The Type Ia Supernova Rate in High Redshift Galaxy Clusters

Kyle H. Barbary; G. Aldering; R. Amanullah; L. F. Barrientos; M. Brodwin; N. Connolly; K. S. Dawson; M. Doi; M. Donahue; P. Eisenhardt; E. Ellingson; L. Faccioli; V. Fadeyev; H. K. Fakhouri; A. S. Fruchter; D. Gilbank; M. D. Gladders; G. Goldhaber; A. Goobar; A. Gude; J. Hennawi; H. Hoekstra; E. Hsiao; Y. Ihara; B. T. Jannuzi; B. Koester; M. Kowalski; C. Lidman; E. V. Linder; L. Lubin; J. Meyers; T. Morokuma; S. Perlmutter; M. Postman; J. Rhodes; P. Rosati; D. Rubin; D. J. Schlegel; A. L. Spadafora; S. Stanford; M. Strovink; N. Takanashi; N. Yasuda; H. K. Yee

The Type Ia Supernova Rate in High Redshift Galaxy Clusters

Kyle H. Barbary, G. Aldering, R. Amanullah, L. F. Barrientos, M. Brodwin, N. Connolly, K. S. Dawson, M. Doi, M. Donahue, P. Eisenhardt, E. Ellingson, L. Faccioli, V. Fadeyev, H. K. Fakhouri, A. S. Fruchter, D. Gilbank, M. D. Gladders, G. Goldhaber, A. Goobar, A. GudeJ. Hennawi, H. Hoekstra, E. Hsiao, Y. Ihara, B. T. Jannuzi, B. Koester, M. Kowalski, C. Lidman, E. V. Linder, L. Lubin, J. Meyers, T. Morokuma, S. Perlmutter, M. Postman, J. Rhodes, P. Rosati, D. Rubin, D. J. Schlegel, A. L. Spadafora, S. Stanford, M. Strovink, N. Takanashi, N. Yasuda, H. K. Yee

Research School of Astronomy & Astrophysics

Research output: Contribution to conference › Paper

Abstract

The type Ia supernova (SN Ia) rate in galaxy clusters can be a powerful probe of both the SN Ia progenitor system and the intracluster medium of the clusters themselves. The cluster SN Ia rate has recently been measured at redshifts below 0.2, but only weak constraints based on one or two SNe exist at high redshift. We report a measurement of the SN Ia rate in galaxy clusters at 0.9 < z < 1.5 based on 9 cluster SNe Ia from the Hubble Space Telescope Cluster Supernova Survey (PI: Perlmutter; see Dawson et al. 2009), providing statistical errors comparable to low redshift measurements. We also use the fraction of hostless SNe in the clusters to place an upper limit on the amount of intracluster light at z > 0.9. This work has been supported by the Office of Science, U.S. Department of Energy, through contract DE-AC02-05CH11231 and in part by NASA through grants associated with HST-GO-10496.

Original language	English
Pages	343.03
Publication status	Published - 1 Jan 2010

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https://ui.adsabs.harvard.edu/abs/2010AAS...21534303B

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Barbary, K. H., Aldering, G., Amanullah, R., Barrientos, L. F., Brodwin, M., Connolly, N., Dawson, K. S., Doi, M., Donahue, M., Eisenhardt, P., Ellingson, E., Faccioli, L., Fadeyev, V., Fakhouri, H. K., Fruchter, A. S., Gilbank, D., Gladders, M. D., Goldhaber, G., Goobar, A., ... Yee, H. K. (2010). The Type Ia Supernova Rate in High Redshift Galaxy Clusters. 343.03. https://ui.adsabs.harvard.edu/abs/2010AAS...21534303B

@conference{ce8d3d9242894eb5a83e9fcee94ac098,

title = "The Type Ia Supernova Rate in High Redshift Galaxy Clusters",

abstract = "The type Ia supernova (SN Ia) rate in galaxy clusters can be a powerful probe of both the SN Ia progenitor system and the intracluster medium of the clusters themselves. The cluster SN Ia rate has recently been measured at redshifts below 0.2, but only weak constraints based on one or two SNe exist at high redshift. We report a measurement of the SN Ia rate in galaxy clusters at 0.9 < z < 1.5 based on 9 cluster SNe Ia from the Hubble Space Telescope Cluster Supernova Survey (PI: Perlmutter; see Dawson et al. 2009), providing statistical errors comparable to low redshift measurements. We also use the fraction of hostless SNe in the clusters to place an upper limit on the amount of intracluster light at z > 0.9. This work has been supported by the Office of Science, U.S. Department of Energy, through contract DE-AC02-05CH11231 and in part by NASA through grants associated with HST-GO-10496.",

