Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble

O. Graur; S. A. Rodney; D. Maoz; A. G. Riess; S. W. Jha; M. Postman; T. Dahlen; T. W.S. Holoien; C. McCully; B. Patel; L. G. Strolger; N. Benítez; D. Coe; S. Jouvel; E. Medezinski; A. Molino; M. Nonino; L. Bradley; A. Koekemoer; I. Balestra; S. B. Cenko; K. I. Clubb; M. E. Dickinson; A. V. Filippenko; T. F. Frederiksen; P. Garnavich; J. Hjorth; D. O. Jones; B. Leibundgut; T. Matheson; B. Mobasher; P. Rosati; J. M. Silverman; V. U; K. Jedruszczuk; C. Li; K. Lin; M. Mirmelstein; J. Neustadt; A. Ovadia; E. H. Rogers

doi:10.1088/0004-637X/783/1/28

Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble

O. Graur, S. A. Rodney, D. Maoz, A. G. Riess, S. W. Jha, M. Postman, T. Dahlen, T. W.S. Holoien, C. McCully, B. Patel, L. G. Strolger, N. Benítez, D. Coe, S. Jouvel, E. Medezinski, A. Molino, M. Nonino, L. Bradley, A. Koekemoer, I. BalestraS. B. Cenko, K. I. Clubb, M. E. Dickinson, A. V. Filippenko, T. F. Frederiksen, P. Garnavich, J. Hjorth, D. O. Jones, B. Leibundgut, T. Matheson, B. Mobasher, P. Rosati, J. M. Silverman, V. U, K. Jedruszczuk, C. Li, K. Lin, M. Mirmelstein, J. Neustadt, A. Ovadia, E. H. Rogers

School of Physics and Astronomy

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Abstract

We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Supernova survey with Hubble (CLASH). Using the Advanced Camera for Surveys and the Wide Field Camera 3 on the Hubble Space Telescope (HST), we have imaged 25 galaxy-cluster fields and parallel fields of non-cluster galaxies. We report a sample of 27 SNe discovered in the parallel fields. Of these SNe,13 are classified as SN Ia candidates, including four SN Ia candidates at redshifts z > 1.2. We measure volumetric SN Ia rates to redshift 1.8 and add the first upper limit on the SN Ia rate in the range 1.8 < z < 2.4. The results are consistent with the rates measured by the HST/GOODS and Subaru Deep Field SN surveys. We model these results together with previous measurements at z < 1 from the literature. The best-fitting SN Ia delay-time distribution (DTD; the distribution of times that elapse between a short burst of star formation and subsequent SN Ia explosions) is a power law with an index of , where the statistical uncertainty is a result of the 68% and 95% (in parentheses) statistical uncertainties reported for the various SN Ia rates (from this work and from the literature), and the systematic uncertainty reflects the range of possible cosmic star-formation histories. We also test DTD models produced by an assortment of published binary population synthesis (BPS) simulations. The shapes of all BPS double-degenerate DTDs are consistent with the volumetric SN Ia measurements, when the DTD models are scaled up by factors of 3-9. In contrast, all BPS single-degenerate DTDs are ruled out by the measurements at >99% significance level.

Original language	English
Article number	28
Journal	Astrophysical Journal
Volume	783
Issue number	1
DOIs	https://doi.org/10.1088/0004-637X/783/1/28
State	Published - 1 Mar 2014

Keywords

supernovae: general
surveys
white dwarfs

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10.1088/0004-637X/783/1/28

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Graur, O., Rodney, S. A., Maoz, D., Riess, A. G., Jha, S. W., Postman, M., Dahlen, T., Holoien, T. W. S., McCully, C., Patel, B., Strolger, L. G., Benítez, N., Coe, D., Jouvel, S., Medezinski, E., Molino, A., Nonino, M., Bradley, L., Koekemoer, A., ... Rogers, E. H. (2014). Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble. Astrophysical Journal, 783(1), [28]. https://doi.org/10.1088/0004-637X/783/1/28

