Supernova Siblings: Assessing the Consistency of Properties of Type Ia Supernovae that Share the Same Parent Galaxies

被引：25

作者：

Scolnic, D. ^{[1
]}

Smith, M. ^{[2
]}

Massiah, A. ^{[3
]}

Wiseman, P. ^{[2
]}

Brout, D. ^{[4
]}

Kessler, R. ^{[5
,6
]}

Davis, T. M. ^{[7
]}

Foley, R. J. ^{[8
]}

Galbany, L. ^{[9
]}

Hinton, S. R. ^{[7
]}

Hounsell, R. ^{[4
]}

Kelsey, L. ^{[2
]}

Lidman, C. ^{[10
]}

Macaulay, E. ^{[11
]}

Morgan, R. ^{[12
]}

Nichol, R. C. ^{[11
]}

Moller, A. ^{[13
]}

Popovic, B. ^{[1
]}

Sako, M. ^{[4
]}

Sullivan, M. ^{[2
]}

Thomas, B. P. ^{[11
]}

Tucker, B. E. ^{[10
]}

Abbott, T. M. C. ^{[14
]}

Aguena, M. ^{[15
,16
]}

Allam, S. ^{[17
]}

Annis, J. ^{[17
]}

Avila, S. ^{[18
]}

Bechtol, K. ^{[12
,19
]}

Bertin, E. ^{[20
,21
]}

Brooks, D. ^{[22
]}

Burke, D. L. ^{[23
,24
]}

Rosell, A. Carnero ^{[25
]}

Carollo, D. ^{[26
]}

Kind, M. Carrasco ^{[27
,28
]}

Carretero, J. ^{[29
]}

Costanzi, M. ^{[30
,31
]}

da Costa, L. N. ^{[16
,32
]}

De Vicente, J. ^{[25
]}

Desai, S. ^{[33
]}

Diehl, H. T. ^{[17
]}

Doel, P. ^{[22
]}

Drlica-Wagner, A. ^{[5
,6
,17
]}

Eckert, K. ^{[4
]}

Eifler, T. F. ^{[34
,35
]}

Everett, S. ^{[8
]}

Flaugher, B. ^{[17
]}

Fosalba, P. ^{[36
,37
]}

Frieman, J. ^{[6
,17
]}

Garcia-Bellido, J. ^{[18
]}

Gaztanaga, E. ^{[36
,37
]}

机构：

[1] Duke Univ, Dept Phys, Durham, NC 27708 USA

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

[3] Univ Connecticut, Storrs, CT 06269 USA

[4] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA

[5] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA

[6] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA

[7] Univ Queensland, Sch Math & Phys, Brisbane, Qld 4072, Australia

[8] Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA

[9] Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA

[10] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia

[11] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[12] Univ Wisconsin, Phys Dept, 2320 Chamberlin Hall,1150 Univ Ave, Madison, WI 53706 USA

[13] Univ Clermont Auvergne, LPC, CNRS, IN2P3, F-63000 Clermont Ferrand, France

[14] Cerro Tololo Interamer Observ, Natl Opt Astron Observ, Casilla 603, La Serena, Chile

[15] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, CP 66318, BR-05314970 Sao Paulo, SP, Brazil

[16] Lab Interinst & Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[17] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA

[18] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[19] LSST, 933 North Cherry Ave, Tucson, AZ 85721 USA

[20] Inst Astrophys Paris, CNRS, UMR 7095, F-75014 Paris, France

[21] Sorbonne Univ, Inst Astrophys Paris, UMR 7095, UPMC Univ Paris 06, F-75014 Paris, France

[22] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England

[23] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA

[24] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA

[25] Ctr Invest Energet Medioambientales & Tecnol CIEM, Madrid, Spain

[26] Astrophys Observ Turin, INAF, I-10025 Pino Torinese, Italy

[27] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA

[28] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA

[29] Barcelona Inst Sci & Technol, Inst Fis Altes Energies IFAE, Campus UAB, E-08193 Bellaterra, Barcelona, Spain

[30] INAF Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy

[31] Inst Fundamental Phys Universe, Via Beirut 2, I-34014 Trieste, Italy

[32] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil

[33] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana, India

[34] Univ Arizona, Dept Astron, Steward Observ, 933 North Cherry Ave, Tucson, AZ 85721 USA

[35] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA

[36] Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain

[37] CSIC, Inst Space Sci ICE, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain

[38] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA

[39] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA

[40] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia

[41] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA

[42] Swiss Fed Inst Technol, Dept Phys, Wolfgang Pauli Str 16, CH-8093 Zurich, Switzerland

[43] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[44] Ohio State Univ, Dept Phys, 174 W 18th Ave, Columbus, OH 43210 USA

[45] Ctr Astrophys Harvard & Smithsonian, 60 Garden St, Cambridge, MA 02138 USA

[46] Macquarie Univ, Australian Astron Opt, N Ryde, NSW 2113, Australia

[47] Lowell Observ, 1400 Mars Hill Rd, Flagstaff, AZ 86001 USA

[48] Univ Sydney, Sch Phys, Sydney Inst Astron, A28, Sydney, NSW 2006, Australia

[49] Princeton Univ, Dept Astrophys Sci, Peyton Hall, Princeton, NJ 08544 USA

[50] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA

来源：

ASTROPHYSICAL JOURNAL LETTERS | 2020年 / 896卷 / 01期

基金：

澳大利亚研究理事会; 欧盟地平线“2020”; 美国国家科学基金会; 英国科学技术设施理事会; 欧洲研究理事会;

关键词：

Observational cosmology; LUMINOSITY; DISTANCE; SOFTWARE; RATES; MASS;

D O I：

10.3847/2041-8213/ab8735

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

While many studies have shown a correlation between properties of the light curves of SNe Ia and properties of their host galaxies, it remains unclear what is driving these correlations. We introduce a new direct method to study these correlations by analyzing "parent" galaxies that host multiple SNe Ia "siblings." Here, we search the Dark Energy Survey SN sample, one of the largest samples of discovered SNe, and find eight galaxies that hosted two likely SNe Ia. Comparing the light-curve properties of these SNe and recovered distances from the light curves, we find no better agreement between properties of SNe in the same galaxy as any random pair of galaxies, with the exception of the SN light-curve stretch. We show at 2.8 sigma significance that at least one-half of the intrinsic scatter of SNe Ia distance modulus residuals is not from common host properties. We also discuss the robustness with which we could make this evaluation with LSST, which will find 100x more pairs of galaxies, and pave a new line of study on the consistency of SNe Ia in the same parent galaxies. Finally, we argue that it is unlikely that some of these SNe are actually single, lensed SN with multiple images.

引用

页数：9

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