See-Change: an HST program to probe Dark Energy time variation

Brian Hayden; Saul Perlmutter; Jakob Nordin; David Rubin; Chris Lidman; Susana E. Deustua; Andrew S. Fruchter; Greg Scott Aldering; Mark Brodwin; Carlos E. Cunha; Peter R. Eisenhardt; Anthony H. Gonzalez; Myungkook J. Jee; Hendrik Hildebrandt; Henk Hoekstra; Joana Santos; S. Adam Stanford; Daniel Stern; Rene Fassbender; Johan Richard; Piero Rosati; Risa H. Wechsler; Adam Muzzin; Jon Willis; Hans Boehringer; Michael Gladders; Ariel Goobar; Rahman Amanullah; Isobel Hook; Dragan Huterer; Xiaosheng Huang; Alex G. Kim; Marek Kowalski; Eric Linder; Reynald Pain; Clare Saunders; Nao Suzuki; Kyle H. Barbary; Eli S. Rykoff; Joshua Meyers; Caroline Sofiatti; Gillian Wilson; Eduardo Rozo; Matt Hilton; Anthony L. Spadafora

See-Change: an HST program to probe Dark Energy time variation

Brian Hayden, Saul Perlmutter, Jakob Nordin, David Rubin, Chris Lidman, Susana E. Deustua, Andrew S. Fruchter, Greg Scott Aldering, Mark Brodwin, Carlos E. Cunha, Peter R. Eisenhardt, Anthony H. Gonzalez, Myungkook J. Jee, Hendrik Hildebrandt, Henk Hoekstra, Joana Santos, S. Adam Stanford, Daniel Stern, Rene Fassbender, Johan RichardPiero Rosati, Risa H. Wechsler, Adam Muzzin, Jon Willis, Hans Boehringer, Michael Gladders, Ariel Goobar, Rahman Amanullah, Isobel Hook, Dragan Huterer, Xiaosheng Huang, Alex G. Kim, Marek Kowalski, Eric Linder, Reynald Pain, Clare Saunders, Nao Suzuki, Kyle H. Barbary, Eli S. Rykoff, Joshua Meyers, Caroline Sofiatti, Gillian Wilson, Eduardo Rozo, Matt Hilton, Anthony L. Spadafora

Research School of Astronomy & Astrophysics

Research output: Contribution to conference › Paper

Abstract

Using the Hubble Space Telescope, the Supernova Cosmology Project is performing a type Ia supernova search in the highest-redshift, most massive clusters known to date. This program was awarded 174 orbits spanning HST cycles 22-23. It will improve the constraint by a factor of 3 on the Dark Energy equation of state above z ~ 1, allowing an unprecedented probe of Dark Energy time variation. When combined with the improved cluster mass calibration provided by the deep WFC3-IR observations of the clusters, the SNe + clusters observed also will triple the Dark Energy Task Force Figure of Merit. We present the supernova survey strategy and cluster selection criteria, and discuss the first few months of the program.

Original language	English
Pages	255.17
Publication status	Published - 1 Jan 2015

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https://ui.adsabs.harvard.edu/abs/2015AAS...22525517H

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Hayden, B., Perlmutter, S., Nordin, J., Rubin, D., Lidman, C., Deustua, S. E., Fruchter, A. S., Aldering, G. S., Brodwin, M., Cunha, C. E., Eisenhardt, P. R., Gonzalez, A. H., Jee, M. J., Hildebrandt, H., Hoekstra, H., Santos, J., Stanford, S. A., Stern, D., Fassbender, R., ... Spadafora, A. L. (2015). See-Change: an HST program to probe Dark Energy time variation. 255.17. https://ui.adsabs.harvard.edu/abs/2015AAS...22525517H

@conference{4e455151f3724cbdb791a242e2168bdf,

title = "See-Change: an HST program to probe Dark Energy time variation",

abstract = "Using the Hubble Space Telescope, the Supernova Cosmology Project is performing a type Ia supernova search in the highest-redshift, most massive clusters known to date. This program was awarded 174 orbits spanning HST cycles 22-23. It will improve the constraint by a factor of 3 on the Dark Energy equation of state above z \textasciitilde{} 1, allowing an unprecedented probe of Dark Energy time variation. When combined with the improved cluster mass calibration provided by the deep WFC3-IR observations of the clusters, the SNe + clusters observed also will triple the Dark Energy Task Force Figure of Merit. We present the supernova survey strategy and cluster selection criteria, and discuss the first few months of the program.",

