid cases, or SLSNe-II, with weak or little interaction, which may be related to SLSNe-I.
References
Aldering G, Antilogus P, Bailey S et al (2006) Nearby supernova factory observations of SN 2005gj: another type Ia supernova in a massive circumstellar envelope. ApJ 650:510. doi:http://dx.doi.org/10.1086/507020
Angus CR, Levan AJ, Perley DA et al (2016) AHubble Space Telescopesurvey of the host galaxies of Superluminous Supernovae. Mon Not R Astron Soc 458:84. doi:http://dx.doi.org/10.1093/mnras/stw063
Arcavi I, Gal-Yam A, Yaron O et al (2011) SN 2011dh: discovery of a type IIb supernova from a compact progenitor in the nearby galaxy M51. ApJ 742:L18. doi:http://dx.doi.org/10.1088/2041-8205/742/2/l18
Arcavi I, Wolf WM, Howell DA et al (2016) Rapidly rising transients in the supernova—superluminous supernova GAP. ApJ 819:35. doi:http://dx.doi.org/10.3847/0004-637X/819/1/35
Arnett WD (1982) Type I supernovae. I – analytic solutions for the early part of the light curve. ApJ 253:785. doi:http://dx.doi.org/10.1086/159681
Barbary K, Dawson KS, Tokita K et al (2008) Discovery of an unusual optical transient with the hubble space telescope. ApJ 690:1358. doi:http://dx.doi.org/10.1088/0004-637X/690/2/1358
Barkat Z, Rakavy G, Sack N (1967) Dynamics of supernova explosion resulting from pair formation. Phys Rev Lett 18:379. doi:http://dx.doi.org/10.1103/physrevlett.18.379
Ben-Ami S, Gal-Yam A, Mazzali PA et al (2014) SN 2010MB: direct evidence for a supernova interacting with a large amount of hydrogen-free circumstellar material. ApJ 785:37. doi:http://dx.doi.org/10.1088/0004-637x/785/1/37
Benetti S, Nicholl M, Cappellaro E et al (2014) The supernova CSS121015:004244+132827: a clue for understanding superluminous supernovae. Mon Not R Astron Soc 441:289. doi:http://dx.doi.org/10.1093/mnras/stu538
Berger E, Chornock R, Lunnan R et al (2012) Ultraluminous supernovae as a new probe of the interstellar medium in distant galaxies. ApJ 755:L29. doi:http://dx.doi.org/10.1088/2041-8205/755/2/l29
Chatzopoulos E, Wheeler JC (2012) Hydrogen-poor circumstellar shells from pulsational pair-instability supernovae with rapidly rotating progenitors. ApJ 760:154. doi:http://dx.doi.org/10.1088/0004-637X/760/2/154
Chatzopoulos E, Wheeler JC, Couch SM (2013a) Multi-dimensional simulations of rotating pair-instability supernovae. ApJ 776:129. doi:http://dx.doi.org/10.1088/0004-637X/776/2/129
Chatzopoulos E, Wheeler JC, Vinko J, Horvath ZL, Nagy A (2013b) Analytical light curve models of superluminous supernovae: χ 2 -minimization of parameter fits. ApJ 773:76. doi:http://dx.doi.org/10.1088/0004-637X/773/1/76
Chen K-J, Woosley SE, Sukhbold T (2016a) Magnetar-powered supernovae in two dimensions. I. Superluminous supernovae. ArXiv e-prints, arXiv:1604.07989
Chen T-W, Smartt SJ, Yates RM et al (2016b) A sub-solar metallicity is required for superluminous supernova progenitors. ArXiv e-prints, arXiv:1605.04925
Chen T-W, Smartt SJ, Bresolin F et al (2013) The host galaxy of the Super-luminous SN 2010gx and limits on explosive 56 Ni production. ApJ Lett 763:L28. doi:http://dx.doi.org/10.1088/2041-8205/763/2/L28
Chen T-W, Smartt SJ, Jerkstrand A et al (2015) The host galaxy and late-time evolution of the superluminous supernova PTF12dam. Mon Not R Astron Soc 452:1567. doi:http://dx.doi.org/10.1093/mnras/stv1360
