Besøksadresse
Svein Rosselands hus (kart)
Sem Sælands vei 13
0371
OSLO
Masterpresentasjoner
Tidligere
Tid og sted:
7. juli 2021 10:15–10:45,
via Zoom Webinar
A Modular Framework for Studying Neutron Star Structure and Cooling - With Dark Matter Applications
Tid og sted:
6. juli 2021 10:00–10:30,
via Zoom Webinar
Phantom energy: A planet, an atom and a meson walked into the end of the universe
Tid og sted:
30. juni 2021 10:15–10:45,
via Zoom Webinar
An analysis of non-Gaussian models predicting anomalies in the cosmic microwave background
Tid og sted:
25. juni 2021 12:00–12:30,
via Zoom Webinar
Investigating the large scale structure of the universe: The cosmic web as a probe for cosmological parameters.
Tid og sted:
24. juni 2021 11:00–11:30,
via Zoom Webinar
Low-level Data Analysis, Calibration, and Ground Modeling with COMAP
Tid og sted:
24. juni 2021 10:00–10:30,
via Zoom Webinar
The origin of the [CII] emission in high-redshift galaxies
Tid og sted:
23. juni 2021 12:00–12:30,
via Zoom Webinar
Depicting a Black Hole Merger: A Bridge Between Einstein Toolkit and GYOTO
Tid:
22. juni 2021 10:45
Probing Modified Gravity via Cross-Correlations of Galaxies with Gravitational Waves
Tid og sted:
22. juni 2021 10:00–10:30,
via Zoom Webinar
The Sub-mm Emission of a Major Galaxy Merger
Tid og sted:
15. juni 2021 10:00–10:30,
via Zoom Webinar
High-level data analysis in the COMAP intensity mapping experiment
Tid og sted:
14. juni 2021 10:00–10:30,
via Zoom Webinar
Data Analysis and Systematic Error Mitigation in the COMAP Experiment
Tid og sted:
10. juni 2021 10:00–10:30,
Via Zoom Webinar - Klikk her
Hyperspectral detection of spicules in Ca II K
Tid og sted:
8. juni 2021 10:00–10:30,
Via Zoom Webinar - Klikk her
A Neural Network approach to 3D non-LTE Radiative Transfer
Tid og sted:
4. juni 2021 10:00–10:30,
Via Zoom Webinar - Klikk her
Elements of Monte Carlo Radiative Transfer in Stellar Atmospheres
Tid:
16. nov. 2020 10:15–11:00
Cosmic Acceleration from a Two-Component Dark Matter Superfluid
Tid:
25. juni 2020 11:30–12:00
Time-ordered modelling of Zodiacal Emission in BeyondPlanck
Tid:
25. juni 2020 10:30–11:00
Intensity Contrast as a Function of Underlying Magnetic Field Through the Solar Atmosphere
Tid:
24. juni 2020 10:15–10:45
Tracing the Interstellar Medium using extinction and polarisation
Tid:
17. juni 2020 10:15–10:45
Data selection for intensity mapping experiments using machine learning
Tid:
2. juni 2020 11:30–12:00
Charged Black Hole Mergers: Emissions, Orbital Evolution, Gravitational Waveform and Observer Bias
Tid og sted:
13. des. 2019 12:00–12:30,
Rom 304 (peisestua), Svein Rosselands hus, Blindern
Galactic Chemical Evolution of R-process Elements in Cosmological Simulations
Tid og sted:
3. okt. 2019 10:00–10:30,
Songsveien 77B Milky Way auditorium
Space-based weak gravitational lensing measurements of lensing-selected clusters
Tid og sted:
2. juli 2019 10:15–11:15,
Songsveien 77B Milky Way auditorium
Line-Intensity Mapping with COMAP
Tid og sted:
25. juni 2019 13:00–13:45,
Songsveien 77B Milky Way auditorium
Modelling Lyman-α Emission from Star Forming Galaxies at High Redshift Using Cosmological Simulations
Tid og sted:
17. juni 2019 10:00–10:30,
Songsveien 77B Milky Way auditorium
Time Delays and Microlensing of Gravitationally Lensed Quasars