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PRODID:-//LBNL Physics Division Research Progress Meetings - ECPv6.8.3//NONSGML v1.0//EN
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X-ORIGINAL-URL:https://rpm.physics.lbl.gov
X-WR-CALDESC:Events for LBNL Physics Division Research Progress Meetings
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BEGIN:VTIMEZONE
TZID:UTC
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TZOFFSETFROM:+0000
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DTSTART:20190101T000000
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BEGIN:VEVENT
DTSTART;TZID=UTC:20191121T160000
DTEND;TZID=UTC:20191121T170000
DTSTAMP:20260416T213211
CREATED:20191022T015801Z
LAST-MODIFIED:20191115T182640Z
UID:1256-1574352000-1574355600@rpm.physics.lbl.gov
SUMMARY:Zhaodi Pan (U. Chicago) "Instrument and science for the SPT-3G cosmic microwave background receiver"
DESCRIPTION:Abstract:\n\nSPT-3G is a third-generation camera for the 10-meter diameter South Pole Telescope (SPT)\, which is designed to measure the cosmic microwave background (CMB). To achieve a high mapping speed\, we have developed a new multichroic receiver with a total of 16\,000 polarization-sensitive detectors. SPT-3G began a 6-year 1500 square degree survey in February 2018\, which will produce measurements of CMB temperature and polarization anisotropies with an unprecedented combination of angular resolution and sensitivity. In this talk\, I will summarize the instrument status and highlight the development of the most compact millimeter-wavelength Fourier transform spectrometer\, which was used for SPT-3G and is also a prototype for the proposed PIXIE satellite. I will also discuss the science goals and current data analyses\, with a focus on the gravitational lensing analysis using SPT-3G’s first-year data.\n 
URL:https://rpm.physics.lbl.gov/event/reserved-71/
LOCATION:HYBRID 50A-5132 (Sessler Conference Room)\, https://lbnl.zoom.us/j/91782268585\, 50A-5132
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