author = "Brian Hayden and Saul Perlmutter and Jakob Nordin and David Rubin and Chris Lidman and Deustua, \{Susana E.\} and Fruchter, \{Andrew S.\} and Aldering, \{Greg Scott\} and Mark Brodwin and Cunha, \{Carlos E.\} and Eisenhardt, \{Peter R.\} and Gonzalez, \{Anthony H.\} and Jee, \{Myungkook J.\} and Hendrik Hildebrandt and Henk Hoekstra and Joana Santos and Stanford, \{S. Adam\} and Daniel Stern and Rene Fassbender and Johan Richard and Piero Rosati and Wechsler, \{Risa H.\} and Adam Muzzin and Jon Willis and Hans Boehringer and Michael Gladders and Ariel Goobar and Rahman Amanullah and Isobel Hook and Dragan Huterer and Xiaosheng Huang and Kim, \{Alex G.\} and Marek Kowalski and Eric Linder and Reynald Pain and Clare Saunders and Nao Suzuki and Barbary, \{Kyle H.\} and Rykoff, \{Eli S.\} and Joshua Meyers and Caroline Sofiatti and Gillian Wilson and Eduardo Rozo and Matt Hilton and Spadafora, \{Anthony L.\}",

year = "2015",

month = jan,

day = "1",

language = "English",

pages = "255.17",

}

Hayden, B, Perlmutter, S, Nordin, J, Rubin, D, Lidman, C, Deustua, SE, Fruchter, AS, Aldering, GS, Brodwin, M, Cunha, CE, Eisenhardt, PR, Gonzalez, AH, Jee, MJ, Hildebrandt, H, Hoekstra, H, Santos, J, Stanford, SA, Stern, D, Fassbender, R, Richard, J, Rosati, P, Wechsler, RH, Muzzin, A, Willis, J, Boehringer, H, Gladders, M, Goobar, A, Amanullah, R, Hook, I, Huterer, D, Huang, X, Kim, AG, Kowalski, M, Linder, E, Pain, R, Saunders, C, Suzuki, N, Barbary, KH, Rykoff, ES, Meyers, J, Sofiatti, C, Wilson, G, Rozo, E, Hilton, M & Spadafora, AL 2015, 'See-Change: an HST program to probe Dark Energy time variation', pp. 255.17. <https://ui.adsabs.harvard.edu/abs/2015AAS...22525517H>

TY - CONF

T1 - See-Change: an HST program to probe Dark Energy time variation

AU - Hayden, Brian

AU - Perlmutter, Saul

AU - Nordin, Jakob

AU - Rubin, David

AU - Lidman, Chris

AU - Deustua, Susana E.

AU - Fruchter, Andrew S.

AU - Aldering, Greg Scott

AU - Brodwin, Mark

AU - Cunha, Carlos E.

AU - Eisenhardt, Peter R.

AU - Gonzalez, Anthony H.

AU - Jee, Myungkook J.

AU - Hildebrandt, Hendrik

AU - Hoekstra, Henk

AU - Santos, Joana

AU - Stanford, S. Adam

AU - Stern, Daniel

AU - Fassbender, Rene

AU - Richard, Johan

AU - Rosati, Piero

AU - Wechsler, Risa H.

AU - Muzzin, Adam

AU - Willis, Jon

AU - Boehringer, Hans

AU - Gladders, Michael

AU - Goobar, Ariel

AU - Amanullah, Rahman

AU - Hook, Isobel

AU - Huterer, Dragan

AU - Huang, Xiaosheng

AU - Kim, Alex G.

AU - Kowalski, Marek

AU - Linder, Eric

AU - Pain, Reynald

AU - Saunders, Clare

AU - Suzuki, Nao

AU - Barbary, Kyle H.

AU - Rykoff, Eli S.

AU - Meyers, Joshua

AU - Sofiatti, Caroline

AU - Wilson, Gillian

AU - Rozo, Eduardo

AU - Hilton, Matt

AU - Spadafora, Anthony L.

PY - 2015/1/1

Y1 - 2015/1/1

N2 - Using the Hubble Space Telescope, the Supernova Cosmology Project is performing a type Ia supernova search in the highest-redshift, most massive clusters known to date. This program was awarded 174 orbits spanning HST cycles 22-23. It will improve the constraint by a factor of 3 on the Dark Energy equation of state above z ~ 1, allowing an unprecedented probe of Dark Energy time variation. When combined with the improved cluster mass calibration provided by the deep WFC3-IR observations of the clusters, the SNe + clusters observed also will triple the Dark Energy Task Force Figure of Merit. We present the supernova survey strategy and cluster selection criteria, and discuss the first few months of the program.

AB - Using the Hubble Space Telescope, the Supernova Cosmology Project is performing a type Ia supernova search in the highest-redshift, most massive clusters known to date. This program was awarded 174 orbits spanning HST cycles 22-23. It will improve the constraint by a factor of 3 on the Dark Energy equation of state above z ~ 1, allowing an unprecedented probe of Dark Energy time variation. When combined with the improved cluster mass calibration provided by the deep WFC3-IR observations of the clusters, the SNe + clusters observed also will triple the Dark Energy Task Force Figure of Merit. We present the supernova survey strategy and cluster selection criteria, and discuss the first few months of the program.

M3 - Paper

SP - 255.17

ER -

See-Change: an HST program to probe Dark Energy time variation

Abstract

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