We present a detailed overview of the science goals and predictions for the
Prime-Cam receiver being constructed by the CCAT-prime collaboration for
dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST is a
wide-field, 6-m aperture submillimeter telescope being built (first light in
late 2023) by an international consortium of institutions led by Cornell
University and sited at more than 5600 meters on Cerro Chajnantor in northern
Chile. The Prime-Cam receiver is one of two instruments planned for FYST and
will provide unprecedented spectroscopic and broadband measurement capabilities
to address important astrophysical questions ranging from Big Bang cosmology
through reionization and the formation of the first galaxies to star formation
within our own Milky Way galaxy. Prime-Cam on the FYST will have a mapping
speed that is over ten times greater than existing and near-term facilities for
high-redshift science and broadband polarimetric imaging at frequencies above
300 GHz. We describe details of the science program enabled by this system and
our preliminary survey strategies.
Description
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
%0 Generic
%1 collaboration2021ccatprime
%A collaboration, CCAT-Prime
%A Aravena, M.
%A Austermann, J. E.
%A Basu, K.
%A Battaglia, N.
%A Beringue, B.
%A Bertoldi, F.
%A Bigiel, F.
%A Bond, J. R.
%A Breysse, P. C.
%A Broughton, C.
%A Bustos, R.
%A Chapman, S. C.
%A Charmetant, M.
%A Choi, S. K.
%A Chung, D. T.
%A Clark, S. E.
%A Cothard, N. F.
%A Dev, A.
%A Douglas, K.
%A Duell, C. J.
%A Ebina, H.
%A Erler, J.
%A Fich, M.
%A Fissel, L. M.
%A Foreman, S.
%A Gao, J.
%A García, Pablo
%A Giovanelli, R.
%A Haynes, M. P.
%A Hensley, B.
%A Herter, T.
%A Higgins, R.
%A Huber, Z.
%A Hubmayr, J.
%A Johnstone, D.
%A Karoumpis, C.
%A Keating, Laura C.
%A Komatsu, E.
%A Li, Y.
%A Magnelli, Benjamin
%A Matthews, B. C.
%A Meerburg, P. D.
%A Meyers, J.
%A Muralidhara, V.
%A Murray, N. W.
%A Niemack, M. D.
%A Nikola, T.
%A Okada, Y.
%A Riechers, D. A.
%A Rosolowsky, E.
%A Roy, A.
%A Sadavoy, S. I.
%A Schaaf, R.
%A Schilke, P.
%A Scott, D.
%A Simon, R.
%A Sinclair, Adrian K.
%A Sivakoff, G. R.
%A Stacey, G. J.
%A Stutz, Amelia M.
%A Stutzki, J.
%A Tahani, M.
%A Thanjavur, K.
%A Timmermann, R. A.
%A Ullom, J. N.
%A van Engelen, A.
%A Vavagiakis, E. M.
%A Vissers, M. R.
%A Wheeler, J. D.
%A White, S. D. M.
%A Zhu, Y.
%A Zou, B.
%D 2021
%K library
%T CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on
the Fred Young Submillimeter Telescope
%U http://arxiv.org/abs/2107.10364
%X We present a detailed overview of the science goals and predictions for the
Prime-Cam receiver being constructed by the CCAT-prime collaboration for
dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST is a
wide-field, 6-m aperture submillimeter telescope being built (first light in
late 2023) by an international consortium of institutions led by Cornell
University and sited at more than 5600 meters on Cerro Chajnantor in northern
Chile. The Prime-Cam receiver is one of two instruments planned for FYST and
will provide unprecedented spectroscopic and broadband measurement capabilities
to address important astrophysical questions ranging from Big Bang cosmology
through reionization and the formation of the first galaxies to star formation
within our own Milky Way galaxy. Prime-Cam on the FYST will have a mapping
speed that is over ten times greater than existing and near-term facilities for
high-redshift science and broadband polarimetric imaging at frequencies above
300 GHz. We describe details of the science program enabled by this system and
our preliminary survey strategies.
@misc{collaboration2021ccatprime,
abstract = {We present a detailed overview of the science goals and predictions for the
Prime-Cam receiver being constructed by the CCAT-prime collaboration for
dedicated use on the Fred Young Submillimeter Telescope (FYST). The FYST is a
wide-field, 6-m aperture submillimeter telescope being built (first light in
late 2023) by an international consortium of institutions led by Cornell
University and sited at more than 5600 meters on Cerro Chajnantor in northern
Chile. The Prime-Cam receiver is one of two instruments planned for FYST and
will provide unprecedented spectroscopic and broadband measurement capabilities
to address important astrophysical questions ranging from Big Bang cosmology
through reionization and the formation of the first galaxies to star formation
within our own Milky Way galaxy. Prime-Cam on the FYST will have a mapping
speed that is over ten times greater than existing and near-term facilities for
high-redshift science and broadband polarimetric imaging at frequencies above
300 GHz. We describe details of the science program enabled by this system and
our preliminary survey strategies.},
added-at = {2021-07-23T12:01:47.000+0200},
author = {collaboration, CCAT-Prime and Aravena, M. and Austermann, J. E. and Basu, K. and Battaglia, N. and Beringue, B. and Bertoldi, F. and Bigiel, F. and Bond, J. R. and Breysse, P. C. and Broughton, C. and Bustos, R. and Chapman, S. C. and Charmetant, M. and Choi, S. K. and Chung, D. T. and Clark, S. E. and Cothard, N. F. and Dev, A. and Douglas, K. and Duell, C. J. and Ebina, H. and Erler, J. and Fich, M. and Fissel, L. M. and Foreman, S. and Gao, J. and García, Pablo and Giovanelli, R. and Haynes, M. P. and Hensley, B. and Herter, T. and Higgins, R. and Huber, Z. and Hubmayr, J. and Johnstone, D. and Karoumpis, C. and Keating, Laura C. and Komatsu, E. and Li, Y. and Magnelli, Benjamin and Matthews, B. C. and Meerburg, P. D. and Meyers, J. and Muralidhara, V. and Murray, N. W. and Niemack, M. D. and Nikola, T. and Okada, Y. and Riechers, D. A. and Rosolowsky, E. and Roy, A. and Sadavoy, S. I. and Schaaf, R. and Schilke, P. and Scott, D. and Simon, R. and Sinclair, Adrian K. and Sivakoff, G. R. and Stacey, G. J. and Stutz, Amelia M. and Stutzki, J. and Tahani, M. and Thanjavur, K. and Timmermann, R. A. and Ullom, J. N. and van Engelen, A. and Vavagiakis, E. M. and Vissers, M. R. and Wheeler, J. D. and White, S. D. M. and Zhu, Y. and Zou, B.},
biburl = {https://www.bibsonomy.org/bibtex/2cdaa12087be7bd6768227ea4abe31aa2/gpkulkarni},
description = {CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope},
interhash = {42114df3d249f12fd5035e6dd63189db},
intrahash = {cdaa12087be7bd6768227ea4abe31aa2},
keywords = {library},
note = {cite arxiv:2107.10364Comment: 61 pages, 16 figures. Submitted to the Astrophysical Journal July 17, 2021},
timestamp = {2021-07-23T12:01:47.000+0200},
title = {CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on
the Fred Young Submillimeter Telescope},
url = {http://arxiv.org/abs/2107.10364},
year = 2021
}