Chevalier RA, Irwin CM (2011) Shock breakout in dense mass loss: luminous supernovae. ApJ 729:L6. doi:http://dx.doi.org/10.1088/2041-8205/729/1/l6
Chomiuk L, Chornock R, Soderberg AM et al (2011) Pan-starrs1 discovery of two ultraluminous supernovae at z ≈ 0.9. ApJ 743:114. doi:http://dx.doi.org/10.1088/0004-637x/743/2/114
Cooke J, Sullivan M, Gal-Yam A et al (2012) Superluminous supernovae at redshifts of 2.05 and 3.90. Nature 491:228. doi:http://dx.doi.org/10.1038/nature11521
Dessart L, Hillier DJ, Waldman R, Livne E, Blondin S (2012) Superluminous supernovae: 56 Ni power versus magnetar radiation. Mon Not R Astron Soc Lett 426:L76. doi:http://dx.doi.org/10.1111/j.1745-3933.2012.01329.x
Dexter J, Kasen D (2013) Supernova light curves POWERED by fallback accretion. ApJ 772:30. doi:http://dx.doi.org/10.1088/0004-637x/772/1/30
Drout MR, Chornock R, Soderberg AM et al (2014) Rapidly evolving and luminous transients from pan-starrs1. ApJ 794:23. doi:http://dx.doi.org/10.1088/0004-637X/794/1/23
Falk SW (1978) Shock steepening and prompt thermal emission in supernovae. ApJ 225:L133. doi:http://dx.doi.org/10.1086/182810
Gal-Yam A (2012) Luminous Supernovae. Science 337:927. doi:http://dx.doi.org/10.1126/science.1203601
Gal-Yam A, Mazzali P, Ofek EO et al (2009) Supernova 2007bi as a pair-instability explosion. Nature 462:624. doi:http://dx.doi.org/10.1038/nature08579
Gal-Yam A, Arcavi I, Ofek EO et al (2014) A Wolf-Rayet-like progenitor of SN 2013cu from spectral observations of a stellar wind. Nature 509:471. doi:http://dx.doi.org/10.1038/nature13304
Germany LM, Reiss DJ, Sadler EM, Schmidt BP, Stubbs CW (2000) SN 1997cy/GRB 970514: a new piece in the gamma ray burst puzzle? ApJ 533:320. doi:http://dx.doi.org/10.1086/308639
Gezari S, Halpern JP, Grupe D et al (2008) Discovery of the ultra-bright type II-L supernova 2008es. ApJ 690:1313. doi:http://dx.doi.org/10.1088/0004-637x/690/2/1313
Gezari S, Jones DO, Sanders NE et al (2015) Galex detection of shock breakout in type IIP supernova PS1-13arp: implications for the progenitor star wind. ApJ 804:28. doi:http://dx.doi.org/10.1088/0004-637x/804/1/28
Gilkis A, Soker N, Papish O (2016) Explaining the most energetic supernovae with an inefficient jet-feedback mechanism. ApJ 826:178. doi:http://dx.doi.org/10.3847/0004-637x/826/2/178
Ginzburg S, Balberg S (2012) Superluminous light curves from supernovae exploding in a dense wind. ApJ 757:178. doi:http://dx.doi.org/10.1088/0004-637X/757/2/178
Gänsicke BT, Levan AJ, Marsh TR, Wheatley PJ (2009) SCP 06F6: a Carbon-rich extragalactic transient at redshift z ≃ 0.14? ApJ 697:L129. doi:http://dx.doi.org/10.1088/0004-637x/697/2/l129
Graham ML, Sand DJ, Valenti S et al (2014) Clues to the nature of SN 2009ip from photometric and spectroscopic evolution to late times. ApJ 787:163. doi:http://dx.doi.org/10.1088/0004-637x/787/2/163
Greiner J, Mazzali PA, Kann DA et al (2015) A very luminous magnetar-powered supernova associated with an ultra-long γ-ray burst. Nature 523:189. doi:http://dx.doi.org/10.1038/nature14579
Hosseinzadeh G, Arcavi I, Valenti S et al (2016) Type Ibn Supernovae Show Photometric Homogeneity and Evidence for Two Spectral Subclasses. ArXiv e-prints, arXiv:1608.01998
Howell DA, Kasen D, Lidman C et al (2013) Two superluminous supernovae from the early universe discovered by the supernova legacy survey. ApJ 779:98. doi:http://dx.doi.org/10.1088/0004-637x/779/2/98
