Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy

J. D.R. Pierel; A. B. Newman; S. Dhawan; M. Gu; B. A. Joshi; T. Li; S. Schuldt; L. G. Strolger; S. H. Suyu; G. B. Caminha; S. H. Cohen; J. M. Diego; J. C.J. DŚilva; S. Ertl; B. L. Frye; G. Granata; C. Grillo; A. M. Koekemoer; J. Li; A. Robotham; J. Summers; T. Treu; R. A. Windhorst; A. Zitrin; S. Agarwal; A. Agrawal; N. Arendse; S. Belli; C. Burns; R. Cañameras; S. Chakrabarti; W. Chen; T. E. Collett; D. A. Coulter; R. S. Ellis; M. Engesser; N. Foo; O. D. Fox; C. Gall; N. Garuda; S. Gezari; S. Gomez; K. Glazebrook; J. Hjorth; X. Huang; S. W. Jha; P. S. Kamieneski; P. Kelly; C. Larison; L. A. Moustakas; M. Pascale; I. Pérez-Fournon; T. Petrushevska; F. Poidevin; A. Rest; M. Shahbandeh; A. J. Shajib; M. Siebert; C. Storfer; M. Talbot; Q. Wang; T. Wevers; Y. Zenati

doi:10.3847/2041-8213/ad4648

Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy

J. D.R. Pierel
, A. B. Newman
, S. Dhawan
, M. Gu
, B. A. Joshi
, T. Li
, S. Schuldt
, L. G. Strolger
, S. H. Suyu
, G. B. Caminha
, S. H. Cohen
, J. M. Diego
, J. C.J. DŚilva
, S. Ertl
, B. L. Frye
, G. Granata
, C. Grillo
, A. M. Koekemoer
, J. Li
, A. Robotham

J. Summers, T. Treu, R. A. Windhorst, A. Zitrin, S. Agarwal, A. Agrawal, N. Arendse, S. Belli, C. Burns, R. Cañameras, S. Chakrabarti, W. Chen, T. E. Collett, D. A. Coulter, R. S. Ellis, M. Engesser, N. Foo, O. D. Fox, C. Gall, N. Garuda, S. Gezari, S. Gomez, K. Glazebrook, J. Hjorth, X. Huang, S. W. Jha, P. S. Kamieneski, P. Kelly, C. Larison, L. A. Moustakas, M. Pascale, I. Pérez-Fournon, T. Petrushevska, F. Poidevin, A. Rest, M. Shahbandeh, A. J. Shajib, M. Siebert, C. Storfer, M. Talbot, Q. Wang, T. Wevers, Y. Zenati

פרסום מחקרי: פרסום בכתב עת › מאמר › ביקורת עמיתים

תקציר

A bright (m _F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in three locations, and remarkably is the second lensed SN found in the same host galaxy. The previous lensed SN was called “Requiem,” and therefore the new SN is named “Encore.” This makes the MACS J0138.0−2155 cluster the first known system to produce more than one multiply imaged SN. Moreover, both SN Requiem and SN Encore are Type Ia SNe (SNe Ia), making this the most distant case of a galaxy hosting two SNe Ia. Using parametric host fitting, we determine the probability of detecting two SNe Ia in this host galaxy over a ∼10 yr window to be ≈3%. These observations have the potential to yield a Hubble constant (H ₀) measurement with ∼10% precision, only the third lensed SN capable of such a result, using the three visible images of the SN. Both SN Requiem and SN Encore have a fourth image that is expected to appear within a few years of ∼2030, providing an unprecedented baseline for time-delay cosmography.

שפה מקורית	אנגלית
מספר המאמר	L37
כתב עת	Astrophysical Journal Letters
כרך	967
מספר גיליון	2
מזהי עצם דיגיטלי (DOIs)	https://doi.org/10.3847/2041-8213/ad4648
סטטוס פרסום	פורסם - 1 יוני 2024
פורסם באופן חיצוני	כן

הערה ביבליוגרפית

Publisher Copyright:
© 2024. The Author(s). Published by the American Astronomical Society.

