%0 Generic %1 chang2019tomography %A Chang, Tzu-Ching %A Beane, Angus %A Dore, Olivier %A Lidz, Adam %A Mas-Ribas, Lluis %A Sun, Guochao %A Alvarez, Marcelo %A Thakur, Ritoban Basu %A Berger, Philippe %A Bethermin, Matthieu %A Bock, Jamie %A Bradford, Charles M. %A Breysse, Patrick %A Burgarella, Denis %A Charmandaris, Vassilis %A Cheng, Yun-Ting %A Cleary, Kieran %A Cooray, Asantha %A Crites, Abigail %A Ewall-Wice, Aaron %A Fan, Xiaohui %A Finkelstein, Steve %A Furlanetto, Steve %A Hewitt, Jacqueline %A Hunacek, Jonathon %A Korngut, Phil %A Kovetz, Ely %A Hallinan, Gregg %A Heneka, Caroline %A Lagache, Guilaine %A Lawrence, Charles %A Lazio, Joseph %A Liu, Adrian %A Marrone, Dan %A Parsons, Aaron %A Readhead, Anthony %A Rhodes, Jason %A Riechers, Dominik %A Seiffert, Michael %A Stacey, Gordon %A Visbal, Eli %A Wu, Hao-Yi %A Zemcov, Michael %A Zheng, Zheng %D 2019 %K library %T Tomography of the Cosmic Dawn and Reionization Eras with Multiple Tracers %U http://arxiv.org/abs/1903.11744 %X The Cosmic Dawn and Reionization epochs remain a fundamental but challenging frontier of astrophysics and cosmology. We advocate a large-scale, multi-tracer approach to develop a comprehensive understanding of the physics that led to the formation and evolution of the first stars and galaxies. We highlight the line intensity mapping technique to trace the multi-phase reionization topology on large scales, and measure reionization history in detail. Besides 21cm, we advocate for Lya tomography mapping during the epoch of Wouthuysen-Field coupling as an additional probe of the cosmic dawn era.

@misc{chang2019tomography, abstract = {The Cosmic Dawn and Reionization epochs remain a fundamental but challenging frontier of astrophysics and cosmology. We advocate a large-scale, multi-tracer approach to develop a comprehensive understanding of the physics that led to the formation and evolution of the first stars and galaxies. We highlight the line intensity mapping technique to trace the multi-phase reionization topology on large scales, and measure reionization history in detail. Besides 21cm, we advocate for Lya tomography mapping during the epoch of Wouthuysen-Field coupling as an additional probe of the cosmic dawn era.}, added-at = {2019-03-29T06:35:13.000+0100}, author = {Chang, Tzu-Ching and Beane, Angus and Dore, Olivier and Lidz, Adam and Mas-Ribas, Lluis and Sun, Guochao and Alvarez, Marcelo and Thakur, Ritoban Basu and Berger, Philippe and Bethermin, Matthieu and Bock, Jamie and Bradford, Charles M. and Breysse, Patrick and Burgarella, Denis and Charmandaris, Vassilis and Cheng, Yun-Ting and Cleary, Kieran and Cooray, Asantha and Crites, Abigail and Ewall-Wice, Aaron and Fan, Xiaohui and Finkelstein, Steve and Furlanetto, Steve and Hewitt, Jacqueline and Hunacek, Jonathon and Korngut, Phil and Kovetz, Ely and Hallinan, Gregg and Heneka, Caroline and Lagache, Guilaine and Lawrence, Charles and Lazio, Joseph and Liu, Adrian and Marrone, Dan and Parsons, Aaron and Readhead, Anthony and Rhodes, Jason and Riechers, Dominik and Seiffert, Michael and Stacey, Gordon and Visbal, Eli and Wu, Hao-Yi and Zemcov, Michael and Zheng, Zheng}, biburl = {https://www.bibsonomy.org/bibtex/29abe445c9318ec9ab91db0778da951aa/gpkulkarni}, description = {Tomography of the Cosmic Dawn and Reionization Eras with Multiple Tracers}, interhash = {f03c03360a9369012c3740983ec2ccb3}, intrahash = {9abe445c9318ec9ab91db0778da951aa}, keywords = {library}, note = {cite arxiv:1903.11744Comment: Astro2020 Science White Paper; 5 pages, 1 figure}, timestamp = {2019-03-29T06:35:13.000+0100}, title = {Tomography of the Cosmic Dawn and Reionization Eras with Multiple Tracers}, url = {http://arxiv.org/abs/1903.11744}, year = 2019 }