Inserra C, Bulla M, Sim SA, Smartt SJ (2016a) Spectropolarimetry of superluminous supernovae: insight into their geometry. ArXiv e-prints, arXiv:1607.02353
Inserra C, Smartt SJ (2014) Superluminous supernovae as standardizable candles and high-redshift distance probes. ApJ 796:87. doi:http://dx.doi.org/10.1088/0004-637x/796/2/87
Inserra C, Smartt SJ, Jerkstrand A et al (2013) Super-luminous type Ic supernovae: catching a magnetar by the tail. ApJ 770:128. doi:http://dx.doi.org/10.1088/0004-637x/770/2/128
Inserra C, Smartt SJ, Gall EEE et al (2016b) On the nature of Hydrogen-rich Superluminous Supernovae. ArXiv e-prints, arXiv:1604.01226
Jerkstrand A, Smartt SJ, Inserra C et al (2016) Long-duration superluminous supernovae at late times. ArXiv e-prints, arXiv:1608.02994
Kasen D, Bildsten L (2010) Supernova light curves powered by young magnetars. ApJ 717:245. doi:http://dx.doi.org/10.1088/0004-637x/717/1/245
Kasen D, Metzger BD, Bildsten L (2016) Magnetar-driven shock breakout and double-peaked supernova light curves. ApJ 821:36. doi:http://dx.doi.org/10.3847/0004-637X/821/1/36
Kasen D, Woosley SE, Heger A (2011) Pair instability supernovae: light curves spectra and shock breakout. ApJ 734:102. doi:http://dx.doi.org/10.1088/0004-637x/734/2/102
Kelly PL, Kirshner RP (2012) Core-collapse supernovae and host galaxy stellar populations. ApJ 759:107. doi:http://dx.doi.org/10.1088/0004-637x/759/2/107
Khazov D, Yaron O, Gal-Yam A et al (2016) Flash spectroscopy: emission lines from the ionized circumstellar material around < 10-DAY-OLD type II supernovae. ApJ 818:3. doi:http://dx.doi.org/10.3847/0004-637x/818/1/3
Kiewe M, Gal-Yam A, Arcavi I et al (2011) Caltech core-collapse project (CCCP) observations of type IIn supernovae: typical properties and implications for their progenitor stars. ApJ 744:10. doi:http://dx.doi.org/10.1088/0004-637X/744/1/10
Klein RI, Chevalier RA (1978) X-ray bursts from type II supernovae. ApJ 223:L109. doi:http://dx.doi.org/10.1086/182740
Knop R, Aldering G, Deustua S et al (1999) Supernovae 1999as and 1999at in anonymous galaxies. IAU Circulars 7128
Leloudas G, Chatzopoulos E, Dilday B et al (2012) SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey. Astron Astrophys 541:A129. doi:http://dx.doi.org/10.1051/0004-6361/201118498
Leloudas G, Patat F, Maund JR et al (2015a) Polarimetry of the superluminous supernova LSQ14MO: no evidence for significant deviations from spherical symmetry. ApJ 815:L10. doi:http://dx.doi.org/10.1088/2041-8205/815/1/l10
Leloudas G, Schulze S, Kruhler T et al (2015b) Spectroscopy of superluminous supernova host galaxies. A preference of hydrogen-poor events for extreme emission line galaxies. Mon Not R Astron Soc 449:917. doi:http://dx.doi.org/10.1093/mnras/stv320
Leonard DC, Filippenko AV, Ganeshalingam M et al (2006) A non-spherical core in the explosion of supernova SN 2004dj. Nature 440:505. doi:http://dx.doi.org/10.1038/nature04558
Levan AJ, Read AM, Metzger BD, Wheatley PJ, Tanvir NR (2013) Superluminous X-rays from a superluminous supernova. ApJ 771:136. doi:http://dx.doi.org/10.1088/0004-637x/771/2/136
Lunnan R, Chornock R, Berger E et al (2013) PS1-10bzj: a fast hydrogen-poor superluminous supernova in a metal-poor host galaxy. ApJ 771:97. doi:http://dx.doi.org/10.1088/0004-637X/771/2/97
