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SUMMARY:Dark Energy with the Atacama Cosmology Telescope
DTSTART;VALUE=DATE-TIME:20050524T100000Z
DTEND;VALUE=DATE-TIME:20050524T110000Z
DTSTAMP;VALUE=DATE-TIME:20261113T073115Z
UID:indico-event-1433@indico.ific.uv.es
DESCRIPTION:I will describe an ongoing Cosmic Microwave Background experim
 ent (ACT) designed to measure CMB anisotropies on a scale of 1 arcminute a
 nd discover clusters of galaxies through the Sunyaev-Zeldovich effect. I w
 ill discuss how to unveil the nature of dark energy\, in particular how th
 e shape of the potential of the scalar field that is driving expansion tod
 ay can be reconstructed using ACT observations.\n\nhttps://indico.ific.uv.
 es/event/1433/
LOCATION:Edf. Institutos de Investigación Sala Seminarios IFIC
URL:https://indico.ific.uv.es/event/1433/
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