Euclid: Searching for pair-instability supernovae with the Deep Survey

被引：17

作者：

Moriya, T. J. ^{[1
,2
]}

Inserra, C. ^{[3
]}

Tanaka, M. ^{[4
,5
]}

Cappellaro, E. ^{[6
]}

Della Valle, M. ^{[7
,8
,9
]}

Hook, I ^{[10
]}

Kotak, R. ^{[11
]}

Longo, G. ^{[8
,12
]}

Mannucci, F. ^{[13
]}

Mattila, S. ^{[11
]}

Tao, C. ^{[14
]}

Altieri, B. ^{[15
]}

Amara, A. ^{[16
]}

Auricchio, N. ^{[17
]}

Bonino, D. ^{[18
]}

Branchini, E. ^{[19
,20
,21
]}

Brescia, M. ^{[7
]}

Brinchmann, J. ^{[22
]}

Camera, S. ^{[18
,23
,24
]}

Capobianco, V ^{[18
]}

Carbone, C. ^{[25
]}

Carretero, J. ^{[26
,27
]}

Castellano, M. ^{[28
]}

Cavuoti, S. ^{[7
,8
,12
]}

Cimatti, A. ^{[13
,29
]}

Cledassou, R. ^{[30
,31
]}

Congedo, G. ^{[32
]}

Conselice, C. J. ^{[33
]}

Conversi, L. ^{[15
,34
]}

Copin, Y. ^{[35
]}

Corcione, L. ^{[18
]}

Courbin, F. ^{[36
]}

Cropper, M. ^{[37
]}

Da Silva, A. ^{[38
,39
]}

Degaudenzi, H. ^{[40
]}

Douspis, M. ^{[41
]}

Dubath, F. ^{[40
]}

Duncan, C. A. J. ^{[33
,42
]}

Dupac, X. ^{[15
]}

Dusini, S. ^{[43
]}

Ealet, A. ^{[35
]}

Farrens, S. ^{[44
]}

Ferriol, S. ^{[35
]}

Frailis, M. ^{[45
]}

Franceschi, E. ^{[17
]}

Fumana, M. ^{[25
]}

Garilli, B. ^{[25
]}

Gillard, W. ^{[14
]}

Gillis, B. ^{[32
]}

Giocoli, C. ^{[46
,47
]}

机构：

[1] Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan

[2] Monash Univ, Fac Sci, Sch Phys & Astron, Clayton, Vic 3800, Australia

[3] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[4] Tohoku Univ, Astron Inst, Sendai, Miyagi 9808578, Japan

[5] Tohoku Univ, Div Estab Frontier Sci, Org Adv Studies, Sendai, Miyagi 9808577, Japan

[6] INAF Osservatorio Astron Padova, Via Osservatorio 5, I-35122 Padua, Italy

[7] INAF Osservatorio Astron Capodimonte, Via Moiariello 16, I-80131 Naples, Italy

[8] Ist Nazl Fis Nucl, Sect Naples, Via Cinthia 6, I-80126 Naples, Italy

[9] Int Ctr Relativist Astrophys, Piazzale Republ 2, I-65122 Pescara, Italy

[10] Univ Lancaster, Dept Phys, Lancaster LA1 4YB, England

[11] Univ Turku, Dept Phys & Astron, Turku 20014, Finland

[12] Univ Federico II, Dept Phys E Pancini, Via Cinthia 6, I-80126 Naples, Italy

[13] INAF Osservatorio Astrofis Arcetri, Largo E Fermi 5, I-50125 Florence, Italy

[14] Aix Marseille Univ, CPPM, CNRS IN2P3, Marseille, France

[15] ESAC ESA, Camino Bajo del Castillo S-N, Madrid 28692, Spain

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

[17] INAF Osservatorio Astrofis & Sci Spazio Bologna, Via Piero Gobetti 93-3, I-40129 Bologna, Italy

[18] INAF Osservatorio Astrofis Torino, Via Osservatorio 20, I-10025 Pino Torinese, TO, Italy