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title = "Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble",

abstract = "We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Supernova survey with Hubble (CLASH). Using the Advanced Camera for Surveys and the Wide Field Camera 3 on the Hubble Space Telescope (HST), we have imaged 25 galaxy-cluster fields and parallel fields of non-cluster galaxies. We report a sample of 27 SNe discovered in the parallel fields. Of these SNe,13 are classified as SN Ia candidates, including four SN Ia candidates at redshifts z > 1.2. We measure volumetric SN Ia rates to redshift 1.8 and add the first upper limit on the SN Ia rate in the range 1.8 < z < 2.4. The results are consistent with the rates measured by the HST/GOODS and Subaru Deep Field SN surveys. We model these results together with previous measurements at z < 1 from the literature. The best-fitting SN Ia delay-time distribution (DTD; the distribution of times that elapse between a short burst of star formation and subsequent SN Ia explosions) is a power law with an index of , where the statistical uncertainty is a result of the 68% and 95% (in parentheses) statistical uncertainties reported for the various SN Ia rates (from this work and from the literature), and the systematic uncertainty reflects the range of possible cosmic star-formation histories. We also test DTD models produced by an assortment of published binary population synthesis (BPS) simulations. The shapes of all BPS double-degenerate DTDs are consistent with the volumetric SN Ia measurements, when the DTD models are scaled up by factors of 3-9. In contrast, all BPS single-degenerate DTDs are ruled out by the measurements at >99% significance level.",

keywords = "supernovae: general, surveys, white dwarfs",

author = "O. Graur and Rodney, {S. A.} and D. Maoz and Riess, {A. G.} and Jha, {S. W.} and M. Postman and T. Dahlen and Holoien, {T. W.S.} and C. McCully and B. Patel and Strolger, {L. G.} and N. Ben{\'i}tez and D. Coe and S. Jouvel and E. Medezinski and A. Molino and M. Nonino and L. Bradley and A. Koekemoer and I. Balestra and Cenko, {S. B.} and Clubb, {K. I.} and Dickinson, {M. E.} and Filippenko, {A. V.} and Frederiksen, {T. F.} and P. Garnavich and J. Hjorth and Jones, {D. O.} and B. Leibundgut and T. Matheson and B. Mobasher and P. Rosati and Silverman, {J. M.} and V. U and K. Jedruszczuk and C. Li and K. Lin and M. Mirmelstein and J. Neustadt and A. Ovadia and Rogers, {E. H.}",

year = "2014",

month = mar,

day = "1",

doi = "10.1088/0004-637X/783/1/28",

language = "אנגלית",

volume = "783",

journal = "Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing Ltd.",

number = "1",

}

Graur, O, Rodney, SA, Maoz, D, Riess, AG, Jha, SW, Postman, M, Dahlen, T, Holoien, TWS, McCully, C, Patel, B, Strolger, LG, Benítez, N, Coe, D, Jouvel, S, Medezinski, E, Molino, A, Nonino, M, Bradley, L, Koekemoer, A, Balestra, I, Cenko, SB, Clubb, KI, Dickinson, ME, Filippenko, AV, Frederiksen, TF, Garnavich, P, Hjorth, J, Jones, DO, Leibundgut, B, Matheson, T, Mobasher, B, Rosati, P, Silverman, JM, U, V, Jedruszczuk, K, Li, C, Lin, K, Mirmelstein, M, Neustadt, J, Ovadia, A & Rogers, EH 2014, 'Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble', Astrophysical Journal, vol. 783, no. 1, 28. https://doi.org/10.1088/0004-637X/783/1/28

TY - JOUR

T1 - Type-Ia supernova rates to redshift 2.4 from clash

T2 - The cluster lensing and supernova survey with Hubble

AU - Graur, O.

AU - Rodney, S. A.

AU - Maoz, D.

AU - Riess, A. G.

AU - Jha, S. W.

AU - Postman, M.

AU - Dahlen, T.

AU - Holoien, T. W.S.

AU - McCully, C.

AU - Patel, B.

AU - Strolger, L. G.

AU - Benítez, N.

AU - Coe, D.

AU - Jouvel, S.

AU - Medezinski, E.

AU - Molino, A.

AU - Nonino, M.

AU - Bradley, L.

AU - Koekemoer, A.

AU - Balestra, I.

AU - Cenko, S. B.

AU - Clubb, K. I.

AU - Dickinson, M. E.

