Difference between revisions of "UChicago-2020: Large Scale Structure Surveys"

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* '''Chihway Chang''': [https://docs.google.com/presentation/d/19_5iFfVxFRBsrKv6FAKtxh6kmyOdxcdfnE6UEhJvv6c/edit?usp=sharing Introduction] (10 min)
 
* '''Chihway Chang''': [https://docs.google.com/presentation/d/19_5iFfVxFRBsrKv6FAKtxh6kmyOdxcdfnE6UEhJvv6c/edit?usp=sharing Introduction] (10 min)
 
* '''Andrina Nicola''': [https://drive.google.com/file/d/1gzCesxfKAkrSP4JXcMiwij7W2LdS_Jz2/view?usp=sharing N x 2pt analysis] (10 min)
 
* '''Andrina Nicola''': [https://drive.google.com/file/d/1gzCesxfKAkrSP4JXcMiwij7W2LdS_Jz2/view?usp=sharing N x 2pt analysis] (10 min)
* '''Emmanuel Schaan''': [https://cmb-s4.org/wiki/images/Schaan_s4_meeting_20200810.pdf Cosmology with kSZ: baryonic effects in weak lensing] [https://drive.google.com/file/d/13Da1m75HlMQNookMtN3Qh9HDwBjNopi-/view?usp=sharing Cosmology with kSZ: baryonic effects in weak lensing] (10 min)
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* '''Emmanuel Schaan''': [https://cmb-s4.org/wiki/images/Schaan_s4_meeting_20200810.pdf Cosmology with kSZ: baryonic effects in weak lensing] (10 min)
 
* '''Srini Raghunathan + Chun-Hao To''': [https://docs.google.com/presentation/d/1uLS1tTI3E_rqoMlKhnyWwTQq392pSNChMQw9cZmMPY8/edit?usp=sharing LSS-clusters connection] (10 min)
 
* '''Srini Raghunathan + Chun-Hao To''': [https://docs.google.com/presentation/d/1uLS1tTI3E_rqoMlKhnyWwTQq392pSNChMQw9cZmMPY8/edit?usp=sharing LSS-clusters connection] (10 min)
 
* '''Marcelo Alvarez, Yuuki Omori, Patricia Larsen''': Correlated simulations update (10 min)
 
* '''Marcelo Alvarez, Yuuki Omori, Patricia Larsen''': Correlated simulations update (10 min)

Revision as of 22:06, 13 August 2020

Synergies of Large Scale Structure Surveys with CMB-S4, Simone Ferraro, Chihway Chang, and Risa Wechsler
We will focus on the synergies of combining tracers of large scale structure as measured at radio through X-ray wavelengths with the wide-field CMB-S4 survey, which will cover ~70% of the sky. We are particularly interested in exploring cosmological analyses that can only be done via the combination of multi-wavelength probes or that are significantly improved through the use of multiple probes (e.g., Nx2 pt, kSZ cosmology, CMB lensing tomography, cosmic shear/WL calibration, cluster cosmology, etc).

Connection Details

Zoom: https://fnal.zoom.us/j/97391022720?pwd=QTE4ZzBzcml4MmlZQ1crWjZib0R1dz09

Time/Date: 10:00am - 11:30am Pacific Time / August 11, 2020

Rapporteurs/Organizers: Simone Ferraro, Chihway Chang, and Risa Wechsler

Agenda

Notes

Real-time notes on this Google doc.