The volumetric rate of superluminous supernovae at z ∼ 1

被引：79

作者：

Prajs, S. ^{[1
]}

Sullivan, M. ^{[1
]}

Smith, M. ^{[1
]}

Levan, A. ^{[2
]}

Karpenka, N. V. ^{[1
]}

Edwards, T. D. P. ^{[3
]}

Walker, C. R. ^{[4
]}

Wolf, W. M. ^{[5
]}

Balland, C. ^{[6
,7
]}

Carlberg, R. ^{[8
]}

Howell, D. A. ^{[9
,10
]}

Lidman, C. ^{[11
]}

Pain, R. ^{[6
,7
]}

Pritchet, C. ^{[12
]}

Ruhlmann-Kleider, V. ^{[13
]}

机构：

[1] Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England

[2] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England

[3] Univ Amsterdam, GRAPPA Inst, Sci Pk 904, NL-1090 GL Amsterdam, Netherlands

[4] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England

[5] Univ Calif Santa Barbara, Kavli Inst Theoret Phys, Santa Barbara, CA 93106 USA

[6] CNRS, IN2P3, LPNHE, F-75005 Paris, France

[7] Univ Paris VI & VII, F-75005 Paris, France

[8] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H8, Canada

[9] Las Cumbres Observ Global Telescope, 6740 Cortona Dr,Suite 102, Goleta, CA 93111 USA

[10] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA

[11] Australian Astron Observ, N Ryde, NSW 2113, Australia

[12] Univ Victoria, Dept Phys & Astron, POB 3055, Victoria, BC V8W 3P6, Canada

[13] CEA, Ctr Saclay, IRFU SPP, F-91191 Gif Sur Yvette, France

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 464卷 / 03期

关键词：

surveys; supernovae: general; GAMMA-RAY BURSTS; MASSIVE BLACK-HOLE; LEGACY SURVEY; LUMINOUS SUPERNOVAE; HIGH-REDSHIFT; IA SUPERNOVAE; LIGHT-CURVE; PHOTOMETRIC REDSHIFTS; OPTICAL TRANSIENT; PAIR-INSTABILITY;

D O I：

10.1093/mnras/stw1942

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a measurement of the volumetric rate of superluminous supernovae (SLSNe) at z similar to 1.0, measured using archival data from the first four years of the Canada-France-Hawaii Telescope Supernova Legacy Survey (SNLS). We develop a method for the photometric classification of SLSNe to construct our sample. Our sample includes two previously spectroscopically identified objects, and a further new candidate selected using our classification technique. We use the point-source recovery efficiencies from Perrett et al. and a Monte Carlo approach to calculate the rate based on our SLSN sample. We find that the three identified SLSNe from SNLS give a rate of 91(-36)(+76) SNe yr(-1) Gpc(-3) at a volume-weighted redshift of z = 1.13. This is equivalent to 2.2(-0.9)(+1.8) x 10(-4) of the volumetric core-collapse supernova rate at the same redshift. When combined with other rate measurements from the literature, we show that the rate of SLSNe increases with redshift in a manner consistent with that of the cosmic star formation history. We also estimate the rate of ultra-long gamma-ray bursts based on the events discovered by the Swift satellite, and show that it is comparable to the rate of SLSNe, providing further evidence of a possible connection between these two classes of events. We also examine the host galaxies of the SLSNe discovered in SNLS, and find them to be consistent with the stellar-mass distribution of other published samples of SLSNe.

引用

页码：3568 / 3579

页数：12

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