[19] Ist Nazl Fis Nucl, Sez Roma Tre, Via Vasca Navale 84, I-00146 Rome, Italy

[20] Univ Genoa, Dipartimento Fis, Via Dodecaneso 33, I-16146 Genoa, Italy

[21] Ist Nazl Fis Nucl, Sez Genova, Via Dodecaneso 33, I-16146 Genoa, Italy

[22] Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Porto, Portugal

[23] Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy

[24] Ist Nazl Fis Nucl, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy

[25] INAF IASF Milano, Via Alfonso Corti 12, I-20133 Milan, Italy

[26] Port Informacio Cient, Campus UAB,C Albareda S-N, Barcelona 08193, Spain

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

[28] INAF Osservatorio Astron Roma, Via Frascati 33, I-00078 Monte Porzio Catone, Italy

[29] Alma Mater Studiorum Univ Bologna, Dipartimento Fis & Astron Augusto Righi, Via Piero Gobetti 93-2, I-40129 Bologna, Italy

[30] Inst Natl Phys Nucl & Phys Particules, 3 Rue Michel Ange, F-75794 Paris 16, France

[31] Ctr Natl Etud Spatiales, Toulouse, France

[32] Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland

[33] Univ Manchester, Jodrell Bank Ctr Astrophys, Dept Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs, England

[34] European Space Agcy ESRIN, Largo Galileo Galilei 1, I-00044 Rome, Italy

[35] Univ Lyon, Univ Claude Bernard Lyon 1, IP2I Lyon, CNRS IN2P3,UMR 5822, F-69622 Villeurbanne, France

[36] Ecole Polytech Fed Lausanne EPFL, Observ Sauverny, Lab Astrophys, Inst Phys, CH-1290 Versoix, Switzerland

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

[38] Univ Lisbon, Fac Ciencias, Dept Fis, Edificio C8, P-1749016 Lisbon, Portugal

[39] Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, P-1749016 Lisbon, Portugal

[40] Univ Geneva, Dept Astron, Ch Ecogia 16, CH-1290 Versoix, Switzerland

[41] Univ Paris Saclay, Inst Astrophys Spatiale, CNRS, F-91405 Orsay, France

[42] Univ Oxford, Dept Phys, Keble Rd, Oxford OX1 3RH, England

[43] INFN Padova, Via Marzolo 8, I-35131 Padua, Italy

[44] Univ Paris Saclay, Univ Paris Cite, CEA,CNRS, Astrophys Instrumentat & Modelisat Paris Saclay, F-91191 Gif Sur Yvette, France

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

[46] Ist Nazl Astrofis INAF, Osservatorio Astrofis & Sci Spazio OAS, Via Gobetti 93-3, I-40127 Bologna, Italy

[47] Ist Nazl Fis Nucl, Sez Bologna, Via Irnerio 46, I-40126 Bologna, Italy

[48] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany

[49] Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Fak Phys, Scheinerstr 1, D-81679 Munich, Germany

[50] Univ Oslo, Inst Theoret Astrophys, POB 1029 Blindern, N-0315 Oslo, Norway

来源：

ASTRONOMY & ASTROPHYSICS | 2022年 / 666卷

基金：

日本学术振兴会; 芬兰科学院; 美国国家航空航天局;

关键词：

stars: massive; supernovae: general; surveys; SUPERLUMINOUS SUPERNOVAE; LIGHT; RATES; MASS; ENRICHMENT; EXPLOSION; SIGNATURE; EVOLUTION; SPECTRA; SAMPLE;

D O I：

10.1051/0004-6361/202243810

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Pair-instability supernovae are theorized supernovae that have not yet been observationally confirmed. They are predicted to exist in low-metallicity environments. Because overall metallicity becomes lower at higher redshifts, deep near-infrared transient surveys probing high-redshift supernovae are suitable to discover pair-instability supernovae. The Euclid satellite, which is planned launch in 2023, has a near-infrared wide-field instrument that is suitable for a high-redshift supernova survey. The Euclid Deep Survey is planned to make regular observations of three Euclid Deep Fields (40 deg(2) in total) spanning Euclid's six-year primary mission period. While the observations of the Euclid Deep Fields are not frequent, we show that the predicted long duration of pair-instability supernovae would allow us to search for high-redshift pair-instability supernovae with the Euclid Deep Survey. Based on the current observational plan of the Euclid mission, we conduct survey simulations in order to estimate the expected numbers of pair-instability supernova discoveries. We find that up to several hundred pair-instability supernovae at z less than or similar to 3.5 can be discovered within the Euclid Deep Survey. We also show that pair-instability supernova candidates can be efficiently identified by their duration and color, which can be determined with the current Euclid Deep Survey plan. We conclude that the Euclid mission can lead to the first confirmation of pair-instability supernovae if their event rates are as high as those predicted by recent theoretical studies. We also update the expected numbers of superluminous supernova discoveries in the Euclid Deep Survey based on the latest observational plan.

