High-Redshift SNe with Subaru and HST

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

High-Redshift SNe with Subaru and HST

David Rubin, Nao Suzuki, Nicolas Regnault, Gregory Aldering, Rahman Amanullah, Pierre Antilogus, Pierre Astier, Kyle Barbary, Marc Betoule, Kyle Robert Boone, Miles Currie, Susana Deustua, Mamoru Doi, Andrew Fruchter, Ariel Goobar, Brian Hayden, Francois Hazenberg, Isobel Hook, Xiaosheng Huang, Jian JiangTakahiro Kato, Alex Kim, Marek Kowalski, Chris Lidman, Eric Linder, Keiichi Maeda, Tomoki Morokuma, Jakob Nordin, Reynald Pain, Saul Perlmutter, Pilar Ruiz-Lapuente, Masao Sako, Clare Myers Saunders, Anthony L. Spadafora, Masaomi Tanaka, Nozomu Tominaga, Naoki Yasuda, Naoki Yoshida

Research output: Contribution to conference › Paper

Abstract

High-redshift type Ia supernovae are crucial for constraining any time variation in dark energy. Here, we present the first discoveries and light curves from the SUbaru Supernovae with Hubble Infrared (SUSHI) program, which combines high-redshift SN discoveries from the Subaru Strategic Program (SSP, as well as other Subaru time) with HST WFC3 IR followup. This program efficiently uses the wide field and high collecting area of Subaru Hyper Suprime-Cam for optical light curves, but still obtains a precision NIR color. We are on track to double the number of well-measured SNe Ia at z > 1.1, triggering on 23 SNe Ia in our first season.

Original language	English
Pages	153.21
Publication status	Published - 1 Jan 2018

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https://ui.adsabs.harvard.edu/abs/2018AAS...23115321R

Cite this

@conference{d121753dc8d94ddaa7b9454c77f2d16e,

title = "High-Redshift SNe with Subaru and HST",

abstract = "High-redshift type Ia supernovae are crucial for constraining any time variation in dark energy. Here, we present the first discoveries and light curves from the SUbaru Supernovae with Hubble Infrared (SUSHI) program, which combines high-redshift SN discoveries from the Subaru Strategic Program (SSP, as well as other Subaru time) with HST WFC3 IR followup. This program efficiently uses the wide field and high collecting area of Subaru Hyper Suprime-Cam for optical light curves, but still obtains a precision NIR color. We are on track to double the number of well-measured SNe Ia at z > 1.1, triggering on 23 SNe Ia in our first season.",

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

year = "2018",

month = jan,

day = "1",

language = "English",

pages = "153.21",

}

Rubin, D, Suzuki, N, Regnault, N, Aldering, G, Amanullah, R, Antilogus, P, Astier, P, Barbary, K, Betoule, M, Boone, KR, Currie, M, Deustua, S, Doi, M, Fruchter, A, Goobar, A, Hayden, B, Hazenberg, F, Hook, I, Huang, X, Jiang, J, Kato, T, Kim, A, Kowalski, M, Lidman, C, Linder, E, Maeda, K, Morokuma, T, Nordin, J, Pain, R, Perlmutter, S, Ruiz-Lapuente, P, Sako, M, Myers Saunders, C, Spadafora, AL, Tanaka, M, Tominaga, N, Yasuda, N & Yoshida, N 2018, 'High-Redshift SNe with Subaru and HST', pp. 153.21. <https://ui.adsabs.harvard.edu/abs/2018AAS...23115321R>

TY - CONF

T1 - High-Redshift SNe with Subaru and HST

AU - Rubin, David

AU - Suzuki, Nao

AU - Regnault, Nicolas

AU - Aldering, Gregory

AU - Amanullah, Rahman

AU - Antilogus, Pierre

AU - Astier, Pierre

AU - Barbary, Kyle

AU - Betoule, Marc

AU - Boone, Kyle Robert

AU - Currie, Miles

AU - Deustua, Susana

AU - Doi, Mamoru

AU - Fruchter, Andrew

AU - Goobar, Ariel

AU - Hayden, Brian

AU - Hazenberg, Francois

AU - Hook, Isobel

AU - Huang, Xiaosheng

AU - Jiang, Jian

AU - Kato, Takahiro

AU - Kim, Alex

AU - Kowalski, Marek

AU - Lidman, Chris

AU - Linder, Eric

AU - Maeda, Keiichi

AU - Morokuma, Tomoki

AU - Nordin, Jakob

AU - Pain, Reynald

AU - Perlmutter, Saul

AU - Ruiz-Lapuente, Pilar

AU - Sako, Masao

AU - Myers Saunders, Clare

AU - Spadafora, Anthony L.

AU - Tanaka, Masaomi

AU - Tominaga, Nozomu

AU - Yasuda, Naoki

AU - Yoshida, Naoki

PY - 2018/1/1

Y1 - 2018/1/1

N2 - High-redshift type Ia supernovae are crucial for constraining any time variation in dark energy. Here, we present the first discoveries and light curves from the SUbaru Supernovae with Hubble Infrared (SUSHI) program, which combines high-redshift SN discoveries from the Subaru Strategic Program (SSP, as well as other Subaru time) with HST WFC3 IR followup. This program efficiently uses the wide field and high collecting area of Subaru Hyper Suprime-Cam for optical light curves, but still obtains a precision NIR color. We are on track to double the number of well-measured SNe Ia at z > 1.1, triggering on 23 SNe Ia in our first season.

AB - High-redshift type Ia supernovae are crucial for constraining any time variation in dark energy. Here, we present the first discoveries and light curves from the SUbaru Supernovae with Hubble Infrared (SUSHI) program, which combines high-redshift SN discoveries from the Subaru Strategic Program (SSP, as well as other Subaru time) with HST WFC3 IR followup. This program efficiently uses the wide field and high collecting area of Subaru Hyper Suprime-Cam for optical light curves, but still obtains a precision NIR color. We are on track to double the number of well-measured SNe Ia at z > 1.1, triggering on 23 SNe Ia in our first season.

M3 - Paper

SP - 153.21

ER -

High-Redshift SNe with Subaru and HST

Abstract

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