SUbaru Supernovae with Hubble Infrared (SUSHI)

Nao Suzuki; Greg Aldering; Rahman Amanullah; Pierre Antilogus; Pierre Astier; Kyle Barbary; Marc Betoule; Kyle Boone; Susana E. Deustua; Mamoru Doi; Andrew S. Fruchter; Ariel Goobar; Brian Hayden; Francois Hazenberg; Isobel Hook; Xiaosheng Huang; Ji-an Jiang; Takahiro Kato; Alex G. Kim; Marek Kowalski; Chris E. Lidman; Eric Linder; Keiichi Maeda; Tomoki Morokuma; Jakob Nordin; Reynald Pain; Saul Perlmutter; Nicolas Regnault; David Rubin; Clare Myers Saunders; Anthony L. Spadafora; Masaomi Tanaka; Nozomu Tominaga; Naoki Yasuda; Naoki Yoshida

SUbaru Supernovae with Hubble Infrared (SUSHI)

Nao Suzuki, Greg Aldering, Rahman Amanullah, Pierre Antilogus, Pierre Astier, Kyle Barbary, Marc Betoule, Kyle Boone, Susana E. Deustua, Mamoru Doi, Andrew S. Fruchter, Ariel Goobar, Brian Hayden, Francois Hazenberg, Isobel Hook, Xiaosheng Huang, Ji-an Jiang, Takahiro Kato, Alex G. Kim, Marek KowalskiChris E. Lidman, Eric Linder, Keiichi Maeda, Tomoki Morokuma, Jakob Nordin, Reynald Pain, Saul Perlmutter, Nicolas Regnault, David Rubin, Clare Myers Saunders, Anthony L. Spadafora, Masaomi Tanaka, Nozomu Tominaga, Naoki Yasuda, Naoki Yoshida

Research output: Other contribution

Abstract

During the next two HST Cycles, the Subaru Strategic Program (SSP) will conduct a rolling search with Hyper Suprime-Cam (HSC) that will discover and study scores of very high quality SNe Ia up to redshift of ~1.5. However, above a redshift of one, the Subaru photometry will be limited to the UV and blue rest-frame of the SNe. By combining the HSC light curve with just one non-disruptive ToO observation and a "reference image" (after the SN has faded) from HST for each of 46 SNe, we will improve the dark energy Figure of Merit (FoM) obtainable from all past and present high-redshift SN searches by a factor of 2.3. This opportunity is unique. Because this search requires frequent changes of the massive HSC at the Subaru prime focus, it will not be repeated for the foreseeable future.

Original language	English
Publication status	Published - 1 Jun 2016

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https://ui.adsabs.harvard.edu/abs/2016hst..prop14808S

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Suzuki, N., Aldering, G., Amanullah, R., Antilogus, P., Astier, P., Barbary, K., Betoule, M., Boone, K., Deustua, S. E., Doi, M., Fruchter, A. S., Goobar, A., Hayden, B., Hazenberg, F., Hook, I., Huang, X., Jiang, J., Kato, T., Kim, A. G., ... Yoshida, N. (2016, Jun 1). SUbaru Supernovae with Hubble Infrared (SUSHI). https://ui.adsabs.harvard.edu/abs/2016hst..prop14808S

@misc{5b775471da3342dea3f3c13c73d670a7,

title = "SUbaru Supernovae with Hubble Infrared (SUSHI)",

abstract = "During the next two HST Cycles, the Subaru Strategic Program (SSP) will conduct a rolling search with Hyper Suprime-Cam (HSC) that will discover and study scores of very high quality SNe Ia up to redshift of ~1.5. However, above a redshift of one, the Subaru photometry will be limited to the UV and blue rest-frame of the SNe. By combining the HSC light curve with just one non-disruptive ToO observation and a {"}reference image{"} (after the SN has faded) from HST for each of 46 SNe, we will improve the dark energy Figure of Merit (FoM) obtainable from all past and present high-redshift SN searches by a factor of 2.3. This opportunity is unique. Because this search requires frequent changes of the massive HSC at the Subaru prime focus, it will not be repeated for the foreseeable future.",

