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Semantic Scholar Open Access 2022 8 sitasi

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

T. Moriya C. Inserra M. Tanaka E. Cappellaro M. Valle +376 lainnya
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Abstrak

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 to be launched 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 deg2 in total) spanning the Euclid's 6 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<~ 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 that 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.

Topik & Kata Kunci

Physics

Penulis (381)

T

T. Moriya

C

C. Inserra

M

M. Tanaka

E

E. Cappellaro

M

M. Valle

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I. Hook

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08193 Bellaterra

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E. P. F. Lausanne

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Observatoire de Sauverny

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1290 Versoix

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Switzerland.

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U

U. London

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Holmbury St. Mary

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Departament de F'isica

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F. Ciencias

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Sezione Infn di Bologna

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46 ViaIrnerio

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M. F. P. Physics

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1. Giessenbachstr.

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D. Garching

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Germany

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Universitatssternwarte Munchen

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F. Physik

L

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1. Scheinerstrasse

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8. Munchen

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I. Astrophysics

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U. Oslo

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P. O. B. 1. Blindern

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N. Oslo

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Pasadena

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91109

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Usa

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von Hoerner Sulger GmbH

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8. Schlossplatz

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D-68723 Schwetzingen

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T. Denmark

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2800 Kgs. Lyngby

D

Denmark.

M

M. Astronomie

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17 Konigstuhl

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D. Heidelberg

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H. I. O. Physics

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2. GustafHallstrominkatu

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4. OudeHoogeveensedijk

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7991PD

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Argelander Institut fur Astronomie

U

U. Bonn

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53121 Bonn

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62 vialeBertiPichat

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Institute for Computational Cosmology

D

D. University

S

South Road

D

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I. Paris

U

Umr 7095

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Sorbonne Universit'e

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98 bis boulevard Arago

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7. Paris

U

U. Sciences

A

A. Switzerland

S

School of Electrical Engineering

5

5210 Windisch

E

European Space AgencyESTEC

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1. Keplerlaan

2

2. Noordwijk

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U. Aarhus

N

Ny Munkegade 120

C

C. DK-8000Aarhus

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Institute of Space Science

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Bucharest

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România

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Institute for Fundamental Physics of the Universe

2

2. viaBeirut

3

34127 Trieste

D

Dipartimento di Fisica e AstronomiaG.Galilei

U

U. Padova

C

Centro de Investigaciones Energ'eticas

M

Medioambientales y Tecnol'ogicas

4

40 AvenidaComplutense

2

28014 Madrid

T

Tapada da Ajuda

P

P. Lisboa

U

Universidad Polit'ecnica de Cartagena

D

D. D. E. Y. T. D. Computadoras

3

30202 Cartagena

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A

A. Center

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CA 91125

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Format Sitasi

APA MLA BibTeX
Moriya, T., Inserra, C., Tanaka, M., Cappellaro, E., Valle, M., Hook, I. et al. (2022). Euclid: Searching for pair-instability supernovae with the Deep Survey. https://doi.org/10.1051/0004-6361/202243810

Akses Cepat

Lihat di Sumber doi.org/10.1051/0004-6361/202243810
Informasi Jurnal
Tahun Terbit
2022
Bahasa
en
Total Sitasi
8×
Sumber Database
Semantic Scholar
DOI
10.1051/0004-6361/202243810
Akses
Open Access ✓