Lunnan R, Chornock R, Berger E et al (2014) Hydrogen-poor superluminous supernovae and long-duration gamma-ray bursts have similar host galaxies. ApJ 787:138. doi:http://dx.doi.org/10.1088/0004-637x/787/2/138
Lunnan R, Chornock R, Berger E et al (2015) Zooming in on the progenitors of superluminous supernovae with the HST. ApJ 804:90. doi:http://dx.doi.org/10.1088/0004-637x/804/2/90
Lunnan R, Chornock R, Berger E et al (2016) PS1-14bj: a hydrogen-poor superluminous supernova With a long rise and slow decay. ArXiv e-prints, arXiv:1605.05235
Mazzali PA, Sullivan M, Pian E, Greiner J, Kann DA (2016) Spectrum formation in superluminous supernovae (Type I). Mon. Not. R. Astron Soc 458:3455. doi:http://dx.doi.org/10.1093/mnras/stw512
McCrum M, Smartt SJ, Kotak R et al (2014) The superluminous supernova PS1-11ap: bridging the gap between low and high redshift. Mon Not R Astron Soc 437:656
McCrum M, Smartt SJ, Rest A et al (2015) Selecting superluminous supernovae in faint galaxies from the first year of the Pan-STARRS1 Medium Deep Survey. Mon Not R Astron Soc 448:1206. doi:http://dx.doi.org/10.1093/mnras/stv034
Metzger BD, Margalit B, Kasen D, Quataert E (2015) The diversity of transients from magnetar birth in core collapse supernovae. Mon Not R Astron Soc 454:3311. doi:http://dx.doi.org/10.1093/mnras/stv2224
Metzger BD, Vurm I, Hascoët R, Beloborodov AM (2014) Ionization break-out from millisecond pulsar wind nebulae: an X-ray probe of the origin of superluminous supernovae. Mon Not R Astron Soc 437:703
Milisavljevic D, Soderberg AM, Margutti R et al (2013) SN 2012au: a golden link between superluminous supernovae and their lower-luminosity counterparts. ApJ 770:L38. doi:http://dx.doi.org/10.1088/2041-8205/770/2/l38
Miller AA, Chornock R, Perley DA et al (2008) The exceptionally luminous type II-linear supernova 2008es. ApJ 690:1303. doi:http://dx.doi.org/10.1088/0004-637x/690/2/1303
Modjaz M, Kewley L, Bloom JS et al (2011) Progenitor diagnostics for stripped core-collapse supernovae: measured metallicities at explosion sites. ApJ 731:L4. doi:http://dx.doi.org/10.1088/2041-8205/731/1/l4
Moriya T, Tominaga N, Tanaka M, Maeda K, Nomoto K (2010) A core-collapse supernova model for the extremely luminous type Ic supernova 2007bi: an alternative to the pair-instability supernova model. ApJ 717:L83. doi:http://dx.doi.org/10.1088/2041-8205/717/2/l83
Moriya TJ, Liu Z-W, Mackey J, Chen T-W, Langer N (2015) Revealing the binary origin of Type Ic superluminous supernovae through nebular hydrogen emission. Astron Astrophys 584:L5
Moriya TJ, Maeda K (2012) A DIP after the early emission of superluminous supernovae: a signature of shock breakout within dense circumstellar media. ApJ 756:L22. doi:http://dx.doi.org/10.1088/2041-8205/756/1/l22
Moriya TJ, Metzger BD, Blinnikov SI (2016) Supernovae powered by magnetars that transform into black holes. ArXiv e-prints, arXiv:1606.09316
Neill JD, Sullivan M, Gal-Yam A et al (2010) The extremehosts of extreme supernovae. ApJ 727:15. doi:http://dx.doi.org/10.1088/0004-637x/727/1/15
Nicholl M, Smartt SJ (2016) Seeing double: the frequency and detectability of double-peaked superluminous supernova light curves. Mon Not R Astron Soc Lett 457:L79. doi:http://dx.doi.org/10.1093/mnrasl/slv210
