Cosmic evolution and metal aversion in superluminous supernova host galaxies

被引：101

作者：

Schulze, S. ^{[1
,2
,3
]}

Kruehler, T. ^{[4
]}

Leloudas, G. ^{[1
,5
]}

Gorosabel, J. ^{[6
,7
,8
]}

Mehner, A. ^{[9
]}

Buchner, J. ^{[2
,3
]}

Kim, S. ^{[2
]}

Ibar, E. ^{[10
]}

Amorin, R. ^{[11
,12
]}

Herrero-Illana, R. ^{[8
,9
]}

Anderson, J. P. ^{[9
]}

Bauer, F. E. ^{[2
,3
,13
]}

Christensen, L. ^{[5
]}

de Pasquale, M. ^{[14
]}

de Ugarte Postigo, A. ^{[8
]}

Gallazzi, A. ^{[15
]}

Hjorth, J. ^{[5
]}

Morrell, N. ^{[16
]}

Malesani, D. ^{[5
]}

Sparre, M. ^{[17
]}

Stalder, B. ^{[18
]}

Stark, A. A. ^{[19
]}

Thone, C. C. ^{[8
]}

Wheeler, J. C. ^{[20
]}

机构：

[1] Weizmann Inst Sci, Dept Particle Phys & Astrophys, IL-7610001 Rehovot, Israel

[2] Pontificia Univ Catolica Chile, Inst Astrofis, Fac Fis, Vicuna Mackenna 4860, Santiago 7820436, Chile

[3] Millennium Inst Astrophys, Vicuna Mackenna 4860, Santiago 7820436, Chile

[4] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

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

[6] Univ Basque Country, UPV EHU, ETS Ingn,IAA CSIC, Dept Fis Aplicada 1,Unidad Asociada Grp Ciencia P, Alameda Urquijo S-N, E-48013 Bilbao, Spain

[7] Basque Fdn Sci, Ikerbasque, Alameda Urquijo 36-5, E-48008 Bilbao, Spain

[8] CSIC, IAA, Glorieta Astron S-N, E-18008 Granada, Spain

[9] ESO, Alonso Cordova 3107, Vitacura, Santiago De Chi, Chile

[10] Univ Valparaiso, Inst Fis & Astron, Avda Gran Bretana 1111, Valparaiso, Chile

[11] Univ Cambridge, Cavendish Lab, 19 JJ Thomson Ave, Cambridge CB3 0HE, England

[12] Univ Cambridge, Kavli Inst Cosmol, Madingley Rd, Cambridge CB3 0HA, England

[13] Space Sci Inst, 4750 Walnut St,Suite 205, Boulder, CO 80301 USA

[14] Univ Coll London, Mullard Space Sci Lab, Holmbury Rd, Dorking RH5 6NT, Surrey, England

[15] INAF, Osservatorio Astrofis Arcetri, Largo Enrico Fermi 5, I-50125 Florence, Italy

[16] Carnegie Observ, Las Campanas Observ, Casilla 601, La Serena, Chile

[17] Heidelberger Inst Theoret Studien, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany

[18] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA

[19] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA

[20] Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2018年 / 473卷 / 01期

基金：

美国国家科学基金会; 欧洲研究理事会; 美国国家航空航天局;

关键词：

galaxies: evolution; galaxies: high-redshift; galaxies: luminosity function; mass function; galaxies: starburst; galaxies: star formation; DIGITAL SKY SURVEY; MASS-METALLICITY RELATION; CORE-COLLAPSE SUPERNOVAE; HUBBLE-SPACE-TELESCOPE; RADIO IMAGING SURVEY; PAIR-INSTABILITY; STAR-FORMATION; LUMINOSITY FUNCTIONS; STELLAR MASS; DEEP SURVEY;

D O I：

10.1093/mnras/stx2352

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The SUperluminous Supernova Host galaxIES survey aims to provide strong new constraints on the progenitors of superluminous supernovae (SLSNe) by understanding the relationship to their host galaxies. We present the photometric properties of 53 H-poor and 16 H-rich SLSN host galaxies out to z similar to 4. We model their spectral energy distributions to derive physical properties, which we compare with other galaxy populations. At low redshift, H-poor SLSNe are preferentially found in very blue, low-mass galaxies with high average specific star formation rates. As redshift increases, the host population follows the general evolution of star-forming galaxies towards more luminous galaxies. After accounting for secular evolution, we find evidence for differential evolution in galaxy mass, but not in the B band and the farultraviolet luminosity (3 sigma confidence). Most remarkable is the scarcity of hosts with stellar masses above 10(10) M-circle dot for both classes of SLSNe. In case of H-poor SLSNe, we attribute this to a stifled production efficiency above similar to 0.4 solar metallicity. However, we argue that, in addition to lowmetallicity, a short-lived stellar population is also required to regulate the SLSN production. H-rich SLSNe are found in a very diverse population of star-forming galaxies. Still, the scarcity of massive hosts suggests a stifled production efficiency above similar to 0.8 solar metallicity. The large dispersion of the H-rich SLSNe host properties is in stark contrast to those of gamma-ray burst, regular core-collapse SN, and H-poor SLSNe host galaxies. We propose that multiple progenitor channels give rise to this subclass.

引用

页码：1258 / 1285

页数：28

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