author = "Barbary, {Kyle H.} and G. Aldering and R. Amanullah and Barrientos, {L. F.} and M. Brodwin and N. Connolly and Dawson, {K. S.} and M. Doi and M. Donahue and P. Eisenhardt and E. Ellingson and L. Faccioli and V. Fadeyev and Fakhouri, {H. K.} and Fruchter, {A. S.} and D. Gilbank and Gladders, {M. D.} and G. Goldhaber and A. Goobar and A. Gude and J. Hennawi and H. Hoekstra and E. Hsiao and Y. Ihara and Jannuzi, {B. T.} and B. Koester and M. Kowalski and C. Lidman and Linder, {E. V.} and L. Lubin and J. Meyers and T. Morokuma and S. Perlmutter and M. Postman and J. Rhodes and P. Rosati and D. Rubin and Schlegel, {D. J.} and Spadafora, {A. L.} and S. Stanford and M. Strovink and N. Takanashi and N. Yasuda and Yee, {H. K.}",

year = "2010",

month = jan,

day = "1",

language = "English",

pages = "343.03",

}

Barbary, KH, Aldering, G, Amanullah, R, Barrientos, LF, Brodwin, M, Connolly, N, Dawson, KS, Doi, M, Donahue, M, Eisenhardt, P, Ellingson, E, Faccioli, L, Fadeyev, V, Fakhouri, HK, Fruchter, AS, Gilbank, D, Gladders, MD, Goldhaber, G, Goobar, A, Gude, A, Hennawi, J, Hoekstra, H, Hsiao, E, Ihara, Y, Jannuzi, BT, Koester, B, Kowalski, M, Lidman, C, Linder, EV, Lubin, L, Meyers, J, Morokuma, T, Perlmutter, S, Postman, M, Rhodes, J, Rosati, P, Rubin, D, Schlegel, DJ, Spadafora, AL, Stanford, S, Strovink, M, Takanashi, N, Yasuda, N & Yee, HK 2010, 'The Type Ia Supernova Rate in High Redshift Galaxy Clusters', pp. 343.03. <https://ui.adsabs.harvard.edu/abs/2010AAS...21534303B>

TY - CONF

T1 - The Type Ia Supernova Rate in High Redshift Galaxy Clusters

AU - Barbary, Kyle H.

AU - Aldering, G.

AU - Amanullah, R.

AU - Barrientos, L. F.

AU - Brodwin, M.

AU - Connolly, N.

AU - Dawson, K. S.

AU - Doi, M.

AU - Donahue, M.

AU - Eisenhardt, P.

AU - Ellingson, E.

AU - Faccioli, L.

AU - Fadeyev, V.

AU - Fakhouri, H. K.

AU - Fruchter, A. S.

AU - Gilbank, D.

AU - Gladders, M. D.

AU - Goldhaber, G.

AU - Goobar, A.

AU - Gude, A.

AU - Hennawi, J.

AU - Hoekstra, H.

AU - Hsiao, E.

AU - Ihara, Y.

AU - Jannuzi, B. T.

AU - Koester, B.

AU - Kowalski, M.

AU - Lidman, C.

AU - Linder, E. V.

AU - Lubin, L.

AU - Meyers, J.

AU - Morokuma, T.

AU - Perlmutter, S.

AU - Postman, M.

AU - Rhodes, J.

AU - Rosati, P.

AU - Rubin, D.

AU - Schlegel, D. J.

AU - Spadafora, A. L.

AU - Stanford, S.

AU - Strovink, M.

AU - Takanashi, N.

AU - Yasuda, N.

AU - Yee, H. K.

PY - 2010/1/1

Y1 - 2010/1/1

N2 - The type Ia supernova (SN Ia) rate in galaxy clusters can be a powerful probe of both the SN Ia progenitor system and the intracluster medium of the clusters themselves. The cluster SN Ia rate has recently been measured at redshifts below 0.2, but only weak constraints based on one or two SNe exist at high redshift. We report a measurement of the SN Ia rate in galaxy clusters at 0.9 < z < 1.5 based on 9 cluster SNe Ia from the Hubble Space Telescope Cluster Supernova Survey (PI: Perlmutter; see Dawson et al. 2009), providing statistical errors comparable to low redshift measurements. We also use the fraction of hostless SNe in the clusters to place an upper limit on the amount of intracluster light at z > 0.9. This work has been supported by the Office of Science, U.S. Department of Energy, through contract DE-AC02-05CH11231 and in part by NASA through grants associated with HST-GO-10496.

AB - The type Ia supernova (SN Ia) rate in galaxy clusters can be a powerful probe of both the SN Ia progenitor system and the intracluster medium of the clusters themselves. The cluster SN Ia rate has recently been measured at redshifts below 0.2, but only weak constraints based on one or two SNe exist at high redshift. We report a measurement of the SN Ia rate in galaxy clusters at 0.9 < z < 1.5 based on 9 cluster SNe Ia from the Hubble Space Telescope Cluster Supernova Survey (PI: Perlmutter; see Dawson et al. 2009), providing statistical errors comparable to low redshift measurements. We also use the fraction of hostless SNe in the clusters to place an upper limit on the amount of intracluster light at z > 0.9. This work has been supported by the Office of Science, U.S. Department of Energy, through contract DE-AC02-05CH11231 and in part by NASA through grants associated with HST-GO-10496.

M3 - Paper

SP - 343.03

ER -

The Type Ia Supernova Rate in High Redshift Galaxy Clusters

Abstract

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