Presentasjon av masteroppgave: Synne Sigstad Jørgensen
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«Scanning Strategy Optimisation for Next-Generation CMB Experiments»
(Abstract not available)
Image caption: The anisotropies of the Cosmic microwave background (CMB) as observed by Planck. The CMB is a snapshot of the oldest light in our Universe, imprinted on the sky when the Universe was just 380 000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities, representing the seeds of all future structure: the stars and galaxies of today. CREDIT: ESA and the Planck Collaboration
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More information: https://www.mn.uio.no/astro/studier/aktuelt/arrangementer/masterpresentasjoner/2026/Synne%20Sigstad%20Jørgensen.html
(Abstract not available)
Image caption: The anisotropies of the Cosmic microwave background (CMB) as observed by Planck. The CMB is a snapshot of the oldest light in our Universe, imprinted on the sky when the Universe was just 380 000 years old. It shows tiny temperature fluctuations that correspond to regions of slightly different densities, representing the seeds of all future structure: the stars and galaxies of today. CREDIT: ESA and the Planck Collaboration
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More information: https://www.mn.uio.no/astro/studier/aktuelt/arrangementer/masterpresentasjoner/2026/Synne%20Sigstad%20Jørgensen.html
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Institute of Theoretical Astrophysics, University of Oslo, Sognsveien 77B, 0855 Oslo, Norge, Oslo, Norway
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Host or PublisherInstitute of Theoretical Astrophysics, University of Oslo
