Sökning: "lensed supernovae"
Hittade 5 avhandlingar innehållade orden lensed supernovae.
1. Supernovae seen through gravitational telescopes
Sammanfattning : Galaxies, and clusters of galaxies, can act as gravitational lenses and magnify the light of objects behind them. The effect enables observations of very distant supernovae, that otherwise would be too faint to be detected by existing telescopes, and allows studies of the frequency and properties of these rare phenomena when the universe was young. LÄS MER
2. Search for lensed supernovae behind the galaxy cluster Abell 1689
Sammanfattning : Distant supernovae probe the history of cosmic expansion and star formation, and provide important information on their progenitor models. Investigation of supernovae type Ia for are needed to reveal any evolution in their intrinsic properties, and thus their utility as existing distance indicators. LÄS MER
3. Observations of distant supernovae and cosmological implications
Sammanfattning : Type Ia supernovae can be used as distance indicators for probing the expansion history of the Universe. The method has proved to be an efficient tool in cosmology and played a decisive role in the discovery of a yet unknown energy form, dark energy, that drives the accelerated expansion of the Universe. LÄS MER
4. Properties of Type Ia Supernovae : From the (intermediate) Palomar Transient Factory
Sammanfattning : Type Ia Supernovae (SNe) have been used to discover the accelerated expansion of the universe but many open questions remain unanswered. These include the stellar progenitor, extinction and possible systematic trends in the supernova brightness for different host galaxy environments or cosmic time. LÄS MER
5. Gravitational lensing as a probe of the first stars and galaxies
Sammanfattning : This thesis investigates the potential for detection and identification of primordial stars, galaxies, and supernovae at high redshift.Simulations indicate that the first Population III stars should appear in minihalos of mass M = 105-106 Msol at z ≈ 10-30. LÄS MER