CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope

CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
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DOI：
10.3847/1538-4365/ac9838
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发表时间：
2021-07
期刊：
The Astrophysical Journal Supplement Series
影响因子：
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通讯作者：
CCAT-Prime Collaboration;M. Aravena;J. Austermann;K. Basu;N. Battaglia;B. Beringue;F. Bertoldi;F. Bigiel;J. Bond;P. Breysse;Colton Broughton;R. Bustos;S. Chapman;Maude Charmetant;Steve K. Choi;D. Chung;S. Clark;N. Cothard;A. Crites;Ankur Dev;K. Douglas;C. Duell;R. Dünner;Haruki Ebina;J. Erler;M. Fich;L. Fissel;S. Foreman;R. Freundt;P. Gallardo;Jiansong Gao;P. García;R. Giovanelli;J. Golec;C. Groppi;M. Haynes;D. Henke;B. Hensley;T. Herter;Ronan Higgins;R. Hložek;A. Huber;Z. Huber;J. Hubmayr;Rebecca Jackson;D. Johnstone;C. Karoumpis;L. Keating;E. Komatsu;Yaqiong Li;B. Magnelli;B. Matthews;P. Mauskopf;J. McMahon;P. Meerburg;Joel Meyers;V. Muralidhara;N. Murray;M. Niemack;T. Nikola;Y. Okada;R. Puddu;D. Riechers;E. Rosolowsky;K. Rossi;K. Rotermund;A. Roy;S. Sadavoy;R. Schaaf;P. Schilke;D. Scott;R. Simon;A. Sinclair;G. Sivakoff;G. Stacey;A. Stutz;J. Stutzki;M. Tahani;K. Thanjavur;R. Timmermann;J. Ullom;A. V. Engelen;E. Vavagiakis;M. Vissers;J. Wheeler;S. White;Yijie Zhu;B. Zou
CCAT-Prime Collaboration;M. Aravena;J. Austermann;K. Basu;N. Battaglia;B. Beringue;F. Bertoldi;F. Bigiel;J. Bond;P. Breysse;Colton Broughton;R. Bustos;S. Chapman;Maude Charmetant;Steve K. Choi;D. Chung;S. Clark;N. Cothard;A. Crites;Ankur Dev;K. Douglas;C. Duell;R. Dünner;Haruki Ebina;J. Erler;M. Fich;L. Fissel;S. Foreman;R. Freundt;P. Gallardo;Jiansong Gao;P. García;R. Giovanelli;J. Golec;C. Groppi;M. Haynes;D. Henke;B. Hensley;T. Herter;Ronan Higgins;R. Hložek;A. Huber;Z. Huber;J. Hubmayr;Rebecca Jackson;D. Johnstone;C. Karoumpis;L. Keating;E. Komatsu;Yaqiong Li;B. Magnelli;B. Matthews;P. Mauskopf;J. McMahon;P. Meerburg;Joel Meyers;V. Muralidhara;N. Murray;M. Niemack;T. Nikola;Y. Okada;R. Puddu;D. Riechers;E. Rosolowsky;K. Rossi;K. Rotermund;A. Roy;S. Sadavoy;R. Schaaf;P. Schilke;D. Scott;R. Simon;A. Sinclair;G. Sivakoff;G. Stacey;A. Stutz;J. Stutzki;M. Tahani;K. Thanjavur;R. Timmermann;J. Ullom;A. V. Engelen;E. Vavagiakis;M. Vissers;J. Wheeler;S. White;Yijie Zhu;B. Zou
中科院分区：
其他
文献类型：
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作者：
CCAT-Prime Collaboration;M. Aravena;J. Austermann;K. Basu;N. Battaglia;B. Beringue;F. Bertoldi;F. Bigiel;J. Bond;P. Breysse;Colton Broughton;R. Bustos;S. Chapman;Maude Charmetant;Steve K. Choi;D. Chung;S. Clark;N. Cothard;A. Crites;Ankur Dev;K. Douglas;C. Duell;R. Dünner;Haruki Ebina;J. Erler;M. Fich;L. Fissel;S. Foreman;R. Freundt;P. Gallardo;Jiansong Gao;P. García;R. Giovanelli;J. Golec;C. Groppi;M. Haynes;D. Henke;B. Hensley;T. Herter;Ronan Higgins;R. Hložek;A. Huber;Z. Huber;J. Hubmayr;Rebecca Jackson;D. Johnstone;C. Karoumpis;L. Keating;E. Komatsu;Yaqiong Li;B. Magnelli;B. Matthews;P. Mauskopf;J. McMahon;P. Meerburg;Joel Meyers;V. Muralidhara;N. Murray;M. Niemack;T. Nikola;Y. Okada;R. Puddu;D. Riechers;E. Rosolowsky;K. Rossi;K. Rotermund;A. Roy;S. Sadavoy;R. Schaaf;P. Schilke;D. Scott;R. Simon;A. Sinclair;G. Sivakoff;G. Stacey;A. Stutz;J. Stutzki;M. Tahani;K. Thanjavur;R. Timmermann;J. Ullom;A. V. Engelen;E. Vavagiakis;M. Vissers;J. Wheeler;S. White;Yijie Zhu;B. Zou

文献摘要

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我们详细概述了由CCAT-prime合作建造的用于弗雷德·杨亚毫米望远镜（FYST）的Prime-Cam直接探测相机-光谱仪的科学目标和预测。FYST是一个宽视场，6米口径的亚毫米望远镜，由康奈尔大学领导的国际机构联盟正在建造（2023年底首次使用），位于智利北部的Cerro Chajnantor，海拔5600多米。Prime-Cam是FYST计划的两种仪器之一，将提供前所未有的光谱和宽带测量能力，以解决重要的天体物理学问题，从大爆炸宇宙学到再电离和第一个星系的形成，再到我们银河系内的恒星形成。FYST上的Prime-Cam的测绘速度将比现有的和近期的高红移科学和300 GHz以上频率的宽带极化成像设备快10倍以上。我们详细描述了由该系统实现的科学计划和我们的初步调查策略。
We present a detailed overview of the science goals and predictions for the Prime-Cam direct-detection camera–spectrometer 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 m on Cerro Chajnantor in northern Chile. Prime-Cam 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. Prime-Cam on the FYST will have a mapping speed that is over 10 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.