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UID:3a1c891d-c4d6-49b6-8056-cb044f39ada4@nexttoyou
DTSTAMP:20261107T013914Z
DTSTART:20261112T180000Z
DTEND:20261112T190000Z
SUMMARY:NPA Seminar: Zeeshan Ahmed\, Kavli Institute\, SLAC National Lab a
 nd Stanford
LOCATION:Wright Laboratory WLE 102\, 272 Whitney Avenue\, New Haven\, CT 0
 6511
DESCRIPTION:Talk Title: "Mapping large-scale structure with the Simons Obs
 ervatory: from multiplexed readout to early science"\n\nThe Simons Observ
 atory (SO)\, now in full science operations in Chile\, will drive major a
 dvances in cosmic microwave background (CMB) science over the next decade
 . This talk describes the microwave-multiplexed readout that made SO’s ro
 ughly 100\,000-detector deployment possible\, and highlights preliminary 
 SO collaboration results on CMB lensing that preview the observatory’s 10
 -year survey of large-scale structure.\n\nHost: Laura Newburgh\n\nFull ab
 stract: Ground-based cosmic microwave background (CMB) science will see s
 ignificant advances over the next decade from the Simons Observatory (SO)
  in Chile’s Atacama Desert and the South Pole Observatory (SPO)\, even th
 ough the agencies are not pursuing CMB-S4 for now. SO entered full scienc
 e operations this fall\, and its 6-meter Large Aperture Telescope (LAT) w
 ill map about 60% of the sky at arcminute resolution through 2034\, measu
 ring how the CMB is gravitationally lensed by intervening mass. Together 
 with the Dark Energy Spectroscopic Instrument (DESI) and the Rubin Observ
 atory\, these maps will trace the growth of structure and constrain the s
 um of neutrino masses and the effects of dark energy.\n\nThe survey rests
  on roughly 100\,000 transition-edge sensor (TES) bolometers across SO’s 
 four telescopes\, read out with microwave superconducting quantum interfe
 rence device (SQUID) multiplexing and the SLAC Microresonator RF (SMu\n\n
 http://next-to-u.app/events/3a1c891d-c4d6-49b6-8056-cb044f39ada4
URL:http://next-to-u.app/events/3a1c891d-c4d6-49b6-8056-cb044f39ada4
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