AU - Filippenko, A. V.

AU - Frederiksen, T. F.

AU - Garnavich, P.

AU - Hjorth, J.

AU - Jones, D. O.

AU - Leibundgut, B.

AU - Matheson, T.

AU - Mobasher, B.

AU - Rosati, P.

AU - Silverman, J. M.

AU - U, V.

AU - Jedruszczuk, K.

AU - Li, C.

AU - Lin, K.

AU - Mirmelstein, M.

AU - Neustadt, J.

AU - Ovadia, A.

AU - Rogers, E. H.

PY - 2014/3/1

Y1 - 2014/3/1

N2 - We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Supernova survey with Hubble (CLASH). Using the Advanced Camera for Surveys and the Wide Field Camera 3 on the Hubble Space Telescope (HST), we have imaged 25 galaxy-cluster fields and parallel fields of non-cluster galaxies. We report a sample of 27 SNe discovered in the parallel fields. Of these SNe,13 are classified as SN Ia candidates, including four SN Ia candidates at redshifts z > 1.2. We measure volumetric SN Ia rates to redshift 1.8 and add the first upper limit on the SN Ia rate in the range 1.8 < z < 2.4. The results are consistent with the rates measured by the HST/GOODS and Subaru Deep Field SN surveys. We model these results together with previous measurements at z < 1 from the literature. The best-fitting SN Ia delay-time distribution (DTD; the distribution of times that elapse between a short burst of star formation and subsequent SN Ia explosions) is a power law with an index of , where the statistical uncertainty is a result of the 68% and 95% (in parentheses) statistical uncertainties reported for the various SN Ia rates (from this work and from the literature), and the systematic uncertainty reflects the range of possible cosmic star-formation histories. We also test DTD models produced by an assortment of published binary population synthesis (BPS) simulations. The shapes of all BPS double-degenerate DTDs are consistent with the volumetric SN Ia measurements, when the DTD models are scaled up by factors of 3-9. In contrast, all BPS single-degenerate DTDs are ruled out by the measurements at >99% significance level.

AB - We present the supernova (SN) sample and Type-Ia SN (SN Ia) rates from the Cluster Lensing And Supernova survey with Hubble (CLASH). Using the Advanced Camera for Surveys and the Wide Field Camera 3 on the Hubble Space Telescope (HST), we have imaged 25 galaxy-cluster fields and parallel fields of non-cluster galaxies. We report a sample of 27 SNe discovered in the parallel fields. Of these SNe,13 are classified as SN Ia candidates, including four SN Ia candidates at redshifts z > 1.2. We measure volumetric SN Ia rates to redshift 1.8 and add the first upper limit on the SN Ia rate in the range 1.8 < z < 2.4. The results are consistent with the rates measured by the HST/GOODS and Subaru Deep Field SN surveys. We model these results together with previous measurements at z < 1 from the literature. The best-fitting SN Ia delay-time distribution (DTD; the distribution of times that elapse between a short burst of star formation and subsequent SN Ia explosions) is a power law with an index of , where the statistical uncertainty is a result of the 68% and 95% (in parentheses) statistical uncertainties reported for the various SN Ia rates (from this work and from the literature), and the systematic uncertainty reflects the range of possible cosmic star-formation histories. We also test DTD models produced by an assortment of published binary population synthesis (BPS) simulations. The shapes of all BPS double-degenerate DTDs are consistent with the volumetric SN Ia measurements, when the DTD models are scaled up by factors of 3-9. In contrast, all BPS single-degenerate DTDs are ruled out by the measurements at >99% significance level.

KW - supernovae: general

KW - surveys

KW - white dwarfs

UR - http://www.scopus.com/inward/record.url?scp=84894384534&partnerID=8YFLogxK

U2 - 10.1088/0004-637X/783/1/28

DO - 10.1088/0004-637X/783/1/28

M3 - מאמר

AN - SCOPUS:84894384534

VL - 783

JO - Astrophysical Journal

JF - Astrophysical Journal

SN - 0004-637X

IS - 1

M1 - 28

ER -

Type-Ia supernova rates to redshift 2.4 from clash: The cluster lensing and supernova survey with Hubble

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Keywords

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