גישה למסמך

10.3847/2041-8213/ad4648

קבצים וקישורים אחרים

Link to publication in Scopus

פורמט ציטוט ביבליוגרפי

Pierel, J. D. R., Newman, A. B., Dhawan, S., Gu, M., Joshi, B. A., Li, T., Schuldt, S., Strolger, L. G., Suyu, S. H., Caminha, G. B., Cohen, S. H., Diego, J. M., DŚilva, J. C. J., Ertl, S., Frye, B. L., Granata, G., Grillo, C., Koekemoer, A. M., Li, J., ... Zenati, Y. (2024). Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy. Astrophysical Journal Letters, 967(2), המאמר L37. https://doi.org/10.3847/2041-8213/ad4648

@article{5c6bd0c05fb84ca1a81153b7f75f2b2a,

title = "Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy",

abstract = "A bright (m F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in three locations, and remarkably is the second lensed SN found in the same host galaxy. The previous lensed SN was called “Requiem,” and therefore the new SN is named “Encore.” This makes the MACS J0138.0−2155 cluster the first known system to produce more than one multiply imaged SN. Moreover, both SN Requiem and SN Encore are Type Ia SNe (SNe Ia), making this the most distant case of a galaxy hosting two SNe Ia. Using parametric host fitting, we determine the probability of detecting two SNe Ia in this host galaxy over a ∼10 yr window to be ≈3\%. These observations have the potential to yield a Hubble constant (H 0) measurement with ∼10\% precision, only the third lensed SN capable of such a result, using the three visible images of the SN. Both SN Requiem and SN Encore have a fourth image that is expected to appear within a few years of ∼2030, providing an unprecedented baseline for time-delay cosmography.",

author = "Pierel, \{J. D.R.\} and Newman, \{A. B.\} and S. Dhawan and M. Gu and Joshi, \{B. A.\} and T. Li and S. Schuldt and Strolger, \{L. G.\} and Suyu, \{S. H.\} and Caminha, \{G. B.\} and Cohen, \{S. H.\} and Diego, \{J. M.\} and D{\'S}ilva, \{J. C.J.\} and S. Ertl and Frye, \{B. L.\} and G. Granata and C. Grillo and Koekemoer, \{A. M.\} and J. Li and A. Robotham and J. Summers and T. Treu and Windhorst, \{R. A.\} and A. Zitrin and S. Agarwal and A. Agrawal and N. Arendse and S. Belli and C. Burns and R. Ca{\~n}ameras and S. Chakrabarti and W. Chen and Collett, \{T. E.\} and Coulter, \{D. A.\} and Ellis, \{R. S.\} and M. Engesser and N. Foo and Fox, \{O. D.\} and C. Gall and N. Garuda and S. Gezari and S. Gomez and K. Glazebrook and J. Hjorth and X. Huang and Jha, \{S. W.\} and Kamieneski, \{P. S.\} and P. Kelly and C. Larison and Moustakas, \{L. A.\} and M. Pascale and I. P{\'e}rez-Fournon and T. Petrushevska and F. Poidevin and A. Rest and M. Shahbandeh and Shajib, \{A. J.\} and M. Siebert and C. Storfer and M. Talbot and Q. Wang and T. Wevers and Y. Zenati",

note = "Publisher Copyright: {\textcopyright} 2024. The Author(s). Published by the American Astronomical Society.",

year = "2024",

month = jun,

day = "1",

doi = "10.3847/2041-8213/ad4648",

language = "אנגלית",

volume = "967",

journal = "Astrophysical Journal Letters",

issn = "2041-8205",

publisher = "American Astronomical Society",

number = "2",

}

Pierel, JDR, Newman, AB, Dhawan, S, Gu, M, Joshi, BA, Li, T, Schuldt, S, Strolger, LG, Suyu, SH, Caminha, GB, Cohen, SH, Diego, JM, DŚilva, JCJ, Ertl, S, Frye, BL, Granata, G, Grillo, C, Koekemoer, AM, Li, J, Robotham, A, Summers, J, Treu, T, Windhorst, RA, Zitrin, A, Agarwal, S, Agrawal, A, Arendse, N, Belli, S, Burns, C, Cañameras, R, Chakrabarti, S, Chen, W, Collett, TE, Coulter, DA, Ellis, RS, Engesser, M, Foo, N, Fox, OD, Gall, C, Garuda, N, Gezari, S, Gomez, S, Glazebrook, K, Hjorth, J, Huang, X, Jha, SW, Kamieneski, PS, Kelly, P, Larison, C, Moustakas, LA, Pascale, M, Pérez-Fournon, I, Petrushevska, T, Poidevin, F, Rest, A, Shahbandeh, M, Shajib, AJ, Siebert, M, Storfer, C, Talbot, M, Wang, Q, Wevers, T & Zenati, Y 2024, 'Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy', Astrophysical Journal Letters, כרך 967, מס' 2, L37. https://doi.org/10.3847/2041-8213/ad4648

TY - JOUR

T1 - Lensed Type Ia Supernova “Encore” at z = 2

T2 - The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy

AU - Pierel, J. D.R.

