Gas contents of the low-redshift Universe from the Sunyaev-Zeldovich effect
Event Start:
2019-10-21T15:00:00
Event End:
2019-10-21T16:00:00
Event Information:
The Sunyaev-Zeldovich effect (SZE) provides a promising avenue to explore the properties of gas associated with halos and large-scale structures. However, due to contamination by the primary CMB, as well as foregrounds, projection effects, halo identification, and the beam size of current CMB surveys, it is not a trivial task to extract the signal precisely and accurately.
Event Location:
Hennings 318
Speaker:
Seunghwan Lim
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Event Start:
2019-10-21T15:00:00
Event End:
2019-10-21T16:00:00
Gas contents of the low-redshift Universe from the Sunyaev-Zeldovich effect
Event Information:
The Sunyaev-Zeldovich effect (SZE) provides a promising avenue to explore the properties of gas associated with halos and large-scale structures. However, due to contamination by the primary CMB, as well as foregrounds, projection effects, halo identification, and the beam size of current CMB surveys, it is not a trivial task to extract the signal precisely and accurately.
Event Location:
Hennings 318