Prospects for detecting dipolar asymmetry in Planck polarization data
Studiearrangementer
Tidligere
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
Tid og sted:
13. juni 2019 10:15–10:45,
Songsveien 77B Milky Way auditorium
Quantized Vortices in Superfluid Dark Matter
Tid og sted:
11. juni 2019 10:15–10:45,
Songsveien 77B Milky Way auditorium
Thermal Dust Emission in the Microwave Frequency Range
Tid og sted:
9. apr. 2019 12:15–12:45,
Sognsveien 77B Milky Way auditorium
Spherical collapse in ΛCDM, Chameleon and Symmetron models
Tid og sted:
15. feb. 2019 09:15–10:45,
Songsveien 77B Milky Way auditorium
Investigating the stability of neutron stars subject to small radial oscillations under the presence of the Symmetron
Tid og sted:
28. nov. 2018 13:00–13:30,
Rom 209 (auditoriet), Svein Rosselands hus
Tid og sted:
21. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
Origins, distribution and kinematics of circumgalactic O VI around L* galaxies
Tid og sted:
20. juni 2018 11:00–11:30,
Rom 209 (auditoriet), Svein Rosselands hus
Multi-layer Observations of Sunspot Waves at High Resolution
Tid og sted:
18. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
Improving the Planck sky maps with Bayesian component separation
Tid og sted:
15. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
Modelling uncertainty of the Rhenium-Osmium cosmic clock
Tid og sted:
14. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
Acceleration of High-Energy Electrons by Magnetic Reconnection in Coronal Nanoflares
Tid og sted:
13. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
On the theory of dark matter superfluidity
Tid og sted:
12. juni 2018 13:00–13:30,
Rom 209 (auditoriet), Svein Rosselands hus
A numerical model for heating by nanoflares in 3D MHD simulations of the solar atmosphere
Tid og sted:
11. juni 2018 10:15–10:45,
Rom 209 (auditoriet), Svein Rosselands hus
Probing Modified Gravity in Cosmic Filaments
Tid og sted:
27. sep. 2017 12:30–13:00,
Rom 209 (auditoriet), Svein Rosselands hus
Testing quadru- and octopolar asymmetry in Planck data.