Nicholl M, Smartt SJ, Jerkstrand A et al (2013) Slowly fading super-luminous supernovae that are not pair-instability explosions. Nature 502:346. doi:http://dx.doi.org/10.1038/nature12569
Nicholl M, Smartt SJ, Jerkstrand A et al (2015a) On the diversity of superluminous supernovae: ejected mass as the dominant factor. Mon Not R Astron Soc 452:3869. doi:http://dx.doi.org/10.1093/mnras/stv1522
Nicholl M, Smartt SJ, Jerkstrand A et al (2015b) LSQ14bdq: a type Ic super-luminous supernova with a double-peaked light curve. ApJ 807:L18. doi:http://dx.doi.org/10.1088/2041-8205/807/1/L18
Nicholl M, Berger E, Smartt SJ et al (2016a) SN 2015bn: a detailed multi-wavelength view of a nearby superluminous supernova. ApJ 826:39. doi:http://dx.doi.org/10.3847/0004-637X/826/1/39
Nicholl M, Berger E, Margutti R et al (2016b) Superluminous supernova SN 2015bn in the nebular phase: evidence for the engine-powered explosion of a stripped massive star. ApJ 828:L18. doi:http://dx.doi.org/10.3847/2041-8205/828/2/l18
Nugent P, Aldering G, Phillips MM et al (1999) Supernovae 1999bc and 1999bd. IAU Circulars 7133
Ofek EO, Cameron PB, Kasliwal MM et al (2007) SN 2006gy: an extremely luminous supernova in the galaxy NGC 1260. ApJ 659:L13. doi:http://dx.doi.org/10.1086/516749
Papadopoulos A, D’Andrea CB, Sullivan M et al (2015) DES13S2cmm: the first superluminous supernova from the Dark Energy Survey. Monthly Notices of the Royal Astronomical Society 449:1215. doi:http://dx.doi.org/10.1093/mnras/stv174
Pastorello A, Smartt SJ, Botticella MT et al (2010) Ultra-bright optical transients are linked with type Ic supernovae. ApJ 724:L16. doi:http://dx.doi.org/10.1088/2041-8205/724/1/l16
Pastorello A, Wang X-F, Ciabattari F et al (2015) Massive stars exploding in a He-rich circumstellar medium – IX. SN 2014av and characterization of Type Ibn SNe. Mon Not R Astron Soc 456:853. doi:http://dx.doi.org/10.1093/mnras/stv2634
Perley DA, Quimby RM, Yan L et al (2016) Host-galaxy properties of 32 low-redshift superluminous supernovae from the palomar transient factory. ApJ 830:13. doi:http://dx.doi.org/10.3847/0004-637X/830/1/13
Piro AL (2015) Using double-peaked supernova light curves to study extended material. ApJ 808:L51. doi:http://dx.doi.org/10.1088/2041-8205/808/2/L51
Prajs S, Sullivan M, Smith M et al (2016) The volumetric rate of superluminous supernovae at z ∼ 1. ArXiv e-prints, arXiv:1605.05250
Quimby RM, Aldering G, Wheeler JC et al (2007) SN 2005ap: a most brilliant explosion. ApJ 668:L99. doi:http://dx.doi.org/10.1086/522862
Quimby RM, Yuan F, Akerlof C, Wheeler JC (2013) Rates of superluminous supernovae at z 0.2. Mon Not R Astron Soc 431:912. doi:http://dx.doi.org/10.1093/mnras/stt213
Quimby RM, Kulkarni SR, Kasliwal MM et al (2011) Hydrogen-poor superluminous stellar explosions. Nature 474:487. doi:http://dx.doi.org/10.1038/nature10095
Rabinak I, Waxman E (2011) The early UV/optical emission from core-collapse supernovae. ApJ 728:63. doi:http://dx.doi.org/10.1088/0004-637x/728/1/63
Rakavy G, Shaviv G (1967) Instabilities in highly evolved stellar models. ApJ 148:803. doi:http://dx.doi.org/10.1086/149204
Roy R, Sollerman J, Silverman JM et al (2016) SN 2012aa – a transient between Type Ibc core-collapse and superluminous supernovae. ArXiv e-prints, arXiv:1607.00924