AU - Newman, A. B.

AU - Dhawan, S.

AU - Gu, M.

AU - Joshi, B. A.

AU - Li, T.

AU - Schuldt, S.

AU - Strolger, L. G.

AU - Suyu, S. H.

AU - Caminha, G. B.

AU - Cohen, S. H.

AU - Diego, J. M.

AU - DŚilva, J. C.J.

AU - Ertl, S.

AU - Frye, B. L.

AU - Granata, G.

AU - Grillo, C.

AU - Koekemoer, A. M.

AU - Li, J.

AU - Robotham, A.

AU - Summers, J.

AU - Treu, T.

AU - Windhorst, R. A.

AU - Zitrin, A.

AU - Agarwal, S.

AU - Agrawal, A.

AU - Arendse, N.

AU - Belli, S.

AU - Burns, C.

AU - Cañameras, R.

AU - Chakrabarti, S.

AU - Chen, W.

AU - Collett, T. E.

AU - Coulter, D. A.

AU - Ellis, R. S.

AU - Engesser, M.

AU - Foo, N.

AU - Fox, O. D.

AU - Gall, C.

AU - Garuda, N.

AU - Gezari, S.

AU - Gomez, S.

AU - Glazebrook, K.

AU - Hjorth, J.

AU - Huang, X.

AU - Jha, S. W.

AU - Kamieneski, P. S.

AU - Kelly, P.

AU - Larison, C.

AU - Moustakas, L. A.

AU - Pascale, M.

AU - Pérez-Fournon, I.

AU - Petrushevska, T.

AU - Poidevin, F.

AU - Rest, A.

AU - Shahbandeh, M.

AU - Shajib, A. J.

AU - Siebert, M.

AU - Storfer, C.

AU - Talbot, M.

AU - Wang, Q.

AU - Wevers, T.

AU - Zenati, Y.

PY - 2024/6/1

Y1 - 2024/6/1

N2 - A bright (m F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in three locations, and remarkably is the second lensed SN found in the same host galaxy. The previous lensed SN was called “Requiem,” and therefore the new SN is named “Encore.” This makes the MACS J0138.0−2155 cluster the first known system to produce more than one multiply imaged SN. Moreover, both SN Requiem and SN Encore are Type Ia SNe (SNe Ia), making this the most distant case of a galaxy hosting two SNe Ia. Using parametric host fitting, we determine the probability of detecting two SNe Ia in this host galaxy over a ∼10 yr window to be ≈3%. These observations have the potential to yield a Hubble constant (H 0) measurement with ∼10% precision, only the third lensed SN capable of such a result, using the three visible images of the SN. Both SN Requiem and SN Encore have a fourth image that is expected to appear within a few years of ∼2030, providing an unprecedented baseline for time-delay cosmography.

AB - A bright (m F150W,AB = 24 mag), z = 1.95 supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detected in three locations, and remarkably is the second lensed SN found in the same host galaxy. The previous lensed SN was called “Requiem,” and therefore the new SN is named “Encore.” This makes the MACS J0138.0−2155 cluster the first known system to produce more than one multiply imaged SN. Moreover, both SN Requiem and SN Encore are Type Ia SNe (SNe Ia), making this the most distant case of a galaxy hosting two SNe Ia. Using parametric host fitting, we determine the probability of detecting two SNe Ia in this host galaxy over a ∼10 yr window to be ≈3%. These observations have the potential to yield a Hubble constant (H 0) measurement with ∼10% precision, only the third lensed SN capable of such a result, using the three visible images of the SN. Both SN Requiem and SN Encore have a fourth image that is expected to appear within a few years of ∼2030, providing an unprecedented baseline for time-delay cosmography.

UR - https://www.scopus.com/pages/publications/85195099247

U2 - 10.3847/2041-8213/ad4648

DO - 10.3847/2041-8213/ad4648

M3 - ???researchoutput.researchoutputtypes.contributiontojournal.article???

AN - SCOPUS:85195099247

SN - 2041-8205

VL - 967

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

M1 - L37

ER -

Lensed Type Ia Supernova “Encore” at z = 2: The First Instance of Two Multiply Imaged Supernovae in the Same Host Galaxy

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