author = "Nao Suzuki and Greg Aldering and Rahman Amanullah and Pierre Antilogus and Pierre Astier and Kyle Barbary and Marc Betoule and Kyle Boone and Deustua, {Susana E.} and Mamoru Doi and Fruchter, {Andrew S.} and Ariel Goobar and Brian Hayden and Francois Hazenberg and Isobel Hook and Xiaosheng Huang and Ji-an Jiang and Takahiro Kato and Kim, {Alex G.} and Marek Kowalski and Lidman, {Chris E.} and Eric Linder and Keiichi Maeda and Tomoki Morokuma and Jakob Nordin and Reynald Pain and Saul Perlmutter and Nicolas Regnault and David Rubin and Saunders, {Clare Myers} and Spadafora, {Anthony L.} and Masaomi Tanaka and Nozomu Tominaga and Naoki Yasuda and Naoki Yoshida",

year = "2016",

month = jun,

day = "1",

language = "English",

type = "Other",

}

Suzuki, N, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Barbary, K, Betoule, M, Boone, K, Deustua, SE, Doi, M, Fruchter, AS, Goobar, A, Hayden, B, Hazenberg, F, Hook, I, Huang, X, Jiang, J, Kato, T, Kim, AG, Kowalski, M, Lidman, CE, Linder, E, Maeda, K, Morokuma, T, Nordin, J, Pain, R, Perlmutter, S, Regnault, N, Rubin, D, Saunders, CM, Spadafora, AL, Tanaka, M, Tominaga, N, Yasuda, N & Yoshida, N 2016, SUbaru Supernovae with Hubble Infrared (SUSHI).. <https://ui.adsabs.harvard.edu/abs/2016hst..prop14808S>

TY - GEN

T1 - SUbaru Supernovae with Hubble Infrared (SUSHI)

AU - Suzuki, Nao

AU - Aldering, Greg

AU - Amanullah, Rahman

AU - Antilogus, Pierre

AU - Astier, Pierre

AU - Barbary, Kyle

AU - Betoule, Marc

AU - Boone, Kyle

AU - Deustua, Susana E.

AU - Doi, Mamoru

AU - Fruchter, Andrew S.

AU - Goobar, Ariel

AU - Hayden, Brian

AU - Hazenberg, Francois

AU - Hook, Isobel

AU - Huang, Xiaosheng

AU - Jiang, Ji-an

AU - Kato, Takahiro

AU - Kim, Alex G.

AU - Kowalski, Marek

AU - Lidman, Chris E.

AU - Linder, Eric

AU - Maeda, Keiichi

AU - Morokuma, Tomoki

AU - Nordin, Jakob

AU - Pain, Reynald

AU - Perlmutter, Saul

AU - Regnault, Nicolas

AU - Rubin, David

AU - Saunders, Clare Myers

AU - Spadafora, Anthony L.

AU - Tanaka, Masaomi

AU - Tominaga, Nozomu

AU - Yasuda, Naoki

AU - Yoshida, Naoki

PY - 2016/6/1

Y1 - 2016/6/1

N2 - During the next two HST Cycles, the Subaru Strategic Program (SSP) will conduct a rolling search with Hyper Suprime-Cam (HSC) that will discover and study scores of very high quality SNe Ia up to redshift of ~1.5. However, above a redshift of one, the Subaru photometry will be limited to the UV and blue rest-frame of the SNe. By combining the HSC light curve with just one non-disruptive ToO observation and a "reference image" (after the SN has faded) from HST for each of 46 SNe, we will improve the dark energy Figure of Merit (FoM) obtainable from all past and present high-redshift SN searches by a factor of 2.3. This opportunity is unique. Because this search requires frequent changes of the massive HSC at the Subaru prime focus, it will not be repeated for the foreseeable future.

AB - During the next two HST Cycles, the Subaru Strategic Program (SSP) will conduct a rolling search with Hyper Suprime-Cam (HSC) that will discover and study scores of very high quality SNe Ia up to redshift of ~1.5. However, above a redshift of one, the Subaru photometry will be limited to the UV and blue rest-frame of the SNe. By combining the HSC light curve with just one non-disruptive ToO observation and a "reference image" (after the SN has faded) from HST for each of 46 SNe, we will improve the dark energy Figure of Merit (FoM) obtainable from all past and present high-redshift SN searches by a factor of 2.3. This opportunity is unique. Because this search requires frequent changes of the massive HSC at the Subaru prime focus, it will not be repeated for the foreseeable future.

M3 - Other contribution

ER -

SUbaru Supernovae with Hubble Infrared (SUSHI)

Abstract

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