Schawinski K, Justham S, Wolf C et al (2008) Supernova shock breakout from a red supergiant. Science 321:223. doi:http://dx.doi.org/10.1126/science.1160456
Silverman JM, Nugent PE, Gal-Yam A et al (2013) Type Ia supernovae strongly interacting with their circumstellar medium. ApJS 207:3. doi:http://dx.doi.org/10.1088/0067-0049/207/1/3
Smith M, Sullivan M, D’Andrea CB et al (2016) DES14X3taz: a type I superluminous supernova showing a luminous rapidly cooling initial pre-peak bump. ApJ 818:L8. doi:http://dx.doi.org/10.3847/2041-8205/818/1/L8
Smith N, Li W, Foley RJ et al (2007) SN 2006gy: discovery of the most luminous supernova ever recorded powered by the death of an extremely massive star like η carinae. ApJ 666:1116. doi:http://dx.doi.org/10.1086/519949
Soderberg AM, Berger E, Page KL et al (2008) An extremely luminous X-ray outburst at the birth of a supernova. Nature 453:469. doi:http://dx.doi.org/10.1038/nature06997
Soker N (2016) Jets launched at magnetar birth cannot be ignored. New Astron 47:88. doi:http://dx.doi.org/10.1016/j.newast.2016.02.009
Sorokina E, Blinnikov S, Nomoto K, Quimby R, Tolstov A (2016) Type I superluminous supernovae as explosions inside non-hydrogen circumstellar envelopes. ApJ 829:17. doi:http://dx.doi.org/10.3847/0004-637X/829/1/17
Taddia F, Stritzinger MD, Sollerman J et al (2013) Carnegie supernova project: observations of type IIn supernovae. Astron Astrophys 555:A10. doi:http://dx.doi.org/10.1051/0004-6361/201321180
Taddia F, Sollerman J, Leloudas G et al (2015) Early-time light curves of Type Ib/c supernovae from the SDSS-II Supernova Survey. Astron Astrophys 574:A60. doi:http://dx.doi.org/10.1051/0004-6361/201423915
Valenti S, Taubenberger S, Pastorello A et al (2012) A spectroscopically normal type Ic supernova from a very massive progenitor. ApJ 749:L28. doi:http://dx.doi.org/10.1088/2041-8205/749/2/l28
Vreeswijk PM, Savaglio S, Gal-Yam A et al (2014) The hydrogen-poor superluminous supernova iPTF 13ajg and its host galaxy in absorption and emission. ApJ 797:24. doi:http://dx.doi.org/10.1088/0004-637X/797/1/24
Wang SQ, Wang LJ, Dai ZG, Wu XF (2015) Superluminous supernovae powered by magnetars: late-time light curves and hard emission leakage. ApJ 799:107. doi:http://dx.doi.org/10.1088/0004-637X/799/1/107
Woosley SE (2010) Bright supernovae from magnetar birth. ApJ 719:L204. doi:http://dx.doi.org/10.1088/2041-8205/719/2/l204
Woosley SE, Blinnikov S, Heger A (2007) Pulsational pair instability as an explanation for the most luminous supernovae. Nature 450:390. doi:http://dx.doi.org/10.1038/nature06333
Yan L, Quimby R, Ofek E et al (2015) Detection of broad Hα emission lines in the late-time spectra of a hydrogen-poor superluminous supernova. ApJ 814:108. doi:http://dx.doi.org/10.1088/0004-637x/814/2/108
Acknowledgements
I would like to thank Matt Nicholl and Cosimo Inserra for the use of figures and helpful discussions and Iair Arcavi, Manos Chatzopoulos, Janet Chen, Jeff Cooke, Griffin Hosseinzadeh, Brian Metzger, Takashi Moriya, Stefano Valenti, and Stan Woosley for comments that improved the manuscript.
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Howell, D.A. (2017). Superluminous Supernovae. In: Alsabti, A., Murdin, P. (eds) Handbook of Supernovae. Springer, Cham. https://doi.org/10.1007/978-3-319-21846-5_41
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