引用

页数：12

共 85 条

[1] A chemical signature of first-generation very massive stars [J].

Aoki, W. ;

Tominaga, N. ;

Beers, T. C. ;

Honda, S. ;

Lee, Y. S. .

SCIENCE, 2014, 345 (6199) :912-915

[2] Extending the supernova Hubble diagram to z ∼ 1.5 with the Euclid space mission [J].

Astier, P. ;

Balland, C. ;

Brescia, M. ;

Cappellaro, E. ;

Carlberg, R. G. ;

Cavuoti, S. ;

Della Valle, M. ;

Gangler, E. ;

Goobar, A. ;

Guy, J. ;

Hardin, D. ;

Hook, I. M. ;

Kessler, R. ;

Kim, A. ;

Linder, E. ;

Longo, G. ;

Maguire, K. ;

Mannucci, F. ;

Mattila, S. ;

Nichol, R. ;

Pain, R. ;

Regnault, N. ;

Spiro, S. ;

Sullivan, M. ;

Tao, C. ;

Turatto, M. ;

Wang, X. F. ;

Wood-Vasey, W. M. .

ASTRONOMY & ASTROPHYSICS, 2014, 572

[3] DYNAMICS OF SUPERNOVA EXPLOSION RESULTING FROM PAIR FORMATION [J].

BARKAT, Z ;

RAKAVY, G ;

SACK, N .

PHYSICAL REVIEW LETTERS, 1967, 18 (10) :379-&

[4] New Determinations of the UV Luminosity Functions from z ∼ 9 to 2 Show a Remarkable Consistency with Halo Growth and a Constant Star Formation Efficiency [J].

Bouwens, R. J. ;

Oesch, P. A. ;

Stefanon, M. ;

Illingworth, G. ;

Labbe, I ;

Reddy, N. ;

Atek, H. ;

Montes, M. ;

Naidu, R. ;

Nanayakkara, T. ;

Nelson, E. ;

Wilkins, S. .

ASTRONOMICAL JOURNAL, 2021, 162 (02)

[5] Estimating transient rates from cosmological simulations and BPASS [J].

Briel, Max M. ;

Eldridge, J. J. ;

Stanway, Elizabeth R. ;

Stevance, H. F. ;

Chrimes, A. A. .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2022, 514 (01) :1315-1334

[6] EFFECTS OF ROTATION ON THE MINIMUM MASS OF PRIMORDIAL PROGENITORS OF PAIR-INSTABILITY SUPERNOVAE [J].

Chatzopoulos, E. ;

Wheeler, J. Craig .

ASTROPHYSICAL JOURNAL, 2012, 748 (01)

[7]

Chen Z, 2022, Arxiv, DOI arXiv:2202.02060

[8]

Chen ZH, 2022, Arxiv, DOI arXiv:2202.02059

[9] Metallicity of stars formed throughout the cosmic history based on the observational properties of star-forming galaxies [J].

Chruslinska, Martyna ;

Nelemans, Gijs .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 488 (04) :5300-5326

[10] Light Curves of Hydrogen-poor Superluminous Supernovae from the Palomar Transient Factory [J].

De Cia, Annalisa ;

Gal-Yam, A. ;

Rubin, A. ;

Leloudas, G. ;

Vreeswijk, P. ;

Perley, D. A. ;

Quimby, R. ;

Yan, Lin ;

Sullivan, M. ;

Floers, A. ;

Sollerman, J. ;

Bersier, D. ;

Cenko, S. B. ;

Gal-Yam, M. ;

Maguire, K. ;

Ofek, E. O. ;

Prentice, S. ;

Schulze, S. ;

Spyromilio, J. ;

Valenti, S. ;

Arcavi, I. ;

Corsi, A. ;

Howell, D. A. ;

Mazzali, P. ;

Kasliwal, M. M. ;

Taddia, F. ;

Yaron, O. .

ASTROPHYSICAL JOURNAL, 2018, 860 (02)

← 1 2 3 4 5 6 7 8 9 →