A Hubble Space Telescope survey of the host galaxies of Superluminous Supernovae

被引：89

作者：

Angus, C. R. ^{[1
]}

Levan, A. J. ^{[1
]}

Perley, D. A. ^{[2
,3
]}

Tanvir, N. R. ^{[4
]}

Lyman, J. D. ^{[1
]}

Stanway, E. R. ^{[1
]}

Fruchter, A. S. ^{[5
]}

机构：

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

[2] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Maries Vej 30, DK-2100 Copenhagen, Denmark

[3] CALTECH, Dept Astron, Pasadena, CA 91106 USA

[4] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England

[5] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2016年 / 458卷 / 01期

关键词：

supernovae: general; galaxies: dwarf; galaxies: luminosity function; mass function; galaxies: starburst; GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; DIGITAL SKY SURVEY; LUMINOUS SUPERNOVA; STAR-FORMATION; IA SUPERNOVAE; LIGHT CURVES; PROGENITOR MASS; IC SUPERNOVAE; DATA RELEASE;

D O I：

10.1093/mnras/stw063

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present Hubble Space Telescope (HST) Wide Field Camera 3 UV and near-IR (nIR) imaging of 21 Superluminous Supernovae (SLSNe) host galaxies, providing a sensitive probe of star formation and stellar mass within the hosts. Comparing the photometric and morphological properties of these host galaxies with those of core-collapse supernovae (CCSNe) and long duration gamma-ray bursts (LGRBs), we find SLSN hosts are fainter and more compact at both UV and nIR wavelengths, in some cases we barely recover hosts with absolute magnitude around My ti 14. With the addition of ground based optical observations and archival results, we produce spectral energy distribution fits to these hosts, and show that SLSN hosts possess lower stellar mass and star formation rates. This is most pronounced for the hydrogen deficient Type-I SLSN hosts, although Type-II H-rich SLSN host galaxies remain distinct from the bulk of CCSNe, spanning a remarkably broad range of absolute magnitudes, with similar to 30 per cent of SLSNe-II arising from galaxies fainter than M-nIR similar to -14. The detection of our faintest SLSN hosts increases the confidence that SLSNe-I hosts are distinct from those of LGRBs in star formation rate and stellar mass, and suggests that apparent similarities in metallicity may be due to the limited fraction of hosts for which emission line metallicity measurements are feasible. The broad range of luminosities of SLSN-II hosts is difficult to describe by metallicity cuts, and does not match the expectations of any reasonable UV-weighted luminosity function, suggesting additional environmental constraints are likely necessary to yield hydrogen rich SLSNe.

引用

页码：84 / 104

页数：21

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